Abstract
| Lingua originale | English |
|---|---|
| Numero di pagine | 17 |
| Rivista | Default journal |
| Volume | 62 |
| Stato di pubblicazione | Published - 2019 |
All Science Journal Classification (ASJC) codes
- Physics and Astronomy(all)
Cita questo
Dense matter with eXTP. / Gambino, Angelo Francesco; Iaria, Rosario; Di Salvo, Tiziana; Song, Liming; Bhattacharyya, Sudip; Ferdman, Robert D.; Linares, Manuel; Riggio, Alessandro; Hebeler, Kai; Lu, Fangjun; Kurkela, Aleksi; Bakala, Pavel; Stiele, Holger; Xu, Renxin; Hartmann, Dieter H.; Guillot, Sebastien; Lai, Xiaoyu; Degenaar, Nathalie; Urbanec, Martin; Prescod-Weinstein, Chanda; Falanga, Maurizio; Mahmoodifar, Simin; Cavecchi, Yuri; Xu, Yupeng; Heger, Alexander; Salmi, Tuomo; Sanna, Andrea; Zheng, Shijie; Ge, Mingyu; Zhang, Guobao; Zhou, Xia; Ji, Long; Tews, Ingo; Gungor, Can; Šrámková, Eva; Nättilä, Joonas; Li, Zhaosheng; Li, Ang; Li, Xiangdong; Zhang, Wenda; Zhang, Shuangnan; Zhang, Shu; Santangelo, Andrea; Homan, Jeroen; Schatz, Hendrik; Riley, Thomas E.; Brown, Edward; Coleman Miller; Greif, Svenja K.; Baykal, Altan; Morsink, Sharon; Kargaltsev, Oleg; Tolos, Laura; Zand, Jean In’T; Bombaci, Ignazio; Del Santo, Melania; Zane, Silvia; Strohmayer, Tod; Poutanen, Juri; Stappers, Benjamin; Possenti, Andrea; Bernardini, Federico; Tsang, David; Feroci, Marco; Schwenk, Achim; Vacchi, Andrea; Chakrabarty, Deepto; Doroshenko, Victor; Qu, Jinlu; Watts, Anna L.; Méndez, Mariano; Yu, Wenfei; Chenevez, Jérôme; Bogdanov, Slavko; Patruno, Alessandro; Török, Gabriel.
In: Default journal, Vol. 62, 2019.Risultato della ricerca: Book/Film/Article review
}
TY - JOUR
T1 - Dense matter with eXTP
AU - Gambino, Angelo Francesco
AU - Iaria, Rosario
AU - Di Salvo, Tiziana
AU - Song, Liming
AU - Bhattacharyya, Sudip
AU - Ferdman, Robert D.
AU - Linares, Manuel
AU - Riggio, Alessandro
AU - Hebeler, Kai
AU - Lu, Fangjun
AU - Kurkela, Aleksi
AU - Bakala, Pavel
AU - Stiele, Holger
AU - Xu, Renxin
AU - Hartmann, Dieter H.
AU - Guillot, Sebastien
AU - Lai, Xiaoyu
AU - Degenaar, Nathalie
AU - Urbanec, Martin
AU - Prescod-Weinstein, Chanda
AU - Falanga, Maurizio
AU - Mahmoodifar, Simin
AU - Cavecchi, Yuri
AU - Xu, Yupeng
AU - Heger, Alexander
AU - Salmi, Tuomo
AU - Sanna, Andrea
AU - Zheng, Shijie
AU - Ge, Mingyu
AU - Zhang, Guobao
AU - Zhou, Xia
AU - Ji, Long
AU - Tews, Ingo
AU - Gungor, Can
AU - Šrámková, Eva
AU - Nättilä, Joonas
AU - Li, Zhaosheng
AU - Li, Ang
AU - Li, Xiangdong
AU - Zhang, Wenda
AU - Zhang, Shuangnan
AU - Zhang, Shu
AU - Santangelo, Andrea
AU - Homan, Jeroen
AU - Schatz, Hendrik
AU - Riley, Thomas E.
AU - Brown, Edward
AU - Coleman Miller, null
AU - Greif, Svenja K.
AU - Baykal, Altan
AU - Morsink, Sharon
AU - Kargaltsev, Oleg
AU - Tolos, Laura
AU - Zand, Jean In’T
AU - Bombaci, Ignazio
AU - Del Santo, Melania
AU - Zane, Silvia
AU - Strohmayer, Tod
AU - Poutanen, Juri
AU - Stappers, Benjamin
AU - Possenti, Andrea
AU - Bernardini, Federico
AU - Tsang, David
AU - Feroci, Marco
AU - Schwenk, Achim
AU - Vacchi, Andrea
AU - Chakrabarty, Deepto
AU - Doroshenko, Victor
AU - Qu, Jinlu
AU - Watts, Anna L.
AU - Méndez, Mariano
AU - Yu, Wenfei
AU - Chenevez, Jérôme
AU - Bogdanov, Slavko
AU - Patruno, Alessandro
AU - Török, Gabriel
PY - 2019
Y1 - 2019
N2 - 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.
AB - 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.
KW - Physics and Astronomy (all)
KW - X-rays
KW - dense matter
KW - equation of state
KW - neutron
UR - http://hdl.handle.net/10447/338147
UR - http://www.springer.com/physics/journal/11433
M3 - Book/Film/Article review
VL - 62
JO - Default journal
JF - Default journal
ER -