Holographic neutrino transport in dense strongly-coupled matter

被引:6
|
作者
Jarvinen, M. [1 ,2 ]
Kiritsis, E. [3 ,4 ]
Nitti, F. [3 ]
Preau, E. [3 ]
机构
[1] Asia Pacific Ctr Theoret Phys, Pohang 37673, South Korea
[2] Pohang Univ Sci & Technol, Dept Phys, Pohang 37673, South Korea
[3] Univ Paris Cite, CNRS, Astroparticule & Cosmol, F-75006 Paris, France
[4] Univ Crete, Inst Theoret & Computat Phys, Crete Ctr Theoret Phys, Dept Phys, POB 2208, Iraklion 70013, Greece
基金
新加坡国家研究基金会; 欧洲研究理事会;
关键词
Holography and Hydrodynamics; Neutrino Interactions; Non-Equilibrium Field Theory; Nonperturbative Effects; BETA-DECAY; CORE-COLLAPSE; QCD; EMISSION; PHYSICS; STARS; PION;
D O I
10.1007/JHEP11(2023)139
中图分类号
O412 [相对论、场论]; O572.2 [粒子物理学];
学科分类号
摘要
A (toy) model for cold and luke-warm strongly-coupled nuclear matter at finite baryon density, is used to study neutrino transport. The complete charged current two-point correlators are computed in the strongly-coupled medium and their impact on neutrino transport is analyzed. The full result is compared with various approximations for the current correlators and the distributions, including the degenerate approximation, the hydrodynamic approximation as well as the diffusive approximation and we comment on their successes. Further improvements are discussed.
引用
收藏
页数:85
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