Zobrazeno 1 - 10
of 26
pro vyhledávání: '"Inchauspe, Henri"'
Autor:
Inchauspé, Henri, Gasparotto, Silvia, Blas, Diego, Heisenberg, Lavinia, Zosso, Jann, Tiwari, Shubhanshu
Gravitational wave (GW) astronomy has revolutionized our capacity to explore nature. The next generation of observatories, among which the space-borne detector Laser Interferometer Space Antenna LISA, is expected to yield orders of magnitude of signa
Externí odkaz:
http://arxiv.org/abs/2406.09228
Autor:
D'Ambrosio, Fabio, Gozzini, Francesco, Heisenberg, Lavinia, Inchauspé, Henri, Maibach, David, Zosso, Jann
We perform a comprehensive analysis of state-of-the-art waveform models, focusing on their predictions concerning kick velocity and inferred gravitational wave memory. In our investigation we assess the accuracy of waveform models using energy-moment
Externí odkaz:
http://arxiv.org/abs/2402.19397
We propose a diagnostic tool for future analyses of stochastic gravitational wave background signals of extra-galactic origin in LISA data. Next-generation gravitational wave detectors hold the capability to track unresolved gravitational waves bundl
Externí odkaz:
http://arxiv.org/abs/2401.14849
Finding a stochastic gravitational-wave background (SGWB) of astrophysical or primordial origin is one of the quests of current and future gravitational-wave observatories. While detector networks such as LIGO-Virgo-Kagra or pulsar timing arrays can
Externí odkaz:
http://arxiv.org/abs/2307.00649
Autor:
Heisenberg, Lavinia, Inchauspé, Henri, Nam, Dam Quang, Sauter, Orion, Waibel, Ricardo, Wass, Peter
The Laser Interferometer Space Antenna (LISA), space-based gravitational wave observatory involves a complex multidimensional closed-loop dynamical system. Its instrument performance is expected to be less efficiently isolated from platform motion th
Externí odkaz:
http://arxiv.org/abs/2306.17262
Publikováno v:
JCAP04(2023)066
Detecting stochastic background radiation of cosmological origin is an exciting possibility for current and future gravitational-wave (GW) detectors. However, distinguishing it from other stochastic processes, such as instrumental noise and astrophys
Externí odkaz:
http://arxiv.org/abs/2302.12573
Publikováno v:
Phys. Rev. D 106, 022006 (2022)
The Drag-Free and Attitude Control System is a central element of LISA technology, ensuring the very high dynamic stability of spacecraft and test masses required in order to reach the sensitivity that gravitational wave astronomy in space requires.
Externí odkaz:
http://arxiv.org/abs/2202.12735
Autor:
Inchauspé, Henri, Olatunde, Taiwo, Apple, Stephen, Parry, Samantha, Letson, Ben, Turetta, Nicholas, Mueller, Guido, Wass, Peter J, Conklin, John W
Publikováno v:
Phys. Rev. D 102, 042002 (2020)
Electrostatic charge control of isolated free-falling test masses is a key enabling technology for space-based gravitational missions. Contact-free electrostatic charge control can be achieved using photoelectron emission from metal surfaces under il
Externí odkaz:
http://arxiv.org/abs/2005.00917
Autor:
Armano, Michele, Audley, Heather, Baird, Jonathon, Binetruy, Pierre, Born, Michael, Bortoluzzi, Daniele, Castelli, Eleanora, Cavalleri, Antonella, Cesarini, Andrea, Cruise, Mike, Danzmann, Karsten, Silva, Marcus de Deus, Diepholz, Ingo, Dixon, George, Dolesi, Rita, Ferraioli, Luigi, Ferroni, Valerio, Fitzsimons, Ewan, Freschi, Mario, Gesa, Luis, Gibert, Ferran, Giardini, Domenico, Giusteri, Roberta, Grimani, Catia, Grzymisch, Jonathan, Harrison, Ian, Heinzel, Gerhard, Hewitson, Martin, Hollington, Daniel, Hoyland, David, Hueller, Mauro, Inchauspe, Henri, Jennrich, Oliver, Jetzer, Philippe, Karnesis, Nikolaos, Kaune, Brigitte, Korsakova, Natalia, Killow, Christian J, Lobo, Alberto, Lloro, Ivan, Liu, Li, Lopez-Zaragoza, Juan-Pedro, Maarschalkerweerd, Rolf, Mance, Davor, Meshksar, Neda, Martın, V, Martin-Polo, L, Martino, Joseph, Martin-Porqueras, Fernando, Mateos, Ignacio, McNamara, Paul, Mendes, Jose, Mendes, Luis, Nofrarias, Miquel, Paczkowski, Sarah, Perreur-Lloyd, Michael, Petiteau, Antoine, Pivato, Paolo, Plagnol, Eric, Ramos-Castro, Jose, Reiche, Jens, Robertson, David, Rivas, Francisco, Russano, Giuliana, Slutsky, Jacob, Sopuerta, Carlos, Sumner, Timothy, Texier, Daniel, Thorpe, Ira, Vetrugno, Daniele, Vitale, Stefano, Wanner, Gudrun, Ward, Harry, Wass, Peter, Weber, William, Wissel, Lennart, Wittchen, Andreas, Zweifel, Peter
Since the 2017 Nobel Prize in Physics was awarded for the observation of gravitational waves, it is fair to say that the epoch of gravitational wave astronomy (GWs) has begun. However, a number of interesting sources of GWs can only be observed from
Externí odkaz:
http://arxiv.org/abs/1903.08924
Autor:
Armano, Michele, Audley, Heather, Baird, Jonathon, Binetruy, Pierre, Born, Michael, Bortoluzzi, Daniele, Castelli, Eleanora, Cavalleri, Antonella, Cesarini, Andrea, Cruise, Mike, Danzmann, Karsten, Silva, Marcus de Deus, Diepholz, Igo, Dixon, George, Dolesi, Rita, Ferraioli, Luigi, Ferroni, Valerio, Fitzsimons, Ewan, Freschi, Mario, Gesa, Luis, Gibert, Ferran, Giardini, Domenico, Giusteri, Roberta, Grimani, Catia, Grzymisch, Jonathan, Harrison, Ian, Heinzel, Gerhard, Hewitson, Martin, Hollington, Daniel, Hoyland, David, Hueller, Mauro, Inchauspe, Henri, Jennrich, Oliver, Jetzer, Philippe, Karnesis, Nikolaos, Kaune, Brigitte, Korsakova, Natalia, Killow, Christian J, Lobo, Alberto, Lloro, Ivan, Liu, Li, Lopez-Zaragoza, Juan-Pedro P, Maarschalkerweerd, Rolf, Mance, Davor, Meshksar, Neda, Martın, V, Martin-Polo, L, Martino, Joseph, Martin-Porqueras, Fernando, Mateos, Ignacio, McNamara, Paul, Mendes, Jose, Mendes, Luis, Nofrarias, Miquel, Paczkowski, Sarah, Perreur-Lloyd, Michael, Petiteau, Antoine, Pivato, Paolo, Plagnol, Eric, Ramos-Castro, Jose, Reiche, Jens, Robertson, David, Rivas, Francisco, Russano, Giuliana, Slutsky, Jacob, Sopuerta, Carlos, Sumner, Timothy, Texier, Daniel, Thorpe, Ira, Vetrugno, Daniele, Vitale, Stefano, Wanner, Gudrun, Ward, Harry, Wass, Peter, Weber, William, Wissel, Lennart, Wittchen, Andreas, Zweifel, Peter
Publikováno v:
Phys. Rev. D 99, 082001 (2019)
The science operations of the LISA Pathfinder mission has demonstrated the feasibility of sub-femto-g free-fall of macroscopic test masses necessary to build a LISA-like gravitational wave observatory in space. While the main focus of interest, i.e.
Externí odkaz:
http://arxiv.org/abs/1812.05491