期刊
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS
卷 -, 期 10, 页码 -出版社
IOP PUBLISHING LTD
DOI: 10.1088/1475-7516/2013/10/021
关键词
modified gravity; magnetic fields; neutron stars; massive stars
资金
- US Department of Energy [DE-SC0010137]
- US National Science Foundation [PHY-1342611]
- National Research Foundation of Korea [20110003188, 2011-0015467, 2012M7A1A2055605]
- JSPS [20244035]
- Ministry of Education, Science and Culture of Japan [20244035, 21540412]
- Scientific Research on Innovative Area of MEXT [20105004]
- Heiwa Nakajima Foundation
- U.S. Department of Energy under Nuclear Theory Grant [DE-FG02-95-ER40934]
- Grants-in-Aid for Scientific Research [21540412] Funding Source: KAKEN
In Kaluza-Klein electromagnetism it is natural to associate modified gravity with strong electromagnetic fields. Hence, in this paper we investigate the combined effects of a strong magnetic field and perturbative f(R) gravity on the structure of neutron stars. The effect of an interior strong magnetic field of about 10(17-18) G on the equation of state is derived in the context of a quantum hadrodynamics (QHD) equation of state (EoS) including effects of the magnetic pressure and energy along with occupied Landau levels. Adopting a random orientation of interior field domains, we solve the modified spherically symmetric hydrostatic equilibrium equations derived for a gravity model with f(R) = R + alpha R-2. Effects of both the finite magnetic field and the modified gravity are detailed for various values of the magnetic field and the perturbation parameter a along with a discussion of their physical implications. We show that there exists a parameter space of the modified gravity and the magnetic field strength, in which even a soft equation of state can accommodate a large (>2 M-circle dot) maximum neutron star mass.
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