Zobrazeno 1 - 10
of 1 906
pro vyhledávání: '"BROWN, EDWARD"'
Autor:
Cullen, Luke, Smith, Andy W, Galib, Asadullah H, Varshney, Debvrat, Brown, Edward J E, Chi, Peter J, Chu, Xiangning, Svoboda, Filip
Local ionospheric density anomalies have been reported in the days prior to major earthquakes. This global study statistically investigates whether consistent ionospheric anomalies occur in the 24 hours prior to earthquakes across different regions,
Externí odkaz:
http://arxiv.org/abs/2401.01773
Autor:
Benson, Bernard, Brown, Edward, Bonasera, Stefano, Acciarini, Giacomo, Pérez-Hernández, Jorge A., Sutton, Eric, Jah, Moriba K., Bridges, Christopher, Jin, Meng, Baydin, Atılım Güneş
Solar radio flux along with geomagnetic indices are important indicators of solar activity and its effects. Extreme solar events such as flares and geomagnetic storms can negatively affect the space environment including satellites in low-Earth orbit
Externí odkaz:
http://arxiv.org/abs/2112.09051
Autor:
Abeysekera, Kush, Marjot, Tom, Brennan, Paul, Mahgoub, Sara, Cacciottolo, Tessa, Hydes, Theresa, Hardy, Tim, McGinty, Gio, Tavabie, Oliver, Cathcart, Jennifer, Premathilaka, Chirantha, Mukhopadhya, Ashis, Bhat, Arshiya, Begum, Shahnaz, Abushaban, Bashar, Bhuva, Meha, Sinclair, Sophie, Leith, Damien, McCulloch, Cullen, Leithead, Joanna, Fox, Richard, Shah, Muhammad Haris, Campbell, Eugene, Brown, Edward, Mansour, Dina, Shah, Fatma, Allison, Michael, Chan, Jonathan, Roberts, Victoria, Appanna, Gautham, Mandour, Mandour Omer, Slee, Georgina, Wong, Vicki, Kotha, Sreelakshmi, Pekarska, Katrina, Parker, Richard, Sieberhagen, Cyril, Ngan, Thomas, Asilmaz, Esra, Miller, Hamish, Cobbold, Jeremy, Crocombe, Dom, Tsochatzis, Manolis, Tanwar, Sudeep, Dias, Aruna, Singh, Gurmit, Agrawal, Swastik, Chhabra, Puneet, Gurung, Amrita, Veettil, Rajesh, Abeles, Robin Daniel, Chatterjee, Devnandan, Carbonell, Michael, Mohamed, Zameer, El-Sayed, Ahmed, Johnson, Amy, Barclay, Stephen, Kelly, Katherine, Munonye, Joshua, Coates, Dominic, Bamidele, Opeyemi, Johnston, Thomas, Samuel, David, Ball, Belinda, Arscott-Samuel, Rebecca, Hams, Pamela, Armstrong, Matthew, Elkhol, Ayman, Shailesh, Karanth, Bains, Vikram, Manousou, Pinelopi, Gupta, Tarun, Than, Sophia, Unitt, Esther, Gordon, Victoria, Wakefield, Alice, Gilchrist, Sian, Cozma, Ioana, Saeed, Sohaib, Umrani, Salman, Olsen, Kathryn, Li, Wenhao, Sheridan, David, McPherson, Stuart, Alazawi, William
Publikováno v:
In JHEP Reports December 2023 5(12)
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:
http://arxiv.org/abs/1906.01535
Autor:
Zand, Jean J. M. in 't, Bozzo, Enrico, Qu, Jinlu, Li, Xiang-Dong, Amati, Lorenzo, Chen, Yang, Donnarumma, Immacolata, Doroshenko, Victor, Drake, Stephen A., Hernanz, Margarita, Jenke, Peter A., Maccarone, Thomas J., Mahmoodifar, Simin, de Martino, Domitilla, De Rosa, Alessandra, Rossi, Elena M., Rowlinson, Antonia, Sala, Gloria, Stratta, Giulia, Tauris, Thomas M., Wilms, Joern, Wu, Xuefeng, Zhou, Ping, Agudo, Iván, Altamirano, Diego, Atteia, Jean-Luc, Andersson, Nils A., Baglio, M. Cristina, Ballantyne, David R., Baykal, Altan, Behar, Ehud, Belloni, Tomaso, Bhattacharyya, Sudip, Bianchi, Stefano, Bilous, Anna, Blay, Pere, Braga, João, Brandt, Søren, Brown, Edward F., Bucciantini, Niccolò, Burderi, Luciano, Cackett, Edward M., Campana, Riccardo, Campana, Sergio, Casella, Piergiorgio, Cavecchi, Yuri, Chambers, Frank, Chen, Liang, Chen, Yu-Peng, Chenevez, Jérôme, Chernyakova, Maria, Chichuan, Jin, Ciolfi, Riccardo, Costantini, Elisa, Cumming, Andrew, D'Aı, Antonino, Dai, Zi-Gao, D'Ammando, Filippo, De Pasquale, Massimiliano, Degenaar, Nathalie, Del Santo, Melania, D'Elia, Valerio, Di Salvo, Tiziana, Doyle, Gerry, Falanga, Maurizio, Fan, Xilong, Ferdman, Robert D., Feroci, Marco, Fraschetti, Federico, Galloway, Duncan K., Gambino, Angelo F., Gandhi, Poshak, Ge, Mingyu, Gendre, Bruce, Gill, Ramandeep, Götz, Diego, Gouiffès, Christian, Grandi, Paola, Granot, Jonathan, Güdel, Manuel, Heger, Alexander, Heinke, Craig O., Homan, Jeroen, Iaria, Rosario, Iwasawa, Kazushi, Izzo, Luca, Ji, Long, Jonker, Peter G., José, Jordi, Kaastra, Jelle S., Kalemci, Emrah, Kargaltsev, Oleg, Kawai, Nobuyuki, Keek, Laurens, Komossa, Stefanie, Kreykenbohm, Ingo, Kuiper, Lucien, Kunneriath, Devaky, Li, Gang, Liang, En-Wei, Linares, Manuel, Longo, Francesco, Lu, Fangjun, Lutovinov, Alexander A., Malyshev, Denys, Malzac, Julien, Manousakis, Antonios, McHardy, Ian, Mehdipour, Missagh, Men, Yunpeng, Méndez, Mariano, Mignani, Roberto P., Mikusincova, Romana, Miller, M. Coleman, Miniutti, Giovanni, Motch, Christian, Nättilä, Joonas, Nardini, Emanuele, Neubert, Torsten, O'Brien, Paul T., Orlandini, Mauro, Osborne, Julian P., Pacciani, Luigi, Paltani, Stéphane, Paolillo, Maurizio, Papadakis, Iossif E., Paul, Biswajit, Pellizzoni, Alberto, Peretz, Uria, Torres, Miguel A. Pérez, Perinati, Emanuele, Prescod-Weinstein, Chanda, Reig, Pablo, Riggio, Alessandro, Rodriguez, Jerome, Rodrıguez-Gil, Pablo, Romano, Patrizia, Różańska, Agata, Sakamoto, Takanori, Salmi, Tuomo, Salvaterra, Ruben, Sanna, Andrea, Santangelo, Andrea, Savolainen, Tuomas, Schanne, Stéphane, Schatz, Hendrik, Shao, Lijing, Shearer, Andy, Shore, Steven N., Stappers, Ben W., Strohmayer, Tod E., Suleimanov, Valery F., Svoboda, Jirı, Thielemann, F. -K., Tombesi, Francesco, Torres, Diego F., Torresi, Eleonora, Turriziani, Sara, Vacchi, Andrea, Vercellone, Stefano, Vink, Jacco, Wang, Jian-Min, Wang, Junfeng, Watts, Anna L., Weng, Shanshan, Weinberg, Nevin N., Wheatley, Peter J., Wijnands, Rudy, Woods, Tyrone E., Woosley, Stan E., Xiong, Shaolin, Xu, Yupeng, Yan, Zhen, Younes, George, Yu, Wenfei, Yuan, Feng, Zampieri, Luca, Zane, Silvia, Zdziarski, Andrzej A., Zhang, Shuang-Nan, Zhang, Shu, Zhang, Shuo, Zhang, Xiao, Zingale, Michael
In this White Paper we present the potential of the enhanced X-ray Timing and Polarimetry (eXTP) mission for studies related to Observatory Science targets. These include flaring stars, supernova remnants, accreting white dwarfs, low and high mass X-
Externí odkaz:
http://arxiv.org/abs/1812.04023
Autor:
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, 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, Zand, Jean in 't, Kargaltsev, Oleg, Kurkela, Aleksi, Lai, Xiaoyu, Li, Ang, Li, XiangDong, Li, Zhaosheng, Linares, Manuel, Lu, FangJun, Mahmoodifar, Simin, Méndez, Mariano, Miller, M. Coleman, 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, Ypeng, Zane, Silvia, Zhang, Guobao, Zhang, ShuangNan, Zhang, Wenda, Zheng, ShiJie, Zhou, Xia
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:
http://arxiv.org/abs/1812.04021
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Autor:
Brown, Edward F., Cumming, Andrew, Fattoyev, Farrukh J., Horowitz, C. J., Page, Dany, Reddy, Sanjay
Publikováno v:
Phys. Rev. Lett. 120, 182701 (2018)
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:
http://arxiv.org/abs/1801.00041
Autor:
Horbal, Steven R., Brown, Edward, Derstine, Brian A., Zhang, Peng, Bidulescu, Aurelian, Sullivan, June A., Ross, Brian E., Su, Grace L., Holcombe, Sven A., Wang, Stewart C.
Publikováno v:
In Clinical Imaging March 2022 83:51-55
Autor:
Fattoyev, F. J., Brown, Edward F., Cumming, Andrew, Deibel, Alex, Horowitz, C. J., Li, Bao-An, Lin, Zidu
Publikováno v:
Phys. Rev. C 98, 025801 (2018)
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
Externí odkaz:
http://arxiv.org/abs/1710.10367