LISA Definition Study Report Article Swipe
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Monica Colpi
,
K. Danzmann
,
M. Hewitson
,
Kelly Holley‐Bockelmann
,
Philippe Jetzer
,
G. Nelemans
,
Antoine Petiteau
,
D. H. Shoemaker
,
Carlos F. Sopuerta
,
R. T. Stebbins
,
N. R. Tanvir
,
Henry Ward
,
W. J. Weber
,
Ira Thorpe
,
Anna Daurskikh
,
Atul Deep
,
Ignacio Fernández Núñez
,
C García Marirrodriga
,
Martin Gehler
,
Jean-Philippe Halain
,
O. Jennrich
,
U. Lammers
,
Jonan Larrañaga
,
Maike Lieser
,
Nora Lützgendorf
,
Waldemar Martens
,
Linda Mondin
,
Ana Piris Niño
,
Pau Amaro‐Seoane
,
Manuel Arca Sedda
,
Pierre Auclair
,
S. Babak
,
Quentin Baghi
,
Vishal Baibhav
,
Tessa Baker
,
Jean-Baptiste Bayle
,
C. P. L. Berry
,
Emanuele Berti
,
Guillaume Boileau
,
Matteo Bonetti
,
Richard Brito
,
R. Buscicchio
,
Gianluca Calcagni
,
Pedro R. Capelo
,
Chiara Caprini
,
Andrea Caputo
,
E. Castelli
,
Hsin-Yu Chen
,
Xian Chen
,
Alvin Chua
,
Gareth M. Davies
,
Andrea Derdzinski
,
Valerie Domcke
,
Daniela D. Doneva
,
Irna Dvorkin
,
José María Ezquiaga
,
Jonathan Gair
,
Zoltán Haiman
,
I. W. Harry
,
Olaf Hartwig
,
Aurelien Hees
,
Anna Heffernan
,
S. Husa
,
David Izquierdo
,
Nikolaos Karnesis
,
Antoine Klein
,
Valeriya Korol
,
Natalia Korsakova
,
Thomas Kupfer
,
D. Laghi
,
A. Lamberts
,
Shane Larson
,
M. Le Jeune
,
Marek Lewicki
,
T. B. Littenberg
,
Eric Madge
,
Alberto Mangiagli
,
S. Marsat
,
Iván Martín Vílchez
,
Andrea Maselli
,
Josh Mathews
,
Maarten van de Meent
,
M. Muratore
,
Germano Nardini
,
Paolo Pani
,
Marco Peloso
,
Mauro Pieroni
,
Adam Pound
,
Hippolyte Quelquejay-Leclere
,
Angelo Ricciardone
,
Elena M. Rossi
,
Andrea Sartirana
,
Etienne Savalle
,
Laura Sberna
,
Alberto Sesana
,
Deirdre Shoemaker
,
Jacob Slutsky
,
Thomas P. Sotiriou
,
Lorenzo Speri
,
Martin Staab
·
YOU?
·
· 2024
· Open Access
·
· DOI: https://doi.org/10.48550/arxiv.2402.07571
· OA: W4391799184
YOU?
·
· 2024
· Open Access
·
· DOI: https://doi.org/10.48550/arxiv.2402.07571
· OA: W4391799184
The Laser Interferometer Space Antenna (LISA) is the first scientific endeavour to detect and study gravitational waves from space. LISA will survey the sky for Gravitational Waves in the 0.1 mHz to 1 Hz frequency band which will enable the study of a vast number of objects ranging from Galactic binaries and stellar mass black holes in the Milky Way, to distant massive black-hole mergers and the expansion of the Universe. This definition study report, or Red Book, presents a summary of the very large body of work that has been undertaken on the LISA mission over the LISA definition phase.
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