Zobrazeno 1 - 10
of 113
pro vyhledávání: '"Dvorkin, Irina"'
Recent discoveries of gravitational wave sources have advanced our knowledge about the formation of compact object binaries. At present, many questions about the stellar origins of binary neutron stars remain open. We explore the evolution of binary
Externí odkaz:
http://arxiv.org/abs/2411.04563
Autor:
Liu, Boyuan, Hartwig, Tilman, Sartorio, Nina S., Dvorkin, Irina, Costa, Guglielmo, Santoliquido, Filippo, Fialkov, Anastasia, Klessen, Ralf S., Bromm, Volker
The gravitational wave (GW) signal from binary black hole (BBH) mergers is a promising probe of Population III (Pop III) stars. To fully unleash the power of the GW probe, one important step is to understand the relative importance and features of di
Externí odkaz:
http://arxiv.org/abs/2406.17397
We investigate the Stochastic Gravitational Wave Background (SGWB) produced by merging binary black holes (BBHs) and binary neutron stars (BNSs) in the frequency ranges of LIGO/Virgo/Kagra and LISA. We develop three analytical models, that are calibr
Externí odkaz:
http://arxiv.org/abs/2306.09861
Autor:
Renzini, Arianna I., Romero-Rodrguez, Alba, Talbot, Colm, Lalleman, Max, Kandhasamy, Shivaraj, Turbang, Kevin, Biscoveanu, Sylvia, Martinovic, Katarina, Meyers, Patrick, Tsukada, Leo, Janssens, Kamiel, Davis, Derek, Matas, Andrew, Charlton, Philip, Liu, Guo-Chin, Dvorkin, Irina, Banagiri, Sharan, Bose, Sukanta, Callister, Thomas, De Lillo, Federico, D'Onofrio, Luca, Garufi, Fabio, Harry, Gregg, Lawrence, Jessica, Mandic, Vuk, Macquet, Adrian, Michaloliakos, Ioannis, Mitra, Sanjit, Pham, Kiet, Poggiani, Rosa, Regimbau, Tania, Romano, Joseph D., van Remortel, Nick, Zhong, Haowen
The collection of gravitational waves (GWs) that are either too weak or too numerous to be individually resolved is commonly referred to as the gravitational-wave background (GWB). A confident detection and model-driven characterization of such a sig
Externí odkaz:
http://arxiv.org/abs/2303.15696
Autor:
Seoane, Pau Amaro, Andrews, Jeff, Sedda, Manuel Arca, Askar, Abbas, Baghi, Quentin, Balasov, Razvan, Bartos, Imre, Bavera, Simone S., Bellovary, Jillian, Berry, Christopher P. L., Berti, Emanuele, Bianchi, Stefano, Blecha, Laura, Blondin, Stephane, Bogdanović, Tamara, Boissier, Samuel, Bonetti, Matteo, Bonoli, Silvia, Bortolas, Elisa, Breivik, Katelyn, Capelo, Pedro R., Caramete, Laurentiu, Cattorini, Federico, Charisi, Maria, Chaty, Sylvain, Chen, Xian, Chruślińska, Martyna, Chua, Alvin J. K., Church, Ross, Colpi, Monica, D'Orazio, Daniel, Danielski, Camilla, Davies, Melvyn B., Dayal, Pratika, De Rosa, Alessandra, Derdzinski, Andrea, Destounis, Kyriakos, Dotti, Massimo, Duţan, Ioana, Dvorkin, Irina, Fabj, Gaia, Foglizzo, Thierry, Ford, Saavik, Fouvry, Jean-Baptiste, Franchini, Alessia, Fragos, Tassos, Fryer, Chris, Gaspari, Massimo, Gerosa, Davide, Graziani, Luca, Groot, Paul, Habouzit, Melanie, Haggard, Daryl, Haiman, Zoltan, Han, Wen-Biao, Istrate, Alina, Johansson, Peter H., Khan, Fazeel Mahmood, Kimpson, Tomas, Kokkotas, Kostas, Kong, Albert, Korol, Valeriya, Kremer, Kyle, Kupfer, Thomas, Lamberts, Astrid, Larson, Shane, Lau, Mike, Liu, Dongliang, Lloyd-Ronning, Nicole, Lodato, Giuseppe, Lupi, Alessandro, Ma, Chung-Pei, Maccarone, Tomas, Mandel, Ilya, Mangiagli, Alberto, Mapelli, Michela, Mathis, Steéphane, Mayer, Lucio, McGee, Sean, McKernan, Berry, Miller, M. Coleman, Mota, David F., Mumpower, Matthew, Nasim, Syeda S, Nelemans, Gijs, Noble, Scott, Pacucci, Fabio, Panessa, Francesca, Paschalidis, Vasileio, Pfister, Hugo, Porquet, Delphine, Quenby, John, Ricarte, Angelo, Röpke, Friedrich K., Regan, John, Rosswog, Stephan, Ruiter, Ashley, Ruiz, Milton, Runnoe, Jessie, Schneider, Raffaella, Schnittman, Jeremy, Secunda, Amy, Sesana, Alberto, Seto, Naoki, Shao, Lijing, Shapiro, Stuart, Sopuerta, Carlos, Stone, Nicholas C., Suvorov, Arthur, Tamanini, Nicola, Tamfal, Tomas, Tauris, Thomas, Temmink, Karel, Tomsick, John, Toonen, Silvia, Torres-Orjuela, Alejandro, Toscani, Martina, Tsokaros, Antonios, Unal, Caner, Vázquez-Aceves, Verónica, Valiante, Rosa, van Putten, Maurice, van Roestel, Jan, Vignali, Christian, Volonteri, Marta, Wu, Kinwah, Younsi, Ziri, Yu, Shenghua, Zane, Silvia, Zwick, Lorenz, Antonini, Fabio, Baibhav, Vishal, Barausse, Enrico, Rivera, Alexander Bonilla, Branchesi, Marica, Branduardi-Raymont, Graziella, Burdge, Kevin, Chakraborty, Srija, Cuadra, Jorge, Dage, Kristen, Davis, Benjamin, de Mink, Selma E., Decarli, Roberto, Doneva, Daniela, Escoffier, Stephanie, Fragione, Giacomo, Gandhi, Poshak, Haardt, Francesco, Lousto, Carlos O., Nissanke, Samaya, Nordhaus, Jason, O'Shaughnessy, Richard, Zwart, Simon Portegies, Pound, Adam, Schussler, Fabian, Sergijenko, Olga, Spallicci, Alessandro, Vernieri, Daniele, Vigna-Gómez, Alejandro
Publikováno v:
Living Reviews in Relativity, Volume 26, Article number: 2 (2023)
The Laser Interferometer Space Antenna (LISA) will be a transformative experiment for gravitational wave astronomy, and, as such, it will offer unique opportunities to address many key astrophysical questions in a completely novel way. The synergy wi
Externí odkaz:
http://arxiv.org/abs/2203.06016
Autor:
Seoane, Pau Amaro, Sedda, Manuel Arca, Babak, Stanislav, Berry, Christopher P. L., Berti, Emanuele, Bertone, Gianfranco, Blas, Diego, Bogdanović, Tamara, Bonetti, Matteo, Breivik, Katelyn, Brito, Richard, Caldwell, Robert, Capelo, Pedro R., Caprini, Chiara, Cardoso, Vitor, Carson, Zack, Chen, Hsin-Yu, Chua, Alvin J. K., Dvorkin, Irina, Haiman, Zoltan, Heisenberg, Lavinia, Isi, Maximiliano, Karnesis, Nikolaos, Kavanagh, Bradley J., Littenberg, Tyson B., Mangiagli, Alberto, Marcoccia, Paolo, Maselli, Andrea, Nardini, Germano, Pani, Paolo, Peloso, Marco, Pieroni, Mauro, Ricciardone, Angelo, Sesana, Alberto, Tamanini, Nicola, Toubiana, Alexandre, Valiante, Rosa, Vretinaris, Stamatis, Weir, David, Yagi, Kent, Zimmerman, Aaron
The science objectives of the LISA mission have been defined under the implicit assumption of a 4 yr continuous data stream. Based on the performance of LISA Pathfinder, it is now expected that LISA will have a duty cycle of $\approx 0.75$, which wou
Externí odkaz:
http://arxiv.org/abs/2107.09665
We study the enrichment of the interstellar medium with rapid neutron capture (r-process) elements produced in binary neutron star (BNS) mergers. We use a semi-analytic model to describe galactic evolution, with merger rates and time delay distributi
Externí odkaz:
http://arxiv.org/abs/2010.00625
Publikováno v:
Astrophys. J., 904, 16 (2020)
We revisit the predictions for the merger rate of massive black hole binaries detectable by the Laser Interferometer Space Antenna (LISA) and their background signal for pulsar-timing arrays. We focus on the effect of the delays between the merger of
Externí odkaz:
http://arxiv.org/abs/2006.03065
In this paper we study gravitational lensing of gravitational wave events. The main point of the present work is to introduce a semi-analytic approach so that each ingredient can be varied and tested individually. Our analytic model for the source po
Externí odkaz:
http://arxiv.org/abs/1912.11916
Autor:
Baker, John, Baker, Tessa, Carbone, Carmelita, Congedo, Giuseppe, Contaldi, Carlo, Dvorkin, Irina, Gair, Jonathan, Haiman, Zoltan, Mota, David F., Renzini, Arianna, Buis, Ernst-Jan, Cusin, Giulia, Ezquiaga, Jose Maria, Mueller, Guido, Pieroni, Mauro, Quenby, John, Ricciardone, Angelo, Saltas, Ippocratis D., Shao, Lijing, Tamanini, Nicola, Tasinato, Gianmassimo, Zumalacárregui, Miguel
Since the very beginning of astronomy the location of objects on the sky has been a fundamental observational quantity that has been taken for granted. While precise two dimensional positional information is easy to obtain for observations in the ele
Externí odkaz:
http://arxiv.org/abs/1908.11410