Dense matter with eXTP

eXTP collaboration

doi:10.1007/s11433-017-9188-4

Dense matter with eXTP

eXTP collaboration

Vrije Universiteit Amsterdam
Shanghai Astronomical Observatory Chinese Academy of Sciences
University of Turku
AlbaNova University Center
Chinese Academy of Sciences
Tata Institute of Fundamental Research, Hyderabad
Columbia University
University of Tübingen
Leiden University
Silesian University in Opava
Middle East Technical University
INAF-Osservatorio Astronomico di Roma
New York University Abu Dhabi
University of Pisa
Istituto Nazionale di Fisica Nucleare - Sezione di Pisa
Michigan State University
Princeton University
University of Southampton
MIT Kavli Institute for Astrophysics and Space Research
Technical University of Denmark
INAF - Istituto di Astrofisica Spaziale e Fisica Cosmica di Palermo
Università di Palermo
International Space Science Institute
University of East Anglia
INAF-Istituto di Astrofisica e Planetologia Spaziali
Technische Universität Darmstadt
GSI Helmholtzzentrum fur Schwerionenforschung GmbH
Pontificia Universidad Católica de Chile
Clemson University
Monash University
SRON Netherlands Institute for Space Research
George Washington University
CERN
University of Stavanger
Hubei University of Education
Xiamen University
Nanjing University
Xiangtan University
Universitat Politècnica de Catalunya
NASA Goddard Space Flight Center
Rijksuniversiteit Groningen
Space Science Institute
University of Alberta
INAF - Osservatorio Astronomico di Cagliari

Research output: Contribution to journal › Review article › peer-review

126 Citations (SciVal)

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
Journal	Science China: Physics, Mechanics and Astronomy
Volume	62
Issue number	2
Early online date	20 Aug 2018
DOIs	https://doi.org/10.1007/s11433-017-9188-4
Publication status	Published - 1 Feb 2019

Bibliographical note

Funding Information:
ALW and TER acknowledge support from ERC Starting (Grant No. 639217 CSINEUTRONSTAR). AP acknowledges support from a Netherlands Organization for Scientific Research (NWO) Vidi Fellowship. YC is suported by the European Union Horizon 2020 research and innovation programme under the Marie Sklodowska-Curie Global Fellowship (Grant No. 703916). SKG, KH and AS are supported in part by the DFG through Grant SFB 1245 and the ERC (Grant No. 307986 STRONGINT). The Chinese team acknowledges the support of the Chinese Academy of Sciences through the Strategic Priority Research Program of the Chinese Academy of Sciences (Grant No. XDA15020100).

Publisher Copyright:
© 2018, Science China Press and Springer-Verlag GmbH Germany, part of Springer Nature.

Copyright:
Copyright 2020 Elsevier B.V., All rights reserved.

Funding

ALW and TER acknowledge support from ERC Starting (Grant No. 639217 CSINEUTRONSTAR). AP acknowledges support from a Netherlands Organization for Scientific Research (NWO) Vidi Fellowship. YC is suported by the European Union Horizon 2020 research and innovation programme under the Marie Sklodowska-Curie Global Fellowship (Grant No. 703916). SKG, KH and AS are supported in part by the DFG through Grant SFB 1245 and the ERC (Grant No. 307986 STRONGINT). The Chinese team acknowledges the support of the Chinese Academy of Sciences through the Strategic Priority Research Program of the Chinese Academy of Sciences (Grant No. XDA15020100).

Keywords

dense matter
equation of state
neutron
X-rays

ASJC Scopus subject areas

General Physics and Astronomy

Access to Document

10.1007/s11433-017-9188-4

https://eprints.soton.ac.uk/426609/

Cite this

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title = "Dense matter with eXTP",

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.",

keywords = "dense matter, equation of state, neutron, X-rays",

author = "\{eXTP collaboration\} and Watts, \{Anna L.\} and Yu, \{Wen Fei\} and Juri Poutanen and Shu Zhang and Sudip Bhattacharyya and Slavko Bogdanov and Long Ji and Alessandro Patruno and Riley, \{Thomas E.\} and Pavel Bakala and Altan Baykal and Federico Bernardini and Ignazio Bombaci and Edward Brown and Yuri Cavecchi and Deepto Chakrabarty and J{\'e}r{\^o}me Chenevez and Nathalie Degenaar and \{Del Santo\}, Melania and \{Di Salvo\}, Tiziana and Victor Doroshenko and Maurizio Falanga and Ferdman, \{Robert D.\} and Marco Feroci and Gambino, \{Angelo F.\} and Ge, \{Ming Yu\} and Greif, \{Svenja K.\} and Sebastien Guillot and Can Gungor and Hartmann, \{Dieter H.\} and Kai Hebeler and Alexander Heger and Jeroen Homan and Rosario Iaria and Zand, \{Jean in{\textquoteright}t\} and Oleg Kargaltsev and Aleksi Kurkela and Lai, \{Xiao Yu\} and Ang Li and Li, \{Xiang Dong\} and Li, \{Zhao Sheng\} and Manuel Linares and Lu, \{Fang Jun\} and Simin Mahmoodifar and Mariano M{\'e}ndez and \{Coleman Miller\}, M. and Sharon Morsink and Joonas N{\"a}ttil{\"a} and Andrea Possenti and David Tsang",

note = "Funding Information: ALW and TER acknowledge support from ERC Starting (Grant No. 639217 CSINEUTRONSTAR). AP acknowledges support from a Netherlands Organization for Scientific Research (NWO) Vidi Fellowship. YC is suported by the European Union Horizon 2020 research and innovation programme under the Marie Sklodowska-Curie Global Fellowship (Grant No. 703916). SKG, KH and AS are supported in part by the DFG through Grant SFB 1245 and the ERC (Grant No. 307986 STRONGINT). The Chinese team acknowledges the support of the Chinese Academy of Sciences through the Strategic Priority Research Program of the Chinese Academy of Sciences (Grant No. XDA15020100). Publisher Copyright: {\textcopyright} 2018, Science China Press and Springer-Verlag GmbH Germany, part of Springer Nature. Copyright: Copyright 2020 Elsevier B.V., All rights reserved.",

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doi = "10.1007/s11433-017-9188-4",

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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

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AU - Coleman Miller, M.

AU - Morsink, Sharon

AU - Nättilä, Joonas

AU - Possenti, Andrea

AU - Tsang, David

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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

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DO - 10.1007/s11433-017-9188-4

M3 - Review article

AN - SCOPUS:85052728338

SN - 1674-7348

VL - 62

JO - Science China: Physics, Mechanics and Astronomy

JF - Science China: Physics, Mechanics and Astronomy

IS - 2

M1 - 29503

ER -

Dense matter with eXTP

Abstract

Bibliographical note

Funding

Keywords

ASJC Scopus subject areas

Access to Document

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Cite this