WATTS, Anna L., WenFei YU, Juri POUTANEN, Shu ZHANG, Sudip BHATTACHARYYA, Slavko BOGDANOV, Long JI, Alessandro PATRUNO, Thomas E. RILEY, Pavel BAKALA (203 Česká republika, domácí), Altan BAYKAL, Federico BERNARDINI, Ignazio BOMBACI, Edward BROWN, Yuri CAVECCHI, Deepto CHAKRABARTY, Jérome CHENEVEZ, Nathalie DEGENAAR, Melania DEL SANTO, Tiziana DI SALVO, Victor DOROSHENKO, Maurizio FALANGA (756 Švýcarsko), Robert D. FERDMAN, Marco FEROCI, Angelo F. GAMBINO, MingYu GE, Svenja K. GREIF, Sebastien GUILLOT, Can GUNGOR, Dieter H. HARTMANN, Kai HEBELER, Alexander HEGER, Jeroen HOMAN, Rosario IARIA, Jean IN ’T ZAND, Oleg KARGALTSEV, Aleksi KURKELA, XiaoYu LAI, Ang LI, XiangDong LI, ZhaoSheng LI, Manuel LINARES, FangJun LU, Simin MAHMOODIFAR, Mariano MÉNDEZ, Coleman MILLER, Sharon MORSINK, Joonas NATTILA, Andrea POSSENTI, Chand PRESCOD-WEINSTEIN, JinLu QU, Alessandro RIGGIO, Tuomo SALMI, Andrea SANNA, Andrea SANTANGELO, Hendrik SCHATZ, Achim SCHWENK, LiMing SONG, Eva ŠRÁMKOVÁ (203 Česká republika, domácí), Benjamin STAPPERS, Holger STIELE, Tod STROHMAYER, Ingo TEWS, Laura TOLOS, Gabriel TÖRÖK (203 Česká republika, domácí), David TSANG, Martin URBANEC (203 Česká republika, domácí), Andrea VACCHI, RenXin XU, YuPeng XU, Silvia ZANE, GuoBao ZHANG, ShuangNan ZHANG, WenDa ZHANG, ShiJie ZHENG a Xia ZHOU
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.
WATTS, Anna L., WenFei YU, Juri POUTANEN, Shu ZHANG, Sudip BHATTACHARYYA, Slavko BOGDANOV, Long JI, Alessandro PATRUNO, Thomas E. RILEY, Pavel BAKALA, Altan BAYKAL, Federico BERNARDINI, Ignazio BOMBACI, Edward BROWN, Yuri CAVECCHI, Deepto CHAKRABARTY, Jérome CHENEVEZ, Nathalie DEGENAAR, Melania DEL SANTO, Tiziana DI SALVO, Victor DOROSHENKO, Maurizio FALANGA, Robert D. FERDMAN, Marco FEROCI, Angelo F. GAMBINO, MingYu GE, Svenja K. GREIF, Sebastien GUILLOT, Can GUNGOR, Dieter H. HARTMANN, Kai HEBELER, Alexander HEGER, Jeroen HOMAN, Rosario IARIA, Jean IN ’T ZAND, Oleg KARGALTSEV, Aleksi KURKELA, XiaoYu LAI, Ang LI, XiangDong LI, ZhaoSheng LI, Manuel LINARES, FangJun LU, Simin MAHMOODIFAR, Mariano MÉNDEZ, Coleman MILLER, Sharon MORSINK, Joonas NATTILA, Andrea POSSENTI, Chand PRESCOD-WEINSTEIN, JinLu QU, Alessandro RIGGIO, Tuomo SALMI, Andrea SANNA, Andrea SANTANGELO, Hendrik SCHATZ, Achim SCHWENK, LiMing SONG, Eva ŠRÁMKOVÁ, Benjamin STAPPERS, Holger STIELE, Tod STROHMAYER, Ingo TEWS, Laura TOLOS, Gabriel TÖRÖK, David TSANG, Martin URBANEC, Andrea VACCHI, RenXin XU, YuPeng XU, Silvia ZANE, GuoBao ZHANG, ShuangNan ZHANG, WenDa ZHANG, ShiJie ZHENG a Xia ZHOU. Dense matter with eXTP. Science China. Physics, Mechanics & Astronomy. 2019, roč. 62, č. 2, s. "029503-1"-"029503-17", 17 s. ISSN 1674-7348. Dostupné z: https://dx.doi.org/10.1007/s11433-017-9188-4.
@article{37861, author = {Watts, Anna L. and Yu, WenFei and Poutanen, Juri and Zhang, Shu and Bhattacharyya, Sudip and Bogdanov, Slavko and Ji, Long and Patruno, Alessandro and Riley, Thomas E. and Bakala, Pavel and Baykal, Altan and Bernardini, Federico and Bombaci, Ignazio and Brown, Edward and Cavecchi, Yuri and Chakrabarty, Deepto and Chenevez, Jérome and Degenaar, Nathalie and Del Santo, Melania and Di Salvo, Tiziana and Doroshenko, Victor and Falanga, Maurizio and Ferdman, Robert D. and Feroci, Marco and Gambino, Angelo F. and Ge, MingYu and Greif, Svenja K. and Guillot, Sebastien and Gungor, Can and Hartmann, Dieter H. and Hebeler, Kai and Heger, Alexander and Homan, Jeroen and Iaria, Rosario and in ’t Zand, Jean and Kargaltsev, Oleg and Kurkela, Aleksi and Lai, XiaoYu and Li, Ang and Li, XiangDong and Li, ZhaoSheng and Linares, Manuel and Lu, FangJun and Mahmoodifar, Simin and Méndez, Mariano and Miller, Coleman and Morsink, Sharon and Nattila, Joonas and Possenti, Andrea and PrescodandWeinstein, Chand and Qu, JinLu and Riggio, Alessandro and Salmi, Tuomo and Sanna, Andrea and Santangelo, Andrea and Schatz, Hendrik and Schwenk, Achim and Song, LiMing and Šrámková, Eva and Stappers, Benjamin and Stiele, Holger and Strohmayer, Tod and Tews, Ingo and Tolos, Laura and Török, Gabriel and Tsang, David and Urbanec, Martin and Vacchi, Andrea and Xu, RenXin and Xu, YuPeng and Zane, Silvia and Zhang, GuoBao and Zhang, ShuangNan and Zhang, WenDa and Zheng, ShiJie and Zhou, Xia}, article_number = {2}, doi = {http://dx.doi.org/10.1007/s11433-017-9188-4}, keywords = {Enhanced X-ray Timing and Polarimetry (eXTP) mission; dense matter; neutron stars; equation of state; accretion flows}, language = {eng}, issn = {1674-7348}, journal = {Science China. Physics, Mechanics & Astronomy}, title = {Dense matter with eXTP}, url = {https://link.springer.com/article/10.1007%2Fs11433-017-9188-4}, volume = {62}, year = {2019} }
TY - JOUR ID - 37861 AU - 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, Jérome - Degenaar, Nathalie - Del Santo, Melania - Di 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 - Miller, Coleman - Morsink, Sharon - Nattila, Joonas - Possenti, Andrea - Prescod-Weinstein, Chand - 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 PY - 2019 TI - Dense matter with eXTP JF - Science China. Physics, Mechanics & Astronomy VL - 62 IS - 2 SP - "029503-1"-"029503-17" EP - "029503-1"-"029503-17" SN - 16747348 KW - Enhanced X-ray Timing and Polarimetry (eXTP) mission KW - dense matter KW - neutron stars KW - equation of state KW - accretion flows UR - https://link.springer.com/article/10.1007%2Fs11433-017-9188-4 L2 - https://link.springer.com/article/10.1007%2Fs11433-017-9188-4 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. ER -
WATTS, Anna L., WenFei YU, Juri POUTANEN, Shu ZHANG, Sudip BHATTACHARYYA, Slavko BOGDANOV, Long JI, Alessandro PATRUNO, Thomas E. RILEY, Pavel BAKALA, Altan BAYKAL, Federico BERNARDINI, Ignazio BOMBACI, Edward BROWN, Yuri CAVECCHI, Deepto CHAKRABARTY, Jérome CHENEVEZ, Nathalie DEGENAAR, Melania DEL SANTO, Tiziana DI SALVO, Victor DOROSHENKO, Maurizio FALANGA, Robert D. FERDMAN, Marco FEROCI, Angelo F. GAMBINO, MingYu GE, Svenja K. GREIF, Sebastien GUILLOT, Can GUNGOR, Dieter H. HARTMANN, Kai HEBELER, Alexander HEGER, Jeroen HOMAN, Rosario IARIA, Jean IN ’T ZAND, Oleg KARGALTSEV, Aleksi KURKELA, XiaoYu LAI, Ang LI, XiangDong LI, ZhaoSheng LI, Manuel LINARES, FangJun LU, Simin MAHMOODIFAR, Mariano MÉNDEZ, Coleman MILLER, Sharon MORSINK, Joonas NATTILA, Andrea POSSENTI, Chand PRESCOD-WEINSTEIN, JinLu QU, Alessandro RIGGIO, Tuomo SALMI, Andrea SANNA, Andrea SANTANGELO, Hendrik SCHATZ, Achim SCHWENK, LiMing SONG, Eva ŠRÁMKOVÁ, Benjamin STAPPERS, Holger STIELE, Tod STROHMAYER, Ingo TEWS, Laura TOLOS, Gabriel TÖRÖK, David TSANG, Martin URBANEC, Andrea VACCHI, RenXin XU, YuPeng XU, Silvia ZANE, GuoBao ZHANG, ShuangNan ZHANG, WenDa ZHANG, ShiJie ZHENG a Xia ZHOU. Dense matter with eXTP. \textit{Science China. Physics, Mechanics \&{} Astronomy}. 2019, roč.~62, č.~2, s.~''029503-1''-''029503-17'', 17 s. ISSN~1674-7348. Dostupné z: https://dx.doi.org/10.1007/s11433-017-9188-4.