Publication:
Studying the onset of deconfinement with multi-messenger astronomy of neutron stars

Дата
2021
Авторы
Cierniak, M.
Blaschke, D.
Journal Title
Journal ISSN
Volume Title
Издатель
Научные группы
Организационные подразделения
Организационная единица
Институт лазерных и плазменных технологий
Стратегическая цель Института ЛаПлаз – стать ведущей научной школой и ядром развития инноваций по лазерным, плазменным, радиационным и ускорительным технологиям, с уникальными образовательными программами, востребованными на российском и мировом рынке образовательных услуг.
Выпуск журнала
Аннотация
© 2021 Wiley-VCH GmbHWith the first multi-messenger observation of a binary neutron star merger (GW170817), new constraints became available for masses and radii of neutron stars. We introduce a class of hybrid EoS that fulfills all these constraints and predicts a region in the mass-radius diagram that could be populated only by hybrid neutron stars with quark matter cores. A confirmation of this conjecture would be provided when the NICER radius measurement for the high-mass pulsar PSR J0740 + 6620 yields a radius significantly less than 11 km. Would this radius measurement yield a result in excess of 12 km, this would allow for both, a purely hadronic and a hybrid nature of this star. In the latter case, the maximum mass could reach 2.6 M⊙ so that the lighter object in the asymmetric binary merger GW190814 could have been a hybrid star. We demonstrate that this high mass can be compatible with an early onset of deconfinement for stars with masses below 1 M⊙ and the occurrence of low-mass twin stars. In such a case, the remnant of GW170817 could be a long-lived hypermassive pulsar.
Описание
Ключевые слова
Цитирование
Cierniak, M. Studying the onset of deconfinement with multi-messenger astronomy of neutron stars / Cierniak, M., Blaschke, D. // Astronomische Nachrichten. - 2021. - 10.1002/asna.202113909
Коллекции