会议论文详细信息
5th Compact Stars in the QCD Phase Diagram
A self-consistent study of magnetic field effects on hybrid stars
Dexheimer, V.^1 ; Franzon, B.^2 ; Schramm, S.^2
Department of Physics, Kent State University, Kent
OH
44242, United States^1
FIAS, Ruth-Moufang 1, Frankfurt am Main
60438, Germany^2
关键词: Einstein's equations;    Magnetized neutron stars;    Neutron stars;    Stellar populations;    Strong magnetic fields;    Symmetric solution;    Temperature profiles;   
Others  :  https://iopscience.iop.org/article/10.1088/1742-6596/861/1/012012/pdf
DOI  :  10.1088/1742-6596/861/1/012012
来源: IOP
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【 摘 要 】

It is understood that strong magnetic fields affect the structure of neutron stars. Nevertheless, many calculations for magnetized neutron stars are still being performed using symmetric solutions of Einstein's equations. In this conference proceeding, we review why this is not the correct procedure and we also discuss the effects of magnetic fields on the stellar population and temperature profiles.

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