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-Weinstein; Maurizio 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; null 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

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

Fisica e Chimica - Emilio Segrè

Risultato della ricerca: Article › peer 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 originale	English
Numero di pagine	17
Rivista	SCIENCE CHINA. PHYSICS, MECHANICS & ASTRONOMY
Volume	62
Stato di pubblicazione	Published - 2019

All Science Journal Classification (ASJC) codes

Physics and Astronomy(all)

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Dense matter with eXTP. / Di Salvo, Tiziana ; Iaria, Rosario ; Gambino, Angelo Francesco; 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; Zhang, Wenda; 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.; Schatz, Hendrik; Méndez, Mariano; Yu, Wenfei; Chenevez, Jérôme; Bogdanov, Slavko; Patruno, Alessandro; Török, Gabriel.

In: SCIENCE CHINA. PHYSICS, MECHANICS & ASTRONOMY, Vol. 62, 2019.

Risultato della ricerca: Article › peer review

Di Salvo, T , Iaria, R , Gambino, AF, Song, L, Bhattacharyya, S, Ferdman, RD, Linares, M, Riggio, A, Hebeler, K, Lu, F, Kurkela, A, Bakala, P, Stiele, H, Xu, R, Hartmann, DH, Guillot, S, Lai, X, Degenaar, N, Urbanec, M, Prescod-Weinstein, C, Falanga, M, Mahmoodifar, S, Cavecchi, Y, Xu, Y, Heger, A, Salmi, T, Sanna, A, Zheng, S, Ge, M, Zhang, G, Zhou, X, Zhang, W, Ji, L, Tews, I, Gungor, C, Šrámková, E, Nättilä, J, Li, Z, Li, A, Li, X, Zhang, W, Zhang, S, Zhang, S, Santangelo, A, Homan, J, Schatz, H, Riley, TE, Brown, E, Coleman Miller, Greif, SK, Baykal, A, Morsink, S, Kargaltsev, O, Tolos, L, Zand, JIT, Bombaci, I, Del Santo, M, Zane, S, Strohmayer, T, Poutanen, J, Stappers, B, Possenti, A, Bernardini, F, Tsang, D, Feroci, M, Schwenk, A, Vacchi, A, Chakrabarty, D, Doroshenko, V, Qu, J, Watts, AL, Schatz, H, Méndez, M, Yu, W, Chenevez, J, Bogdanov, S, Patruno, A & Török, G 2019, 'Dense matter with eXTP', SCIENCE CHINA. PHYSICS, MECHANICS & ASTRONOMY, vol. 62.

Di Salvo, Tiziana ; Iaria, Rosario ; Gambino, Angelo Francesco ; 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 ; Zhang, Wenda ; 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. ; Schatz, Hendrik ; Méndez, Mariano ; Yu, Wenfei ; Chenevez, Jérôme ; Bogdanov, Slavko ; Patruno, Alessandro ; Török, Gabriel. / Dense matter with eXTP. In: SCIENCE CHINA. PHYSICS, MECHANICS & ASTRONOMY. 2019 ; Vol. 62.

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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.",

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

year = "2019",

language = "English",

volume = "62",

journal = "SCIENCE CHINA. PHYSICS, MECHANICS & ASTRONOMY",

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TY - JOUR

T1 - Dense matter with eXTP

AU - Di Salvo, Tiziana

AU - Iaria, Rosario

AU - Gambino, Angelo Francesco

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 - Zhang, Wenda

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 - Schatz, Hendrik

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

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 - Article

VL - 62

JO - SCIENCE CHINA. PHYSICS, MECHANICS & ASTRONOMY

JF - SCIENCE CHINA. PHYSICS, MECHANICS & ASTRONOMY

SN - 1674-7348

ER -