Abstract
A Boltzmann equation, used to describe the evolution of the density function of a gas of photons interacting by Compton scattering with electrons at low density and non relativistic equilibrium, is considered. A truncation of the very singular redistribution function is introduced and justified. The existence of weak solutions is proved for a large set of initial data. A simplified equation, where only the quadratic terms are kept and that appears at very low temperature of the electron gas, for small values of the photon’s energies, is also studied. The existence of weak solutions, and also of more regular solutions that are very flat near the origin, is proved. The long time asymptotic behavior of weak solutions of the simplified equation is described.
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References
Ballew, J., Iyer, G., Pego, R.L.: Bose–Einstein condensation in a hyperbolic model for the Kompaneets equation. SIAM J. Math. Anal. 48, 3840–3859 (2016)
Barik, P.K., Giri, A.K., Laurençot, P.: Mass-conserving solutions to the Smoluchowski coagulation equation with singular kernel. (2018) ArXiv e-prints, arXiv:1804.00853
Birkinshaw, M.: The Sunyaev–Zeldovich effect. Phys. Rep. 310(2), 97–195 (1999)
Bogachev, V.I.: Measure Theory, vol. 2. Springer, Berlin (2007)
Brown, L.M., Feynman, R.P.: Radiative corrections to Compton scattering. Phys. Rev. 85, 231–244 (1952)
Buet, C., Després, B., Leroy, T.: Anisotropic models and angular moments methods for the Compton scattering. E-prints, hal-01717173 (2018)
Caflisch, R.E., Levermore, C.D.: Equilibrium for radiation in a homogeneous plasma. Phys. Fluids 29(3), 748–752 (1986)
Camejo, C.C., Gröpler, R., Warnecke, G.: Regular solutions to the coagulation equations with singular kernels. Math. Methods Appl. Sci. 38(11), 2171–2184 (2015)
Chane-Yook, M., Nouri, A.: On a quantum kinetic equation linked to the Compton effect. Transp. Theory Stat. Phys. 33(5–7), 403–427 (2004)
Cortés, E., Escobedo, M.: On a system of equations for the normal fluid-condensate interaction in a Bose gas. ArXiv e-prints, (2018)
Dreicer, H.: Kinetic theory of an electron–photon gas. Phys. Fluids 7, 735–753 (1964)
Escobedo, M., Herrero, M.A., Velázquez, J.J.L.: A nonlinear Fokker–Planck equation modelling the approach to thermal equilibrium in a homogeneous plasma. Trans. Am. Math. Soc. 350(10), 3837–3901 (1998)
Escobedo, M., Mischler, S.: On a quantum Boltzmann equation for a gas of photons. J. Math. Pures Appl. 80(5), 471–515 (2001)
Escobedo, M., Mischler, S., Valle, M.A.: Homogeneous Boltzmann equation in quantum relativistic kinetic theory. Electron. J. Diff. Equ. Monogr. 4(2), 1–85 (2003)
Escobedo, M., Mischler, S., Velázquez, J.J.L.: Asymptotic description of Dirac mass formation in kinetic equations for quantum particles. J. Diff. Equ. 202(2), 208–230 (2004)
Ferrari, E., Nouri, A.: On the Cauchy problem for a quantum kinetic equation linked to the Compton effect. Math. Comput. Modell. 43, 838–853 (2006)
Folland, G.B.: Real Analysis: Modern Techniques and Their Applications. Pure and Applied Mathematics. Wiley, New York (1999)
Fournier, N., Laurençot, P.: Well-posedness of Smoluchowski’s coagulation equation for a class of homogeneous kernels. J. Funct. Anal. 233(2), 351–379 (2006)
Grachev, S.I.: Nonstationary radiative transfer: evolution of a spectrum by multiple compton scattering. Astrophysics 57(4), 550–558 (2014)
Kavian, O.: Remarks on the Kompaneets Equation, a Simplified Model of the Fokker–Planck Equation. Studies in Applied Mathematics. North-Holland (2002)
Klenke, A.: Probability Theory: A Comprehensive Course (Universitext). Springer, London (2013)
Kompaneets, A.S.: The establishment of thermal equilibrium between quanta and electrons. Soviet J. Exp. Theor. Phys. 4, 730–737 (1957)
Levermore, C.D., Liu, H., Pego, R.L.: Global dynamics of Bose–Einstein condensation for a model of the Kompaneets equation. SIAM J. Math. Anal. 48(4), 2454–2494 (2016)
Mészáros, P., Bussard, R.W.: The angle-dependent Compton redistribution function in X-ray sources. Astrophys. J. 306, 238–247 (1986)
Norris, J.R.: Smoluchowski’s coagulation equation: uniqueness, nonuniqueness and a hydrodynamic limit for the stochastic coalescent. Ann. Appl. Probab. 9(1), 78–109 (1999)
Weyman, R.: Diffusion approximation for a photon gas interacting with a plasma via the compton effect. Phys. Fluids 8, 2112–2114 (1965)
Zel’Dovich, Y.B.: Reviews of topical problems: interaction of free electrons with electromagnetic radiation. Sov. Phys. Uspekhi 18, 79–98 (1975)
Zel’Dovich, Y.B., Levich, E.V.: Bose condensation and shock waves in photon spectra. Sov. J. Exp. Theor. Phys. 28, 1287–1290 (1969)
Zel’Dovich, Y.B., Levich, E.V., Syunyaev, R.A.: Stimulated compton interaction between Maxwellian electrons and spectrally narrow radiation. Sov. J. Exp. Theor. Phys. 35, 733–740 (1972)
Zel’Dovich, Y.B., Syunyaev, R.A.: Shock wave structure in the radiation spectrum during bose condensation of photons. Sov. J. Exp. Theor. Phys. 35, 81–85 (1972)
Acknowledgements
The research of the first author is supported by the Basque Government through the BERC 2014-2017 program, by the Spanish Ministry of Economy and Competitiveness MINECO: BCAM Severo Ochoa accreditation SEV-2013-0323, and by MTM2014-52347-C2-1-R of DGES. The research of the second author is supported by Grants MTM2014-52347-C2-1-R of DGES and IT641-13 of the Basque Government. The authors gratefully thank the referees for their careful reading of the manuscript and their valuable comments and recommendations.
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Appendices
Appendix A: Some Useful Estimates
Lemma A.1
If B satisfies (2.5)–(2.10), and \(\varphi \) is L-Lipschitz on \([0,\infty )\), then for all \((x,y)\in \Gamma \):
Moreover, the function \(\mathcal {L}_{\varphi }\) given in (2.31) is continuous on \([0,\infty )\) and for all \(x\in [0,\infty )\),
In particular, \(\mathcal {L}_{\varphi }(0)=0\).
Proof
We first prove (A.1). Let \((x,y)\in {\text {supp}}(B)=\Gamma \), and assume, by the symmetry of \(k_{\varphi }\), that \(0\le y\le x\). By the mean value theo, \(|e^{-x}-e^{-y}|\le e^{-y}(x-y)\), and from (2.11) and the Lipschitz condition,
and (A.1) follows.
In order to prove (A.2) we use (2.11) and the Lipschitz condition to have, for all \((x,y)\in \Gamma \),
Using that \(\Gamma \subset \{(x,y)\in [0,\infty )^2:\theta x\le y\le \theta ^{-1}x\}\), then
and (A.2) follows. We obtain (A.3) directly from (A.2) and Remark 2.1.
We finally prove the continuity of \(\mathcal {L}_{\varphi }\) on \([0,\infty )\). By (2.7)–(2.10), \(\mathcal {L}_{\varphi }(x)\) is continuous for all \(x>0\), so we only need to prove \(\mathcal {L}_{\varphi }(x)\rightarrow 0\) as \(x\rightarrow 0\). This follows from (A.3) and the mean value theo, using \( \gamma _2(x)-\gamma _1(x)\le (\theta ^{-1}-\theta )x. \)\(\square \)
Remark A.2
Under the hypothesis of Lemma A.1, the function \(k_{\varphi }\) could not be continuous at the origin \((x,y)=(0,0)\), since we do not know if \(\lim _{(x,y)\rightarrow (0,0)}k_{\varphi }(x,y)=0\). However we have the following.
Lemma A.3
If B satisfies (2.5)–(2.10), then \(k_{\varphi }\in C([0,\infty )^2)\) for all \(\varphi \in C^1([0,\infty ))\) with \(\varphi '(0)=0\), and \(k_{\varphi }(0,0)=0\).
Proof
By definition and (2.7), it is clear that \(k_{\varphi }\in C([0,\infty )^2\setminus \{0\})\). If we prove that \(\lim _{(x,y)\rightarrow (0,0)}k_{\varphi }(x,y)=0\), the continuity at the origin follows. To this end we mimic the proof of (A.1) using \(\varphi (x)-\varphi (y)=\varphi '(\xi )(x-y)\) for some \(\xi \in (\min \{x,y\},\max \{x,y\})\) instead of the Lipschitz condition, and we obtain
for all \((x,y)\in \Gamma \) and all \(\varphi \in C^1([0,\infty )).\) If \(\varphi '(0)=0\), it follows from (A.4) that \(\lim _{(x,y)\rightarrow (0,0)}k_{\varphi }(x,y)=0\). \(\square \)
Proposition A.4
Suppose that B satisfies (2.5)–(2.10), \(\varphi \) is L-Lipschitz on \([0,\infty )\), and \(u\in \mathscr {M}_+([0,\infty ))\). Then
where A is given in (A.1).
Proof
In order to prove (A.5), we use Remarks 2.1, 2.3 and (A.1):
from where (A.5) follows. The estimate (A.6) follows directly from (A.3). \(\square \)
Let us define now
Remark A.5
Since \(\phi _n\le x^{-1}\), the estimates (A.1)–(A.3) in Lemma A.1 hold for \(k_{\varphi ,n}\), \(\ell _{\varphi ,n}\) and \(\mathcal {L}_{\varphi ,n}\) respectively, and estimates (A.5) and (A.6) in Lemma A.4 hold for \(K_{\varphi ,n}(u,u)\) and \(L_{\varphi ,n}(u)\) respectively, for all \(n\in \mathbb {N}\).
Lemma A.6
\(\mathcal {L}_{\varphi ,n}\rightarrow \mathcal {L}_{\varphi }\) as \(n\rightarrow \infty \) uniformly on the compact sets of \([0,\infty )\) for all \(\varphi \)L-Lipschitz on \([0,\infty )\).
Proof
Let \(R>0\) and \(x\in [0,R]\). On the one hand, if \(x\in [0,1/n]\), we have \(|\mathcal {L}_{\varphi }(x)-\mathcal {L}_{\varphi ,n}(x)|\le 2|\mathcal {L}_{\varphi }(x)|\rightarrow 0\) as \(n\rightarrow \infty \), since \(\mathcal {L}_{\varphi }(0)=0\) (cf. Lemma A.1). On the other hand, if \(x\in [1/n,R]\) and \(y\in [1/n,n]\), by definition \(\phi _n(x)\phi _n(y)=(xy)^{-1}\), and then
The two integrals in the right hand side above are treated in the same way. Using \(|\ell _{\varphi }(x,y)-\ell _{\varphi ,n}(x,y)|\le |\ell _{\varphi }(x,y)|\) and (A.2),
and the result follows. \(\square \)
Appendix B: The Function \(\mathcal {B} _{ \beta }\), Properties and Scalings
In this Section, we describe several properties of the function \(\mathcal {B}_\beta \). First, the parameter \(\beta \) is used to scale the variables, in such a way that the total mass of the solution is conserved. Then, for each \(\beta >0\) fixed, the behavior of \(\mathcal {B}_\beta (k, k')\) is studied when k and \(k'\) are varying on \((0, \infty )\).
1.1 B.1 \(\beta \)-Scalings of \(\mathcal {B}_\beta \)
It looks natural from (1.2) to introduce the scaled variable
and define
The scaling (B.2) preserves the total number of particles:
In terms of F,
and if we define
that is,
the Eq. (1.2) then reads
If we now define
then from (B.5) we finally obtain
The second term in the right hand side of (B.7) seems then negligible when \(\beta \) tends to \(\infty \), but no rigorous result on that direction is known.
1.2 B.2 The Function \(B_\beta (x, x')\) for \(\beta \) Fixed.
In this Section we show some properties of the kernel \(B_{\beta }\) defined in (B.4).
Proposition B.1
For all \(\beta >0\), \(x>0\) and \(x'>0\),
and for all \(x>0,\;x'>0\) with \(x\ne x'\),
Proof
For all \(x>0\) and \(x'>0\),
and then (B.8) holds. If \(x'\not =x\), we have first
and since
then (B.9) follows from Lebesgue’s convergence Theorem. \(\square \)
Proposition B.2
Proof
By definition, for all \(x>0\),
and the result follows. \(\square \)
The function \(B_\beta \) is exponentially decreasing in the direction orthogonal to the first diagonal, as shown in the next two Propositions.
Proposition B.3
For all \(\beta >0\),
Proof
It is only a straightforward calculation. With the help of Mathematica, using the change of variables \(t=\cos \theta \),
The expression of \(\frac{\partial B_\beta }{\partial x'}\) is obtained from (B.15) and (B.16) using the permutation \(x\leftrightarrow x'\). Then,
and the result follows. \(\square \)
Proposition B.4
For all \(\beta >0\), \(x>0\) and \(x'>0\),
where
Proof
For all \(\mathbf x \in \mathbb {R}^3\) and \(\mathbf x '\in \mathbb {R}^3\) such that \(|\mathbf x |=x\), \(|\mathbf x '|=x'\),
Therefore,
and the result follows using (B.10). \(\square \)
Corollary B.5
as \(x+x'\rightarrow \infty \), and
If \(x+x'\rightarrow \infty \), and \(|x-x'|\le \theta x\):
For all \(\rho >0\) fixed and \(x>0\), \(x'>0\) such that \(x+x'=\rho \),
Proof
By Proposition B.3, the function \(B_\beta \) is strictly decreasing in the direction orthogonal to the first diagonal, and then property (B.21) follows. In order to prove (B.22) we have first, when \(x+x'\rightarrow \infty \),
If moreover, \(0\le x'-x \le \theta x\) then
If \(-\theta x \le x'-x\le 0\) then,
and (B.22) follows. \(\square \)
Proposition B.6
For all \(\varphi \in C_c((0, \infty )\times (0, \infty ))\):
Proof
Define the new variables
and denote \(\Psi _{\beta }(\xi ,\zeta )=\Phi _{\beta }(x,y)\). Then,
where \(D=\{(\zeta ,\xi )\in \mathbb {R}^2:\zeta >0,\;-\zeta<\xi <\zeta \}\). We write now,
and the change of variables:
whose Jacobian is \(\sqrt{2m/\beta }\, z_2\) and,
Due to the cut off function \(\Phi _\beta (x, y)\), the actual domain of integration \(\Omega _\beta \) is:
where \(\Omega \) is the domain where \(z_2>0\), \(z_1\in (-1, 1)\). As \(\beta \rightarrow \infty \),
On the other hand, using (B.12), for all \(z_1, z_2\),
By definition of \(\Psi \), for all \(z_1\in \mathbb {R}\) and \(z_2>0\) fixed, if \(\beta \) is sufficiently large,
Then,
\(\square \)
The function \(B_\beta (x, y)\ge 0\) coincides with \(\mathscr {B}_\beta (x, y)\) for \(x=y\) and is below that function, that tends to a Dirac measure along the first diagonal as \(\beta \rightarrow \infty \). From properties (B.9) and (B.24), the truncation of \(\mathcal {B}_\beta \) may then be seen as reasonable.
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Cortés, E., Escobedo, M. On a Boltzmann Equation for Compton Scattering from Non relativistic Electrons at Low Density. J Stat Phys 175, 819–878 (2019). https://doi.org/10.1007/s10955-019-02230-6
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DOI: https://doi.org/10.1007/s10955-019-02230-6