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.
| Original language | English |
|---|---|
| Article number | 29503 |
| Number of pages | 17 |
| Journal | Science China: Physics, Mechanics and Astronomy |
| Volume | 62 |
| Issue number | 2 |
| DOIs | |
| Publication status | Published - 1 Feb 2019 |
Keywords
- dense matter
- equation of state
- neutron
- X-rays
Cite this
}
Dense matter with eXTP. / Watts, Anna L.; Yu, Wen Fei; Poutanen, Juri; Zhang, Shu; Bhattacharyya, Sudip; Bogdanov, Slavko; Ji, Long; Patruno, Alessandro; Riley, Thomas E.; Bakala, Pavel; Baykal, Altan; Bernardini, Federico; Bombaci, Ignazio; Brown, Edward; Cavecchi, Yuri; Chakrabarty, Deepto; Chenevez, Jérôme; Degenaar, Nathalie; Del Santo, Melania; Di Salvo, Tiziana; Doroshenko, Victor; Falanga, Maurizio; Ferdman, Robert D.; Feroci, Marco; Gambino, Angelo F.; Ge, Ming Yu; Greif, Svenja K.; Guillot, Sebastien; Gungor, Can; Hartmann, Dieter H.; Hebeler, Kai; Heger, Alexander; Homan, Jeroen; Iaria, Rosario; Zand, Jean in’t; Kargaltsev, Oleg; Kurkela, Aleksi; Lai, Xiao Yu; Li, Ang; Li, Xiang Dong; Li, Zhao Sheng; Linares, Manuel; Lu, Fang Jun; Mahmoodifar, Simin; Méndez, Mariano; Coleman Miller, M.; Morsink, Sharon; Nättilä, Joonas; Possenti, Andrea; Prescod-Weinstein, Chanda; Qu, Jin Lu; Riggio, Alessandro; Salmi, Tuomo; Sanna, Andrea; Santangelo, Andrea; Schatz, Hendrik; Schwenk, Achim; Song, Li Ming; Šrámková, Eva; Stappers, Benjamin; Stiele, Holger; Strohmayer, Tod; Tews, Ingo; Tolos, Laura; Török, Gabriel; Tsang, David; Urbanec, Martin; Vacchi, Andrea; Xu, Ren Xin; Xu, Yu Peng; Zane, Silvia; Zhang, Guo Bao; Zhang, Shuang Nan; Zhang, Wen Da; Zheng, Shi Jie; Zhou, Xia.
In: Science China: Physics, Mechanics and Astronomy, Vol. 62, No. 2, 29503, 01.02.2019.Research output: Contribution to journal › Review Article › Research › peer-review
TY - JOUR
T1 - Dense matter with eXTP
AU - Watts, Anna L.
AU - Yu, Wen Fei
AU - Poutanen, Juri
AU - Zhang, Shu
AU - Bhattacharyya, Sudip
AU - Bogdanov, Slavko
AU - Ji, Long
AU - Patruno, Alessandro
AU - Riley, Thomas E.
AU - Bakala, Pavel
AU - Baykal, Altan
AU - Bernardini, Federico
AU - Bombaci, Ignazio
AU - Brown, Edward
AU - Cavecchi, Yuri
AU - Chakrabarty, Deepto
AU - Chenevez, Jérôme
AU - Degenaar, Nathalie
AU - Del Santo, Melania
AU - Di Salvo, Tiziana
AU - Doroshenko, Victor
AU - Falanga, Maurizio
AU - Ferdman, Robert D.
AU - Feroci, Marco
AU - Gambino, Angelo F.
AU - Ge, Ming Yu
AU - Greif, Svenja K.
AU - Guillot, Sebastien
AU - Gungor, Can
AU - Hartmann, Dieter H.
AU - Hebeler, Kai
AU - Heger, Alexander
AU - Homan, Jeroen
AU - Iaria, Rosario
AU - Zand, Jean in’t
AU - Kargaltsev, Oleg
AU - Kurkela, Aleksi
AU - Lai, Xiao Yu
AU - Li, Ang
AU - Li, Xiang Dong
AU - Li, Zhao Sheng
AU - Linares, Manuel
AU - Lu, Fang Jun
AU - Mahmoodifar, Simin
AU - Méndez, Mariano
AU - Coleman Miller, M.
AU - Morsink, Sharon
AU - Nättilä, Joonas
AU - Possenti, Andrea
AU - Prescod-Weinstein, Chanda
AU - Qu, Jin Lu
AU - Riggio, Alessandro
AU - Salmi, Tuomo
AU - Sanna, Andrea
AU - Santangelo, Andrea
AU - Schatz, Hendrik
AU - Schwenk, Achim
AU - Song, Li Ming
AU - Šrámková, Eva
AU - Stappers, Benjamin
AU - Stiele, Holger
AU - Strohmayer, Tod
AU - Tews, Ingo
AU - Tolos, Laura
AU - Török, Gabriel
AU - Tsang, David
AU - Urbanec, Martin
AU - Vacchi, Andrea
AU - Xu, Ren Xin
AU - Xu, Yu Peng
AU - Zane, Silvia
AU - Zhang, Guo Bao
AU - Zhang, Shuang Nan
AU - Zhang, Wen Da
AU - Zheng, Shi Jie
AU - Zhou, Xia
PY - 2019/2/1
Y1 - 2019/2/1
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 - dense matter
KW - equation of state
KW - neutron
KW - X-rays
UR - http://www.scopus.com/inward/record.url?scp=85052728338&partnerID=8YFLogxK
U2 - 10.1007/s11433-017-9188-4
DO - 10.1007/s11433-017-9188-4
M3 - Review Article
VL - 62
JO - Science China Physics, Mechanics & Astronomy
JF - Science China Physics, Mechanics & Astronomy
SN - 1674-7348
IS - 2
M1 - 29503
ER -