Slowly rotating anisotropic neutron stars in general relativity and scalar-tensor theory

Some models (such as the Skyrme model, a low-energy effective field theory for quantum chromodynamics) suggest that the high-density matter prevailing in neutron star (NS) interiors may be significantly anisotropic. Anisotropy is known to affect the bulk properties of nonrotating NSs in general rela...

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Veröffentlicht in:	Classical and quantum gravity 2015-07, Vol.32 (14), p.145008-145025
Hauptverfasser:	Silva, Hector O, Macedo, Caio F B, Berti, Emanuele, Crispino, Luís C B
Format:	Artikel
Sprache:	eng
Schlagworte:	Anisotropy equation of state general relativity Mathematical models modified theories of gravity Neutron stars Pulsars Quantum gravity relativistic stars Relativity Rotating Spontaneous
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