How to Integrate the Boltzmann Equation Over Heavy Momenta in Cosmology?

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Homework Help Overview

The discussion revolves around integrating the Boltzmann equation in the context of cosmology, specifically focusing on heavy momenta associated with particle interactions. The original poster seeks assistance with the integration process involving Dirac delta functions and the properties of heavy and light particles in a reaction involving neutrinos, protons, and electrons.

Discussion Character

  • Exploratory, Assumption checking, Problem interpretation

Approaches and Questions Raised

  • Participants discuss the integration of the Boltzmann equation, questioning the notation and the role of different particle momenta. There are attempts to clarify the use of Dirac delta functions and how they relate to the integration process. Some participants suggest simplifying the integrals by considering the properties of heavy and light particles.

Discussion Status

The discussion is ongoing, with participants exploring various interpretations of the problem and attempting to clarify the notation and assumptions involved. Some guidance has been offered regarding the use of Dirac delta functions and the implications of heavy versus light momenta, but no consensus has been reached on the integration approach.

Contextual Notes

There are indications of confusion regarding the setup of the reaction and the number of phase space integrals involved. Participants are also grappling with the implications of the heavy momenta in the context of the Boltzmann equation.

alejandrito29
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I need integrate "over heavy momenta" the following equation
\sigma v>=
&lt;\sigma v&gt;= \frac{1}{n^{(0)}_1n^{(0}}_2 \int \frac{d^3p_1}{(2Pi)^3 2 E_1} \int \frac{d^3p_2}{(2Pi)^3 2 E_2} \int \frac{d^3p_3 }{(2Pi)^3 2 E_3} \int \frac{d^3p_4}{(2Pi)^3 2 E_4} e^{-(E_1+E_2)/T} \\<br /> <br /> \cdot (2 Pi)^4 \delta^3 (p_1+p_2-p_3-p_4) \delta (E_1+E_2-E_3-E_4) M^2

where n+ \nu \rightarrow p+ e^-

I need to find that_

n_{\nu}^{(0)}&lt; \sigma v&gt;= \frac{Pi}{4m^2}\int \frac{d^3p_\nu}{(2Pi)^3 2 p_\nu} e^{-p_\nu/T}\int \frac{d^3p_e}{(2Pi)^3 2 p_e} \delta (Q-p_\nu-p_e) M^2

where Q=m_n-m_p

I tried very ways, for example using \delta^3 (p_1+p_2+p_3+p_4)= \delta(p_1)\delta(p_2)\delta(p_3)\delta(p_4) but i have very problems with the integration and with the propierties of Dirac Delta...

Help please
 
Last edited:
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I tried very ways, for example using \delta^3 (p_1+p_2+p_3+p_4)= \delta(p_1)\delta(p_2)\delta(p_3)\delta(p_4) but i have very problems with the integration and with the propierties of Dirac Delta...

Help please

You are confusing your notation here. pn are not different components of a 4-vector, they are 3-vectors corresponding to different particle species.


Now, let's start from the beginning. What are Ep, En, Ev and Ee? Replace them in your equation, and you should only have particle momenta left. Then consider integrating.
 
Last edited:
clamtrox said:
You are confusing your notation here. pn are not different components of a 4-vector, they are 3-vectors corresponding to different particle species.


Now, let's start from the beginning. What are Ep, En, Ev and Ee? Replace them in your equation, and you should only have particle momenta left. Then consider integrating.

i think that if the particle is heavym (proton and neutron)

E=\sqrt{m^2+p^2} = m\sqrt{1+\frac{p^2}{m^2}} \approx m

\delta^3 (p_1+p_2-p_3-p_4) \delta (m_n+E_\nu-m_p-E_e) M^2

\int \frac{d^3p_e}{(2Pi)^3 2 E_e} e^{-(E_n+E_\nu)/T} \delta^3 (p_n+p_\nu-p_p-p_e) \delta (Q+E_\nu-E_e) M^2

but ¿how i use de Dirac Delta? ¿what is the propierty?
 
That's good! And also for the relativistic particles, Ee = pe and same for neutrino.

Now you notice that your integrand does not depend on the heavy momenta at all. So let's look at the standard delta function identity
\int d^3 x \delta^3(x-a) = 1 if a is in the integral domain. Use this to get rid of one of the integrals (it's really that easy!).

Then you're left with another integral over a heavy momentum, but the integrand still doesn't depend on the integral variable. This integral looks a lot like a phase space number density, so maybe you can find a nice identity for that one somewhere from your material.
 
clamtrox said:
That's good! And also for the relativistic particles, Ee = pe and same for neutrino.

Now you notice that your integrand does not depend on the heavy momenta at all. So let's look at the standard delta function identity
\int d^3 x \delta^3(x-a) = 1 if a is in the integral domain. Use this to get rid of one of the integrals (it's really that easy!).

Then you're left with another integral over a heavy momentum, but the integrand still doesn't depend on the integral variable. This integral looks a lot like a phase space number density, so maybe you can find a nice identity for that one somewhere from your material.

very thanks, but if Ee = pe then my equation is


\int \frac{d^3p_e}{(2Pi)^3 2 p_e} e^{-(E_n+E_\nu)/T} \delta^3 (p_n+p_\nu-p_p-p_e) \delta (Q+p_\nu-p_e) M^2

but, the integrand \frac{1}{p_e} itself depends on the heavy momentum pe..

then \int \frac{d^3p_e}{(2Pi)^3 2 p_e} \delta^3 (p_n+p_\nu-p_p-p_e) \neq 1

¿ how i use \int d^3 x \delta^3(x-a) = 1 ?
 
alejandrito29 said:
... but, the integrand \frac{1}{p_e} itself depends on the heavy momentum pe..

Assume that proton and neutron are heavy, p << m, and that electron and neutrino are light, p >> m.
 
thank, but my problem is the integral of last post,
 
  • #10
alejandrito29 said:
I need integrate "over heavy momenta" the following equation
\sigma v>=
&lt;\sigma v&gt;= \frac{1}{n^{(0)}_1n^{(0}}_2 \int \frac{d^3p_1}{(2Pi)^3 2 E_1} \int \frac{d^3p_2}{(2Pi)^3 2 E_2} \int \frac{d^3p_3 }{(2Pi)^3 2 E_3} \int \frac{d^3p_4}{(2Pi)^3 2 E_4} e^{-(E_1+E_2)/T} \\<br /> <br /> \cdot (2 Pi)^4 \delta^3 (p_1+p_2-p_3-p_4) \delta (E_1+E_2-E_3-E_4) M^2

where n+ \nu \rightarrow p+ e^-

I need to find that_

n_{\nu}^{(0)}&lt; \sigma v&gt;= \frac{Pi}{4m^2}\int \frac{d^3p_\nu}{(2Pi)^3 2 p_\nu} e^{-p_\nu/T}\int \frac{d^3p_e}{(2Pi)^3 2 p_e} \delta (Q-p_\nu-p_e) M^2

where Q=m_n-m_p

I tried very ways, for example using \delta^3 (p_1+p_2+p_3+p_4)= \delta(p_1)\delta(p_2)\delta(p_3)\delta(p_4) but i have very problems with the integration and with the propierties of Dirac Delta...
First of all, i have problems here regarding the reaction.It should be probably
n→p+e- +v-(however it does not seem from the delta function you have written).Anyway,you are probably calculating cross section,right?So why are there 4 phase space integrals.There should be only two for your reaction and three for mine but there are four?the way to handle the space δ is to integrate over anyone of the three variable,which will left only two momentum integral(according to me) then you have to move forward to time delta function with relation E=√p2+m2.
 
  • #11
alejandrito29 said:
thank, but my problem is the integral of last post,

You are not asked to calculate that integral in this problem.
 

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