Zobrazeno 1 - 10
of 142
pro vyhledávání: '"Edward F. Brown"'
Autor:
C. J. Prokop, R. Lewis, Christoph Langer, F. Montes, S. Gupta, J. Pereira, K. Childers, F. Naqvi, B. P. Crider, Sean Liddick, Stephanie Lyons, W.-J. Ong, D. Richman, S. Ahn, J. Browne, Alexander Dombos, A. Spyrou, Edward F. Brown, Peter Möller, G. W. Hitt, Zach Meisel, K. Schmidt, Hendrik Schatz
Publikováno v:
Physical Review Letters. 125
The interpretation of observations of cooling neutron star crusts in quasipersistent x-ray transients is affected by predictions of the strength of neutrino cooling via crust Urca processes. The strength of crust Urca neutrino cooling depends sensiti
Autor:
Sanjay Reddy, Michael Scott Smith, Brian W. O'Shea, Falk Herwig, Remco Zegers, J. C. Blackmon, R. E. Rutledge, D. W. Bardayan, Madappa Prakash, Francis Timmes, Arthur E Champagne, Timothy C. Beers, Pawel Danielewicz, Boris Pritychenko, Gail C. McLaughlin, Filomena Nunes, Brian D. Fields, Dean M. Townsley, Anthony Mezzacappa, Almudena Arcones, Mounib El-Eid, Grigory Rogachev, Jutta Escher, Roland Diehl, Bronson Messer, Hendrik Schatz, B. Alex Brown, L. A. Bernstein, Michael Zingale, Christian Iliadis, William Raphael Hix, Andrew W. Steiner, Carl R. Brune, Aaron Couture, Tod E. Strohmayer, Michael Wiescher, Ernst Rehm, Carla Fröhlich, Edward F. Brown, Alessandro Chieffi, Bradley S. Meyer, W. G. Lynch, Ingrid H. Stairs
Publikováno v:
Progress in Particle and Nuclear Physics. 94:1-67
This white paper informs the nuclear astrophysics community and funding agencies about the scientific directions and priorities of the field and provides input from this community for the 2015 Nuclear Science Long Range Plan. It summarizes the outcom
Neutron stars cooling after sustained accretion outbursts provide unique information about the neutron star crust and underlying dense matter. Comparisons between astronomical observations of these cooling transients and model calculations of neutron
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::04241a45aea645d317803e410981920b
Autor:
Xiang-Dong Li, Jean in 't Zand, B. W. Stappers, Sudip Bhattacharyya, Slavko Bogdanov, Holger Stiele, Sharon M. Morsink, Tiziana Di Salvo, Zhaosheng Li, Robert D. Ferdman, Alessandro Riggio, Jin-Lu Qu, Wenfei Yu, Oleg Kargaltsev, R. Iaria, Xia Zhou, Joonas Nättilä, Gabriel Török, David Tsang, Aleksi Kurkela, Laura Tolos, Achim Schwenk, Ingo Tews, Ypeng Xu, Andrea Vacchi, Martin Urbanec, Andrea Santangelo, Xiao Yu Lai, Manuel Linares, Pavel Bakala, Altan Baykal, Anna L. Watts, Alexander Heger, Eva Šrámková, Andrea Sanna, Maurizio Falanga, Ang Li, M. Coleman Miller, Federico Bernardini, Edward F. Brown, Yuri Cavecchi, Jérôme Chenevez, Long Ji, Dieter H. Hartmann, Hendrik Schatz, Ignazio Bombaci, Shuang-Nan Zhang, Silvia Zane, Chanda Prescod-Weinstein, Victor Doroshenko, Kai Hebeler, Guobao Zhang, Tuomo Salmi, Fangjun Lu, Ming-Yu Ge, Melania Del Santo, Deepto Chakrabarty, Mariano Mendez, ShiJie Zheng, Wenda Zhang, S. K. Greif, Alessandro Patruno, Angelo Gambino, Nathalie Degenaar, Simin Mahmoodifar, Juri Poutanen, Marco Feroci, Thomas E. Riley, Shu Zhang, Andrea Possenti, Sebastien Guillot, Tod E. Strohmayer, Jeroen Homan, Can Güngör, Li-Ming Song, Renxin Xu
Publikováno v:
Recercat. Dipósit de la Recerca de Catalunya
instname
Science China-Physics, Mechanics & Astronomy
Science China: Physics, Mechanics and Astronomy, 62(2):29503. Science in China Press
UPCommons. Portal del coneixement obert de la UPC
Universitat Politècnica de Catalunya (UPC)
Science China Physics, Mechanics & Astronomy
Science china-Physics mechanics & astronomy, 62(2):029503. Science Press
arXiv
instname
Science China-Physics, Mechanics & Astronomy
Science China: Physics, Mechanics and Astronomy, 62(2):29503. Science in China Press
UPCommons. Portal del coneixement obert de la UPC
Universitat Politècnica de Catalunya (UPC)
Science China Physics, Mechanics & Astronomy
Science china-Physics mechanics & astronomy, 62(2):029503. Science Press
arXiv
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 laborat
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::fb45e6ab162de9f7132515101d200f0c
http://hdl.handle.net/20.500.12386/29101
http://hdl.handle.net/20.500.12386/29101
Autor:
Diego Altamirano, Edward F. Brown, Rudy Wijnands, A.C. Waterhouse, Nathalie Degenaar, Jon M. Miller, Manuel Linares
Publikováno v:
Monthly Notices of the Royal Astronomical Society, 456(4), 4001-4014. Oxford University Press
Aql X-1 is a prolific transient neutron star low-mass X-ray binary that exhibits an accretion outburst approximately once every year. Whether the thermal X-rays detected in intervening quiescent episodes are the result of cooling of the neutron star
Autor:
Andrew Cumming, Edward F. Brown, Zidu Lin, Bao-An Li, Alex Deibel, Charles Horowitz, Farrukh J. Fattoyev
Publikováno v:
NASA Astrophysics Data System
We present a new mechanism for deep crustal heating in accreting neutron stars. Charged pions ($\pi^+$) are produced in nuclear collisions on the neutron star surface during active accretion and upon decay they provide a flux of neutrinos into the ne
Autor:
Arash Bahramian, Edward F. Brown, Andrew Cumming, L. S. Ootes, Craig O. Heinke, Edward M. Cackett, M. J. P. Wijngaarden, Jeroen Homan, A. Rouco Escorial, Dany Page, Aastha S. Parikh, Rudy Wijnands, Nathalie Degenaar
Publikováno v:
Astronomy & Astrophysics, 624:A84. EDP Sciences
Monitoring the cooling of neutron-star crusts heated during accretion outbursts allows us to infer the physics of the dense matter present in the crust. We examine the crust cooling evolution of the low-mass X-ray binary MXB 1659-29 up to ~505 days a
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::13ee42052c0e5e442d0ab0312b105aa5
Autor:
Leandro Gasques, R. Lau, A. V. Afanasjev, Alex Deibel, Hendrik Schatz, P. Möller, S. S. Gupta, M. Beard, Michael Wiescher, William Raphael Hix, Andrew W. Steiner, Laurens Keek, Y. Xu, Edward F. Brown, Peter Shternin, G. W. Hitt
Publikováno v:
NASA Astrophysics Data System
X-ray observations of transiently accreting neutron stars during quiescence provide information about the structure of neutron star crusts and the properties of dense matter. Interpretation of the observational data requires an understanding of the n
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5429310f616710f51298e740e34828be
Autor:
Dany Page, Charles Horowitz, Edward F. Brown, Sanjay Reddy, Andrew Cumming, Farrukh J. Fattoyev
Publikováno v:
NASA Astrophysics Data System
We show that the neutron star in the transient system MXB~1659-29 has a core neutrino luminosity that substantially exceeds that of the modified Urca reactions (i.e., $n+n\to n+p+e^{-}+\bar{\nu}_{e}$ and inverse) and is consistent with the direct Urc
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f036e333741b1451cdb707e9686d9965
http://arxiv.org/abs/1801.00041
http://arxiv.org/abs/1801.00041
Autor:
Diego Altamirano, Gregory R. Sivakoff, Joel K. Fridriksson, Nathalie Degenaar, Jeroen Homan, Andrew Cumming, Edward F. Brown, Jon M. Miller, Craig O. Heinke, Edward M. Cackett, Arash Bahramian, David Pooley, Rudy Wijnands
Publikováno v:
Monthly Notices of the Royal Astronomical Society, 451(2), 2071-2081. Oxford University Press
When neutron stars reside in transient X-ray binaries, their crustal layers become heated during accretion outbursts and subsequently cool in quiescence. Observing and modeling this thermal response has yielded valuable insight into the physics of ne