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Dense matter with eXTP
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 d...
Autores principales: | , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , |
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Lenguaje: | eng |
Publicado: |
2019
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Materias: | |
Acceso en línea: | https://dx.doi.org/10.1007/s11433-017-9188-4 http://cds.cern.ch/record/2671647 |
_version_ | 1780962428911091712 |
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author | Watts, Anna L Yu, WenFei 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 Santo, Melania Salvo, Tiziana Doroshenko, Victor Falanga, Maurizio Ferdman, Robert D Feroci, Marco Gambino, Angelo F Ge, MingYu Greif, Svenja K Guillot, Sebastien Gungor, Can Hartmann, Dieter H Hebeler, Kai Heger, Alexander Homan, Jeroen Iaria, Rosario in't Zand, Jean Kargaltsev, Oleg Kurkela, Aleksi Lai, XiaoYu Li, Ang Li, XiangDong Li, ZhaoSheng Linares, Manuel Lu, FangJun Mahmoodifar, Simin Méndez, Mariano Coleman Miller, M Morsink, Sharon Nättilä, Joonas Possenti, Andrea Prescod-Weinstein, Chanda Qu, JinLu Riggio, Alessandro Salmi, Tuomo Sanna, Andrea Santangelo, Andrea Schatz, Hendrik Schwenk, Achim Song, LiMing Šrámková, Eva Stappers, Benjamin Stiele, Holger Strohmayer, Tod Tews, Ingo Tolos, Laura Török, Gabriel Tsang, David Urbanec, Martin Vacchi, Andrea Xu, RenXin Xu, YuPeng Zane, Silvia Zhang, GuoBao Zhang, ShuangNan Zhang, WenDa Zheng, ShiJie Zhou, Xia |
author_facet | Watts, Anna L Yu, WenFei 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 Santo, Melania Salvo, Tiziana Doroshenko, Victor Falanga, Maurizio Ferdman, Robert D Feroci, Marco Gambino, Angelo F Ge, MingYu Greif, Svenja K Guillot, Sebastien Gungor, Can Hartmann, Dieter H Hebeler, Kai Heger, Alexander Homan, Jeroen Iaria, Rosario in't Zand, Jean Kargaltsev, Oleg Kurkela, Aleksi Lai, XiaoYu Li, Ang Li, XiangDong Li, ZhaoSheng Linares, Manuel Lu, FangJun Mahmoodifar, Simin Méndez, Mariano Coleman Miller, M Morsink, Sharon Nättilä, Joonas Possenti, Andrea Prescod-Weinstein, Chanda Qu, JinLu Riggio, Alessandro Salmi, Tuomo Sanna, Andrea Santangelo, Andrea Schatz, Hendrik Schwenk, Achim Song, LiMing Šrámková, Eva Stappers, Benjamin Stiele, Holger Strohmayer, Tod Tews, Ingo Tolos, Laura Török, Gabriel Tsang, David Urbanec, Martin Vacchi, Andrea Xu, RenXin Xu, YuPeng Zane, Silvia Zhang, GuoBao Zhang, ShuangNan Zhang, WenDa Zheng, ShiJie Zhou, Xia |
author_sort | Watts, Anna L |
collection | CERN |
description | 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. |
id | oai-inspirehep.net-1703092 |
institution | Organización Europea para la Investigación Nuclear |
language | eng |
publishDate | 2019 |
record_format | invenio |
spelling | oai-inspirehep.net-17030922022-01-14T15:04:52Zdoi:10.1007/s11433-017-9188-4http://cds.cern.ch/record/2671647engWatts, Anna LYu, WenFeiPoutanen, JuriZhang, ShuBhattacharyya, SudipBogdanov, SlavkoJi, LongPatruno, AlessandroRiley, Thomas EBakala, PavelBaykal, AltanBernardini, FedericoBombaci, IgnazioBrown, EdwardCavecchi, YuriChakrabarty, DeeptoChenevez, JérômeDegenaar, NathalieSanto, MelaniaSalvo, TizianaDoroshenko, VictorFalanga, MaurizioFerdman, Robert DFeroci, MarcoGambino, Angelo FGe, MingYuGreif, Svenja KGuillot, SebastienGungor, CanHartmann, Dieter HHebeler, KaiHeger, AlexanderHoman, JeroenIaria, Rosarioin't Zand, JeanKargaltsev, OlegKurkela, AleksiLai, XiaoYuLi, AngLi, XiangDongLi, ZhaoShengLinares, ManuelLu, FangJunMahmoodifar, SiminMéndez, MarianoColeman Miller, MMorsink, SharonNättilä, JoonasPossenti, AndreaPrescod-Weinstein, ChandaQu, JinLuRiggio, AlessandroSalmi, TuomoSanna, AndreaSantangelo, AndreaSchatz, HendrikSchwenk, AchimSong, LiMingŠrámková, EvaStappers, BenjaminStiele, HolgerStrohmayer, TodTews, IngoTolos, LauraTörök, GabrielTsang, DavidUrbanec, MartinVacchi, AndreaXu, RenXinXu, YuPengZane, SilviaZhang, GuoBaoZhang, ShuangNanZhang, WenDaZheng, ShiJieZhou, XiaDense matter with eXTPAstrophysics and AstronomyIn 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.oai:inspirehep.net:17030922019 |
spellingShingle | Astrophysics and Astronomy Watts, Anna L Yu, WenFei 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 Santo, Melania Salvo, Tiziana Doroshenko, Victor Falanga, Maurizio Ferdman, Robert D Feroci, Marco Gambino, Angelo F Ge, MingYu Greif, Svenja K Guillot, Sebastien Gungor, Can Hartmann, Dieter H Hebeler, Kai Heger, Alexander Homan, Jeroen Iaria, Rosario in't Zand, Jean Kargaltsev, Oleg Kurkela, Aleksi Lai, XiaoYu Li, Ang Li, XiangDong Li, ZhaoSheng Linares, Manuel Lu, FangJun Mahmoodifar, Simin Méndez, Mariano Coleman Miller, M Morsink, Sharon Nättilä, Joonas Possenti, Andrea Prescod-Weinstein, Chanda Qu, JinLu Riggio, Alessandro Salmi, Tuomo Sanna, Andrea Santangelo, Andrea Schatz, Hendrik Schwenk, Achim Song, LiMing Šrámková, Eva Stappers, Benjamin Stiele, Holger Strohmayer, Tod Tews, Ingo Tolos, Laura Török, Gabriel Tsang, David Urbanec, Martin Vacchi, Andrea Xu, RenXin Xu, YuPeng Zane, Silvia Zhang, GuoBao Zhang, ShuangNan Zhang, WenDa Zheng, ShiJie Zhou, Xia Dense matter with eXTP |
title | Dense matter with eXTP |
title_full | Dense matter with eXTP |
title_fullStr | Dense matter with eXTP |
title_full_unstemmed | Dense matter with eXTP |
title_short | Dense matter with eXTP |
title_sort | dense matter with extp |
topic | Astrophysics and Astronomy |
url | https://dx.doi.org/10.1007/s11433-017-9188-4 http://cds.cern.ch/record/2671647 |
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