Stellar matter with pseudoscalar condensates

The European Physical Journal C

D. Espriu¹  S. S. Kolevatov²  V. A. Andrianov²  A. A. Andrianov³ 

[1] Departament d’Estructura i Constituents de la Matèria and Institut de Ciències del Cosmos (ICCUB), Universitat de Barcelona, Martí i Franquès 1, 08028, Barcelona, Catalonia, Spain;Saint-Petersburg State University, 7/9 Universitetskaya nab, 199034, St.Petersburg, Russia;Saint-Petersburg State University, 7/9 Universitetskaya nab, 199034, St.Petersburg, Russia;Departament d’Estructura i Constituents de la Matèria and Institut de Ciències del Cosmos (ICCUB), Universitat de Barcelona, Martí i Franquès 1, 08028, Barcelona, Catalonia, Spain;

关键词: Neutron Star;    White Dwarf;    Compact Star;    Parity Breaking;    Axion Condensate;   

DOI  :  10.1140/epjc/s10052-016-4012-1

来源: Springer

【 摘 要 】

In this work we consider how the appearance of gradients of pseudoscalar condensates in dense systems may possibly influence the transport properties of photons in such a medium as well as other thermodynamic characteristics. We adopt the hypothesis that in regions where the pseudoscalar density gradient is large the properties of photons and fermions are governed by the usual lagrangian extended with a Chern–Simons interaction for photons and a constant axial field for fermions. We find that these new pieces in the lagrangian produce non-trivial reflection coefficients both for photons and fermions when entering or leaving a region where the pseudoscalar has a non-zero gradient. A varying pseudoscalar density may also lead to instability of some fermion and boson modes and modify some properties of the Fermi sea. We speculate that some of these modifications could influence the cooling rate of stellar matter (for instance in compact stars) and have other observable consequences. While quantitative results may depend on the precise astrophysical details most of the consequences are quite universal and consideration should be given to this possibility.

【 授权许可】

CC BY