2015/04/02 by Stefan Schramm, S. Schramm, Abhijit Bhattacharyya +9
Earth and Planetary Sciences · Engineering · Physics and Astronomy · #FOS: Physical sciences #High-pressure geophysics and materials #Nuclear Theory (nucl-th) #Pulsars and Gravitational Waves Research #Solar and Stellar Astrophysics (astro-ph.SR) #Superconducting Materials and Applications #astro-ph.SR #nucl-th
paper · pdf · doi:10.48550/arxiv.1504.00451
Contribution to the Proceedings of CSQCD IV, Prerow (2014)
arxiv created 2015/04/02 · openalex publication_date 2015/04/02 · arxiv updated 2015/04/03 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
Neutron stars feature extremely high magnetic fields with deduced field strengths of 1015 G in the case of magnetars and potentially much higher values inside of the star. In this context we consider the appearance of ρ- meson condensation taking into account the effect of the magnetic field. The results show that, depending on parameters, such a condensation in magnetized neutron stars might (just) occur.