How to prove that $int_0^inftyln^2(x)sin(x^2)dx=frac132sqrtfracpi2(2gamma-pi+ln16)^2$ Announcing the arrival of Valued Associate #679: Cesar Manara Planned maintenance scheduled April 17/18, 2019 at 00:00UTC (8:00pm US/Eastern)Mellin transform of $sin x$ aka $int^infty_0 x^s-1sin x dx $Solving $int_0^infty ln^m(x)sinleft(x^nright):dx$Solving used Real Based Methods: $int_0^x fract^kleft(t^n + aright)^m:dt$Proving $ int_0^infty fracln(t)sqrtte^-t mathrm dt=-sqrtpi(gamma+ln4)$How to prove $int_0^inftyfrace^-left(sqrtx-a/sqrtxright)^2sqrtxdx=sqrtpi,,a>0$?Solve: $int_0^infty left( cos left( … right)+sin left( … right) right) frace^-u^2(u^2+ fracalpha4t)^2 ~mathrmdu$Prove $Gamma^2(1/4)over 4sqrt2pi=prod_n=1^inftyleft(2n+1over 2nright)^(-1)^n+1$Proof $int_-infty^inftyfracdxleft(e^x+e^-x+e^ixsqrt3right)^2=frac13$How do I Evaluate the Integral $int_-infty ^infty frac1e^x^2+1 , dx$?Evaluate $int_0^infty sinleft(frac1xright)sinleft(x^2right),dx$What did I do wrong in calculating $int_-infty^inftyfracsinxxmathrmdx$ via $oint_gammafracsinzzmathrmdz$?How to prove $int_0^+infty fracsin(x)x^s = cos(fracpi s2) Gamma(1-s)$Using the result $g(omega)=frac1sqrt2pifrac2alphaalpha^2 + omega^2$ evaluate $int_-infty^inftyfrac11+x^2e^-ixdx$
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How to prove that $int_0^inftyln^2(x)sin(x^2)dx=frac132sqrtfracpi2(2gamma-pi+ln16)^2$
Announcing the arrival of Valued Associate #679: Cesar Manara
Planned maintenance scheduled April 17/18, 2019 at 00:00UTC (8:00pm US/Eastern)Mellin transform of $sin x$ aka $int^infty_0 x^s-1sin x dx $Solving $int_0^infty ln^m(x)sinleft(x^nright):dx$Solving used Real Based Methods: $int_0^x fract^kleft(t^n + aright)^m:dt$Proving $ int_0^infty fracln(t)sqrtte^-t mathrm dt=-sqrtpi(gamma+ln4)$How to prove $int_0^inftyfrace^-left(sqrtx-a/sqrtxright)^2sqrtxdx=sqrtpi,,a>0$?Solve: $int_0^infty left( cos left( … right)+sin left( … right) right) frace^-u^2(u^2+ fracalpha4t)^2 ~mathrmdu$Prove $Gamma^2(1/4)over 4sqrt2pi=prod_n=1^inftyleft(2n+1over 2nright)^(-1)^n+1$Proof $int_-infty^inftyfracdxleft(e^x+e^-x+e^ixsqrt3right)^2=frac13$How do I Evaluate the Integral $int_-infty ^infty frac1e^x^2+1 , dx$?Evaluate $int_0^infty sinleft(frac1xright)sinleft(x^2right),dx$What did I do wrong in calculating $int_-infty^inftyfracsinxxmathrmdx$ via $oint_gammafracsinzzmathrmdz$?How to prove $int_0^+infty fracsin(x)x^s = cos(fracpi s2) Gamma(1-s)$Using the result $g(omega)=frac1sqrt2pifrac2alphaalpha^2 + omega^2$ evaluate $int_-infty^inftyfrac11+x^2e^-ixdx$
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Wolfram Alpha provides
$$int_0^inftyln^2(x)sin(x^2)dx=frac132sqrtfracpi2(2gamma-pi+ln16)^2tag1$$
But I haven't figured out the way to verify this result.
I know Frullani's Integral
$$ln(x)= int_0^inftyfrace^-t-e^-xttdt$$
I also know
$$int_0^inftysin(x^2)~dx=frac12int_0^inftyx^-1/2sin(x)~dx$$
Then,
$$beginalign
int_0^inftyln^2(x)sin(x^2)dx&=int_0^inftyleft(int_0^inftyfrace^-t-e^-xttdtright)left(int_0^inftyfrace^-n-e^-xnndnright)sin(x^2)~dx\
&=frac12int_0^inftyleft(int_0^inftyfrace^-t-e^-xttdtright)left(int_0^inftyfrace^-n-e^-xnndnright)fracsin(x)sqrtxdx\
&=frac12int_0^inftyint_0^inftyint_0^inftyfrace^-t-e^-xttfrace^-n-e^-xnnfracsin(x)sqrtx~dx~dn~dt\
&=frac12int_0^inftyfrac1tint_0^inftyfrac1nint_0^infty(e^-t-e^-xt)(e^-n-e^-xn)fracsin(x)sqrtx~dx~dn~dt\
&=frac12int_0^inftyfrac1tint_0^inftyfrac1nint_0^infty(e^-t-n-e^-xn-t-e^-xt-n+e^-xt-xn)fracsin(x)sqrtx~dx~dn~dt
endalign$$
What should I do next?
There is also a general case
$$int_0^inftyln^2(x^a)sin(x^2)dx=fraca^232sqrtfracpi2(2gamma-pi+ln16)^2tag2$$
But I think $(2)$ becomes easy to prove if we can prove $(1)$.
calculus integration
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|
show 2 more comments
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Wolfram Alpha provides
$$int_0^inftyln^2(x)sin(x^2)dx=frac132sqrtfracpi2(2gamma-pi+ln16)^2tag1$$
But I haven't figured out the way to verify this result.
I know Frullani's Integral
$$ln(x)= int_0^inftyfrace^-t-e^-xttdt$$
I also know
$$int_0^inftysin(x^2)~dx=frac12int_0^inftyx^-1/2sin(x)~dx$$
Then,
$$beginalign
int_0^inftyln^2(x)sin(x^2)dx&=int_0^inftyleft(int_0^inftyfrace^-t-e^-xttdtright)left(int_0^inftyfrace^-n-e^-xnndnright)sin(x^2)~dx\
&=frac12int_0^inftyleft(int_0^inftyfrace^-t-e^-xttdtright)left(int_0^inftyfrace^-n-e^-xnndnright)fracsin(x)sqrtxdx\
&=frac12int_0^inftyint_0^inftyint_0^inftyfrace^-t-e^-xttfrace^-n-e^-xnnfracsin(x)sqrtx~dx~dn~dt\
&=frac12int_0^inftyfrac1tint_0^inftyfrac1nint_0^infty(e^-t-e^-xt)(e^-n-e^-xn)fracsin(x)sqrtx~dx~dn~dt\
&=frac12int_0^inftyfrac1tint_0^inftyfrac1nint_0^infty(e^-t-n-e^-xn-t-e^-xt-n+e^-xt-xn)fracsin(x)sqrtx~dx~dn~dt
endalign$$
What should I do next?
There is also a general case
$$int_0^inftyln^2(x^a)sin(x^2)dx=fraca^232sqrtfracpi2(2gamma-pi+ln16)^2tag2$$
But I think $(2)$ becomes easy to prove if we can prove $(1)$.
calculus integration
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Computer algebra solves this instantly: $frac132 sqrtfracpi 2 (2 gamma -pi +log (16))^2$. Is there really a need to perform this by hand? ted.com/talks/…
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– David G. Stork
Jan 26 at 20:10
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It is an interesting video. "Hand calculating procedures teach understanding."
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– Larry
Jan 26 at 20:16
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Did you actually watch the full video? One of Wolfram's key points was exposing the fallacy in "hand calculating procedures teach understanding." Very convincing.
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– David G. Stork
Jan 26 at 20:29
2
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@DavidG.Stork I entirely disagree. I personally am interested in knowing how to preform such manual calculations as they teach me new techniques which I can apply to other problems. Also, what is the point of knowing that $int_0^infty ln^2(x)sin(x^2)mathrm dx$ has a closed form (or exact evaluation instead of a decimal expansion) if one cannot prove it? Without a proof it is just a useless fact.
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– clathratus
Jan 26 at 20:51
2
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Ok, I see. That is actually a good point. I will keep that in mind.
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– Larry
Jan 26 at 21:12
|
show 2 more comments
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Wolfram Alpha provides
$$int_0^inftyln^2(x)sin(x^2)dx=frac132sqrtfracpi2(2gamma-pi+ln16)^2tag1$$
But I haven't figured out the way to verify this result.
I know Frullani's Integral
$$ln(x)= int_0^inftyfrace^-t-e^-xttdt$$
I also know
$$int_0^inftysin(x^2)~dx=frac12int_0^inftyx^-1/2sin(x)~dx$$
Then,
$$beginalign
int_0^inftyln^2(x)sin(x^2)dx&=int_0^inftyleft(int_0^inftyfrace^-t-e^-xttdtright)left(int_0^inftyfrace^-n-e^-xnndnright)sin(x^2)~dx\
&=frac12int_0^inftyleft(int_0^inftyfrace^-t-e^-xttdtright)left(int_0^inftyfrace^-n-e^-xnndnright)fracsin(x)sqrtxdx\
&=frac12int_0^inftyint_0^inftyint_0^inftyfrace^-t-e^-xttfrace^-n-e^-xnnfracsin(x)sqrtx~dx~dn~dt\
&=frac12int_0^inftyfrac1tint_0^inftyfrac1nint_0^infty(e^-t-e^-xt)(e^-n-e^-xn)fracsin(x)sqrtx~dx~dn~dt\
&=frac12int_0^inftyfrac1tint_0^inftyfrac1nint_0^infty(e^-t-n-e^-xn-t-e^-xt-n+e^-xt-xn)fracsin(x)sqrtx~dx~dn~dt
endalign$$
What should I do next?
There is also a general case
$$int_0^inftyln^2(x^a)sin(x^2)dx=fraca^232sqrtfracpi2(2gamma-pi+ln16)^2tag2$$
But I think $(2)$ becomes easy to prove if we can prove $(1)$.
calculus integration
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Wolfram Alpha provides
$$int_0^inftyln^2(x)sin(x^2)dx=frac132sqrtfracpi2(2gamma-pi+ln16)^2tag1$$
But I haven't figured out the way to verify this result.
I know Frullani's Integral
$$ln(x)= int_0^inftyfrace^-t-e^-xttdt$$
I also know
$$int_0^inftysin(x^2)~dx=frac12int_0^inftyx^-1/2sin(x)~dx$$
Then,
$$beginalign
int_0^inftyln^2(x)sin(x^2)dx&=int_0^inftyleft(int_0^inftyfrace^-t-e^-xttdtright)left(int_0^inftyfrace^-n-e^-xnndnright)sin(x^2)~dx\
&=frac12int_0^inftyleft(int_0^inftyfrace^-t-e^-xttdtright)left(int_0^inftyfrace^-n-e^-xnndnright)fracsin(x)sqrtxdx\
&=frac12int_0^inftyint_0^inftyint_0^inftyfrace^-t-e^-xttfrace^-n-e^-xnnfracsin(x)sqrtx~dx~dn~dt\
&=frac12int_0^inftyfrac1tint_0^inftyfrac1nint_0^infty(e^-t-e^-xt)(e^-n-e^-xn)fracsin(x)sqrtx~dx~dn~dt\
&=frac12int_0^inftyfrac1tint_0^inftyfrac1nint_0^infty(e^-t-n-e^-xn-t-e^-xt-n+e^-xt-xn)fracsin(x)sqrtx~dx~dn~dt
endalign$$
What should I do next?
There is also a general case
$$int_0^inftyln^2(x^a)sin(x^2)dx=fraca^232sqrtfracpi2(2gamma-pi+ln16)^2tag2$$
But I think $(2)$ becomes easy to prove if we can prove $(1)$.
calculus integration
calculus integration
edited Jan 26 at 20:18
user
6,57011031
6,57011031
asked Jan 26 at 19:48
LarryLarry
2,55031131
2,55031131
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Computer algebra solves this instantly: $frac132 sqrtfracpi 2 (2 gamma -pi +log (16))^2$. Is there really a need to perform this by hand? ted.com/talks/…
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– David G. Stork
Jan 26 at 20:10
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It is an interesting video. "Hand calculating procedures teach understanding."
$endgroup$
– Larry
Jan 26 at 20:16
$begingroup$
Did you actually watch the full video? One of Wolfram's key points was exposing the fallacy in "hand calculating procedures teach understanding." Very convincing.
$endgroup$
– David G. Stork
Jan 26 at 20:29
2
$begingroup$
@DavidG.Stork I entirely disagree. I personally am interested in knowing how to preform such manual calculations as they teach me new techniques which I can apply to other problems. Also, what is the point of knowing that $int_0^infty ln^2(x)sin(x^2)mathrm dx$ has a closed form (or exact evaluation instead of a decimal expansion) if one cannot prove it? Without a proof it is just a useless fact.
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– clathratus
Jan 26 at 20:51
2
$begingroup$
Ok, I see. That is actually a good point. I will keep that in mind.
$endgroup$
– Larry
Jan 26 at 21:12
|
show 2 more comments
$begingroup$
Computer algebra solves this instantly: $frac132 sqrtfracpi 2 (2 gamma -pi +log (16))^2$. Is there really a need to perform this by hand? ted.com/talks/…
$endgroup$
– David G. Stork
Jan 26 at 20:10
$begingroup$
It is an interesting video. "Hand calculating procedures teach understanding."
$endgroup$
– Larry
Jan 26 at 20:16
$begingroup$
Did you actually watch the full video? One of Wolfram's key points was exposing the fallacy in "hand calculating procedures teach understanding." Very convincing.
$endgroup$
– David G. Stork
Jan 26 at 20:29
2
$begingroup$
@DavidG.Stork I entirely disagree. I personally am interested in knowing how to preform such manual calculations as they teach me new techniques which I can apply to other problems. Also, what is the point of knowing that $int_0^infty ln^2(x)sin(x^2)mathrm dx$ has a closed form (or exact evaluation instead of a decimal expansion) if one cannot prove it? Without a proof it is just a useless fact.
$endgroup$
– clathratus
Jan 26 at 20:51
2
$begingroup$
Ok, I see. That is actually a good point. I will keep that in mind.
$endgroup$
– Larry
Jan 26 at 21:12
$begingroup$
Computer algebra solves this instantly: $frac132 sqrtfracpi 2 (2 gamma -pi +log (16))^2$. Is there really a need to perform this by hand? ted.com/talks/…
$endgroup$
– David G. Stork
Jan 26 at 20:10
$begingroup$
Computer algebra solves this instantly: $frac132 sqrtfracpi 2 (2 gamma -pi +log (16))^2$. Is there really a need to perform this by hand? ted.com/talks/…
$endgroup$
– David G. Stork
Jan 26 at 20:10
$begingroup$
It is an interesting video. "Hand calculating procedures teach understanding."
$endgroup$
– Larry
Jan 26 at 20:16
$begingroup$
It is an interesting video. "Hand calculating procedures teach understanding."
$endgroup$
– Larry
Jan 26 at 20:16
$begingroup$
Did you actually watch the full video? One of Wolfram's key points was exposing the fallacy in "hand calculating procedures teach understanding." Very convincing.
$endgroup$
– David G. Stork
Jan 26 at 20:29
$begingroup$
Did you actually watch the full video? One of Wolfram's key points was exposing the fallacy in "hand calculating procedures teach understanding." Very convincing.
$endgroup$
– David G. Stork
Jan 26 at 20:29
2
2
$begingroup$
@DavidG.Stork I entirely disagree. I personally am interested in knowing how to preform such manual calculations as they teach me new techniques which I can apply to other problems. Also, what is the point of knowing that $int_0^infty ln^2(x)sin(x^2)mathrm dx$ has a closed form (or exact evaluation instead of a decimal expansion) if one cannot prove it? Without a proof it is just a useless fact.
$endgroup$
– clathratus
Jan 26 at 20:51
$begingroup$
@DavidG.Stork I entirely disagree. I personally am interested in knowing how to preform such manual calculations as they teach me new techniques which I can apply to other problems. Also, what is the point of knowing that $int_0^infty ln^2(x)sin(x^2)mathrm dx$ has a closed form (or exact evaluation instead of a decimal expansion) if one cannot prove it? Without a proof it is just a useless fact.
$endgroup$
– clathratus
Jan 26 at 20:51
2
2
$begingroup$
Ok, I see. That is actually a good point. I will keep that in mind.
$endgroup$
– Larry
Jan 26 at 21:12
$begingroup$
Ok, I see. That is actually a good point. I will keep that in mind.
$endgroup$
– Larry
Jan 26 at 21:12
|
show 2 more comments
6 Answers
6
active
oldest
votes
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$$I=int_0^inftyln^2(x)sin(x^2)dx oversetx^2=t=int_0^infty frac12sqrt t ln^2 (sqrt t) sin t dt =frac18 int_0^infty t^-1/2sin t ln^2 t ,dt$$
Note that the last integral is the Mellin transform in $s=frac12 $ of the sine after being differentiated twice.
See for example here a proof for:
$$int_0^infty x^s-1sin x dx= Gamma(s) sinleft(fracpi s2right)$$
$$Rightarrow I=frac18fracd^2ds^2Gamma(s) sinleft(fracpi s2right)bigg|_s=frac12$$
It's not the end of the world to differentiate that twice since the digamma function comes in our help.
From the wiki page we have:
$Gamma'(x)=Gamma(x)psi(x)$
$$Rightarrow fracddsGamma(s) sinleft(fracpi s2right)=Gamma(s)psi(s)sinleft(fracpi s2right) +fracpi2Gamma(s)cosleft(fracpi s2right)$$
$$Rightarrow fracd^2ds^2Gamma(s) sinleft(fracpi s2right)=fracddsGamma(s)left(psi(s)sinleft(fracpi s2right)+fracpi2cosleft(fracpi s2right)right)$$
$$=Gamma(x)psi(x)left(psi(s)sinleft(fracpi s2right)+fracpi2cosleft(fracpi s2right)right)+Gamma(s)left(psi_1(x)sinleft(fracpi s2right)+fracpi2Gamma(s)cosleft(fracpi s2right)-fracpi^24sinleft(fracpi s2right)right)$$
And now setting $s=frac12$ we get using $Gammaleft(frac12right)=sqrtpi$, $psileft(frac12 right)=-gamma -2ln 2 $,$ psi_1left(frac12right)=fracpi^22$ the result.
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2
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Note that the identity used by @Zacky applied is a direct application of Ramanujan's Master Theorem: en.wikipedia.org/wiki/Ramanujan%27s_master_theorem
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– user150203
Jan 28 at 9:09
add a comment |
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We have
$$ F(alpha)=int_0^+infty x^alpha sin(x^2),dx = frac12int_0^+infty x^alpha/2-1sin(x),dx\=frac12Gamma(1-alpha/2)int_0^+infty fracdss^alpha/2(s^2+1) $$
by the properties of the Laplace transform. The last integral can be computed through the Beta and Gamma functions, producing
$$ F(alpha) = frac12,Gammaleft(frac1+alpha2right)sinleft(fracpi4(1+alpha)right) $$
for any $alpha$ such that $textRe(alpha)in(-3,1)$. In order to prove the claim, it is enough to apply $lim_alphato 0fracd^2dalpha^2$ to both sides of the last identity and recall the special values of $Gamma,psi$ and $psi'$ at $frac12$.
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add a comment |
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Let us rewrite your integral as
$$int_0^infty ln^2(x)sin(x^2)dx=frac18int_0^infty fracln^2(x)sin(x)sqrtxdx$$
To solve this integral, you can employ the following identity, which holds for any $pin (0,1)$:
$$int_0^infty x^p-1sin(x)dx=Gamma(p)sin(pi p/2)$$
The value of your integral can be obtained from this by differentiating both sides of this equation twice with respect to $p$, moving the derivative inside of the definite integral on the LHS, and making use of the known special values of the Digamma function.
This can be done by hand, but it requires a lot of algebra and would be best left to a CAS, as suggested in the comments.
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add a comment |
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Just a generalization of @Zacky's answer
$$F(a)=int_0^inftylog^2(x^a)sin(x^2)mathrm dx$$
Since $log(x^a)=log(e^alog x)=alog x$,
$$F(a)=a^2int_0^inftylog^2(x)sin(x^2)mathrm dx$$
$$F(a)=a^2F(1)$$
And as @Zacky showed,
$$F(1)=frac18mathrmD^2_s=frac12Gamma(s)sinfracpi s2=frac132sqrtfracpi2(2gamma-pi+log16)^2$$
So
$$F(a)=fraca^232sqrtfracpi2(2gamma-pi+log16)^2$$
I will edit my answer to include a proof of my own once I find one.
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Nice, I forgot the fact that $log(x^a)=alog(x)$.
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– Larry
Jan 26 at 21:14
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@Larry I legitimately can't tell if you're being sarcastic or not
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– clathratus
Jan 26 at 21:15
1
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I am not being sarcastic.
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– Larry
Jan 26 at 21:18
1
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@Larry Thank you for the clarification. You were very right when you mentioned that $(2)$ would be easy to prove once one had proven $(1)$.
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– clathratus
Jan 26 at 21:20
add a comment |
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An alternative approach is to employ Feynman's Trick and Laplace Transforms to solve:
beginequation
I = int_0^inftyln^2(x)sinleft(x^2right):dx
endequation
We first observe that:
beginequation
I = int_0^inftyln^2(x)sinleft(x^2right):dx = lim_krightarrow 0^+ fracd^2dk^2int_0^infty x^ksinleft(x^2right):dx = lim_krightarrow 0^+ fracd^2dk^2 H(k)
endequation
We proceed by solving $H(k)$. To do so, we introduce a new parameter $'t'$:
beginequation
J(t; k) = int_0^infty x^ksinleft(tx^2right):dx
endequation
(This is allowable through the Dominated Convergence Theorem). Thus:
beginequation
H(k) = lim_trightarrow 1^+ J(t; k)
endequation
Using Fubini's Theorem we now take the Laplace Transform with respect to '$t$'
beginalign
mathscrL_tleft[J(t;k) right] &= int_0^infty x^kmathscrL_tleft[sinleft(tx^2right)right]:dx = int_0^infty fracx^k + 2s^2 + x^4:dx
endalign
As I address here we find this becomes:
beginalign
mathscrL_tleft[J(t;k) right] &= frac14cdot left(s^2right)^frack + 2 + 12 - 1 cdot Bleft(1 - frack + 2 + 1 4, frack + 2 + 1 4 right) = frac14 s^frack - 12 Bleft(1 - frack + 34 , frack + 34right)
endalign
Using the relationship between the Gamma and Beta Function we find:
beginequation
mathscrL_tleft[J(t;k) right] = frac14 s^frack - 12 Gammaleft(1 - frack + 34right) Gammaleft( frack + 34right)
endequation
Using Euler's Reflection Formula we find:
beginequation
mathscrL_tleft[J(t;k) right] = frac14 s^frack - 12 fracpisinleft(pileft(frack + 34right) right)
endequation
Taking the inverse Laplace Transforms is rather tricky here. To evaluate recall that:
beginequation
I = lim_krightarrow 0^+ fracd^2dk^2 H(k) = lim_krightarrow 0^+ fracd^2dk^2left[ lim_trightarrow 1^+ J(t;k)right]
endequation
In this process we solve for $H(k)$ using
beginequation
H(k) = lim_trightarrow 1^+ mathscrL_s^-1left[mathscrL_tleft[J(t; k)right]right]
endequation
Thus, our definition of $I$ becomes:
beginalign
I &= lim_krightarrow 0^+ fracd^2dk^2 H(k) = lim_krightarrow 0^+ fracd^2dk^2left[ lim_trightarrow 1^+ J(t;k)right] = lim_krightarrow 0^+ fracd^2dk^2left[ lim_trightarrow 1^+ mathscrL_s^-1left[mathscrL_tleft[J(t; k)right]right]right] \
&= lim_trightarrow 1^+ mathscrL_s^-1left[ lim_krightarrow 0^+ fracd^2dk^2mathscrL_tleft[J(t; k)right]right] = lim_trightarrow 1^+ mathscrL_s^-1left[ lim_krightarrow 0^+ fracd^2dk^2left[ frac14 s^frack - 12 fracpisinleft(pileft(frack + 34right) right)right]right]
endalign
Because I'm lazy, I used Wolframalpha to evaluate the second derivate at $0$:
beginalign
I &= lim_trightarrow 1^+ mathscrL_s^-1left[ lim_krightarrow 0^+ fracd^2dk^2left[ frac14 s^frack - 12 fracpisinleft(pileft(frack + 34right) right)right]right] = lim_trightarrow 1^+ mathscrL_s^-1left[ fracpi4left( frac3pi^28sqrt2sqrts + fracln^2(s)2sqrt2sqrts + fracpiln(s)2sqrt2sqrtsright)right] \
&= lim_trightarrow 1^+ left[ frac3pi^332sqrt2 mathscrL_s^-1left[ frac1sqrtsright] + fracpi8sqrt2 mathscrL_s^-1left[ fracln^2(s)sqrtsright]+ fracpi^28sqrt2 mathscrL_s^-1left[ fracln(s)sqrtsright]right] \
&= lim_trightarrow 1^+ left[ frac3pi^332sqrt2 left[ frac1sqrtpisqrttright] + fracpi32sqrt2 left[ frac
left(psi^(0)left(frac12right)-ln(t)right)^2 -fracpi^22sqrtpisqrttright]+ fracpi^216sqrt2 left[ frac
psi^(0)left(frac12right)-ln(t)sqrtpisqrttright]right] \
&= frac3pi^332sqrt2 left[ frac1sqrtpiright] + fracpi32sqrt2 left[ frac
psi^(0)left(frac12right)^2 -fracpi^22sqrtpiright]+ fracpi^216sqrt2 left[ frac
psi^(0)left(frac12right)sqrtpiright]
endalign
Noting that
beginequation
psi^(0)left(frac12right) = -gamma - 2ln(2)
endequation
Where $gamma$ is the Euler–Mascheroni constant.
Thus,
beginalign
I = frac3pi^332sqrt2 left[ frac1sqrtpiright] + fracpi32sqrt2 left[ frac
left(gamma + 2ln(2)right)^2 -fracpi^22sqrtpiright]+ fracpi^216sqrt2 left[ frac
gamma - 2ln(2)sqrtpiright] = frac132sqrtfracpi2(2gamma-pi+4ln2)^2
endalign
$endgroup$
$begingroup$
Very nice solution! I am a fan of your method.
$endgroup$
– clathratus
Jan 28 at 16:07
$begingroup$
Do you use a similar technique to evaluate $$F(n)=int_0^infty cos(x^n)mathrm dx$$
$endgroup$
– clathratus
Feb 6 at 20:58
$begingroup$
@clathratus You definitely can
$endgroup$
– user150203
Feb 7 at 0:09
add a comment |
$begingroup$
$newcommandbbx[1],bbox[15px,border:1px groove navy]displaystyle#1,
newcommandbraces[1]leftlbrace,#1,rightrbrace
newcommandbracks[1]leftlbrack,#1,rightrbrack
newcommandddmathrmd
newcommandds[1]displaystyle#1
newcommandexpo[1],mathrme^#1,
newcommandicmathrmi
newcommandmc[1]mathcal#1
newcommandmrm[1]mathrm#1
newcommandpars[1]left(,#1,right)
newcommandpartiald[3][]fracpartial^#1 #2partial #3^#1
newcommandroot[2][],sqrt[#1],#2,,
newcommandtotald[3][]fracmathrmd^#1 #2mathrmd #3^#1
newcommandverts[1]leftvert,#1,rightvert$
With $dsR > 0$ and $dsnu in pars0,1$:
beginalign
&bbox[10px,#ffd]int_0^Rx^nuexpparsic x^2dd x
\[5mm] = &
-int_0^pi/4parsRexpoic theta^nu
expparsic R^2expo2icthetaRexpoicthetaic,ddtheta -
int_R^0parsrexpoicpi/4^nu
expparsicbracksrexpoicpi/4^2expoicpi/4,dd r
\[8mm] = &
-overbraceR^nu + 1,icint_0^pi/4
expparsicbracksnutheta + R^2cospars2theta + theta
exppars-R^2sinpars2thetaddtheta^dsequiv mcIparsR,nu
\[2mm] + &
expoicparsnu + 1pi/4int_0^Rr^nuexpo-r^2dd r
endalign
Since $dsnu in pars0,1$, note that
beginalign
0 & < vertsmcIparsR,nu <
R^nu + 1int_0^pi/4expo-4R^2theta/piddtheta =
pi over 4,1 - exppars-R^2 over R^1 - nu
,,,stackrelmrmas R to inftyLARGEto,,,
colorredlarge 0
endalign
Then,
beginalign
&bbox[10px,#ffd]int_0^inftyx^nusinparsx^2dd x =
sinparsbracksnu + 1,pi over 4
int_0^inftyr^nuexpo-r^2dd r
\[5mm] stackrelr^2 mapsto r=,,,&
1 over 2,sinparsbracksnu + 1,pi over 4
int_0^inftyr^nu/2 - 1/2expo-rdd r =
1 over 2,sinparsbracksnu + 1,pi over 4
Gammaparsnu over 2 + 1 over 2
endalign
and
beginalign
&bbox[10px,#ffd]int_0^inftyln^2parsxsinparsx^2dd x =
lim_nu to 0^+
totald[2]nu
braces1 over 2,sinparsbracksnu + 1,pi over 4
Gammaparsnu over 2 + 1 over 2
\[5mm] = &
bbx1 over 32rootpi over 2
bracksvphantomLarge A2gamma - pi + lnpars16^2 approx 0.0242
endalign
$endgroup$
add a comment |
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6 Answers
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$begingroup$
$$I=int_0^inftyln^2(x)sin(x^2)dx oversetx^2=t=int_0^infty frac12sqrt t ln^2 (sqrt t) sin t dt =frac18 int_0^infty t^-1/2sin t ln^2 t ,dt$$
Note that the last integral is the Mellin transform in $s=frac12 $ of the sine after being differentiated twice.
See for example here a proof for:
$$int_0^infty x^s-1sin x dx= Gamma(s) sinleft(fracpi s2right)$$
$$Rightarrow I=frac18fracd^2ds^2Gamma(s) sinleft(fracpi s2right)bigg|_s=frac12$$
It's not the end of the world to differentiate that twice since the digamma function comes in our help.
From the wiki page we have:
$Gamma'(x)=Gamma(x)psi(x)$
$$Rightarrow fracddsGamma(s) sinleft(fracpi s2right)=Gamma(s)psi(s)sinleft(fracpi s2right) +fracpi2Gamma(s)cosleft(fracpi s2right)$$
$$Rightarrow fracd^2ds^2Gamma(s) sinleft(fracpi s2right)=fracddsGamma(s)left(psi(s)sinleft(fracpi s2right)+fracpi2cosleft(fracpi s2right)right)$$
$$=Gamma(x)psi(x)left(psi(s)sinleft(fracpi s2right)+fracpi2cosleft(fracpi s2right)right)+Gamma(s)left(psi_1(x)sinleft(fracpi s2right)+fracpi2Gamma(s)cosleft(fracpi s2right)-fracpi^24sinleft(fracpi s2right)right)$$
And now setting $s=frac12$ we get using $Gammaleft(frac12right)=sqrtpi$, $psileft(frac12 right)=-gamma -2ln 2 $,$ psi_1left(frac12right)=fracpi^22$ the result.
$endgroup$
2
$begingroup$
Note that the identity used by @Zacky applied is a direct application of Ramanujan's Master Theorem: en.wikipedia.org/wiki/Ramanujan%27s_master_theorem
$endgroup$
– user150203
Jan 28 at 9:09
add a comment |
$begingroup$
$$I=int_0^inftyln^2(x)sin(x^2)dx oversetx^2=t=int_0^infty frac12sqrt t ln^2 (sqrt t) sin t dt =frac18 int_0^infty t^-1/2sin t ln^2 t ,dt$$
Note that the last integral is the Mellin transform in $s=frac12 $ of the sine after being differentiated twice.
See for example here a proof for:
$$int_0^infty x^s-1sin x dx= Gamma(s) sinleft(fracpi s2right)$$
$$Rightarrow I=frac18fracd^2ds^2Gamma(s) sinleft(fracpi s2right)bigg|_s=frac12$$
It's not the end of the world to differentiate that twice since the digamma function comes in our help.
From the wiki page we have:
$Gamma'(x)=Gamma(x)psi(x)$
$$Rightarrow fracddsGamma(s) sinleft(fracpi s2right)=Gamma(s)psi(s)sinleft(fracpi s2right) +fracpi2Gamma(s)cosleft(fracpi s2right)$$
$$Rightarrow fracd^2ds^2Gamma(s) sinleft(fracpi s2right)=fracddsGamma(s)left(psi(s)sinleft(fracpi s2right)+fracpi2cosleft(fracpi s2right)right)$$
$$=Gamma(x)psi(x)left(psi(s)sinleft(fracpi s2right)+fracpi2cosleft(fracpi s2right)right)+Gamma(s)left(psi_1(x)sinleft(fracpi s2right)+fracpi2Gamma(s)cosleft(fracpi s2right)-fracpi^24sinleft(fracpi s2right)right)$$
And now setting $s=frac12$ we get using $Gammaleft(frac12right)=sqrtpi$, $psileft(frac12 right)=-gamma -2ln 2 $,$ psi_1left(frac12right)=fracpi^22$ the result.
$endgroup$
2
$begingroup$
Note that the identity used by @Zacky applied is a direct application of Ramanujan's Master Theorem: en.wikipedia.org/wiki/Ramanujan%27s_master_theorem
$endgroup$
– user150203
Jan 28 at 9:09
add a comment |
$begingroup$
$$I=int_0^inftyln^2(x)sin(x^2)dx oversetx^2=t=int_0^infty frac12sqrt t ln^2 (sqrt t) sin t dt =frac18 int_0^infty t^-1/2sin t ln^2 t ,dt$$
Note that the last integral is the Mellin transform in $s=frac12 $ of the sine after being differentiated twice.
See for example here a proof for:
$$int_0^infty x^s-1sin x dx= Gamma(s) sinleft(fracpi s2right)$$
$$Rightarrow I=frac18fracd^2ds^2Gamma(s) sinleft(fracpi s2right)bigg|_s=frac12$$
It's not the end of the world to differentiate that twice since the digamma function comes in our help.
From the wiki page we have:
$Gamma'(x)=Gamma(x)psi(x)$
$$Rightarrow fracddsGamma(s) sinleft(fracpi s2right)=Gamma(s)psi(s)sinleft(fracpi s2right) +fracpi2Gamma(s)cosleft(fracpi s2right)$$
$$Rightarrow fracd^2ds^2Gamma(s) sinleft(fracpi s2right)=fracddsGamma(s)left(psi(s)sinleft(fracpi s2right)+fracpi2cosleft(fracpi s2right)right)$$
$$=Gamma(x)psi(x)left(psi(s)sinleft(fracpi s2right)+fracpi2cosleft(fracpi s2right)right)+Gamma(s)left(psi_1(x)sinleft(fracpi s2right)+fracpi2Gamma(s)cosleft(fracpi s2right)-fracpi^24sinleft(fracpi s2right)right)$$
And now setting $s=frac12$ we get using $Gammaleft(frac12right)=sqrtpi$, $psileft(frac12 right)=-gamma -2ln 2 $,$ psi_1left(frac12right)=fracpi^22$ the result.
$endgroup$
$$I=int_0^inftyln^2(x)sin(x^2)dx oversetx^2=t=int_0^infty frac12sqrt t ln^2 (sqrt t) sin t dt =frac18 int_0^infty t^-1/2sin t ln^2 t ,dt$$
Note that the last integral is the Mellin transform in $s=frac12 $ of the sine after being differentiated twice.
See for example here a proof for:
$$int_0^infty x^s-1sin x dx= Gamma(s) sinleft(fracpi s2right)$$
$$Rightarrow I=frac18fracd^2ds^2Gamma(s) sinleft(fracpi s2right)bigg|_s=frac12$$
It's not the end of the world to differentiate that twice since the digamma function comes in our help.
From the wiki page we have:
$Gamma'(x)=Gamma(x)psi(x)$
$$Rightarrow fracddsGamma(s) sinleft(fracpi s2right)=Gamma(s)psi(s)sinleft(fracpi s2right) +fracpi2Gamma(s)cosleft(fracpi s2right)$$
$$Rightarrow fracd^2ds^2Gamma(s) sinleft(fracpi s2right)=fracddsGamma(s)left(psi(s)sinleft(fracpi s2right)+fracpi2cosleft(fracpi s2right)right)$$
$$=Gamma(x)psi(x)left(psi(s)sinleft(fracpi s2right)+fracpi2cosleft(fracpi s2right)right)+Gamma(s)left(psi_1(x)sinleft(fracpi s2right)+fracpi2Gamma(s)cosleft(fracpi s2right)-fracpi^24sinleft(fracpi s2right)right)$$
And now setting $s=frac12$ we get using $Gammaleft(frac12right)=sqrtpi$, $psileft(frac12 right)=-gamma -2ln 2 $,$ psi_1left(frac12right)=fracpi^22$ the result.
answered Jan 26 at 20:24
ZackyZacky
7,87511062
7,87511062
2
$begingroup$
Note that the identity used by @Zacky applied is a direct application of Ramanujan's Master Theorem: en.wikipedia.org/wiki/Ramanujan%27s_master_theorem
$endgroup$
– user150203
Jan 28 at 9:09
add a comment |
2
$begingroup$
Note that the identity used by @Zacky applied is a direct application of Ramanujan's Master Theorem: en.wikipedia.org/wiki/Ramanujan%27s_master_theorem
$endgroup$
– user150203
Jan 28 at 9:09
2
2
$begingroup$
Note that the identity used by @Zacky applied is a direct application of Ramanujan's Master Theorem: en.wikipedia.org/wiki/Ramanujan%27s_master_theorem
$endgroup$
– user150203
Jan 28 at 9:09
$begingroup$
Note that the identity used by @Zacky applied is a direct application of Ramanujan's Master Theorem: en.wikipedia.org/wiki/Ramanujan%27s_master_theorem
$endgroup$
– user150203
Jan 28 at 9:09
add a comment |
$begingroup$
We have
$$ F(alpha)=int_0^+infty x^alpha sin(x^2),dx = frac12int_0^+infty x^alpha/2-1sin(x),dx\=frac12Gamma(1-alpha/2)int_0^+infty fracdss^alpha/2(s^2+1) $$
by the properties of the Laplace transform. The last integral can be computed through the Beta and Gamma functions, producing
$$ F(alpha) = frac12,Gammaleft(frac1+alpha2right)sinleft(fracpi4(1+alpha)right) $$
for any $alpha$ such that $textRe(alpha)in(-3,1)$. In order to prove the claim, it is enough to apply $lim_alphato 0fracd^2dalpha^2$ to both sides of the last identity and recall the special values of $Gamma,psi$ and $psi'$ at $frac12$.
$endgroup$
add a comment |
$begingroup$
We have
$$ F(alpha)=int_0^+infty x^alpha sin(x^2),dx = frac12int_0^+infty x^alpha/2-1sin(x),dx\=frac12Gamma(1-alpha/2)int_0^+infty fracdss^alpha/2(s^2+1) $$
by the properties of the Laplace transform. The last integral can be computed through the Beta and Gamma functions, producing
$$ F(alpha) = frac12,Gammaleft(frac1+alpha2right)sinleft(fracpi4(1+alpha)right) $$
for any $alpha$ such that $textRe(alpha)in(-3,1)$. In order to prove the claim, it is enough to apply $lim_alphato 0fracd^2dalpha^2$ to both sides of the last identity and recall the special values of $Gamma,psi$ and $psi'$ at $frac12$.
$endgroup$
add a comment |
$begingroup$
We have
$$ F(alpha)=int_0^+infty x^alpha sin(x^2),dx = frac12int_0^+infty x^alpha/2-1sin(x),dx\=frac12Gamma(1-alpha/2)int_0^+infty fracdss^alpha/2(s^2+1) $$
by the properties of the Laplace transform. The last integral can be computed through the Beta and Gamma functions, producing
$$ F(alpha) = frac12,Gammaleft(frac1+alpha2right)sinleft(fracpi4(1+alpha)right) $$
for any $alpha$ such that $textRe(alpha)in(-3,1)$. In order to prove the claim, it is enough to apply $lim_alphato 0fracd^2dalpha^2$ to both sides of the last identity and recall the special values of $Gamma,psi$ and $psi'$ at $frac12$.
$endgroup$
We have
$$ F(alpha)=int_0^+infty x^alpha sin(x^2),dx = frac12int_0^+infty x^alpha/2-1sin(x),dx\=frac12Gamma(1-alpha/2)int_0^+infty fracdss^alpha/2(s^2+1) $$
by the properties of the Laplace transform. The last integral can be computed through the Beta and Gamma functions, producing
$$ F(alpha) = frac12,Gammaleft(frac1+alpha2right)sinleft(fracpi4(1+alpha)right) $$
for any $alpha$ such that $textRe(alpha)in(-3,1)$. In order to prove the claim, it is enough to apply $lim_alphato 0fracd^2dalpha^2$ to both sides of the last identity and recall the special values of $Gamma,psi$ and $psi'$ at $frac12$.
answered Jan 26 at 20:23
Jack D'AurizioJack D'Aurizio
292k33284673
292k33284673
add a comment |
add a comment |
$begingroup$
Let us rewrite your integral as
$$int_0^infty ln^2(x)sin(x^2)dx=frac18int_0^infty fracln^2(x)sin(x)sqrtxdx$$
To solve this integral, you can employ the following identity, which holds for any $pin (0,1)$:
$$int_0^infty x^p-1sin(x)dx=Gamma(p)sin(pi p/2)$$
The value of your integral can be obtained from this by differentiating both sides of this equation twice with respect to $p$, moving the derivative inside of the definite integral on the LHS, and making use of the known special values of the Digamma function.
This can be done by hand, but it requires a lot of algebra and would be best left to a CAS, as suggested in the comments.
$endgroup$
add a comment |
$begingroup$
Let us rewrite your integral as
$$int_0^infty ln^2(x)sin(x^2)dx=frac18int_0^infty fracln^2(x)sin(x)sqrtxdx$$
To solve this integral, you can employ the following identity, which holds for any $pin (0,1)$:
$$int_0^infty x^p-1sin(x)dx=Gamma(p)sin(pi p/2)$$
The value of your integral can be obtained from this by differentiating both sides of this equation twice with respect to $p$, moving the derivative inside of the definite integral on the LHS, and making use of the known special values of the Digamma function.
This can be done by hand, but it requires a lot of algebra and would be best left to a CAS, as suggested in the comments.
$endgroup$
add a comment |
$begingroup$
Let us rewrite your integral as
$$int_0^infty ln^2(x)sin(x^2)dx=frac18int_0^infty fracln^2(x)sin(x)sqrtxdx$$
To solve this integral, you can employ the following identity, which holds for any $pin (0,1)$:
$$int_0^infty x^p-1sin(x)dx=Gamma(p)sin(pi p/2)$$
The value of your integral can be obtained from this by differentiating both sides of this equation twice with respect to $p$, moving the derivative inside of the definite integral on the LHS, and making use of the known special values of the Digamma function.
This can be done by hand, but it requires a lot of algebra and would be best left to a CAS, as suggested in the comments.
$endgroup$
Let us rewrite your integral as
$$int_0^infty ln^2(x)sin(x^2)dx=frac18int_0^infty fracln^2(x)sin(x)sqrtxdx$$
To solve this integral, you can employ the following identity, which holds for any $pin (0,1)$:
$$int_0^infty x^p-1sin(x)dx=Gamma(p)sin(pi p/2)$$
The value of your integral can be obtained from this by differentiating both sides of this equation twice with respect to $p$, moving the derivative inside of the definite integral on the LHS, and making use of the known special values of the Digamma function.
This can be done by hand, but it requires a lot of algebra and would be best left to a CAS, as suggested in the comments.
answered Jan 26 at 20:17
FrpzzdFrpzzd
23k841112
23k841112
add a comment |
add a comment |
$begingroup$
Just a generalization of @Zacky's answer
$$F(a)=int_0^inftylog^2(x^a)sin(x^2)mathrm dx$$
Since $log(x^a)=log(e^alog x)=alog x$,
$$F(a)=a^2int_0^inftylog^2(x)sin(x^2)mathrm dx$$
$$F(a)=a^2F(1)$$
And as @Zacky showed,
$$F(1)=frac18mathrmD^2_s=frac12Gamma(s)sinfracpi s2=frac132sqrtfracpi2(2gamma-pi+log16)^2$$
So
$$F(a)=fraca^232sqrtfracpi2(2gamma-pi+log16)^2$$
I will edit my answer to include a proof of my own once I find one.
$endgroup$
$begingroup$
Nice, I forgot the fact that $log(x^a)=alog(x)$.
$endgroup$
– Larry
Jan 26 at 21:14
$begingroup$
@Larry I legitimately can't tell if you're being sarcastic or not
$endgroup$
– clathratus
Jan 26 at 21:15
1
$begingroup$
I am not being sarcastic.
$endgroup$
– Larry
Jan 26 at 21:18
1
$begingroup$
@Larry Thank you for the clarification. You were very right when you mentioned that $(2)$ would be easy to prove once one had proven $(1)$.
$endgroup$
– clathratus
Jan 26 at 21:20
add a comment |
$begingroup$
Just a generalization of @Zacky's answer
$$F(a)=int_0^inftylog^2(x^a)sin(x^2)mathrm dx$$
Since $log(x^a)=log(e^alog x)=alog x$,
$$F(a)=a^2int_0^inftylog^2(x)sin(x^2)mathrm dx$$
$$F(a)=a^2F(1)$$
And as @Zacky showed,
$$F(1)=frac18mathrmD^2_s=frac12Gamma(s)sinfracpi s2=frac132sqrtfracpi2(2gamma-pi+log16)^2$$
So
$$F(a)=fraca^232sqrtfracpi2(2gamma-pi+log16)^2$$
I will edit my answer to include a proof of my own once I find one.
$endgroup$
$begingroup$
Nice, I forgot the fact that $log(x^a)=alog(x)$.
$endgroup$
– Larry
Jan 26 at 21:14
$begingroup$
@Larry I legitimately can't tell if you're being sarcastic or not
$endgroup$
– clathratus
Jan 26 at 21:15
1
$begingroup$
I am not being sarcastic.
$endgroup$
– Larry
Jan 26 at 21:18
1
$begingroup$
@Larry Thank you for the clarification. You were very right when you mentioned that $(2)$ would be easy to prove once one had proven $(1)$.
$endgroup$
– clathratus
Jan 26 at 21:20
add a comment |
$begingroup$
Just a generalization of @Zacky's answer
$$F(a)=int_0^inftylog^2(x^a)sin(x^2)mathrm dx$$
Since $log(x^a)=log(e^alog x)=alog x$,
$$F(a)=a^2int_0^inftylog^2(x)sin(x^2)mathrm dx$$
$$F(a)=a^2F(1)$$
And as @Zacky showed,
$$F(1)=frac18mathrmD^2_s=frac12Gamma(s)sinfracpi s2=frac132sqrtfracpi2(2gamma-pi+log16)^2$$
So
$$F(a)=fraca^232sqrtfracpi2(2gamma-pi+log16)^2$$
I will edit my answer to include a proof of my own once I find one.
$endgroup$
Just a generalization of @Zacky's answer
$$F(a)=int_0^inftylog^2(x^a)sin(x^2)mathrm dx$$
Since $log(x^a)=log(e^alog x)=alog x$,
$$F(a)=a^2int_0^inftylog^2(x)sin(x^2)mathrm dx$$
$$F(a)=a^2F(1)$$
And as @Zacky showed,
$$F(1)=frac18mathrmD^2_s=frac12Gamma(s)sinfracpi s2=frac132sqrtfracpi2(2gamma-pi+log16)^2$$
So
$$F(a)=fraca^232sqrtfracpi2(2gamma-pi+log16)^2$$
I will edit my answer to include a proof of my own once I find one.
answered Jan 26 at 21:05
clathratusclathratus
5,1441439
5,1441439
$begingroup$
Nice, I forgot the fact that $log(x^a)=alog(x)$.
$endgroup$
– Larry
Jan 26 at 21:14
$begingroup$
@Larry I legitimately can't tell if you're being sarcastic or not
$endgroup$
– clathratus
Jan 26 at 21:15
1
$begingroup$
I am not being sarcastic.
$endgroup$
– Larry
Jan 26 at 21:18
1
$begingroup$
@Larry Thank you for the clarification. You were very right when you mentioned that $(2)$ would be easy to prove once one had proven $(1)$.
$endgroup$
– clathratus
Jan 26 at 21:20
add a comment |
$begingroup$
Nice, I forgot the fact that $log(x^a)=alog(x)$.
$endgroup$
– Larry
Jan 26 at 21:14
$begingroup$
@Larry I legitimately can't tell if you're being sarcastic or not
$endgroup$
– clathratus
Jan 26 at 21:15
1
$begingroup$
I am not being sarcastic.
$endgroup$
– Larry
Jan 26 at 21:18
1
$begingroup$
@Larry Thank you for the clarification. You were very right when you mentioned that $(2)$ would be easy to prove once one had proven $(1)$.
$endgroup$
– clathratus
Jan 26 at 21:20
$begingroup$
Nice, I forgot the fact that $log(x^a)=alog(x)$.
$endgroup$
– Larry
Jan 26 at 21:14
$begingroup$
Nice, I forgot the fact that $log(x^a)=alog(x)$.
$endgroup$
– Larry
Jan 26 at 21:14
$begingroup$
@Larry I legitimately can't tell if you're being sarcastic or not
$endgroup$
– clathratus
Jan 26 at 21:15
$begingroup$
@Larry I legitimately can't tell if you're being sarcastic or not
$endgroup$
– clathratus
Jan 26 at 21:15
1
1
$begingroup$
I am not being sarcastic.
$endgroup$
– Larry
Jan 26 at 21:18
$begingroup$
I am not being sarcastic.
$endgroup$
– Larry
Jan 26 at 21:18
1
1
$begingroup$
@Larry Thank you for the clarification. You were very right when you mentioned that $(2)$ would be easy to prove once one had proven $(1)$.
$endgroup$
– clathratus
Jan 26 at 21:20
$begingroup$
@Larry Thank you for the clarification. You were very right when you mentioned that $(2)$ would be easy to prove once one had proven $(1)$.
$endgroup$
– clathratus
Jan 26 at 21:20
add a comment |
$begingroup$
An alternative approach is to employ Feynman's Trick and Laplace Transforms to solve:
beginequation
I = int_0^inftyln^2(x)sinleft(x^2right):dx
endequation
We first observe that:
beginequation
I = int_0^inftyln^2(x)sinleft(x^2right):dx = lim_krightarrow 0^+ fracd^2dk^2int_0^infty x^ksinleft(x^2right):dx = lim_krightarrow 0^+ fracd^2dk^2 H(k)
endequation
We proceed by solving $H(k)$. To do so, we introduce a new parameter $'t'$:
beginequation
J(t; k) = int_0^infty x^ksinleft(tx^2right):dx
endequation
(This is allowable through the Dominated Convergence Theorem). Thus:
beginequation
H(k) = lim_trightarrow 1^+ J(t; k)
endequation
Using Fubini's Theorem we now take the Laplace Transform with respect to '$t$'
beginalign
mathscrL_tleft[J(t;k) right] &= int_0^infty x^kmathscrL_tleft[sinleft(tx^2right)right]:dx = int_0^infty fracx^k + 2s^2 + x^4:dx
endalign
As I address here we find this becomes:
beginalign
mathscrL_tleft[J(t;k) right] &= frac14cdot left(s^2right)^frack + 2 + 12 - 1 cdot Bleft(1 - frack + 2 + 1 4, frack + 2 + 1 4 right) = frac14 s^frack - 12 Bleft(1 - frack + 34 , frack + 34right)
endalign
Using the relationship between the Gamma and Beta Function we find:
beginequation
mathscrL_tleft[J(t;k) right] = frac14 s^frack - 12 Gammaleft(1 - frack + 34right) Gammaleft( frack + 34right)
endequation
Using Euler's Reflection Formula we find:
beginequation
mathscrL_tleft[J(t;k) right] = frac14 s^frack - 12 fracpisinleft(pileft(frack + 34right) right)
endequation
Taking the inverse Laplace Transforms is rather tricky here. To evaluate recall that:
beginequation
I = lim_krightarrow 0^+ fracd^2dk^2 H(k) = lim_krightarrow 0^+ fracd^2dk^2left[ lim_trightarrow 1^+ J(t;k)right]
endequation
In this process we solve for $H(k)$ using
beginequation
H(k) = lim_trightarrow 1^+ mathscrL_s^-1left[mathscrL_tleft[J(t; k)right]right]
endequation
Thus, our definition of $I$ becomes:
beginalign
I &= lim_krightarrow 0^+ fracd^2dk^2 H(k) = lim_krightarrow 0^+ fracd^2dk^2left[ lim_trightarrow 1^+ J(t;k)right] = lim_krightarrow 0^+ fracd^2dk^2left[ lim_trightarrow 1^+ mathscrL_s^-1left[mathscrL_tleft[J(t; k)right]right]right] \
&= lim_trightarrow 1^+ mathscrL_s^-1left[ lim_krightarrow 0^+ fracd^2dk^2mathscrL_tleft[J(t; k)right]right] = lim_trightarrow 1^+ mathscrL_s^-1left[ lim_krightarrow 0^+ fracd^2dk^2left[ frac14 s^frack - 12 fracpisinleft(pileft(frack + 34right) right)right]right]
endalign
Because I'm lazy, I used Wolframalpha to evaluate the second derivate at $0$:
beginalign
I &= lim_trightarrow 1^+ mathscrL_s^-1left[ lim_krightarrow 0^+ fracd^2dk^2left[ frac14 s^frack - 12 fracpisinleft(pileft(frack + 34right) right)right]right] = lim_trightarrow 1^+ mathscrL_s^-1left[ fracpi4left( frac3pi^28sqrt2sqrts + fracln^2(s)2sqrt2sqrts + fracpiln(s)2sqrt2sqrtsright)right] \
&= lim_trightarrow 1^+ left[ frac3pi^332sqrt2 mathscrL_s^-1left[ frac1sqrtsright] + fracpi8sqrt2 mathscrL_s^-1left[ fracln^2(s)sqrtsright]+ fracpi^28sqrt2 mathscrL_s^-1left[ fracln(s)sqrtsright]right] \
&= lim_trightarrow 1^+ left[ frac3pi^332sqrt2 left[ frac1sqrtpisqrttright] + fracpi32sqrt2 left[ frac
left(psi^(0)left(frac12right)-ln(t)right)^2 -fracpi^22sqrtpisqrttright]+ fracpi^216sqrt2 left[ frac
psi^(0)left(frac12right)-ln(t)sqrtpisqrttright]right] \
&= frac3pi^332sqrt2 left[ frac1sqrtpiright] + fracpi32sqrt2 left[ frac
psi^(0)left(frac12right)^2 -fracpi^22sqrtpiright]+ fracpi^216sqrt2 left[ frac
psi^(0)left(frac12right)sqrtpiright]
endalign
Noting that
beginequation
psi^(0)left(frac12right) = -gamma - 2ln(2)
endequation
Where $gamma$ is the Euler–Mascheroni constant.
Thus,
beginalign
I = frac3pi^332sqrt2 left[ frac1sqrtpiright] + fracpi32sqrt2 left[ frac
left(gamma + 2ln(2)right)^2 -fracpi^22sqrtpiright]+ fracpi^216sqrt2 left[ frac
gamma - 2ln(2)sqrtpiright] = frac132sqrtfracpi2(2gamma-pi+4ln2)^2
endalign
$endgroup$
$begingroup$
Very nice solution! I am a fan of your method.
$endgroup$
– clathratus
Jan 28 at 16:07
$begingroup$
Do you use a similar technique to evaluate $$F(n)=int_0^infty cos(x^n)mathrm dx$$
$endgroup$
– clathratus
Feb 6 at 20:58
$begingroup$
@clathratus You definitely can
$endgroup$
– user150203
Feb 7 at 0:09
add a comment |
$begingroup$
An alternative approach is to employ Feynman's Trick and Laplace Transforms to solve:
beginequation
I = int_0^inftyln^2(x)sinleft(x^2right):dx
endequation
We first observe that:
beginequation
I = int_0^inftyln^2(x)sinleft(x^2right):dx = lim_krightarrow 0^+ fracd^2dk^2int_0^infty x^ksinleft(x^2right):dx = lim_krightarrow 0^+ fracd^2dk^2 H(k)
endequation
We proceed by solving $H(k)$. To do so, we introduce a new parameter $'t'$:
beginequation
J(t; k) = int_0^infty x^ksinleft(tx^2right):dx
endequation
(This is allowable through the Dominated Convergence Theorem). Thus:
beginequation
H(k) = lim_trightarrow 1^+ J(t; k)
endequation
Using Fubini's Theorem we now take the Laplace Transform with respect to '$t$'
beginalign
mathscrL_tleft[J(t;k) right] &= int_0^infty x^kmathscrL_tleft[sinleft(tx^2right)right]:dx = int_0^infty fracx^k + 2s^2 + x^4:dx
endalign
As I address here we find this becomes:
beginalign
mathscrL_tleft[J(t;k) right] &= frac14cdot left(s^2right)^frack + 2 + 12 - 1 cdot Bleft(1 - frack + 2 + 1 4, frack + 2 + 1 4 right) = frac14 s^frack - 12 Bleft(1 - frack + 34 , frack + 34right)
endalign
Using the relationship between the Gamma and Beta Function we find:
beginequation
mathscrL_tleft[J(t;k) right] = frac14 s^frack - 12 Gammaleft(1 - frack + 34right) Gammaleft( frack + 34right)
endequation
Using Euler's Reflection Formula we find:
beginequation
mathscrL_tleft[J(t;k) right] = frac14 s^frack - 12 fracpisinleft(pileft(frack + 34right) right)
endequation
Taking the inverse Laplace Transforms is rather tricky here. To evaluate recall that:
beginequation
I = lim_krightarrow 0^+ fracd^2dk^2 H(k) = lim_krightarrow 0^+ fracd^2dk^2left[ lim_trightarrow 1^+ J(t;k)right]
endequation
In this process we solve for $H(k)$ using
beginequation
H(k) = lim_trightarrow 1^+ mathscrL_s^-1left[mathscrL_tleft[J(t; k)right]right]
endequation
Thus, our definition of $I$ becomes:
beginalign
I &= lim_krightarrow 0^+ fracd^2dk^2 H(k) = lim_krightarrow 0^+ fracd^2dk^2left[ lim_trightarrow 1^+ J(t;k)right] = lim_krightarrow 0^+ fracd^2dk^2left[ lim_trightarrow 1^+ mathscrL_s^-1left[mathscrL_tleft[J(t; k)right]right]right] \
&= lim_trightarrow 1^+ mathscrL_s^-1left[ lim_krightarrow 0^+ fracd^2dk^2mathscrL_tleft[J(t; k)right]right] = lim_trightarrow 1^+ mathscrL_s^-1left[ lim_krightarrow 0^+ fracd^2dk^2left[ frac14 s^frack - 12 fracpisinleft(pileft(frack + 34right) right)right]right]
endalign
Because I'm lazy, I used Wolframalpha to evaluate the second derivate at $0$:
beginalign
I &= lim_trightarrow 1^+ mathscrL_s^-1left[ lim_krightarrow 0^+ fracd^2dk^2left[ frac14 s^frack - 12 fracpisinleft(pileft(frack + 34right) right)right]right] = lim_trightarrow 1^+ mathscrL_s^-1left[ fracpi4left( frac3pi^28sqrt2sqrts + fracln^2(s)2sqrt2sqrts + fracpiln(s)2sqrt2sqrtsright)right] \
&= lim_trightarrow 1^+ left[ frac3pi^332sqrt2 mathscrL_s^-1left[ frac1sqrtsright] + fracpi8sqrt2 mathscrL_s^-1left[ fracln^2(s)sqrtsright]+ fracpi^28sqrt2 mathscrL_s^-1left[ fracln(s)sqrtsright]right] \
&= lim_trightarrow 1^+ left[ frac3pi^332sqrt2 left[ frac1sqrtpisqrttright] + fracpi32sqrt2 left[ frac
left(psi^(0)left(frac12right)-ln(t)right)^2 -fracpi^22sqrtpisqrttright]+ fracpi^216sqrt2 left[ frac
psi^(0)left(frac12right)-ln(t)sqrtpisqrttright]right] \
&= frac3pi^332sqrt2 left[ frac1sqrtpiright] + fracpi32sqrt2 left[ frac
psi^(0)left(frac12right)^2 -fracpi^22sqrtpiright]+ fracpi^216sqrt2 left[ frac
psi^(0)left(frac12right)sqrtpiright]
endalign
Noting that
beginequation
psi^(0)left(frac12right) = -gamma - 2ln(2)
endequation
Where $gamma$ is the Euler–Mascheroni constant.
Thus,
beginalign
I = frac3pi^332sqrt2 left[ frac1sqrtpiright] + fracpi32sqrt2 left[ frac
left(gamma + 2ln(2)right)^2 -fracpi^22sqrtpiright]+ fracpi^216sqrt2 left[ frac
gamma - 2ln(2)sqrtpiright] = frac132sqrtfracpi2(2gamma-pi+4ln2)^2
endalign
$endgroup$
$begingroup$
Very nice solution! I am a fan of your method.
$endgroup$
– clathratus
Jan 28 at 16:07
$begingroup$
Do you use a similar technique to evaluate $$F(n)=int_0^infty cos(x^n)mathrm dx$$
$endgroup$
– clathratus
Feb 6 at 20:58
$begingroup$
@clathratus You definitely can
$endgroup$
– user150203
Feb 7 at 0:09
add a comment |
$begingroup$
An alternative approach is to employ Feynman's Trick and Laplace Transforms to solve:
beginequation
I = int_0^inftyln^2(x)sinleft(x^2right):dx
endequation
We first observe that:
beginequation
I = int_0^inftyln^2(x)sinleft(x^2right):dx = lim_krightarrow 0^+ fracd^2dk^2int_0^infty x^ksinleft(x^2right):dx = lim_krightarrow 0^+ fracd^2dk^2 H(k)
endequation
We proceed by solving $H(k)$. To do so, we introduce a new parameter $'t'$:
beginequation
J(t; k) = int_0^infty x^ksinleft(tx^2right):dx
endequation
(This is allowable through the Dominated Convergence Theorem). Thus:
beginequation
H(k) = lim_trightarrow 1^+ J(t; k)
endequation
Using Fubini's Theorem we now take the Laplace Transform with respect to '$t$'
beginalign
mathscrL_tleft[J(t;k) right] &= int_0^infty x^kmathscrL_tleft[sinleft(tx^2right)right]:dx = int_0^infty fracx^k + 2s^2 + x^4:dx
endalign
As I address here we find this becomes:
beginalign
mathscrL_tleft[J(t;k) right] &= frac14cdot left(s^2right)^frack + 2 + 12 - 1 cdot Bleft(1 - frack + 2 + 1 4, frack + 2 + 1 4 right) = frac14 s^frack - 12 Bleft(1 - frack + 34 , frack + 34right)
endalign
Using the relationship between the Gamma and Beta Function we find:
beginequation
mathscrL_tleft[J(t;k) right] = frac14 s^frack - 12 Gammaleft(1 - frack + 34right) Gammaleft( frack + 34right)
endequation
Using Euler's Reflection Formula we find:
beginequation
mathscrL_tleft[J(t;k) right] = frac14 s^frack - 12 fracpisinleft(pileft(frack + 34right) right)
endequation
Taking the inverse Laplace Transforms is rather tricky here. To evaluate recall that:
beginequation
I = lim_krightarrow 0^+ fracd^2dk^2 H(k) = lim_krightarrow 0^+ fracd^2dk^2left[ lim_trightarrow 1^+ J(t;k)right]
endequation
In this process we solve for $H(k)$ using
beginequation
H(k) = lim_trightarrow 1^+ mathscrL_s^-1left[mathscrL_tleft[J(t; k)right]right]
endequation
Thus, our definition of $I$ becomes:
beginalign
I &= lim_krightarrow 0^+ fracd^2dk^2 H(k) = lim_krightarrow 0^+ fracd^2dk^2left[ lim_trightarrow 1^+ J(t;k)right] = lim_krightarrow 0^+ fracd^2dk^2left[ lim_trightarrow 1^+ mathscrL_s^-1left[mathscrL_tleft[J(t; k)right]right]right] \
&= lim_trightarrow 1^+ mathscrL_s^-1left[ lim_krightarrow 0^+ fracd^2dk^2mathscrL_tleft[J(t; k)right]right] = lim_trightarrow 1^+ mathscrL_s^-1left[ lim_krightarrow 0^+ fracd^2dk^2left[ frac14 s^frack - 12 fracpisinleft(pileft(frack + 34right) right)right]right]
endalign
Because I'm lazy, I used Wolframalpha to evaluate the second derivate at $0$:
beginalign
I &= lim_trightarrow 1^+ mathscrL_s^-1left[ lim_krightarrow 0^+ fracd^2dk^2left[ frac14 s^frack - 12 fracpisinleft(pileft(frack + 34right) right)right]right] = lim_trightarrow 1^+ mathscrL_s^-1left[ fracpi4left( frac3pi^28sqrt2sqrts + fracln^2(s)2sqrt2sqrts + fracpiln(s)2sqrt2sqrtsright)right] \
&= lim_trightarrow 1^+ left[ frac3pi^332sqrt2 mathscrL_s^-1left[ frac1sqrtsright] + fracpi8sqrt2 mathscrL_s^-1left[ fracln^2(s)sqrtsright]+ fracpi^28sqrt2 mathscrL_s^-1left[ fracln(s)sqrtsright]right] \
&= lim_trightarrow 1^+ left[ frac3pi^332sqrt2 left[ frac1sqrtpisqrttright] + fracpi32sqrt2 left[ frac
left(psi^(0)left(frac12right)-ln(t)right)^2 -fracpi^22sqrtpisqrttright]+ fracpi^216sqrt2 left[ frac
psi^(0)left(frac12right)-ln(t)sqrtpisqrttright]right] \
&= frac3pi^332sqrt2 left[ frac1sqrtpiright] + fracpi32sqrt2 left[ frac
psi^(0)left(frac12right)^2 -fracpi^22sqrtpiright]+ fracpi^216sqrt2 left[ frac
psi^(0)left(frac12right)sqrtpiright]
endalign
Noting that
beginequation
psi^(0)left(frac12right) = -gamma - 2ln(2)
endequation
Where $gamma$ is the Euler–Mascheroni constant.
Thus,
beginalign
I = frac3pi^332sqrt2 left[ frac1sqrtpiright] + fracpi32sqrt2 left[ frac
left(gamma + 2ln(2)right)^2 -fracpi^22sqrtpiright]+ fracpi^216sqrt2 left[ frac
gamma - 2ln(2)sqrtpiright] = frac132sqrtfracpi2(2gamma-pi+4ln2)^2
endalign
$endgroup$
An alternative approach is to employ Feynman's Trick and Laplace Transforms to solve:
beginequation
I = int_0^inftyln^2(x)sinleft(x^2right):dx
endequation
We first observe that:
beginequation
I = int_0^inftyln^2(x)sinleft(x^2right):dx = lim_krightarrow 0^+ fracd^2dk^2int_0^infty x^ksinleft(x^2right):dx = lim_krightarrow 0^+ fracd^2dk^2 H(k)
endequation
We proceed by solving $H(k)$. To do so, we introduce a new parameter $'t'$:
beginequation
J(t; k) = int_0^infty x^ksinleft(tx^2right):dx
endequation
(This is allowable through the Dominated Convergence Theorem). Thus:
beginequation
H(k) = lim_trightarrow 1^+ J(t; k)
endequation
Using Fubini's Theorem we now take the Laplace Transform with respect to '$t$'
beginalign
mathscrL_tleft[J(t;k) right] &= int_0^infty x^kmathscrL_tleft[sinleft(tx^2right)right]:dx = int_0^infty fracx^k + 2s^2 + x^4:dx
endalign
As I address here we find this becomes:
beginalign
mathscrL_tleft[J(t;k) right] &= frac14cdot left(s^2right)^frack + 2 + 12 - 1 cdot Bleft(1 - frack + 2 + 1 4, frack + 2 + 1 4 right) = frac14 s^frack - 12 Bleft(1 - frack + 34 , frack + 34right)
endalign
Using the relationship between the Gamma and Beta Function we find:
beginequation
mathscrL_tleft[J(t;k) right] = frac14 s^frack - 12 Gammaleft(1 - frack + 34right) Gammaleft( frack + 34right)
endequation
Using Euler's Reflection Formula we find:
beginequation
mathscrL_tleft[J(t;k) right] = frac14 s^frack - 12 fracpisinleft(pileft(frack + 34right) right)
endequation
Taking the inverse Laplace Transforms is rather tricky here. To evaluate recall that:
beginequation
I = lim_krightarrow 0^+ fracd^2dk^2 H(k) = lim_krightarrow 0^+ fracd^2dk^2left[ lim_trightarrow 1^+ J(t;k)right]
endequation
In this process we solve for $H(k)$ using
beginequation
H(k) = lim_trightarrow 1^+ mathscrL_s^-1left[mathscrL_tleft[J(t; k)right]right]
endequation
Thus, our definition of $I$ becomes:
beginalign
I &= lim_krightarrow 0^+ fracd^2dk^2 H(k) = lim_krightarrow 0^+ fracd^2dk^2left[ lim_trightarrow 1^+ J(t;k)right] = lim_krightarrow 0^+ fracd^2dk^2left[ lim_trightarrow 1^+ mathscrL_s^-1left[mathscrL_tleft[J(t; k)right]right]right] \
&= lim_trightarrow 1^+ mathscrL_s^-1left[ lim_krightarrow 0^+ fracd^2dk^2mathscrL_tleft[J(t; k)right]right] = lim_trightarrow 1^+ mathscrL_s^-1left[ lim_krightarrow 0^+ fracd^2dk^2left[ frac14 s^frack - 12 fracpisinleft(pileft(frack + 34right) right)right]right]
endalign
Because I'm lazy, I used Wolframalpha to evaluate the second derivate at $0$:
beginalign
I &= lim_trightarrow 1^+ mathscrL_s^-1left[ lim_krightarrow 0^+ fracd^2dk^2left[ frac14 s^frack - 12 fracpisinleft(pileft(frack + 34right) right)right]right] = lim_trightarrow 1^+ mathscrL_s^-1left[ fracpi4left( frac3pi^28sqrt2sqrts + fracln^2(s)2sqrt2sqrts + fracpiln(s)2sqrt2sqrtsright)right] \
&= lim_trightarrow 1^+ left[ frac3pi^332sqrt2 mathscrL_s^-1left[ frac1sqrtsright] + fracpi8sqrt2 mathscrL_s^-1left[ fracln^2(s)sqrtsright]+ fracpi^28sqrt2 mathscrL_s^-1left[ fracln(s)sqrtsright]right] \
&= lim_trightarrow 1^+ left[ frac3pi^332sqrt2 left[ frac1sqrtpisqrttright] + fracpi32sqrt2 left[ frac
left(psi^(0)left(frac12right)-ln(t)right)^2 -fracpi^22sqrtpisqrttright]+ fracpi^216sqrt2 left[ frac
psi^(0)left(frac12right)-ln(t)sqrtpisqrttright]right] \
&= frac3pi^332sqrt2 left[ frac1sqrtpiright] + fracpi32sqrt2 left[ frac
psi^(0)left(frac12right)^2 -fracpi^22sqrtpiright]+ fracpi^216sqrt2 left[ frac
psi^(0)left(frac12right)sqrtpiright]
endalign
Noting that
beginequation
psi^(0)left(frac12right) = -gamma - 2ln(2)
endequation
Where $gamma$ is the Euler–Mascheroni constant.
Thus,
beginalign
I = frac3pi^332sqrt2 left[ frac1sqrtpiright] + fracpi32sqrt2 left[ frac
left(gamma + 2ln(2)right)^2 -fracpi^22sqrtpiright]+ fracpi^216sqrt2 left[ frac
gamma - 2ln(2)sqrtpiright] = frac132sqrtfracpi2(2gamma-pi+4ln2)^2
endalign
edited Jan 31 at 12:44
answered Jan 28 at 12:51
user150203
$begingroup$
Very nice solution! I am a fan of your method.
$endgroup$
– clathratus
Jan 28 at 16:07
$begingroup$
Do you use a similar technique to evaluate $$F(n)=int_0^infty cos(x^n)mathrm dx$$
$endgroup$
– clathratus
Feb 6 at 20:58
$begingroup$
@clathratus You definitely can
$endgroup$
– user150203
Feb 7 at 0:09
add a comment |
$begingroup$
Very nice solution! I am a fan of your method.
$endgroup$
– clathratus
Jan 28 at 16:07
$begingroup$
Do you use a similar technique to evaluate $$F(n)=int_0^infty cos(x^n)mathrm dx$$
$endgroup$
– clathratus
Feb 6 at 20:58
$begingroup$
@clathratus You definitely can
$endgroup$
– user150203
Feb 7 at 0:09
$begingroup$
Very nice solution! I am a fan of your method.
$endgroup$
– clathratus
Jan 28 at 16:07
$begingroup$
Very nice solution! I am a fan of your method.
$endgroup$
– clathratus
Jan 28 at 16:07
$begingroup$
Do you use a similar technique to evaluate $$F(n)=int_0^infty cos(x^n)mathrm dx$$
$endgroup$
– clathratus
Feb 6 at 20:58
$begingroup$
Do you use a similar technique to evaluate $$F(n)=int_0^infty cos(x^n)mathrm dx$$
$endgroup$
– clathratus
Feb 6 at 20:58
$begingroup$
@clathratus You definitely can
$endgroup$
– user150203
Feb 7 at 0:09
$begingroup$
@clathratus You definitely can
$endgroup$
– user150203
Feb 7 at 0:09
add a comment |
$begingroup$
$newcommandbbx[1],bbox[15px,border:1px groove navy]displaystyle#1,
newcommandbraces[1]leftlbrace,#1,rightrbrace
newcommandbracks[1]leftlbrack,#1,rightrbrack
newcommandddmathrmd
newcommandds[1]displaystyle#1
newcommandexpo[1],mathrme^#1,
newcommandicmathrmi
newcommandmc[1]mathcal#1
newcommandmrm[1]mathrm#1
newcommandpars[1]left(,#1,right)
newcommandpartiald[3][]fracpartial^#1 #2partial #3^#1
newcommandroot[2][],sqrt[#1],#2,,
newcommandtotald[3][]fracmathrmd^#1 #2mathrmd #3^#1
newcommandverts[1]leftvert,#1,rightvert$
With $dsR > 0$ and $dsnu in pars0,1$:
beginalign
&bbox[10px,#ffd]int_0^Rx^nuexpparsic x^2dd x
\[5mm] = &
-int_0^pi/4parsRexpoic theta^nu
expparsic R^2expo2icthetaRexpoicthetaic,ddtheta -
int_R^0parsrexpoicpi/4^nu
expparsicbracksrexpoicpi/4^2expoicpi/4,dd r
\[8mm] = &
-overbraceR^nu + 1,icint_0^pi/4
expparsicbracksnutheta + R^2cospars2theta + theta
exppars-R^2sinpars2thetaddtheta^dsequiv mcIparsR,nu
\[2mm] + &
expoicparsnu + 1pi/4int_0^Rr^nuexpo-r^2dd r
endalign
Since $dsnu in pars0,1$, note that
beginalign
0 & < vertsmcIparsR,nu <
R^nu + 1int_0^pi/4expo-4R^2theta/piddtheta =
pi over 4,1 - exppars-R^2 over R^1 - nu
,,,stackrelmrmas R to inftyLARGEto,,,
colorredlarge 0
endalign
Then,
beginalign
&bbox[10px,#ffd]int_0^inftyx^nusinparsx^2dd x =
sinparsbracksnu + 1,pi over 4
int_0^inftyr^nuexpo-r^2dd r
\[5mm] stackrelr^2 mapsto r=,,,&
1 over 2,sinparsbracksnu + 1,pi over 4
int_0^inftyr^nu/2 - 1/2expo-rdd r =
1 over 2,sinparsbracksnu + 1,pi over 4
Gammaparsnu over 2 + 1 over 2
endalign
and
beginalign
&bbox[10px,#ffd]int_0^inftyln^2parsxsinparsx^2dd x =
lim_nu to 0^+
totald[2]nu
braces1 over 2,sinparsbracksnu + 1,pi over 4
Gammaparsnu over 2 + 1 over 2
\[5mm] = &
bbx1 over 32rootpi over 2
bracksvphantomLarge A2gamma - pi + lnpars16^2 approx 0.0242
endalign
$endgroup$
add a comment |
$begingroup$
$newcommandbbx[1],bbox[15px,border:1px groove navy]displaystyle#1,
newcommandbraces[1]leftlbrace,#1,rightrbrace
newcommandbracks[1]leftlbrack,#1,rightrbrack
newcommandddmathrmd
newcommandds[1]displaystyle#1
newcommandexpo[1],mathrme^#1,
newcommandicmathrmi
newcommandmc[1]mathcal#1
newcommandmrm[1]mathrm#1
newcommandpars[1]left(,#1,right)
newcommandpartiald[3][]fracpartial^#1 #2partial #3^#1
newcommandroot[2][],sqrt[#1],#2,,
newcommandtotald[3][]fracmathrmd^#1 #2mathrmd #3^#1
newcommandverts[1]leftvert,#1,rightvert$
With $dsR > 0$ and $dsnu in pars0,1$:
beginalign
&bbox[10px,#ffd]int_0^Rx^nuexpparsic x^2dd x
\[5mm] = &
-int_0^pi/4parsRexpoic theta^nu
expparsic R^2expo2icthetaRexpoicthetaic,ddtheta -
int_R^0parsrexpoicpi/4^nu
expparsicbracksrexpoicpi/4^2expoicpi/4,dd r
\[8mm] = &
-overbraceR^nu + 1,icint_0^pi/4
expparsicbracksnutheta + R^2cospars2theta + theta
exppars-R^2sinpars2thetaddtheta^dsequiv mcIparsR,nu
\[2mm] + &
expoicparsnu + 1pi/4int_0^Rr^nuexpo-r^2dd r
endalign
Since $dsnu in pars0,1$, note that
beginalign
0 & < vertsmcIparsR,nu <
R^nu + 1int_0^pi/4expo-4R^2theta/piddtheta =
pi over 4,1 - exppars-R^2 over R^1 - nu
,,,stackrelmrmas R to inftyLARGEto,,,
colorredlarge 0
endalign
Then,
beginalign
&bbox[10px,#ffd]int_0^inftyx^nusinparsx^2dd x =
sinparsbracksnu + 1,pi over 4
int_0^inftyr^nuexpo-r^2dd r
\[5mm] stackrelr^2 mapsto r=,,,&
1 over 2,sinparsbracksnu + 1,pi over 4
int_0^inftyr^nu/2 - 1/2expo-rdd r =
1 over 2,sinparsbracksnu + 1,pi over 4
Gammaparsnu over 2 + 1 over 2
endalign
and
beginalign
&bbox[10px,#ffd]int_0^inftyln^2parsxsinparsx^2dd x =
lim_nu to 0^+
totald[2]nu
braces1 over 2,sinparsbracksnu + 1,pi over 4
Gammaparsnu over 2 + 1 over 2
\[5mm] = &
bbx1 over 32rootpi over 2
bracksvphantomLarge A2gamma - pi + lnpars16^2 approx 0.0242
endalign
$endgroup$
add a comment |
$begingroup$
$newcommandbbx[1],bbox[15px,border:1px groove navy]displaystyle#1,
newcommandbraces[1]leftlbrace,#1,rightrbrace
newcommandbracks[1]leftlbrack,#1,rightrbrack
newcommandddmathrmd
newcommandds[1]displaystyle#1
newcommandexpo[1],mathrme^#1,
newcommandicmathrmi
newcommandmc[1]mathcal#1
newcommandmrm[1]mathrm#1
newcommandpars[1]left(,#1,right)
newcommandpartiald[3][]fracpartial^#1 #2partial #3^#1
newcommandroot[2][],sqrt[#1],#2,,
newcommandtotald[3][]fracmathrmd^#1 #2mathrmd #3^#1
newcommandverts[1]leftvert,#1,rightvert$
With $dsR > 0$ and $dsnu in pars0,1$:
beginalign
&bbox[10px,#ffd]int_0^Rx^nuexpparsic x^2dd x
\[5mm] = &
-int_0^pi/4parsRexpoic theta^nu
expparsic R^2expo2icthetaRexpoicthetaic,ddtheta -
int_R^0parsrexpoicpi/4^nu
expparsicbracksrexpoicpi/4^2expoicpi/4,dd r
\[8mm] = &
-overbraceR^nu + 1,icint_0^pi/4
expparsicbracksnutheta + R^2cospars2theta + theta
exppars-R^2sinpars2thetaddtheta^dsequiv mcIparsR,nu
\[2mm] + &
expoicparsnu + 1pi/4int_0^Rr^nuexpo-r^2dd r
endalign
Since $dsnu in pars0,1$, note that
beginalign
0 & < vertsmcIparsR,nu <
R^nu + 1int_0^pi/4expo-4R^2theta/piddtheta =
pi over 4,1 - exppars-R^2 over R^1 - nu
,,,stackrelmrmas R to inftyLARGEto,,,
colorredlarge 0
endalign
Then,
beginalign
&bbox[10px,#ffd]int_0^inftyx^nusinparsx^2dd x =
sinparsbracksnu + 1,pi over 4
int_0^inftyr^nuexpo-r^2dd r
\[5mm] stackrelr^2 mapsto r=,,,&
1 over 2,sinparsbracksnu + 1,pi over 4
int_0^inftyr^nu/2 - 1/2expo-rdd r =
1 over 2,sinparsbracksnu + 1,pi over 4
Gammaparsnu over 2 + 1 over 2
endalign
and
beginalign
&bbox[10px,#ffd]int_0^inftyln^2parsxsinparsx^2dd x =
lim_nu to 0^+
totald[2]nu
braces1 over 2,sinparsbracksnu + 1,pi over 4
Gammaparsnu over 2 + 1 over 2
\[5mm] = &
bbx1 over 32rootpi over 2
bracksvphantomLarge A2gamma - pi + lnpars16^2 approx 0.0242
endalign
$endgroup$
$newcommandbbx[1],bbox[15px,border:1px groove navy]displaystyle#1,
newcommandbraces[1]leftlbrace,#1,rightrbrace
newcommandbracks[1]leftlbrack,#1,rightrbrack
newcommandddmathrmd
newcommandds[1]displaystyle#1
newcommandexpo[1],mathrme^#1,
newcommandicmathrmi
newcommandmc[1]mathcal#1
newcommandmrm[1]mathrm#1
newcommandpars[1]left(,#1,right)
newcommandpartiald[3][]fracpartial^#1 #2partial #3^#1
newcommandroot[2][],sqrt[#1],#2,,
newcommandtotald[3][]fracmathrmd^#1 #2mathrmd #3^#1
newcommandverts[1]leftvert,#1,rightvert$
With $dsR > 0$ and $dsnu in pars0,1$:
beginalign
&bbox[10px,#ffd]int_0^Rx^nuexpparsic x^2dd x
\[5mm] = &
-int_0^pi/4parsRexpoic theta^nu
expparsic R^2expo2icthetaRexpoicthetaic,ddtheta -
int_R^0parsrexpoicpi/4^nu
expparsicbracksrexpoicpi/4^2expoicpi/4,dd r
\[8mm] = &
-overbraceR^nu + 1,icint_0^pi/4
expparsicbracksnutheta + R^2cospars2theta + theta
exppars-R^2sinpars2thetaddtheta^dsequiv mcIparsR,nu
\[2mm] + &
expoicparsnu + 1pi/4int_0^Rr^nuexpo-r^2dd r
endalign
Since $dsnu in pars0,1$, note that
beginalign
0 & < vertsmcIparsR,nu <
R^nu + 1int_0^pi/4expo-4R^2theta/piddtheta =
pi over 4,1 - exppars-R^2 over R^1 - nu
,,,stackrelmrmas R to inftyLARGEto,,,
colorredlarge 0
endalign
Then,
beginalign
&bbox[10px,#ffd]int_0^inftyx^nusinparsx^2dd x =
sinparsbracksnu + 1,pi over 4
int_0^inftyr^nuexpo-r^2dd r
\[5mm] stackrelr^2 mapsto r=,,,&
1 over 2,sinparsbracksnu + 1,pi over 4
int_0^inftyr^nu/2 - 1/2expo-rdd r =
1 over 2,sinparsbracksnu + 1,pi over 4
Gammaparsnu over 2 + 1 over 2
endalign
and
beginalign
&bbox[10px,#ffd]int_0^inftyln^2parsxsinparsx^2dd x =
lim_nu to 0^+
totald[2]nu
braces1 over 2,sinparsbracksnu + 1,pi over 4
Gammaparsnu over 2 + 1 over 2
\[5mm] = &
bbx1 over 32rootpi over 2
bracksvphantomLarge A2gamma - pi + lnpars16^2 approx 0.0242
endalign
answered Mar 26 at 6:28
Felix MarinFelix Marin
69k7110147
69k7110147
add a comment |
add a comment |
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$begingroup$
Computer algebra solves this instantly: $frac132 sqrtfracpi 2 (2 gamma -pi +log (16))^2$. Is there really a need to perform this by hand? ted.com/talks/…
$endgroup$
– David G. Stork
Jan 26 at 20:10
$begingroup$
It is an interesting video. "Hand calculating procedures teach understanding."
$endgroup$
– Larry
Jan 26 at 20:16
$begingroup$
Did you actually watch the full video? One of Wolfram's key points was exposing the fallacy in "hand calculating procedures teach understanding." Very convincing.
$endgroup$
– David G. Stork
Jan 26 at 20:29
2
$begingroup$
@DavidG.Stork I entirely disagree. I personally am interested in knowing how to preform such manual calculations as they teach me new techniques which I can apply to other problems. Also, what is the point of knowing that $int_0^infty ln^2(x)sin(x^2)mathrm dx$ has a closed form (or exact evaluation instead of a decimal expansion) if one cannot prove it? Without a proof it is just a useless fact.
$endgroup$
– clathratus
Jan 26 at 20:51
2
$begingroup$
Ok, I see. That is actually a good point. I will keep that in mind.
$endgroup$
– Larry
Jan 26 at 21:12