Talk:Fluctuation–dissipation theorem

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Potential sign error

Depending on which convention one uses for the Fourier transform, the FDT adopts different signs.

Definition (1):

${\hat {A}}(\omega )=\int \limits _{-\infty }^{\infty }\mathrm {e} ^{i\omega t}A(t)\,dt$

gives

$S_{x}(\omega )={\frac {2k_{B}T}{\omega }}\,\mathrm {Im} [{\hat {\chi }}(\omega )].$

Definition (2):

${\hat {A}}(\omega )=\int \limits _{-\infty }^{\infty }\mathrm {e} ^{-i\omega t}A(t)\,dt$

gives

$S_{x}(\omega )=-{\frac {2k_{B}T}{\omega }}\,\mathrm {Im} [{\hat {\chi }}(\omega )].$

The article uses the first form of the FDT, but in its derivation a Fourier transform of form (2) is used. This inconsistency should be corrected, but I wanted to discuss this first. Benjamin.friedrich (talk) 22:30, 6 December 2017 (UTC)

Rewrite

I've changed the headline paragraph for the FDT entry to correct misleading text. The rest of the introductory section is problematic. Please see my Talk page.

-- Pwfen (talk) 14:26, 25 January 2015 (UTC)

I started a major rewrite of this article.

What was the state before: IMO, the second part of the original version was not very clear.

• 'General applicability' did not give a formula of a general FDT
• 'Derivation' did not make it clear to may what actually is the aim of this computation

What I have done: I included a section 'General form' where I give a general FDT in its simplest form; I also included a derivation.

What can be done next:

• remove redundancies
• compare different versions of general FDT (there's a whole plethora in the literature)
• derive the examples from the general form of the FDT

I would appreciate your help.

--Benjamin.friedrich (talk) 12:18, 18 December 2007 (UTC)

Sure, Benjamin, I'll be glad to help you, although I'm apt to over-commit myself. I appreciate all your work so far in shaping up this little article; most of it was just dashed off quickly while I was researching the equipartition theorem. I meant to return to it, but I got distracted... :( I just added some references and touched up the wording in the lead and my derivation section. I think both derivations should go at the end, similar to what I did at Laplace-Runge-Lenz vector. I'll need to read up on the fluctuation dissipation theorem a lot more, though, before I can really give you much help — sorry! I learn pretty fast, though. :) Willow (talk) 01:13, 19 December 2007 (UTC)

"Citation needed" / "Violations in glassy systems": "In the mid 1990s, in the study of non-equilibrium dynamics of spin glass models, a generalization of the fluctuation-dissipation theorem was discovered": I suspect you really intended one of the references you've listed in "Further reading", Cristani A, Ritort F (2003), as your citation for this point? - but I'm not familiar with it so I don't feel free to edit quite so boldly as to just put it in!! SquisherDa (talk) 03:19, 9 April 2012 (UTC)

Definition of the theorem

I actually miss the theorem itself. Only examples, derivation and applications..--85.146.199.125 (talk) 20:22, 20 February 2008 (UTC)

Definition of Linear Response Function fix

Perhaps nitpicking, but: In "general formulation," the perturbing field f seems to be off a minus sign: dp/dt = -dH/dx = -dH0/dx - f(t) as written. So then f is *minus* the applied force. This should be changed to be consistent with the definition of susceptibility in that wikipedia article. Dstrozzi (talk) 00:02, 27 March 2017 (UTC)

The old definition is not correct:

$\langle x(t)\rangle =\langle x\rangle _{0}+\int _{-\infty }^{t}\chi (\tau )f(t-\tau )d\tau \,$ (incorrect)

Rather $f$ and $\chi$ are swapped. It should be:

$\langle x(t)\rangle =\langle x\rangle _{0}+\int _{-\infty }^{t}f(\tau )\chi (t-\tau )d\tau \$

such that $\langle x(t)\rangle$ only depends on the perturbation $f$ before $t$. 76.199.99.43 (talk) 10:41, 21 April 2009 (UTC)

Fix Error in Equation (**) in Derivation

(Note: This is my first attempt at editing a Wikipedia page; I'm still unsure of syntax and etiquette. Advice and/or guidance will be very much appreciated.)

Equation (**) implies a discontinuous step-function response for $\langle x(t)\rangle -\langle x\rangle _{0}$ at t=0, which is incorrect. As t approaches zero from minus infinity, $\langle x(t)\rangle -\langle x\rangle _{0}$ adiabatically approaches $\ \beta f_{0}A(0)$. Equation (**) can be corrected by removing the outer parentheses on the right-hand side. As a consequence of this change, the outer parentheses in the second term on the right-hand side in the final equation of the derivation must also be removed. Thus the derivation beginning with Equation (**) should read:

$(**)-\chi (t)=\beta {\operatorname {d} A(t) \over \operatorname {d} t}\theta (t).$

For stationary processes, the Wiener-Khinchin theorem states that the power spectrum equals twice the Fourier transform of the auto-correlation function

$S_{x}(\omega )=2{\tilde {A}}(\omega ).$

The last step is to Fourier transform equation (**) and to take the imaginary part. For this it is useful to recall that the Fourier transform of a real symmetric function is real, while the Fourier transform of a real antisymmetric function is purely imaginary. We can split ${\operatorname {d} A(t) \over \operatorname {d} t}\theta (t)$ into a symmetric and an anti-symmetric part

$2{\operatorname {d} A(t) \over \operatorname {d} t}\theta (t)\ ={\operatorname {d} A(t) \over \operatorname {d} t}+{\operatorname {d} A(t) \over \operatorname {d} t}{\rm {sign}}(t).$

Now the fluctuation-dissipation theorem follows.

(Remark to reviewer, not to be included in the actual article: Observe that the corrected derivation above does not change the imaginary (absorptive) part of chi, but it does modify the real (dispersive) part.)

PaulH (talk) 01:58, 16 February 2011 (UTC)

Hi Paul, welcome at Wikipedia, and please feel free to correct, improve, expand this article in whatever way. This entire field suffers from a lack of expert attention. -- Marie Poise (talk) 14:40, 16 February 2011 (UTC)

Hey Paul, I think you have the etiquette mastered already! Using this Talk page is excellent, and it was especially kind of you to write. :) I replied on my Talk page, but I neglected to mention there that we also need more references. Willow (talk) 18:51, 16 February 2011 (UTC)

Can you provide a reference why we should have a factor of two between the power spectrum and the Fourier transform of the autocorrelation function? Maybe this is just a matter of defintion, but both this article as well as the article on the Wiener-Khinchin theorem do not have this factor of two. Benjamin.friedrich (talk) 09:44, 7 December 2017 (UTC)

Derivation in trace notation is wrong

I don't like to delete the whole section, but don't see another way. The problem is this one: In order to expand in the pertubation, h and H would have to commute. (cf. Baker-Campbell-Hausdorff formula). But if they commute, A(t) is not anymore time-dependent and there will always hold ${\bar {A}}(t)=\langle A\rangle$

I don't think one can reconcile that and thus I vote for deleting the entire section.

129.206.196.179 (talk) 10:13, 9 June 2011 (UTC)

Correction: Now I think, it's right. But there is a huge lack of explanation. I hope, I'll get back to inserting it.

129.206.91.26 (talk) 16:36, 9 June 2011 (UTC)

Another correction: I checked it, it's definitely wrong. I hope, I'll find the time to point out, why.

129.206.91.26 (talk) 17:49, 9 June 2011 (UTC)

So, here it comes: The Taylor-expansion in numerator and denominator need the following approximation to hold (which is far from obvious for non-commuting H and h, check Baker-Campbell-Hausdorff formula):

${\mbox{tr}}(Ae^{-\beta (H+h)}\approx {\mbox{tr}}(Ae^{-\beta H}e^{-\beta h})$

and in the denominator:

${\mbox{tr}}(e^{-\beta (H+h)}\approx {\mbox{tr}}(e^{-\beta H}e^{-\beta h})$

While the second approximation seems to hold (I checked some matrices with oracle), the first approximation is simply wrong. Demanding A to be small is probably a solution, but it's highly unphysical to expect some observable to be small compared to the Hamiltonian. Another possibility is to demand $H$ and $h$ to commute. But then the time evolution of our equilibrium state is trivial and the FDT states: $0=0$.

For these reasons I will now delete the whole "Derivation in trace notation" - section. Hope, your ok with that. — Preceding unsigned comment added by 129.206.196.143 (talk) 16:10, 12 June 2011 (UTC)

I am trying to comprehend why the field is always taken to be time-independent. I understand why it is turned off at time zero, but there should be a way to derive this without requiring time independence of the field. 129.255.226.50 (talk) 18:06, 19 August 2013 (UTC)

Deletion of partially cited or uncited text from FDT page

There have been edits of this page that delete text in response to old comments about missing citations. An example of this was the deletion of the following statement: "A proof can be found by means of the LSZ reduction, an identity from quantum field theory.[citation needed]"

• There was a partial citation (to the LSZ article in Wikipedia).
• Removing this statement did not improve the quality of the article. It degraded it.
• Please invest the effort find a peer-reviewed article that is missing if that is what bothers you.

This article is not in great shape, and deletions are generally not what is required. The work I did a while back on the Intro was intended to drag the article out of the "catastrophically wrong" category (a quote from a UC Berkeley faculty member, with which I agreed completely at the time).

("Catastrophically wrong" because prior versions of the FDT article had the basis and origin of the theorem completely wrong: e.g. the text appeared to have been written by sitting down with an undergraduate exposition that assumed equilibrium conditions for ease of derivation)

Pwfen (talk) 06:54, 29 August 2018 (UTC)

First Example of the Fluctuation-Dissipation Theorem

The 9 April 2019 version of the FDT page <https://en.wikipedia.org/w/index.php?title=Fluctuation-dissipation_theorem&oldid=891240986) states that "The fluctuation–dissipation theorem was originally formulated by Harry Nyquist in 1928". This is incorrect. Einstein's 1905 Brownian motion paper is the first published example of a fluctuation-dissipation relation. Pwfen (talk) 14:22, 9 April 2019 (UTC)

Detailed balance versus thermal equilibrium

The fluctuation-dissipation theorem does not require thermal equilibrium to hold. It requires detailed balance to hold. Please see https://en.wikipedia.org/wiki/User_talk:Pwfen for a discussion of problems with the FDT page. Pwfen (talk) 09:37, 11 April 2019 (UTC)

Problems with quantum derivation of FDT

There are few things that do not look 100% fine in that section and probably need some adjustment.

• The present strange formula ${\text{Im}}\left[\chi (t)\right]=(\chi (t)-\chi (-t))/2i$ comes from equation (2) in the cited paper... where it is stated that $\chi ^{d}(t)=(\chi (t)-\chi (-t))/2i$ is the "dissipative part" of the response function. I kind of understand what all this means... since the Fourier transform of $\chi ^{d}(t)$ is indeed ${\text{Im}}\left[\chi (\omega )\right]$. However, this looks a bit like a misleading formula to me and anyway calling this ${\text{Im}}\left[\chi (t)\right]$ is really weird since $\chi (t)$ is a real causal funcion and strictly speaking it does not have any imaginary part.

• There seems to be a sign inconsistency between :$\chi (t-t')=i\theta (t-t')\langle [{\hat {x}}(t),{\hat {x}}(t')]\rangle$ and ${\text{Im}}\left[\chi (t)\right]=-{\frac {1}{2}}\left[\langle {\hat {x}}(t){\hat {x}}(0)\rangle -\langle {\hat {x}}(0){\hat {x}}(t)\rangle \right]$

• The final formula with the "+1/2" is just the symmetric part of $S_{x}(\omega )$... indeed $S_{x}(\omega )=2\hbar [n_{BE}(\omega )+1]\chi (\omega )$... plus 1, not plus 1/2.

• sometimes $\hbar$ is dropped, other times it's not... I am ok with $\hbar =1$ but then it should be used all the times.

Suggestions

I am ok with the initial discussion but I would refer to ${\text{Im}}\left[\chi (\omega )\right]$ and just drop this strange ${\text{Im}}\left[\chi (t)\right]$. Then I am ok with Kubo formula, this is a very good starting point

$\chi (t)={\frac {i\theta (t)}{\hbar }}\langle \left[x(t),x(0)\right]\rangle$

if we take Kubo for granted then the final result can be derived just by a simple Fourier transform

$\chi (\omega )={\frac {i}{\hbar }}\int _{0}^{\infty }\langle \left[{\hat {x}}(t),{\hat {x}}(0)\right]\rangle e^{i\omega t}dt$

so

${\text{Im}}\left[\chi (\omega )\right]={\frac {\chi (\omega )-\chi ^{*}(\omega )}{2i}}={\frac {1}{2\hbar }}\int _{0}^{\infty }\langle \left[{\hat {x}}(t),{\hat {x}}(0)\right]\rangle e^{i\omega t}dt+{\frac {1}{2\hbar }}\int _{0}^{\infty }\langle \left[{\hat {x}}(0),{\hat {x}}(t)\right]\rangle e^{-i\omega t}dt={\frac {1}{2\hbar }}\int _{-\infty }^{+\infty }\langle \left[{\hat {x}}(t),{\hat {x}}(0)\right]\rangle e^{i\omega t}dt$

then the following part is very correct: "In the canonical ensemble, the second term can be re-expressed as

$\langle {\hat {x}}(0){\hat {x}}(t)\rangle ={\text{Tr }}e^{-\beta {\hat {H}}}{\hat {x}}(0){\hat {x}}(t)={\text{Tr }}{\hat {x}}(t)e^{-\beta {\hat {H}}}{\hat {x}}(0)={\text{Tr }}e^{-\beta {\hat {H}}}\underbrace {e^{\beta {\hat {H}}}{\hat {x}}(t)e^{-\beta {\hat {H}}}} _{{\hat {x}}(t-i\hbar \beta )}{\hat {x}}(0)=\langle {\hat {x}}(t-i\hbar \beta ){\hat {x}}(0)\rangle$

where in the second equality we re-positioned ${\hat {x}}(t)$ using the cyclic property of trace (in this step we have also assumed that the operator ${\hat {x}}$ is bosonic, i.e. does not introduce a sign change under permutation). Next, in the third equality, we inserted $e^{-\beta {\hat {H}}}e^{\beta {\hat {H}}}$ next to the trace and interpreted $e^{-\beta {\hat {H}}}$ as a time evolution operator $e^{-{\frac {i}{\hbar }}{\hat {H}}\Delta t}$ with imaginary time interval $\Delta t=-i\hbar \beta$."... and if we plug this in the previous equation we get

${\text{Im}}\left[\chi (\omega )\right]={\frac {1}{2\hbar }}\int _{-\infty }^{+\infty }\langle {\hat {x}}(t){\hat {x}}(0)-{\hat {x}}(t-i\hbar \beta ){\hat {x}}(0)\rangle e^{i\omega t}dt={\frac {1-e^{-\beta \hbar \omega }}{2\hbar }}\int _{-\infty }^{+\infty }\langle {\hat {x}}(t){\hat {x}}(0)\rangle e^{i\omega t}dt={\frac {1-e^{-\beta \hbar \omega }}{2\hbar }}S_{x}(\omega )$

and finally, with minor reshuffling of the factors, to

$S_{x}(\omega )=2\hbar \left[n_{\rm {BE}}(\omega )+1\right]{\text{Im}}\left[\chi (\omega )\right]$

where $n_{\rm {BE}}(\omega )=1/\left(e^{\beta \hbar \omega }-1\right)$: note here we have a $+1$, not $+1/2$. The $1/2$ makes sense but only because the same calculation for $-\omega$ yields

$S_{x}(-\omega )=2\hbar \left[n_{\rm {BE}}(\omega )\right]{\text{Im}}\left[\chi (\omega )\right]=e^{-\beta \hbar \omega }S_{x}(\omega )$

without the +1. So the cited formula with $1/2$ is just the symmetric part of power spectral density $(S_{x}(\omega )+S_{x}(-\omega ))/2$. In quantum noise $S_{x}(\omega )$ is not symmetric and, consistently, the autocorrelation $\langle x(t)x(0)\rangle$ contains an imaginary part. This is something that is not particularly trivial/intuitive and might deserve a separate discussion... possible reference/examples here

Wikirod76 (talk) 00:57, 9 January 2021 (UTC)