Zobrazeno 1 - 10
of 121
pro vyhledávání: '"Landry, Philippe"'
Autor:
Somasundaram, Rahul, Svensson, Isak, De, Soumi, Deneris, Andrew E., Dietz, Yannick, Landry, Philippe, Schwenk, Achim, Tews, Ingo
Understanding the interactions between nucleons in dense matter is one of the outstanding challenges of theoretical physics. Effective field theories have emerged as the dominant approach to address this problem at low energies, with many successful
Externí odkaz:
http://arxiv.org/abs/2410.00247
Observations of GW170817 strongly suggest that binary neutron star (BNS) mergers can produce rapid neutron-capture nucleosynthesis (r-process) elements. However, it remains an open question whether BNS mergers can account for all the r-process elemen
Externí odkaz:
http://arxiv.org/abs/2402.03696
Autor:
Gupta, Ish, Afle, Chaitanya, Arun, K. G., Bandopadhyay, Ananya, Baryakhtar, Masha, Biscoveanu, Sylvia, Borhanian, Ssohrab, Broekgaarden, Floor, Corsi, Alessandra, Dhani, Arnab, Evans, Matthew, Hall, Evan D., Hannuksela, Otto A., Kacanja, Keisi, Kashyap, Rahul, Khadkikar, Sanika, Kuns, Kevin, Li, Tjonnie G. F., Miller, Andrew L., Nitz, Alexander Harvey, Owen, Benjamin J., Palomba, Cristiano, Pearce, Anthony, Phurailatpam, Hemantakumar, Rajbhandari, Binod, Read, Jocelyn, Romano, Joseph D., Sathyaprakash, Bangalore S., Shoemaker, David H., Singh, Divya, Vitale, Salvatore, Barsotti, Lisa, Berti, Emanuele, Cahillane, Craig, Chen, Hsin-Yu, Fritschel, Peter, Haster, Carl-Johan, Landry, Philippe, Lovelace, Geoffrey, McClelland, David, Slagmolen, Bram J J, Smith, Joshua, Soares-Santos, Marcelle, Sun, Ling, Tanner, David, Yamamoto, Hiro, Zucker, Michael
Gravitational-wave observations by the Laser Interferometer Gravitational-Wave Observatory (LIGO) and Virgo have provided us a new tool to explore the Universe on all scales from nuclear physics to the cosmos and have the massive potential to further
Externí odkaz:
http://arxiv.org/abs/2307.10421
Publikováno v:
Res. Notes AAS 7 136 (2023)
Compact-object binary mergers consisting of one neutron star and one black hole (NSBHs) have long been considered promising progenitors for gamma-ray bursts, whose central engine remains poorly understood. Using gravitational-wave constraints on the
Externí odkaz:
http://arxiv.org/abs/2306.14974
Autor:
Evans, Matthew, Corsi, Alessandra, Afle, Chaitanya, Ananyeva, Alena, Arun, K. G., Ballmer, Stefan, Bandopadhyay, Ananya, Barsotti, Lisa, Baryakhtar, Masha, Berger, Edo, Berti, Emanuele, Biscoveanu, Sylvia, Borhanian, Ssohrab, Broekgaarden, Floor, Brown, Duncan A., Cahillane, Craig, Campbell, Lorna, Chen, Hsin-Yu, Daniel, Kathryne J., Dhani, Arnab, Driggers, Jennifer C., Effler, Anamaria, Eisenstein, Robert, Fairhurst, Stephen, Feicht, Jon, Fritschel, Peter, Fulda, Paul, Gupta, Ish, Hall, Evan D., Hammond, Giles, Hannuksela, Otto A., Hansen, Hannah, Haster, Carl-Johan, Kacanja, Keisi, Kamai, Brittany, Kashyap, Rahul, Key, Joey Shapiro, Khadkikar, Sanika, Kontos, Antonios, Kuns, Kevin, Landry, Michael, Landry, Philippe, Lantz, Brian, Li, Tjonnie G. F., Lovelace, Geoffrey, Mandic, Vuk, Mansell, Georgia L., Martynov, Denys, McCuller, Lee, Miller, Andrew L., Nitz, Alexander Harvey, Owen, Benjamin J., Palomba, Cristiano, Read, Jocelyn, Phurailatpam, Hemantakumar, Reddy, Sanjay, Richardson, Jonathan, Rollins, Jameson, Romano, Joseph D., Sathyaprakash, Bangalore S., Schofield, Robert, Shoemaker, David H., Sigg, Daniel, Singh, Divya, Slagmolen, Bram, Sledge, Piper, Smith, Joshua, Soares-Santos, Marcelle, Strunk, Amber, Sun, Ling, Tanner, David, van Son, Lieke A. C., Vitale, Salvatore, Willke, Benno, Yamamoto, Hiro, Zucker, Michael
Gravitational-wave astronomy has revolutionized humanity's view of the universe, a revolution driven by observations that no other field can make. This white paper describes an observatory that builds on decades of investment by the National Science
Externí odkaz:
http://arxiv.org/abs/2306.13745
Astrophysical observations of neutron stars probe the structure of dense nuclear matter and have the potential to reveal phase transitions at high densities. Most recent analyses are based on parametrized models of the equation of state with a finite
Externí odkaz:
http://arxiv.org/abs/2305.07411
Autor:
Kumar, Rajesh, Dexheimer, Veronica, Jahan, Johannes, Noronha, Jorge, Noronha-Hostler, Jacquelyn, Ratti, Claudia, Yunes, Nico, Acuna, Angel Rodrigo Nava, Alford, Mark, Anik, Mahmudul Hasan, Chatterjee, Debarati, Chatziioannou, Katerina, Chen, Hsin-Yu, Clevinger, Alexander, Conde, Carlos, Cruz-Camacho, Nikolas, Dore, Travis, Drischler, Christian, Elfner, Hannah, Essick, Reed, Friedenberg, David, Ghosh, Suprovo, Grefa, Joaquin, Haas, Roland, Haber, Alexander, Hammelmann, Jan, Harris, Steven, Haster, Carl-Johan, Hatsuda, Tetsuo, Hippert, Mauricio, Hirayama, Renan, Holt, Jeremy W., Kahangirwe, Micheal, Karthein, Jamie, Kojo, Toru, Landry, Philippe, Lin, Zidu, Luzum, Matthew, Manning, T. Andrew, Martin, Jordi Salinas San, Miller, Cole, Most, Elias Roland, Mroczek, Debora, Muronga, Azwinndini, Patino, Nicolas, Peterson, Jeffrey, Plumberg, Christopher, Price, Damien, Providencia, Constanca, Rougemont, Romulo, Roy, Satyajit, Shah, Hitansh, Shapiro, Stuart, Steiner, Andrew W., Strickland, Michael, Tan, Hung, Togashi, Hajime, Vazquez, Israel Portillo, Wen, Pengsheng, Zhang, Ziyuan
Publikováno v:
Living Reviews in Relativity (2024) 27:3
This review aims at providing an extensive discussion of modern constraints relevant for dense and hot strongly interacting matter. It includes theoretical first-principle results from lattice and perturbative QCD, as well as chiral effective field t
Externí odkaz:
http://arxiv.org/abs/2303.17021
Autor:
Landry, Philippe, Chakravarti, Kabir
Neutron star equations of state with strong phase transitions may support twin stars, hybrid and hadronic stars with the same mass but different tidal deformabilities. The presence of twin stars in the population of merging neutron stars produces dis
Externí odkaz:
http://arxiv.org/abs/2212.09733
Autor:
Lovato, Alessandro, Dore, Travis, Pisarski, Robert D., Schenke, Bjoern, Chatziioannou, Katerina, Read, Jocelyn S., Landry, Philippe, Danielewicz, Pawel, Lee, Dean, Pratt, Scott, Rennecke, Fabian, Elfner, Hannah, Dexheimer, Veronica, Kumar, Rajesh, Strickland, Michael, Jahan, Johannes, Ratti, Claudia, Vovchenko, Volodymyr, Stephanov, Mikhail, Almaalol, Dekrayat, Baym, Gordon, Hippert, Mauricio, Noronha-Hostler, Jacquelyn, Noronha, Jorge, Speranza, Enrico, Yunes, Nicolas, Horowitz, Chuck J., Harris, Steven P., McLerran, Larry, Reddy, Sanjay, Sorensen, Agnieszka, Sen, Srimoyee, Gandolfi, Stefano, Tews, Ingo, Miller, M. Coleman, Chirenti, Cecilia, Davoudi, Zohreh, Karthein, Jamie M., Rajagopal, Krishna, Vitale, Salvatore, Kapusta, Joseph, Basar, Gokce, Schaefer, Thomas, Skokov, Vladimir, Heinz, Ulrich, Drischler, Christian, Phillips, Daniel R., Prakash, Madappa, Fodor, Zoltan, Radice, David, Plumberg, Christopher, Most, Elias R., Raithel, Carolyn A., Fraga, Eduardo S., Kurkela, Aleksi, Lattimer, James M., Steiner, Andrew W., Holt, Jeremy W., Li, Bao-An, Shen, Chun, Alford, Mark, Haber, Alexander, Pastore, Saori, Piarulli, Maria
Since the release of the 2015 Long Range Plan in Nuclear Physics, major events have occurred that reshaped our understanding of quantum chromodynamics (QCD) and nuclear matter at large densities, in and out of equilibrium. The US nuclear community ha
Externí odkaz:
http://arxiv.org/abs/2211.02224
Autor:
Bogdanov, Slavko, Fonseca, Emmanuel, Kashyap, Rahul, Kurkela, Aleksi, Lattimer, James M., Read, Jocelyn S., Sathyaprakash, Bangalore S., Cromartie, H. Thankful, Dietrich, Tim, Dhani, Arnab, Dolch, Timothy, Gorda, Tyler, Guillot, Sebastien, Ho, Wynn C. G., Huxford, Rachael, Lamb, Frederick K., Landry, Philippe, Meyers, Bradley W., Miller, M. Coleman, Nättilä, Joonas, Paatelainen, Risto, Prescod-Weinstein, Chanda, Säppi, Saga, Stairs, Ingrid H., Stergioulas, Nikolaos, Tews, Ingo, Vuorinen, Aleksi, Wadiasingh, Zorawar, Watts, Anna L.
Our limited understanding of the physical properties of matter at ultra-high density, high proton/neutron number asymmetry, and low temperature is presently one of the major outstanding problems in physics. As matter in this extreme state is known to
Externí odkaz:
http://arxiv.org/abs/2209.07412