Open Access
Issue
EPJ Web Conf.
Volume 158, 2017
The XXIII International Workshop “High Energy Physics and Quantum Field Theory” (QFTHEP 2017)
Article Number 05003
Number of page(s) 9
Section Astroparticle physics, Cosmology and Gravity Theory
DOI https://doi.org/10.1051/epjconf/201715805003
Published online 24 October 2017
  1. Ozel F., Freire P. Masses, radii, and equation of state of neutron star. Ann. Rev. Astron. Astrophys., 54, 401–440 (2016). [NASA ADS] [CrossRef]
  2. Weber F., Contera G. A., et al. Properties of high-density matter in neutron stars. Mod. Phys Lett. A, 29, 1430022 (2014). [NASA ADS] [CrossRef]
  3. Potekhin A. Y., Pons J. A., Page D. Neutron stars - cooling and transport. Space. Sci. Rev. 191, 239 (2015). [NASA ADS] [CrossRef]
  4. Turolla R., Zane S., Watts A. Magnetars: the physics behind observations. Rep. Prog. Phys. 78, 116901 (2015). [NASA ADS] [CrossRef]
  5. Iwamoto N. Quark Beta Decay and the Cooling of Neutron Stars. Phys.Rev.Lett., 44, 1637 (1980). [NASA ADS] [CrossRef]
  6. Schmitt A. Dense matter in compact stars. e-Print Arxiv: astro-ph.SR 1001.3294v2., (2010).
  7. Le Bellac M. Thermal Field Theory. ( Cambridge University Press, Cambridge, 1996) 269
  8. Gvozdev A. A., Osokina E. V. Neutrino processes in an external magnetic field in the density matrix formalism, TMP, 170: 3, C pp 354–375 (2012).
  9. Gradshteyn I. S., Ryzhik I.M. Table of Integrals, Series, and Products (7ed) (Academic Press, Oxford, 2007) 1161. [EDP Sciences]
  10. Mikheev N. V., Narynskaya E. N. Neutrino-electron processes in a dense magnetized plasma. Modern Physics Letters A., 15: 25, 1551–1556 (2000). [CrossRef]

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