Physics and astrophysics of strong magnetic field systems with eXTP

Andrea Santangelo; Silvia Zane; Hua Feng; Ren Xin Xu; Victor Doroshenko; Enrico Bozzo; Ilaria Caiazzo; Francesco Coti Zelati; Paolo Esposito; Denis González-Caniulef; Jeremy Heyl; Daniela Huppenkothen; Gianluca Israel; Zhao Sheng Li; Lin Lin; Roberto Mignani; Nanda Rea; Mauro Orlandini; Roberto Taverna; Hao Tong; Roberto Turolla; Cristina Baglio; Federico Bernardini; Niccolo’ Bucciantini; Marco Feroci; Felix Fürst; Ersin Göğüş; Can Güngör; Long Ji; Fang Jun Lu; Antonios Manousakis; Sandro Mereghetti; Romana Mikusincova; Biswajit Paul; Chanda Prescod-Weinstein; George Younes; Andrea Tiengo; Yu Peng Xu; Anna Watts; Shu Zhang; Shuang Nan Zhan

doi:10.1007/s11433-018-9234-3

Physics and astrophysics of strong magnetic field systems with eXTP

Andrea Santangelo, Silvia Zane, Hua Feng, Ren Xin Xu, Victor Doroshenko, Enrico Bozzo, Ilaria Caiazzo, Francesco Coti Zelati, Paolo Esposito, Denis González-Caniulef, Jeremy Heyl, Daniela Huppenkothen, Gianluca Israel, Zhao Sheng Li, Lin Lin, Roberto Mignani, Nanda Rea, Mauro Orlandini, Roberto Taverna, Hao TongRoberto Turolla, Cristina Baglio, Federico Bernardini, Niccolo’ Bucciantini, Marco Feroci, Felix Fürst, Ersin Göğüş, Can Güngör, Long Ji, Fang Jun Lu, Antonios Manousakis, Sandro Mereghetti, Romana Mikusincova, Biswajit Paul, Chanda Prescod-Weinstein, George Younes, Andrea Tiengo, Yu Peng Xu, Anna Watts, Shu Zhang, Shuang Nan Zhan

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

Abstract

In this paper we present the science potential of the enhanced X-ray Timing and Polarimetry (eXTP) mission for studies of strongly magnetized objects. We will focus on the physics and astrophysics of strongly magnetized objects, namely magnetars, accreting X-ray pulsars, and rotation powered pulsars. We also discuss the science potential of eXTP for QED studies. Developed 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 (US)
Article number	29505
Journal	Science China: Physics, Mechanics and Astronomy
Volume	62
Issue number	2
DOIs	https://doi.org/10.1007/s11433-018-9234-3
State	Published - Feb 1 2019

Keywords

QED
accreting pulsars
eXTP
magnetars
neutron stars

ASJC Scopus subject areas

Physics and Astronomy(all)

Access to Document

10.1007/s11433-018-9234-3

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Santangelo, A., Zane, S., Feng, H., Xu, R. X., Doroshenko, V., Bozzo, E., Caiazzo, I., Zelati, F. C., Esposito, P., González-Caniulef, D., Heyl, J., Huppenkothen, D., Israel, G., Li, Z. S., Lin, L., Mignani, R., Rea, N., Orlandini, M., Taverna, R., ... Zhan, S. N. (2019). Physics and astrophysics of strong magnetic field systems with eXTP. Science China: Physics, Mechanics and Astronomy, 62(2), [29505]. https://doi.org/10.1007/s11433-018-9234-3

Physics and astrophysics of strong magnetic field systems with eXTP. / Santangelo, Andrea; Zane, Silvia; Feng, Hua; Xu, Ren Xin; Doroshenko, Victor; Bozzo, Enrico; Caiazzo, Ilaria; Zelati, Francesco Coti; Esposito, Paolo; González-Caniulef, Denis; Heyl, Jeremy; Huppenkothen, Daniela; Israel, Gianluca; Li, Zhao Sheng; Lin, Lin; Mignani, Roberto; Rea, Nanda; Orlandini, Mauro; Taverna, Roberto; Tong, Hao; Turolla, Roberto; Baglio, Cristina; Bernardini, Federico; Bucciantini, Niccolo’; Feroci, Marco; Fürst, Felix; Göğüş, Ersin; Güngör, Can; Ji, Long; Lu, Fang Jun; Manousakis, Antonios; Mereghetti, Sandro; Mikusincova, Romana; Paul, Biswajit; Prescod-Weinstein, Chanda; Younes, George; Tiengo, Andrea; Xu, Yu Peng; Watts, Anna; Zhang, Shu; Zhan, Shuang Nan.

In: Science China: Physics, Mechanics and Astronomy, Vol. 62, No. 2, 29505, 01.02.2019.

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

Santangelo, A, Zane, S, Feng, H, Xu, RX, Doroshenko, V, Bozzo, E, Caiazzo, I, Zelati, FC, Esposito, P, González-Caniulef, D, Heyl, J, Huppenkothen, D, Israel, G, Li, ZS, Lin, L, Mignani, R, Rea, N, Orlandini, M, Taverna, R, Tong, H, Turolla, R, Baglio, C, Bernardini, F, Bucciantini, N, Feroci, M, Fürst, F, Göğüş, E, Güngör, C, Ji, L, Lu, FJ, Manousakis, A, Mereghetti, S, Mikusincova, R, Paul, B, Prescod-Weinstein, C, Younes, G, Tiengo, A, Xu, YP, Watts, A, Zhang, S & Zhan, SN 2019, 'Physics and astrophysics of strong magnetic field systems with eXTP', Science China: Physics, Mechanics and Astronomy, vol. 62, no. 2, 29505. https://doi.org/10.1007/s11433-018-9234-3

Santangelo, Andrea ; Zane, Silvia ; Feng, Hua ; Xu, Ren Xin ; Doroshenko, Victor ; Bozzo, Enrico ; Caiazzo, Ilaria ; Zelati, Francesco Coti ; Esposito, Paolo ; González-Caniulef, Denis ; Heyl, Jeremy ; Huppenkothen, Daniela ; Israel, Gianluca ; Li, Zhao Sheng ; Lin, Lin ; Mignani, Roberto ; Rea, Nanda ; Orlandini, Mauro ; Taverna, Roberto ; Tong, Hao ; Turolla, Roberto ; Baglio, Cristina ; Bernardini, Federico ; Bucciantini, Niccolo’ ; Feroci, Marco ; Fürst, Felix ; Göğüş, Ersin ; Güngör, Can ; Ji, Long ; Lu, Fang Jun ; Manousakis, Antonios ; Mereghetti, Sandro ; Mikusincova, Romana ; Paul, Biswajit ; Prescod-Weinstein, Chanda ; Younes, George ; Tiengo, Andrea ; Xu, Yu Peng ; Watts, Anna ; Zhang, Shu ; Zhan, Shuang Nan. / Physics and astrophysics of strong magnetic field systems with eXTP. In: Science China: Physics, Mechanics and Astronomy. 2019 ; Vol. 62, No. 2.

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abstract = "In this paper we present the science potential of the enhanced X-ray Timing and Polarimetry (eXTP) mission for studies of strongly magnetized objects. We will focus on the physics and astrophysics of strongly magnetized objects, namely magnetars, accreting X-ray pulsars, and rotation powered pulsars. We also discuss the science potential of eXTP for QED studies. Developed 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 = "QED, accreting pulsars, eXTP, magnetars, neutron stars",

author = "Andrea Santangelo and Silvia Zane and Hua Feng and Xu, {Ren Xin} and Victor Doroshenko and Enrico Bozzo and Ilaria Caiazzo and Zelati, {Francesco Coti} and Paolo Esposito and Denis Gonz{\'a}lez-Caniulef and Jeremy Heyl and Daniela Huppenkothen and Gianluca Israel and Li, {Zhao Sheng} and Lin Lin and Roberto Mignani and Nanda Rea and Mauro Orlandini and Roberto Taverna and Hao Tong and Roberto Turolla and Cristina Baglio and Federico Bernardini and Niccolo{\textquoteright} Bucciantini and Marco Feroci and Felix F{\"u}rst and Ersin G{\"o}ğ{\"u}{\c s} and Can G{\"u}ng{\"o}r and Long Ji and Lu, {Fang Jun} and Antonios Manousakis and Sandro Mereghetti and Romana Mikusincova and Biswajit Paul and Chanda Prescod-Weinstein and George Younes and Andrea Tiengo and Xu, {Yu Peng} and Anna Watts and Shu Zhang and Zhan, {Shuang Nan}",

note = "Funding Information: 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). This work was supported by the Bundesministerium fuer Wirtschaft und Technologie through the Deutsches Zentrum fuer Luft-und Raumfahrte.V. (DLR) (Grant No. FKZ 50 OO 1701). Financial contribution from the agreement between the Italian Space Agency and the Istituto Nazionale di Astrofisica ASI-INAF n.2017-14-H.O is acknowledged. Publisher Copyright: {\textcopyright} 2018, Science China Press and Springer-Verlag GmbH Germany, part of Springer Nature.",

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doi = "10.1007/s11433-018-9234-3",

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AU - Santangelo, Andrea

AU - Zane, Silvia

AU - Feng, Hua

AU - Xu, Ren Xin

AU - Doroshenko, Victor

AU - Bozzo, Enrico

AU - Caiazzo, Ilaria

AU - Zelati, Francesco Coti

AU - Esposito, Paolo

AU - González-Caniulef, Denis

AU - Heyl, Jeremy

AU - Huppenkothen, Daniela

AU - Israel, Gianluca

AU - Li, Zhao Sheng

AU - Lin, Lin

AU - Mignani, Roberto

AU - Rea, Nanda

AU - Orlandini, Mauro

AU - Taverna, Roberto

AU - Tong, Hao

AU - Turolla, Roberto

AU - Baglio, Cristina

AU - Bernardini, Federico

AU - Bucciantini, Niccolo’

AU - Feroci, Marco

AU - Fürst, Felix

AU - Göğüş, Ersin

AU - Güngör, Can

AU - Ji, Long

AU - Lu, Fang Jun

AU - Manousakis, Antonios

AU - Mereghetti, Sandro

AU - Mikusincova, Romana

AU - Paul, Biswajit

AU - Prescod-Weinstein, Chanda

AU - Younes, George

AU - Tiengo, Andrea

AU - Xu, Yu Peng

AU - Watts, Anna

AU - Zhang, Shu

AU - Zhan, Shuang Nan

N1 - Funding Information: 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). This work was supported by the Bundesministerium fuer Wirtschaft und Technologie through the Deutsches Zentrum fuer Luft-und Raumfahrte.V. (DLR) (Grant No. FKZ 50 OO 1701). Financial contribution from the agreement between the Italian Space Agency and the Istituto Nazionale di Astrofisica ASI-INAF n.2017-14-H.O is acknowledged. Publisher Copyright: © 2018, Science China Press and Springer-Verlag GmbH Germany, part of Springer Nature.

PY - 2019/2/1

Y1 - 2019/2/1

N2 - In this paper we present the science potential of the enhanced X-ray Timing and Polarimetry (eXTP) mission for studies of strongly magnetized objects. We will focus on the physics and astrophysics of strongly magnetized objects, namely magnetars, accreting X-ray pulsars, and rotation powered pulsars. We also discuss the science potential of eXTP for QED studies. Developed 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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KW - accreting pulsars

KW - eXTP

KW - magnetars

KW - neutron stars

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DO - 10.1007/s11433-018-9234-3

M3 - Review article

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VL - 62

JO - Science in China, Series G: Physics Astronomy

JF - Science in China, Series G: Physics Astronomy

SN - 1674-7348

IS - 2

M1 - 29505

ER -

Physics and astrophysics of strong magnetic field systems with eXTP

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Keywords

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