Zobrazeno 1 - 10
of 445
pro vyhledávání: '"Fryer, Chris L."'
Publikováno v:
A&A 686, L8 (2024)
The $\gamma$-process in core-collapse supernovae (CCSNe) can produce a number of neutron-deficient stable isotopes heavier than iron (p-nuclei). However, current model predictions do to not fully reproduce the solar abundances. We investigate the imp
Externí odkaz:
http://arxiv.org/abs/2405.07783
Autor:
Peng, Yinglei, Ristić, Marko, Kedia, Atul, O'Shaughnessy, Richard, Fontes, Christopher J., Fryer, Chris L., Korobkin, Oleg, Mumpower, Matthew R., Villar, V. Ashley, Wollaeger, Ryan T.
Publikováno v:
Phys. Rev. Res. 6, 033078 (2024)
Kilonovae are the electromagnetic transients created by the radioactive decay of freshly synthesized elements in the environment surrounding a neutron star merger. To study the fundamental physics in these complex environments, kilonova modeling requ
Externí odkaz:
http://arxiv.org/abs/2402.05871
Autor:
Wollaeger, Ryan T., Fryer, Chris L., Chiodi, Robert, Brady, Peter T., Korobkin, Oleg, Harnish, Cale, Fontes, Christopher J., Haack, Jeffrey R., Chapurin, Oleksandr, Koshkarov, Oleksandr, Delzanno, Gian Luca, Livescu, Daniel
The interaction of $\beta$-particles with the weakly ionized plasma background is an important mechanism for powering the kilonova transient signal from neutron star mergers. For this purpose, we present an implementation of the approximate fast-part
Externí odkaz:
http://arxiv.org/abs/2401.11069
Autor:
Fryer, Chris L., Hungerford, Aimee L., Wollaeger, Ryan T., Miller, Jonah M., De, Soumi, Fontes, Christopher J., Korobkin, Oleg, Kedia, Atul, Ristic, Marko, O'Shaugnessy, Richard
The electromagnetic emission from the non-relativistic ejecta launched in neutron star mergers (either dynamically or through a disk wind) has the potential to probe both the total mass and composition of this ejecta. These observations are crucial i
Externí odkaz:
http://arxiv.org/abs/2311.05005
Autor:
Reynolds, Stephen, An, Hongjun, Abdelmaguid, Moaz, Alford, Jason, Fryer, Chris L., Mori, Kaya, Nynka, Melania, Park, Jaegeun, Terada, Yukikatsu, Woo, Jooyun, Bamba, Aya, Bangale, Priyadarshini, Diesing, Rebecca, Eagle, Jordan, Gabici, Stefano, Gelfand, Joseph, Grefenstette, Brian, Garcia, Javier, Kim, Chanho, Kumar, Sajan, Mac Intyre, Brydyn, Madsen, Kristin, Manconi, Silvia, Motogami, Yugo, Ohsumi, Hayato, Olmi, Barbara, Sato, Toshiki, Shang, Ruo-Yu, Stern, Daniel, Tsuji, Naomi, Younes, George, Zoglauer, Andreas
HEX-P is a probe-class mission concept that will combine high spatial resolution X-ray imaging ($<10"$ full width at half maximum) and broad spectral coverage (0.2--80 keV) with an effective area far superior to current facilities (including XMM-Newt
Externí odkaz:
http://arxiv.org/abs/2311.04952
Autor:
Mori, Kaya, Reynolds, Stephen, An, Hongjun, Bamba, Aya, Krivonos, Roman, Tsuji, Naomi, Abdelmaguid, Moaz, Alford, Jason, Bangale, Priyadarshini, Celli, Silvia, Diesing, Rebecca, Eagle, Jordan, Fryer, Chris L., Gabici, Stefano, Gelfand, Joseph, Grefenstette, Brian, Garcia, Javier, Kim, Chanho, Kumar, Sajan, Kuznetsova, Ekaterina, Mac Intyre, Brydyn, Madsen, Kristin, Manconi, Silvia, Motogami, Yugo, Ohsumi, Hayato, Olmi, Barbara, Park, Jaegeun, Ponti, Gabriele, Sato, Toshiki, Shang, Ruo-Yu, Stern, Daniel, Terada, Yukikatsu, Woo, Jooyun, Younes, George, Zoglauer, Andreas
HEX-P is a probe-class mission concept that will combine high spatial resolution X-ray imaging (<10" FWHM) and broad spectral coverage (0.2-80 keV) with an effective area far superior to current facilities (including XMM-Newton and NuSTAR) to enable
Externí odkaz:
http://arxiv.org/abs/2311.04851
Autor:
LISA Consortium Waveform Working Group, Afshordi, Niayesh, Akçay, Sarp, Seoane, Pau Amaro, Antonelli, Andrea, Aurrekoetxea, Josu C., Barack, Leor, Barausse, Enrico, Benkel, Robert, Bernard, Laura, Bernuzzi, Sebastiano, Berti, Emanuele, Bonetti, Matteo, Bonga, Béatrice, Bozzola, Gabriele, Brito, Richard, Buonanno, Alessandra, Cárdenas-Avendaño, Alejandro, Casals, Marc, Chernoff, David F., Chua, Alvin J. K., Clough, Katy, Colleoni, Marta, Dhesi, Mekhi, Druart, Adrien, Durkan, Leanne, Faye, Guillaume, Ferguson, Deborah, Field, Scott E., Gabella, William E., García-Bellido, Juan, Gracia-Linares, Miguel, Gerosa, Davide, Green, Stephen R., Haney, Maria, Hannam, Mark, Heffernan, Anna, Hinderer, Tanja, Helfer, Thomas, Hughes, Scott A., Husa, Sascha, Isoyama, Soichiro, Katz, Michael L., Kavanagh, Chris, Khanna, Gaurav, Kidder, Larry E., Korol, Valeriya, Küchler, Lorenzo, Laguna, Pablo, Larrouturou, François, Tiec, Alexandre Le, Leather, Benjamin, Lim, Eugene A., Lim, Hyun, Littenberg, Tyson B., Long, Oliver, Lousto, Carlos O., Lovelace, Geoffrey, Lukes-Gerakopoulos, Georgios, Lynch, Philip, Macedo, Rodrigo P., Markakis, Charalampos, Maggio, Elisa, Mandel, Ilya, Maselli, Andrea, Mathews, Josh, Mourier, Pierre, Neilsen, David, Nagar, Alessandro, Nichols, David A., Novák, Jan, Okounkova, Maria, O'Shaughnessy, Richard, Oshita, Naritaka, O'Toole, Conor, Pan, Zhen, Pani, Paolo, Pappas, George, Paschalidis, Vasileios, Pfeiffer, Harald P., Pompili, Lorenzo, Pound, Adam, Pratten, Geraint, Rüter, Hannes R., Ruiz, Milton, Sam, Zeyd, Sberna, Laura, Shapiro, Stuart L., Shoemaker, Deirdre M., Sopuerta, Carlos F., Spiers, Andrew, Sundar, Hari, Tamanini, Nicola, Thompson, Jonathan E., Toubiana, Alexandre, Tsokaros, Antonios, Upton, Samuel D., van de Meent, Maarten, Vernieri, Daniele, Wachter, Jeremy M., Warburton, Niels, Wardell, Barry, Witek, Helvi, Witzany, Vojtěch, Yang, Huan, Zilhão, Miguel, Albertini, Angelica, Arun, K. G., Bezares, Miguel, Bonilla, Alexander, Chapman-Bird, Christian, Cownden, Bradley, Cunningham, Kevin, Devitt, Chris, Dolan, Sam, Duque, Francisco, Dyson, Conor, Fryer, Chris L., Gair, Jonathan R., Giacomazzo, Bruno, Gupta, Priti, Han, Wen-Biao, Haas, Roland, Hirschmann, Eric W., Huerta, E. A., Jetzer, Philippe, Kelly, Bernard, Khalil, Mohammed, Lewis, Jack, Lloyd-Ronning, Nicole, Marsat, Sylvain, Nardini, Germano, Neef, Jakob, Ottewill, Adrian, Pantelidou, Christiana, Piovano, Gabriel Andres, Redondo-Yuste, Jaime, Sagunski, Laura, Stein, Leo C., Skoupý, Viktor, Sperhake, Ulrich, Speri, Lorenzo, Spieksma, Thomas F. M., Stevens, Chris, Trestini, David, Vañó-Viñuales, Alex
LISA, the Laser Interferometer Space Antenna, will usher in a new era in gravitational-wave astronomy. As the first anticipated space-based gravitational-wave detector, it will expand our view to the millihertz gravitational-wave sky, where a spectac
Externí odkaz:
http://arxiv.org/abs/2311.01300
Autor:
Burns, Eric, Coughlin, Michael, Ackley, Kendall, Andreoni, Igor, Bizouard, Marie-Anne, Broekgaarden, Floor, Christensen, Nelson L., D'Ammando, Filippo, DeLaunay, James, Fleischhack, Henrike, Frey, Raymond, Fryer, Chris L., Goldstein, Adam, Grossan, Bruce, Hamburg, Rachel, Hartmann, Dieter H., Ho, Anna Y. Q., Howell, Eric J., Hui, C. Michelle, Jenks, Leah, Joens, Alyson, Lesage, Stephen, Levan, Andrew J., Lien, Amy, Meli, Athina, Negro, Michela, Parsotan, Tyler, Roberts, Oliver J., Santander, Marcos, Smith, Jacob R., Tohuvavohu, Aaron, Tomsick, John A., Wadiasingh, Zorawar, Veres, Peter, Villar, Ashley V., Zhang, Haocheng, Zhu, Sylvia J.
The Interplanetary Network (IPN) is a detection, localization and alert system that utilizes the arrival time of transient signals in gamma-ray detectors on spacecraft separated by planetary baselines to geometrically locate the origin of these trans
Externí odkaz:
http://arxiv.org/abs/2308.04485
Autor:
Yang, Yu-Han, Troja, Eleonora, O'Connor, Brendan, Fryer, Chris L., Im, Myungshin, Durbak, Joe, Paek, Gregory S. H., Ricci, Roberto, De Bom, Clécio R., Gillanders, James H., Castro-Tirado, Alberto J., Peng, Zong-Kai, Dichiara, Simone, Ryan, Geoffrey, van Eerten, Hendrik, Dai, Zi-Gao, Chang, Seo-Won, Choi, Hyeonho, De, Kishalay, Hu, Youdong, Kilpatrick, Charles D., Kutyrev, Alexander, Jeong, Mankeun, Lee, Chung-Uk, Makler, Martin, Navarete, Felipe, Pérez-García, Ignacio
Kilonovae are a rare class of astrophysical transients powered by the radioactive decay of nuclei heavier than iron, synthesized in the merger of two compact objects. Over the first few days, the kilonova evolution is dominated by a large number of r
Externí odkaz:
http://arxiv.org/abs/2308.00638
Autor:
Gillanders, James H., Troja, Eleonora, Fryer, Chris L., Ristic, Marko, O'Connor, Brendan, Fontes, Christopher J., Yang, Yu-Han, Domoto, Nanae, Rahmouni, Salma, Tanaka, Masaomi, Fox, Ori D., Dichiara, Simone
Kilonovae are a novel class of astrophysical transients, and the only observationally-confirmed site of rapid neutron capture nucleosynthesis (the r-process) in the Universe. To date, only a handful of kilonovae have been detected, with just a single
Externí odkaz:
http://arxiv.org/abs/2308.00633