Zobrazeno 1 - 10
of 13
pro vyhledávání: '"Arianna I. Renzini"'
Autor:
Pierre Auclair, David Bacon, Tessa Baker, Tiago Barreiro, Nicola Bartolo, Enis Belgacem, Nicola Bellomo, Ido Ben-Dayan, Daniele Bertacca, Marc Besancon, Jose J. Blanco-Pillado, Diego Blas, Guillaume Boileau, Gianluca Calcagni, Robert Caldwell, Chiara Caprini, Carmelita Carbone, Chia-Feng Chang, Hsin-Yu Chen, Nelson Christensen, Sebastien Clesse, Denis Comelli, Giuseppe Congedo, Carlo Contaldi, Marco Crisostomi, Djuna Croon, Yanou Cui, Giulia Cusin, Daniel Cutting, Charles Dalang, Valerio De Luca, Walter Del Pozzo, Vincent Desjacques, Emanuela Dimastrogiovanni, Glauber C. Dorsch, Jose Maria Ezquiaga, Matteo Fasiello, Daniel G. Figueroa, Raphael Flauger, Gabriele Franciolini, Noemi Frusciante, Jacopo Fumagalli, Juan García-Bellido, Oliver Gould, Daniel Holz, Laura Iacconi, Rajeev Kumar Jain, Alexander C. Jenkins, Ryusuke Jinno, Cristian Joana, Nikolaos Karnesis, Thomas Konstandin, Kazuya Koyama, Jonathan Kozaczuk, Sachiko Kuroyanagi, Danny Laghi, Marek Lewicki, Lucas Lombriser, Eric Madge, Michele Maggiore, Ameek Malhotra, Michele Mancarella, Vuk Mandic, Alberto Mangiagli, Sabino Matarrese, Anupam Mazumdar, Suvodip Mukherjee, Ilia Musco, Germano Nardini, Jose Miguel No, Theodoros Papanikolaou, Marco Peloso, Mauro Pieroni, Luigi Pilo, Alvise Raccanelli, Sébastien Renaux-Petel, Arianna I. Renzini, Angelo Ricciardone, Antonio Riotto, Joseph D. Romano, Rocco Rollo, Alberto Roper Pol, Ester Ruiz Morales, Mairi Sakellariadou, Ippocratis D. Saltas, Marco Scalisi, Kai Schmitz, Pedro Schwaller, Olga Sergijenko, Geraldine Servant, Peera Simakachorn, Lorenzo Sorbo, Lara Sousa, Lorenzo Speri, Danièle A. Steer, Nicola Tamanini, Gianmassimo Tasinato, Jesús Torrado, Caner Unal, Vincent Vennin, Daniele Vernieri, Filippo Vernizzi, Marta Volonteri, Jeremy M. Wachter, David Wands, Lukas T. Witkowski, Miguel Zumalacárregui, James Annis, Fëanor Reuben Ares, Pedro P. Avelino, Anastasios Avgoustidis, Enrico Barausse, Alexander Bonilla, Camille Bonvin, Pasquale Bosso, Matteo Calabrese, Mesut Çalışkan, Jose A. R. Cembranos, Mikael Chala, David Chernoff, Katy Clough, Alexander Criswell, Saurya Das, Antonio da Silva, Pratika Dayal, Valerie Domcke, Ruth Durrer, Richard Easther, Stephanie Escoffier, Sandrine Ferrans, Chris Fryer, Jonathan Gair, Chris Gordon, Martin Hendry, Mark Hindmarsh, Deanna C. Hooper, Eric Kajfasz, Joachim Kopp, Savvas M. Koushiappas, Utkarsh Kumar, Martin Kunz, Macarena Lagos, Marc Lilley, Joanes Lizarraga, Francisco S. N. Lobo, Azadeh Maleknejad, C. J. A. P. Martins, P. Daniel Meerburg, Renate Meyer, José Pedro Mimoso, Savvas Nesseris, Nelson Nunes, Vasilis Oikonomou, Giorgio Orlando, Ogan Özsoy, Fabio Pacucci, Antonella Palmese, Antoine Petiteau, Lucas Pinol, Simon Portegies Zwart, Geraint Pratten, Tomislav Prokopec, John Quenby, Saeed Rastgoo, Diederik Roest, Kari Rummukainen, Carlo Schimd, Aurélia Secroun, Alberto Sesana, Carlos F. Sopuerta, Ismael Tereno, Andrew Tolley, Jon Urrestilla, Elias C. Vagenas, Jorinde van de Vis, Rien van de Weygaert, Barry Wardell, David J. Weir, Graham White, Bogumiła Świeżewska, Valery I. Zhdanov, The LISA Cosmology Working Group
Publikováno v:
Living Reviews in Relativity, Vol 26, Iss 1, Pp 1-254 (2023)
Abstract The Laser Interferometer Space Antenna (LISA) has two scientific objectives of cosmological focus: to probe the expansion rate of the universe, and to understand stochastic gravitational-wave backgrounds and their implications for early univ
Externí odkaz:
https://doaj.org/article/cb0550dff7cf4f0d9707d25befc457fc
Autor:
Arianna I. Renzini, Alba Romero-Rodríguez, Colm Talbot, Max Lalleman, Shivaraj Kandhasamy, Kevin Turbang, Sylvia Biscoveanu, Katarina Martinovic, Patrick Meyers, Leo Tsukada, Kamiel Janssens, Derek Davis, Andrew Matas, Philip Charlton, Guo-Chin Liu, Irina Dvorkin, Sharan Banagiri, Sukanta Bose, Thomas Callister, Federico De Lillo, Luca D’Onofrio, Fabio Garufi, Gregg Harry, Jessica Lawrence, Vuk Mandic, Adrian Macquet, Ioannis Michaloliakos, Sanjit Mitra, Kiet Pham, Rosa Poggiani, Tania Regimbau, Joseph D. Romano, Nick van Remortel, Haowen Zhong
Publikováno v:
The Astrophysical Journal, Vol 952, Iss 1, p 25 (2023)
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:
https://doaj.org/article/40fa330a676f45b9a6d6f54efe62ce7f
Publikováno v:
Galaxies, Vol 10, Iss 1, p 34 (2022)
The collection of individually resolvable gravitational wave (GW) events makes up a tiny fraction of all GW signals that reach our detectors, while most lie below the confusion limit and are undetected. Similarly to voices in a crowded room, the coll
Externí odkaz:
https://doaj.org/article/0a429383bdbd4660b9f2aea7fe8fc495
Publikováno v:
Nature Astronomy. 6:1356-1363
Autor:
Jessica Lawrence, Kevin Turbang, Andrew Matas, Arianna I. Renzini, Nick van Remortel, Joseph Romano
Publikováno v:
Physical review D
Physical Review D
Physical Review D
A likely source of a gravitational-wave background (GWB) in the frequency band of the Advanced LIGO, Virgo and KAGRA detectors is the superposition of signals from the population of unresolvable stellar-mass binary-black-hole (BBH) mergers throughout
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7746edcb9d78a0c917e8f7659ee435a7
Autor:
Jean-Baptiste Bayle, Béatrice Bonga, Daniela Doneva, Tanja Hinderer, Archisman Ghosh, Nikolaos Karnesis, Mikhail Korobko, Valeriya Korol, Elisa Maggio, Martina Muratore, Arianna I. Renzini, Angelo Ricciardone, Sweta Shah, Golam Shaifullah, Lijing Shao, Lorenzo Speri, Nicola Tamanini, David Weir
Publikováno v:
Nature Astronomy, 6, 304-305
Nature astronomy
Nature Astronomy, 6, 3, pp. 304-305
Nature astronomy
Nature Astronomy, 6, 3, pp. 304-305
Gravitational wave science is a dynamical, fast-expanding research field founded on results, tools and methodologies drawn from different research areas and communities. Early career scientists entering this field must learn and combine knowledge and
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::97b91a49462420b8b065268dce608412
http://hdl.handle.net/2066/249246
http://hdl.handle.net/2066/249246
Autor:
Miguel Zumalacarregui, Carlo R. Contaldi, John G. Baker, Ippocratis D. Saltas, Lijing Shao, Angelo Ricciardone, Gianmassimo Tasinato, Giulia Cusin, J. J. Quenby, E.-J. Buis, Nicola Tamanini, Arianna I. Renzini, Mauro Pieroni, Tessa Baker, Zoltan Haiman, Jose María Ezquiaga, David F. Mota, Guido Mueller, Irina Dvorkin, Jonathan R. Gair, Carmelita Carbone, G. Congedo
Publikováno v:
Baker, J, Baker, T, Carbone, C, Congedo, G, Contaldi, C, Dvorkin, I, Gair, J, Haiman, Z, Mota, D F, Renzini, A, Buis, E-J, Cusin, G, Ezquiaga, J M, Mueller, G, Pieroni, M, Quenby, J, Ricciardone, A, Saltas, I D, Shao, L, Tamanini, N, Tasinato, G & Zumalacárregui, M 2021, ' High angular resolution gravitational wave astronomy ', Experimental Astronomy . https://doi.org/10.1007/s10686-021-09712-0
Experimental Astronomy
Experimental Astronomy, Springer Link, 2021, 51 (3), pp.1441-1470. ⟨10.1007/s10686-021-09712-0⟩
Experimental Astronomy
Experimental Astronomy, Springer Link, 2021, 51 (3), pp.1441-1470. ⟨10.1007/s10686-021-09712-0⟩
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:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0a5d3bf5adcab09875e97b9952fdd036
https://cronfa.swan.ac.uk/Record/cronfa60805/Download/60805__24910__3c3e521dda4247439c92fda7c92c566f.pdf
https://cronfa.swan.ac.uk/Record/cronfa60805/Download/60805__24910__3c3e521dda4247439c92fda7c92c566f.pdf
Autor:
Carlo R. Contaldi, Mauro Pieroni, Nikos Karnesis, Angelo Ricciardone, Arianna I. Renzini, Giulia Cusin, Marco Peloso, Gianmassimo Tasinato
Publikováno v:
Phys.Rev.D
Phys.Rev.D, 2020, 102 (4), pp.043502. ⟨10.1103/PhysRevD.102.043502⟩
Physical Review D
Physical Review D, American Physical Society, 2020, 102 (4), pp.043502. ⟨10.1103/PhysRevD.102.043502⟩
Phys.Rev.D, 2020, 102 (4), pp.043502. ⟨10.1103/PhysRevD.102.043502⟩
Physical Review D
Physical Review D, American Physical Society, 2020, 102 (4), pp.043502. ⟨10.1103/PhysRevD.102.043502⟩
Given the recent advances in gravitational-wave detection technologies, the detection and characterisation of gravitational-wave backgrounds (GWBs) with the Laser Interferometer Space Antenna (LISA) is a real possibility. To assess the abilities of t
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d79ca97931a21ad1ea9c93812563fbf9
http://arxiv.org/abs/2006.03313
http://arxiv.org/abs/2006.03313
Autor:
Carlo R. Contaldi, Arianna I. Renzini
We integrate the entire, publicly available, Advanced LIGO (ALIGO) data set to obtain maximum-likelihood constraint maps of the Stochastic Gravitational-Wave Background (SGWB). From these we derive limits on the energy density of the stochastic backg
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3cdf15c75a14657767ab75d479c31201
http://arxiv.org/abs/1907.10329
http://arxiv.org/abs/1907.10329
Autor:
Carlo R. Contaldi, Arianna I. Renzini
Given the recent detection of gravitational waves from individual sources it is almost a certainty that some form of background of gravitational waves will be detected in future. The most promising candidate for such a detection are backgrounds made
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5e194717e2702a1c1502b244a7225ff1