Zobrazeno 1 - 10
of 4 087
pro vyhledávání: '"Murphy, A. W."'
Autor:
Murphy, Jeremiah W., Barrientos, Andres F., Andrae, Rene, Guzman, Joseph, Williams, Benjamin F., Dalcanton, Julianne J., Koplitz, Brad
Stellar evolution theory restricted to single stars predicts a minimum mass for core-collapse supernovae (CCSNe) of around eight solar masses; this minimum mass corresponds to a maximum age of around 45 million years for the progenitor and the coeval
Externí odkaz:
http://arxiv.org/abs/2406.04075
Autor:
Murphy, Christopher W.
Lorentz invariant quantum field theories (QFTs) in four spacetime dimensions (4D) have a $\mathbb{Z}_4$ symmetry provided there exists a basis of operators in the QFT where all operators have even operator dimension, $d$, including those with $d > 4$
Externí odkaz:
http://arxiv.org/abs/2402.02195
Most massive stars end their lives with core collapse. However, it is not clear which explode as a Core-collapse Supernova (CCSN), leaving behind a neutron star and which collapse to black hole, aborting the explosion. One path to predict explodabili
Externí odkaz:
http://arxiv.org/abs/2311.02179
In this paper, we introduce curve-lifted codes over fields of arbitrary characteristic, inspired by Hermitian-lifted codes over $\mathbb{F}_{2^r}$. These codes are designed for locality and availability, and their particular parameters depend on the
Externí odkaz:
http://arxiv.org/abs/2307.13183
Autor:
Koplitz, Brad, Johnson, Jared, Williams, Benjamin F., Diaz-Rodriguez, Mariangelly, Murphy, Jeremiah W., Lazzarini, Margaret, Guzman, Joseph, Dalcanton, Julianne J., Dolphin, Andrew, Durbin, Meredith
Using resolved optical stellar photometry from the Panchromatic Hubble Andromeda Treasury Triangulum Extended Region (PHATTER) survey, we measured the star formation history (SFH) near the position of 85 supernova remnants (SNRs) in M33. We constrain
Externí odkaz:
http://arxiv.org/abs/2303.07318
Autor:
Daly, R. Terik, Ernst, Carolyn M., Barnouin, Olivier S., Chabot, Nancy L., Rivkin, Andrew S., Cheng, Andrew F., Adams, Elena Y., Agrusa, Harrison F., Abel, Elisabeth D., Alford, Amy L., Asphaug, Erik I., Atchison, Justin A., Badger, Andrew R., Baki, Paul, Ballouz, Ronald-L., Bekker, Dmitriy L., Bellerose, Julie, Bhaskaran, Shyam, Buratti, Bonnie J., Cambioni, Saverio, Chen, Michelle H., Chesley, Steven R., Chiu, George, Collins, Gareth S., Cox, Matthew W., DeCoster, Mallory E., Ericksen, Peter S., Espiritu, Raymond C., Faber, Alan S., Farnham, Tony L., Ferrari, Fabio, Fletcher, Zachary J., Gaskell, Robert W., Graninger, Dawn M., Haque, Musad A., Harrington-Duff, Patricia A., Hefter, Sarah, Herreros, Isabel, Hirabayashi, Masatoshi, Huang, Philip M., Hsieh, Syau-Yun W., Jacobson, Seth A., Jenkins, Stephen N., Jensenius, Mark A., John, Jeremy W., Jutzi, Martin, Kohout, Tomas, Krueger, Timothy O., Laipert, Frank E., Lopez, Norberto R., Luther, Robert, Lucchetti, Alice, Mages, Declan M., Marchi, Simone, Martin, Anna C., McQuaide, Maria E., Michel, Patrick, Moskovitz, Nicholas A., Murphy, Ian W., Murdoch, Naomi, Naidu, Shantanu P., Nair, Hari, Nolan, Michael C., Ormö, Jens, Pajola, Maurizio, Palmer, Eric E., Peachey, James M., Pravec, Petr, Raducan, Sabina D., Ramesh, K. T., Ramirez, Joshua R., Reynolds, Edward L., Richman, Joshua E., Robin, Colas Q., Rodriguez, Luis M., Roufberg, Lew M., Rush, Brian P., Sawyer, Carolyn A., Scheeres, Daniel J., Scheirich, Petr, Schwartz, Stephen R., Shannon, Matthew P., Shapiro, Brett N., Shearer, Caitlin E., Smith, Evan J., Steele, R. Joshua, Steckloff, Jordan K, Stickle, Angela M., Sunshine, Jessica M., Superfin, Emil A., Tarzi, Zahi B., Thomas, Cristina A., Thomas, Justin R., Trigo-Rodríguez, Josep M., Tropf, B. Teresa, Vaughan, Andrew T., Velez, Dianna, Waller, C. Dany, Wilson, Daniel S., Wortman, Kristin A., Zhang, Yun
While no known asteroid poses a threat to Earth for at least the next century, the catalog of near-Earth asteroids is incomplete for objects whose impacts would produce regional devastation. Several approaches have been proposed to potentially preven
Externí odkaz:
http://arxiv.org/abs/2303.02248
One of the major challenges in Core-collapse Supernova (CCSN) theory is to predict which stars explode and which collapse to black holes. Gogilashvili and Murphy (2022) derived an analytic force explosion condition (FEC) and showed that the FEC is co
Externí odkaz:
http://arxiv.org/abs/2302.04890
Autor:
Alioli, Simone, Boughezal, Radja, Cao, Weiguang, Chala, Mikael, Díaz-Carmona, Álvaro, Bakshi, Supratim Das, Durieux, Gauthier, Gráf, Lukáš, Guedes, Guilherme, Henning, Brian Quinn, Kitahara, Teppei, Li, Hao-Lin, Lu, Xiaochuan, Machado, Camila S., Martin, Adam, Melia, Tom, Mereghetti, Emanuele, Murayama, Hitoshi, Murphy, Christopher W., Nepveu, Jasper Roosmale, Pal, Sridip, Petriello, Frank, Shadmi, Yael, Shu, Jing, Weiss, Yaniv, Xiao, Ming-Lei, Yu, Jiang-Hao
In this contribution to the Snowmass 2021 process we review theoretical developments in the Standard Model Effective Field Theory (SMEFT) with a focus on effects at the dimension-8 level and beyond. We review the theoretical advances that led to the
Externí odkaz:
http://arxiv.org/abs/2203.06771
Autor:
Barry, Tomás, Kasemiire, Alice, Quinn, Martin, Deasy, Conor, Bury, Gerard, Masterson, Siobhan, Segurado, Ricardo, Murphy, Andrew W.
Publikováno v:
In Resuscitation Plus September 2024 19
Autor:
Barry, Tomás, Kasemiire, Alice, Quinn, Martin, Deasy, Conor, Bury, Gerard, Masterson, Siobhan, Segurado, Ricardo, Murphy, Andrew W
Publikováno v:
In Resuscitation Plus September 2024 19