17-21 September 2019
Yerevan, Armenia
Etc/GMT+4 timezone

Astrophysical aspects of general relativistic mass twin stars

20 Sep 2019, 14:30
Yerevan, Armenia

Yerevan, Armenia

Department of Physics, Alex Manoogian str. 1, Yerevan, Armenia


Noshad Khosravi (Alzahra University, Iran)


An effective, multi-polytope equation of state (EoS) model is used to study the so-called “mass twins” scenario, where two compact stars have approximately the same mass but (significant for observation) quite different radii. Stellar mass twin configurations are obtained if a strong first-order phase transition occurs in the interior of a compact star. In the mass-radius diagram of compact stars, this leads to a third branch of gravitationally stable stars with features that are very different from those of white dwarfs and neutron stars. Rotating hybrid star sequences are discussed in the slow rotation approximation and in full general relativity and conclusions are drawn [1] for an upper limit on the maximum mass of nonrotating compact stars that has recently been deduced from the observation of the merger event GW170817.

[1] D. Blaschke et al., arXiv:1906.02522 (2019)

Primary authors

David Blaschke (University of Wroclaw) Noshad Khosravi (Alzahra University, Iran) Dr David Edwin Alvarez Castillo (JINR) Alexander Ayriyan (JINR & AANL) Dr Hovik Grigorian Prof. Fridolin Weber (San Diego State University)

Presentation Materials