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pro vyhledávání: '"Kelley, Luke Z."'
Autor:
Bavera, Simone S., Fragos, Tassos, Zapartas, Emmanouil, Ramirez-Ruiz, Enrico, Marchant, Pablo, Kelley, Luke Z., Zevin, Michael, Andrews, Jeff J., Coughlin, Scott, Dotter, Aaron, Kovlakas, Konstantinos, Misra, Devina, Serra-Perez, Juan G., Qin, Ying, Rocha, Kyle A., Román-Garza, Jaime, Tran, Nam H., Xing, Zepei
Long-duration gamma-ray bursts are thought to be associated with the core-collapse of massive, rapidly spinning stars and the formation of black holes. However, efficient angular momentum transport in stellar interiors, currently supported by asteros
Externí odkaz:
http://arxiv.org/abs/2106.15841
Autor:
Arzoumanian, Zaven, Baker, Paul T., Brazier, Adam, Brook, Paul R., Burke-Spolaor, Sarah, Becsy, Bence, Charisi, Maria, Chatterjee, Shami, Cordes, James M., Cornish, Neil J., Crawford, Fronefield, Cromartie, H. Thankful, DeCesar, Megan E., Demorest, Paul B., Dolch, Timothy, Elliott, Rodney D., Ellis, Justin A., Ferrara, Elizabeth C., Fonseca, Emmanuel, Garver-Daniels, Nathan, Gentile, Peter A., Good, Deborah C., Hazboun, Jeffrey S., Islo, Kristina, Jennings, Ross J., Jones, Megan L., Kaiser, Andrew R., Kaplan, David L., Kelley, Luke Z., Key, Joey Shapiro, Lam, Michael T., Lazio, T. Joseph W., Luo, Jing, Lynch, Ryan S., Ma, Chung-Pei, Madison, Dustin R., McLaughlin, Maura A., Mingarelli, Chiara M. F., Ng, Cherry, Nice, David J., Pennucci, Timothy T., Pol, Nihan S., Ransom, Scott M., Ray, Paul S., Shapiro-Albert, Brent J., Siemens, Xavier, Simon, Joseph, Spiewak, Renee, Stairs, Ingrid H., Stinebring, Daniel R., Stovall, Kevin, Swiggum, Joseph K., Taylor, Stephen R., Vallisneri, Michele, Vigeland, Sarah J., Witt, Caitlin A., Collaboration, The NANOGrav
Supermassive black hole binaries (SMBHBs) should form frequently in galactic nuclei as a result of galaxy mergers. At sub-parsec separations, binaries become strong sources of low-frequency gravitational waves (GWs), targeted by Pulsar Timing Arrays
Externí odkaz:
http://arxiv.org/abs/2101.02716
Autor:
Taylor, Stephen R., Burke-Spolaor, Sarah, Baker, Paul T., Charisi, Maria, Islo, Kristina, Kelley, Luke Z., Madison, Dustin R., Simon, Joseph, Vigeland, Sarah
Precision timing of large arrays (>50) of millisecond pulsars will detect the nanohertz gravitational-wave emission from supermassive binary black holes within the next ~3-7 years. We review the scientific opportunities of these detections, the requi
Externí odkaz:
http://arxiv.org/abs/1903.08183
We discuss two approaches to searches for gravitational-wave (GW) and electromagnetic (EM) counterparts of binary neutron star mergers. The first approach relies on triggering archival searches of GW detector data based on detections of EM transients
Externí odkaz:
http://arxiv.org/abs/1111.0005
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