18-23 March 2018
Florianopolis, Brazil
America/Sao_Paulo timezone

Thermodynamic consistency in magnetized neutron stars

20 Mar 2018, 16:00
Florianopolis, Brazil

Florianopolis, Brazil


Luiz Lopes (Centro Federal de Educação Tecnológica de Minas Gerais)


In this work we show how to indroduce the magnetic field in hadronic matter in a thermodynamically consistent way. We revisit the literature and show that several common results that are derived magnetic field on hadronic matter are thermodynamically inconsistent and that affects the mass-radius results.

Utilizing the so called choatic magnetic field [1,2,3,4] we show that a thermodynamically consistent way is possible and give us more reliable results.

[1] Ya. B. Zel’dovich, I. D. Nivikov it Stars and Relativity, Dover, New York (1996)
[2] C. W. Misner, Kip S. Thorne, J. A. Wheeler Gravitation, Freeman and Company, San Francisco (1973)
[3] L. Lopes, D. Menezes, JCAP 08 (2015) 002
[4] L. Lopes, D. Menezes, Eur. Phys. J. A, 52 2 (2016) 17

Primary authors

Luiz Lopes (Centro Federal de Educação Tecnológica de Minas Gerais) Debora Menezes (UFSC)

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