Influence of the pseudoscalar condensate gradient on the cooling regime of compact stars
From MaRDI portal
Publication:2014437
DOI10.1134/S0040577917020015zbMath1369.85004OpenAlexW2594204612MaRDI QIDQ2014437
S. S. Kolevatov, Domènec Espriu, V. A. Andrianov, Alexander A. Andrianov
Publication date: 25 August 2017
Published in: Theoretical and Mathematical Physics (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1134/s0040577917020015
Related Items (1)
Cites Work
- Unnamed Item
- Search for parity violation in cosmic rays
- Velocity addition and a closed time cycle in Lorentz-noninvariant theories
- The sphaleron rate in SU(\(N\)) gauge theory
- Axion stars in the infrared limit
- Propagation of photons and massive vector mesons between a parity breaking medium and vacuum
- Transmission of vector particles through the interface of a spatial parity-violating medium and the vacuum
- General relativistic boson stars
- Finite-Temperature Field Theory
This page was built for publication: Influence of the pseudoscalar condensate gradient on the cooling regime of compact stars