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@ARTICLE{Afshordi:599177,
author = {Afshordi, Niaesh and Akçay, Sarp and Seoane, Pau Amaro and
Antonelli, Andrea and Aurrekoetxea, Josu C. and Barack, Leor
and Barausse, Enrico and Benkel, Robert and Bernard, Laura
and Bernuzzi, Sebastiano and Berti, Emanuele and Bonetti,
Matteo and Bonga, Béatrice and Bozzola, Gabriele and Brito,
Richard and Buonanno, Alessandra and Cárdenas-Avendaño,
Alejandro and Casals, Marc and Chernoff, David F. and Chua,
Alvin J. K. and Clough, Katy and Colleoni, Marta and Dhesi,
Mekhi and Druart, Adrien and Durkan, Leanne and Faye,
Guillaume and Ferguson, Deborah and Field, Scott E. and
Gabella, William E. and García-Bellido, Juan and
Gracia-Linares, Miguel and Gerosa, Davide and Green, Stephen
R. and Haney, Maria and Hannam, Mark and Heffernan, Anna and
Hinderer, Tanja and Helfer, Thomas and Hughes, Scott A. and
Husa, Sascha and Isoyama, Soichiro and Katz, Michael L. and
Kavanagh, Chris and Khanna, Gaurav and Kidder, Larry E. and
Korol, Valeriya and Küchler, Lorenzo and Laguna, Pablo and
Larrouturou, François and Le Tiec, Alexandre and Leather,
Benjamin and Lim, Eugene A. and Lim, Hyun and Littenberg,
Tyson B. and Long, Oliver and Lousto, Carlos O. and
Lovelace, Geoffrey and Lukes-Gerakopoulos, Georgios and
Lynch, Philip and Macedo, Rodrigo P. and Markakis,
Charalampos and Maggio, Elisa and Mandel, Ilya and Maselli,
Andrea and Mathews, Josh and Mourier, Pierre and Neilsen,
David and Nagar, Alessandro and Nichols, David A. and
Novák, Jan and Okounkova, Maria and O'Shaughnessy, Richard
and Oshita, Naritaka and O'Toole, Conor and Pan, Zhen and
Pani, Paolo and Pappas, George and Paschalidis, Vasileios
and Pfeiffer, Harald P. and Pompili, Lorenzo and Pound, Adam
and Pratten, Geraint and Rüter, Hannes R. and Ruiz, Milton
and Sam, Zeyd and Sberna, Laura and Shapiro, Stuart L. and
Shoemaker, Deirdre M. and Sopuerta, Carlos F. and Spiers,
Andrew and Sundar, Hari and Tamanini, Nicola and Thompson,
Jonathan E. and Toubiana, Alexandre and Tsokaros, Antonios
and Upton, Samuel D. and van de Meent, Maarten and Vernieri,
Daniele and Wachter, Jeremy M. and Warburton, Niels and
Wardell, Barry and Witek, Helvi and Witzany, Vojtˇech and
Yang, Huan and Zilhão, Miguel and Arun, K. G. and Bezares,
Miguel and Bonilla, Alexander and Chapman-Bird, Christian
and Compère, Geoffrey and Cownden, Bradley and Cunningham,
Kevin and Devitt, Chris and Dolan, Sam and Duque, Francisco
and Dyson, Conor and Fryer, Chris L. and Gair, Jonathan R.
and Giacomazzo, Bruno and Gupta, Priti and Han, Wen-Biao and
Haas, Roland and Hirschmann, Eric W. and Huerta, E. A. and
Jetzer, Philippe and Kelly, Bernard and Khalil, Mohammed and
Lloyd-Ronning, Nicole and Marsat, Sylvain and Nardini,
Germano and Neef, Jakob and Ottewill, Adrian and Pantelidou,
Christiana and Piovano, Gabriel Andres and Redondo-Yuste,
Jaime and Sagunski, Laura and Stein, Leo C. and Skoupý,
Viktor and Sperhake, Ulrich and Speri, Lorenzo and Spieksma,
Thomas F. M. and Stevens, Chris and Trestini, David and
Vañó-Viñuales, Alex},
collaboration = {LISA Consortium {Waveform Collaboration}},
title = {{W}aveform {M}odelling for the {L}aser {I}nterferometer
{S}pace {A}ntenna},
reportid = {PUBDB-2023-07201, arXiv:2311.01300},
year = {2023},
note = {237 pages, 11 figures, white paper from the LISA Consortium
Waveform Working Group, invited for submission to Living
Reviews in Relativity},
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: from millions of ultra-compact binaries in our
Galaxy, to mergers of massive black holes at cosmological
distances; from the beginnings of inspirals that will
venture into the ground-based detectors' view to the death
spiral of compact objects into massive black holes, and many
sources in between. Central to realising LISA's discovery
potential are waveform models, the theoretical and
phenomenological predictions of the pattern of gravitational
waves that these sources emit. This white paper is presented
on behalf of the Waveform Working Group for the LISA
Consortium. It provides a review of the current state of
waveform models for LISA sources, and describes the
significant challenges that must yet be overcome.},
keywords = {LISA (INSPIRE) / gravitational radiation: frequency
(INSPIRE) / black hole: binary: coalescence (INSPIRE) /
gravitational radiation detector (INSPIRE) / binary: compact
(INSPIRE) / capture (INSPIRE) / galaxy (INSPIRE) / wave
function (INSPIRE) / black hole: mass (INSPIRE)},
cin = {$Z_THAT$},
cid = {$I:(DE-H253)Z_THAT-20210408$},
pnm = {613 - Matter and Radiation from the Universe (POF4-613)},
pid = {G:(DE-HGF)POF4-613},
experiment = {EXP:(DE-MLZ)NOSPEC-20140101},
typ = {PUB:(DE-HGF)25},
eprint = {2311.01300},
howpublished = {arXiv:2311.01300},
archivePrefix = {arXiv},
SLACcitation = {$\%\%CITATION$ = $arXiv:2311.01300;\%\%$},
doi = {10.3204/PUBDB-2023-07201},
url = {https://bib-pubdb1.desy.de/record/599177},
}
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