Dense matter with eXTP

Tiziana Di Salvo, Rosario Iaria, Angelo Francesco Gambino, Liming Song, Sudip Bhattacharyya, Robert D. Ferdman, Manuel Linares, Alessandro Riggio, Kai Hebeler, Fangjun Lu, Aleksi Kurkela, Pavel Bakala, Holger Stiele, Renxin Xu, Dieter H. Hartmann, Sebastien Guillot, Xiaoyu Lai, Nathalie Degenaar, Martin Urbanec, Chanda Prescod-WeinsteinMaurizio Falanga, Simin Mahmoodifar, Yuri Cavecchi, Yupeng Xu, Alexander Heger, Tuomo Salmi, Andrea Sanna, Shijie Zheng, Mingyu Ge, Guobao Zhang, Xia Zhou, Wenda Zhang, Long Ji, Ingo Tews, Can Gungor, Eva Šrámková, Joonas Nättilä, Zhaosheng Li, Ang Li, Xiangdong Li, Wenda Zhang, Shuangnan Zhang, Shu Zhang, Andrea Santangelo, Jeroen Homan, Hendrik Schatz, Thomas E. Riley, Edward Brown, Coleman Miller, Svenja K. Greif, Altan Baykal, Sharon Morsink, Oleg Kargaltsev, Laura Tolos, Jean In’T Zand, Ignazio Bombaci, Melania Del Santo, Silvia Zane, Tod Strohmayer, Juri Poutanen, Benjamin Stappers, Andrea Possenti, Federico Bernardini, David Tsang, Marco Feroci, Achim Schwenk, Andrea Vacchi, Deepto Chakrabarty, Victor Doroshenko, Jinlu Qu, Anna L. Watts, Hendrik Schatz, Mariano Méndez, Wenfei Yu, Jérôme Chenevez, Slavko Bogdanov, Alessandro Patruno, Gabriel Török

Risultato della ricerca: Articlepeer review

41 Citazioni (Scopus)

Abstract

In this White Paper we present the potential of the Enhanced X-ray Timing and Polarimetry (eXTP) mission for determining the nature of dense matter; neutron star cores host an extreme density regime which cannot be replicated in a terrestrial laboratory. The tightest statistical constraints on the dense matter equation of state will come from pulse profile modelling of accretion-powered pulsars, burst oscillation sources, and rotation-powered pulsars. Additional constraints will derive from spin measurements, burst spectra, and properties of the accretion flows in the vicinity of the neutron star. Under development by an international Consortium led by the Institute of High Energy Physics of the Chinese Academy of Sciences, the eXTP mission is expected to be launched in the mid 2020s.
Lingua originaleEnglish
Numero di pagine17
RivistaSCIENCE CHINA. PHYSICS, MECHANICS & ASTRONOMY
Volume62
Stato di pubblicazionePublished - 2019

All Science Journal Classification (ASJC) codes

  • Physics and Astronomy(all)

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