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2011

Analytical Representation for Equations of State of Dense Matter

Gungor, Can, Eksi, K. Yavuz

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We present an analytical unified representation for 22 equations of state (EoS) of dense matter in neutron stars.

Such analytical representations can be useful for modeling neutron star structure in modified theories of gravity with high order derivatives.

Analytical Representation for Equations of State of Dense Matter · Around

Built on

Oppenheimer, J. R., & Volkoff, G. M. 1939, Physical Review, 55, 374
1939
Earlier work this paper cites.
Tolman, R. C. 1939, Physical Review, 55, 364
Original
1939
Earlier work this paper cites.
Baym, G., Pethick, C., & Sutherland, P. 1971, ApJ, 170, 299
1971
Earlier work this paper cites.

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Negele, J. W., & Vautherin, D. 1973, Nuclear Physics A, 207, 298
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Haensel, P., & Potekhin, A. Y. 2004, A&A, 428, 191
2004
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Then

de Felice, A., & Tsujikawa, S. 2010, Living Reviews in Relativity, 13, 3
2010
Later among the works it cites.
Arapoglu, A. S., Deliduman, C., & Eksi, K. Y. 2011, JCAP, 2011, 020
2011
Closest in time.

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