TY - INPR A1 - Afshordi, Niayesh A1 - Akçay, Sarp A1 - Amaro-Seoane, Pau A1 - Antonelli, Andrea A1 - Aurrekoetxea, Josu C. A1 - Barack, Leor A1 - Barausse, Enrico A1 - Benkel, Robert A1 - Bernard, Laura A1 - Bernuzzi, Sebastiano A1 - Berti, Emanuele A1 - Bonetti, Matteo A1 - Bonga, Béatrice A1 - Bozzola, Gabriele A1 - Brito, Richard A1 - Buonanno, Alessandra A1 - Cárdenas-Avendaño, Alejandro A1 - Casals, Marc A1 - Chernoff, David F. A1 - Chua, Alvin J. K. A1 - Clough, Katy A1 - Colleoni, Marta A1 - Dhesi, Mekhi A1 - Druart, Adrien A1 - Durkan, Leanne A1 - Faye, Guillaume A1 - Ferguson, Deborah A1 - Field, Scott E. A1 - Gabella, William E. A1 - García-Bellido, Juan A1 - Gracia-Linares, Miguel A1 - Gerosa, Davide A1 - Green, Stephen R. A1 - Haney, Maria A1 - Hannam, Mark A1 - Heffernan, Anna A1 - Hinderer, Tanja A1 - Helfer, Thomas A1 - Hughes, Scott A. A1 - Husa, Sascha A1 - Isoyama, Soichiro A1 - Katz, Michael L. A1 - Kavanagh, Chris A1 - Khanna, Gaurav A1 - Kidder, Larry E. A1 - Korol, Valeriya A1 - Küchler, Lorenzo A1 - Laguna, Pablo A1 - Larrouturou, François A1 - Le Tiec, Alexandre A1 - Leather, Benjamin A1 - Lim, Eugene A. A1 - Lim, Hyun A1 - Littenberg, Tyson B. A1 - Long, Oliver A1 - Lousto, Carlos O. A1 - Lovelace, Geoffrey A1 - Lukes-Gerakopoulos, Georgios A1 - Lynch, Philip A1 - Macedo, Rodrigo P. A1 - Markakis, Charalampos A1 - Maggio, Elisa A1 - Mandel, Ilya A1 - Maselli, Andrea A1 - Mathews, Josh A1 - Mourier, Pierre A1 - Neilsen, David A1 - Nagar, Alessandro A1 - Nichols, David A. A1 - Novák, Jan A1 - Okounkova, Maria A1 - O’Shaughnessy, Richard A1 - Oshita, Naritaka A1 - O’Toole, Conor A1 - Pan, Zhen A1 - Pani, Paolo A1 - Pappas, George A1 - Paschalidis, Vasileios A1 - Pfeiffer, Harald P. A1 - Pompili, Lorenzo A1 - Pound, Adam A1 - Pratten, Geraint A1 - Rüter, Hannes A1 - Ruiz, Milton A1 - Sam, Zeyd A1 - Sberna, Laura A1 - Shapiro, Stuart L. A1 - Shoemaker, Deirdre M. A1 - Sopuerta, Carlos F. A1 - Spiers, Andrew A1 - Sundar, Hari A1 - Tamanini, Nicola A1 - Thompson, Jonathan E. A1 - Toubiana, Alexandre A1 - Tsokaros, Antonios A1 - Upton, Samuel D. A1 - Meent, Maarten van de A1 - Vernieri, Daniele A1 - Wachter, Jeremy M. A1 - Warburton, Niels A1 - Wardell, Barry A1 - Witek, Helvi A1 - Witzany, Vojtěch A1 - Yang, Huan A1 - Zilhão, Miguel A1 - Albertini, Angelica A1 - Arun, K. G. A1 - Bezares, Miguel A1 - Bonilla, Alexander Rivera A1 - Chapman-Bird, Christian A1 - Cownden, Bradley A1 - Cunningham, Kevin A1 - Devitt, Chris A1 - Dolan, Sam A1 - Duque, Francisco A1 - Dyson, Conor A1 - Fryer, Chris L. A1 - Gair, Jonathan R. A1 - Giacomazzo, Bruno A1 - Gupta, Priti A1 - Han, Wen-Biao A1 - Haas, Roland A1 - Hirschmann, Eric A1 - Huerta, Eliu A. A1 - Jetzer, Philippe A1 - Kelly, Bernard A1 - Khalil, Mohammed A1 - Lewis, Jack A1 - Lloyd-Ronning, Nicole Marie A1 - Marsat, Sylvain A1 - Nardini, Germano A1 - Neef, Jakob A1 - Ottewill, Adrian A1 - Pantelidou, Christiana A1 - Piovano, Gabriel Andres A1 - Redondo-Yuste, Jaime A1 - Sagunski, Laura A1 - Stein, Leo C. A1 - Skoupý, Viktor A1 - Sperhake, Ulrich A1 - Speri, Lorenzo A1 - Spieksma, Thomas F. M. A1 - Stevens, Chris A1 - Trestini, David A1 - Vañó-Viñuales, Alex T1 - Waveform Modelling for the Laser Interferometer Space Antenna T2 - arXiv N2 - 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. Y1 - 2023 UR - http://publikationen.ub.uni-frankfurt.de/frontdoor/index/index/docId/86869 UR - https://nbn-resolving.org/urn:nbn:de:hebis:30:3-868690 UR - https://arxiv.org/abs/2311.01300v2 IS - 2311.01300v2 PB - arXiv ER -