Maqola

Astrophysical and Theoretical Physics Implications from Multimessenger Neutron Star Observations

Hector O. SilvaMax-Planck-Institut für Gravitationsphysik (Albert-Einstein-Institut), Am Mühlenberg 1, D-14476 Potsdam, GermanyA. M. HolgadoDepartment of Astronomy, University of Illinois at Urbana-Champaign, Urbana, Illinois 61801, USAAlejandro Cárdenas-AvendañoPrograma de Matemática, Fundación Universitaria Konrad Lorenz, 110231 Bogotá, ColombiaNicolás YunesDepartment of Physics and Illinois Center for Advanced Studies of the Universe, University of Illinois at Urbana-Champaign, Urbana, Illinois 61801, USA

2021en

ABI

Annotatsiya

The combination of gravitational-wave and x-ray observations of neutron stars provides new information on the mass distribution in these stars as well as new confirmation of Einstein's theory of gravity.

Hali tarjima qilinmagan

Identifikatorlar

DOI: 10.1103/physrevlett.126.181101

Iqtiboslar va manbalar

2 ta iqtibos0 ta foydalanilgan manba