Valeriya Korol, Riccardo Buscicchio, Ruediger Pakmor, Javier Moran-Fraile, Christopher J. Moore, and Selma E. de Mink
Abstract: The nature of progenitors of Type Ia supernovae has long been debated, primarily due to the elusiveness of the progenitor systems to traditional electromagnetic observation methods. We argue that gravitational wave observations with the upcoming Laser Interferometer Space Antenna (LISA) ..
M. Armano, H. Audley, J. Baird, P. Binetruy, M. Born, D. Bortoluzzi, E. Castelli, A. Cavalleri, A. Cesarini, V. Chiavegato, A. M. Cruise, D. Dal Bosco, K. Danzmann, et al.
Abstract: We present an analysis of the LISA Pathfinder differential acceleration performance over the entire mission. We show that the Brownian noise level, …
LISA Consortium Waveform Working Group, Niayesh Afshordi, Sarp Akçay, Pau Amaro Seoane, Andrea Antonelli, et al.
Abstract: LISA, the Laser Interferometer Space Antenna, will usher in a new era in gravitational-wave astronomy. As the first anticipated space-based gravitational-wave detector, it will expand our view to the millihertz gravitational-wave sky, where a spectacular variety of interesting new sources abound …
Future exploration of the Large Magellanic Cloud (LMC) with LISA will uncover a rich population of binary systems emitting detectable gravitational waves, offering valuable insights into the LMC’s properties and giving a more complete understanding of the Milky Way’s largest satellite galaxy.
Zenodo: https://zenodo.org/record/6918083
Michael L. Katz, Sylvain Marsat, Alvin J. K. Chua, Stanislav Babak, and Shane L. Larson
Abstract: The Laser Interferometer Space Antenna (LISA) is slated for launch in the early 2030s. A main target of the mission is massive black hole binaries that have an expected detection rate of …
Isabel Escudero Sanz*, Astrid Heske and Jeffrey C. Livas
Abstract: Gravitational waves are a prediction of Einstein’s general relativity theory. In autumn 2017, the Laser Interferometer Gravitational-Wave Observatory (LIGO) experiment reported the first detection of gravitational waves in addition to elec- tromagnetic radiation from the collision of two neutron stars …
Stanislav Babak, Jonathan Gair, Alberto Sesana, Enrico Barausse, Carlos F. Sopuerta, Christopher P. L. Berry, Emanuele Berti, Pau Amaro-Seoane, Antoine Petiteau, Antoine Klein
Abstract: The space-based Laser Interferometer Space Antenna (LISA) will be able to observe the gravitational-wave signals from systems comprised of a massive black hole and a stellar-mass compact object. These systems are known as extreme-mass-ratio inspirals …
G Heinzel, V Wand, A García, O Jennrich, C Braxmaier, D Robertson, K Middleton, D Hoyland, A Rüdiger, R Schilling, U Johann and K Danzmann
Abstract: The LISA Technology Package (LTP), to be launched by ESA in 2006/2007, is a technology demonstration mission in preparation for the LISA space-borne gravitational wave detector. A central part of the LTP is the optical metrology package (heterodyne interferometer with phasemeter) which monitors the distance between …