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CERN Accelerating science

Article
Report number arXiv:2001.09793
Title Prospects for Fundamental Physics with LISA
Author(s)

Barausse, Enrico (INFN, Trieste ; SISSA, Trieste ; Trieste U. ; Paris, Inst. Astrophys.) ; Berti, Emanuele (Johns Hopkins U.) ; Hertog, Thomas (Leuven U.) ; Hughes, Scott A. (MIT ; MIT, MKI) ; Jetzer, Philippe (Zurich U.) ; Pani, Paolo (INFN, Rome ; Rome U.) ; Sotiriou, Thomas P. (Nottingham U.) ; Tamanini, Nicola (Potsdam, Max Planck Inst.) ; Witek, Helvi (King's Coll. London ; Illinois U., Urbana) ; Yagi, Kent (Virginia U.) ; Yunes, Nicolás (Montana State U. ; Illinois U., Urbana (main)) ; Abdelsalhin, T. (INFN, Rome ; Rome U.) ; Achucarro, A. (Leiden U.) ; Aelst, K.V. (LUTH, Meudon) ; Afshordi, N. (Perimeter Inst. Theor. Phys.) ; Akcay, S. (Jena U.) ; Annulli, L. (Lisbon, CENTRA) ; Arun, K.G. (Chennai Math. Inst.) ; Ayuso, I. (LUTH, Meudon) ; Baibhav, V. (Johns Hopkins U.) ; Baker, T. (Queen Mary, U. of London) ; Bantilan, H. (Queen Mary, U. of London) ; Barreiro, T. (Lisbon U.) ; Barrera-Hinojosa, C. (Durham U.) ; Bartolo, N. (Swansea U.) ; Baumann, D. (Unlisted, NL) ; Belgacem, E. (Geneva U., CAP ; Geneva U., Dept. Theor. Phys.) ; Bellini, E. (JAI, UK) ; Bellomo, N. (ICC, Barcelona U.) ; Ben-Dayan, I. (Judea and Samaria Coll.) ; Bena, I. (IPhT, Saclay) ; Benkel, R. (APC, Paris) ; Bergshoefs, E. (Nikhef, Amsterdam) ; Bernard, L. (LUTH, Meudon) ; Bernuzzi, S. (Jena U.) ; Bertacca, D. (Swansea U.) ; Besancon, M. (IRFU, Saclay) ; Beutler, F. (Portsmouth U.) ; Beyer, F. (Otago U.) ; Bhagwat, S. (INFN, Rome ; Rome U.) ; Bicak, J. (Prague, Tech. U.) ; Biondini, S. (CERN ; U. Groningen, VSI) ; Bize, S. (SYRTE, Paris) ; Blas, D. (King's Coll. London) ; Boehmer, C. (University Coll. London) ; Boller, K. (Groningen, KVI) ; Bonga, B. (Perimeter Inst. Theor. Phys.) ; Bonvin, C. (Geneva U., CAP ; Geneva U., Dept. Theor. Phys.) ; Bosso, P. (Kuwait U.) ; Bozzola, G. (Arizona U.) ; Brax, P. (IPhT, Saclay) ; Breitbach, M. (Mainz U., Inst. Phys.) ; Brito, R. (INFN, Rome ; Rome U.) ; Bruni, M. (Portsmouth U.) ; Brügmann, B. (Jena U.) ; Bulten, H. (Nikhef, Amsterdam) ; Buonanno, A. (APC, Paris) ; Burke, A.O. (Edinburgh U.) ; Burko, L.M. (Moscow, Gravity Res. Group) ; Burrage, C. (Nottingham U.) ; Cabral, F. (Lisbon U.) ; Calcagni, G. (Madrid, Inst. Estructura Materia) ; Caprini, C. (APC, Paris) ; Cárdenas-Avendaño, A. (Illinois U., Urbana) ; Celoria, M. (INFM, L'Aquila) ; Chatziioannou, K. (CCA, New York) ; Chernoff, D. (Cornell U., Phys. Dept.) ; Clough, K. (JAI, UK) ; Coates, A. (Tubingen U.) ; Comelli, D. (INFM, L'Aquila) ; Compère, G. (Brussels U.) ; Croon, D. (TRIUMF) ; Cruces, D. (ICC, Barcelona U.) ; Cusin, G. (JAI, UK) ; Dalang, C. (Geneva U., CAP ; Geneva U., Dept. Theor. Phys.) ; Danielsson, U. (Uppsala U. (main)) ; Das, S. (Kuwait U.) ; Datta, S. (IUCAA, Pune) ; de Boer, J. (Amsterdam U.) ; De Luca, V. (Geneva U., CAP ; Geneva U., Dept. Theor. Phys.) ; De Rham, C. (Imperial Coll., London) ; Desjacques, V. (Technion) ; Destounis, K. (Lisbon, CFP) ; Di Filippo, F. (SISSA, Trieste) ; Dima, A. (SISSA, Trieste) ; Dimastrogiovanni, E. (Case Western Reserve U.) ; Dolan, S. (Sheffield U.) ; Doneva, D. (Tubingen U.) ; Duque, F. (Lisbon, CFP) ; Durrer, R. (Geneva U., CAP ; Geneva U., Dept. Theor. Phys.) ; East, W. (Perimeter Inst. Theor. Phys.) ; Easther, R. (Auckland U.) ; Elley, M. (King's Coll. London) ; Ellis, J.R. (King's Coll. London) ; Emparan, R. (ICC, Barcelona U.) ; Ezquiaga, J.M. (Chicago U., KICP) ; Fairbairn, M. (King's Coll. London) ; Fairhurst, S. (Cardiff U.) ; Farmer, H.F. ; Fasiello, M.R. (Portsmouth U., ICG) ; Ferrari, V. (INFN, Rome ; Rome U.) ; Ferreira, P.G. (JAI, UK) ; Ficarra, G. (King's Coll. London) ; Figueras, P. (Queen Mary, U. of London) ; Fisenko, S. (Unlisted, RU) ; Foffa, S. (Geneva U., CAP ; Geneva U., Dept. Theor. Phys.) ; Franchini, N. (SISSA, Trieste) ; Franciolini, G. (Geneva U., CAP ; Geneva U., Dept. Theor. Phys.) ; Fransen, K. (Leuven U.) ; Frauendiener, J. (Otago U.) ; Frusciante, N. (Lisbon U.) ; Fujita, R. (Kyoto U., Yukawa Inst., Kyoto) ; Gair, J. (Edinburgh U.) ; Ganz, A. (Swansea U.) ; Garcia, P. (LUTH, Meudon) ; Garcia-Bellido, J. (Madrid, IFT) ; Garriga, J. (ICC, Barcelona U.) ; Geiger, R. (SYRTE, Paris) ; Geng, C. (Taiwan, Natl. Tsing Hua U.) ; Gergely, L.Á. (Szeged U.) ; Germani, C. (ICC, Barcelona U.) ; Gerosa, D. (Birmingham U.) ; Giddings, S.B. (UC, Santa Barbara) ; Gourgoulhon, E. (LUTH, Meudon) ; Grandclement, P. (LUTH, Meudon) ; Graziani, L. (INFN, Rome ; Rome U.) ; Gualtieri, L. (INFN, Rome ; Rome U.) ; Haggard, D. (McGill U.) ; Haino, S. (RCAS, Taipei) ; Halburd, R. (University Coll. London) ; Han, W.-B. (Shanghai, Astron. Observ.) ; Hawken, A.J. (Marseille, CPPM) ; Hees, A. (SYRTE, Paris) ; Heng, I.S. (Glasgow U.) ; Hennig, J. (Otago U.) ; Herdeiro, C. (Aveiro U.) ; Hervik, S. (Stavanger U.) ; Holten, J.v. (Nikhef, Amsterdam) ; Hoyle, C.J.D. (Ohio State U.) ; Hu, Y. (University Coll. London) ; Hull, M. (Portsmouth U.) ; Ikeda, T. (LUTH, Meudon) ; Isi, M. (MIT, MKI) ; Jenkins, A. (King's Coll. London) ; Julié, F. (Johns Hopkins U.) ; Kajfasz, E. (Marseille, CPPM) ; Kalaghatgi, C. (Cardiff U.) ; Kaloper, N. (UC, Davis) ; Kamionkowski, M. (Johns Hopkins U.) ; Karas, V. (Prague, Tech. U.) ; Kastha, S. (Chennai Math. Inst.) ; Keresztes, Z. (Szeged U.) ; Kidder, L. (Cornell U., Phys. Dept.) ; Kimpson, T. (University Coll. London) ; Klein, A. (Birmingham U.) ; Klioner, S. (Lohrmann Observ.) ; Kokkotas, K. (Tubingen U.) ; Kolesova, H. (Stavanger U.) ; Kolkowitz, S. (Wisconsin U., Madison) ; Kopp, J. (Mainz U., Inst. Phys.) ; Koyama, K. (Portsmouth U.) ; Krishnendu, N.V. (Chennai Math. Inst.) ; Kroon, J.A.V. (Queen Mary, U. of London) ; Kunz, M. (Geneva U., CAP ; Geneva U., Dept. Theor. Phys.) ; Lahav, O. (University Coll. London) ; Landragin, A. (SYRTE, Paris) ; Lang, R.N. (MIT) ; Le Poncin-Lafitte, C. (SYRTE, Paris) ; Lemos, J. (LUTH, Meudon) ; Li, B. (Durham U.) ; Liberati, S. (SISSA, Trieste) ; Liguori, M. (Swansea U.) ; Lin, F. (Taiwan, Natl. Taiwan U.) ; Liu, G. (Taiwan, Natl. Taiwan U.) ; Lobo, F.S.N. (Lisbon U.) ; Loll, R. (Nikhef, Amsterdam) ; Lombriser, L. (Geneva U., CAP ; Geneva U., Dept. Theor. Phys.) ; Lovelace, G. (Cal State, Fullerton) ; Macedo, R.P. (Queen Mary, U. of London) ; Madge, E. (Mainz U., Inst. Phys.) ; Maggio, E. (INFN, Rome ; Rome U.) ; Maggiore, M. (Geneva U., CAP ; Geneva U., Dept. Theor. Phys.) ; Marassi, S. (INFN, Rome ; Rome U.) ; Marcoccia, P. (Stavanger U.) ; Markakis, C. (Queen Mary, U. of London) ; Martens, W. (ESOC, Darmstadt) ; Martinovic, K. (King's Coll. London) ; Martins, C.J.A.P. (Porto U., Astron. Dept.) ; Maselli, A. (INFN, Rome ; Rome U.) ; Mastrogiovanni, S. (APC, Paris) ; Matarrese, S. (Swansea U.) ; Matas, A. (APC, Paris) ; Mavromatos, N.E. (King's Coll. London) ; Mazumdar, A. (U. Groningen, VSI) ; Meerburg, P.D. (CERN ; U. Groningen, VSI) ; Megias, E. (CAFPE, Granada) ; Miller, J. (JAI, UK) ; Mimoso, J.P. (Lisbon U.) ; Mittnacht, L. (Mainz U., Inst. Phys.) ; Montero, M.M. (Brussels U.) ; Moore, B. (Montana State U.) ; Martin-Moruno, P. (Madrid U.) ; Musco, I. (Geneva U., CAP ; Geneva U., Dept. Theor. Phys. ; ICC, Barcelona U.) ; Nakano, H. (LISA) ; Nampalliwar, S. (Tubingen U.) ; Nardini, G. (Stavanger U.) ; Nielsen, A. (Stavanger U.) ; Novák, J. (Liberec Tech. U.) ; Nunes, N.J. (Lisbon U.) ; Okounkova, M. (Caltech, JPL) ; Oliveri, R. (Prague, Tech. U.) ; Oppizzi, F. (Swansea U.) ; Orlando, G. (Swansea U.) ; Oshita, N. (Perimeter Inst. Theor. Phys.) ; Pappas, G. (Aristotle U., Thessaloniki) ; Paschalidis, V. (Arizona U.) ; Peiris, H. (University Coll. London) ; Peloso, M. (Swansea U.) ; Perkins, S. (Illinois U., Urbana) ; Pettorino, V. (IRFU, Saclay) ; Pikovski, I. (Harvard-Smithsonian Ctr. Astrophys.) ; Pilo, L. (INFM, L'Aquila) ; Podolsky, J. (Prague, Tech. U.) ; Pontzen, A. (University Coll. London) ; Prabhat, S. (INFN, Rome ; Rome U.) ; Pratten, G. (Birmingham U.) ; Prokopec, T. (Nikhef, Amsterdam) ; Prouza, M. (Prague, Tech. U.) ; Qi, H. (Cardiff U.) ; Raccanelli, A. (CERN) ; Rajantie, A. (Imperial Coll., London) ; Randall, L. (Harvard U.) ; Raposo, G. (INFN, Rome ; Rome U.) ; Raymond, V. (Cardiff U.) ; Renaux-Petel, S. (Paris, Inst. Astrophys.) ; Ricciardone, A. (INFN, Padua) ; Riotto, A. (Geneva U., CAP ; Geneva U., Dept. Theor. Phys.) ; Robson, T. (Montana State U.) ; Roest, D. (CERN ; U. Groningen, VSI) ; Rollo, R. (INFM, L'Aquila) ; Rosofsky, S. (NCSA, Urbana) ; Ruan, J.J. (McGill U.) ; Rubiera-García, D. (Lisbon U. ; Madrid U.) ; Ruiz, M. (Illinois U., Urbana) ; Rusu, M. (Bucharest, Inst. Space Science) ; Sabatie, F. (IRFU, Saclay) ; Sago, N. (LISA) ; Sakellariadou, M. (King's Coll. London) ; Saltas, I.D. (Prague, Tech. U.) ; Sberna, L. (Perimeter Inst. Theor. Phys.) ; Sathyaprakash, B. (Cardiff U.) ; Scheel, M. (Caltech, JPL) ; Schmidt, P. (Birmingham U.) ; Schutz, B. (APC, Paris) ; Schwaller, P. (Mainz U., Inst. Phys.) ; Shao, L. (Peking U., Beijing, KIAA) ; Shapiro, S.L. (Illinois U., Urbana) ; Shoemaker, D. (Georgia Tech) ; Silva, A.d. (Lisbon U.) ; Simpson, C. (Edinburgh U.) ; Sopuerta, C.F. (Barcelona, IEEC ; ICE, Bellaterra) ; Spallicci, A. (LPC2E, Orleans) ; Stefanek, B.A. (Mainz U., Inst. Phys.) ; Stein, L. (Caltech, JPL) ; Stergioulas, N. (Aristotle U., Thessaloniki) ; Stott, M. (King's Coll. London) ; Sutton, P. (Cardiff U.) ; Svarc, R. (Prague, Tech. U.) ; Tagoshi, H. (Tokyo U., ICRR) ; Tahamtan, T. (Prague, Tech. U.) ; Takeda, H. (Wako, RIKEN) ; Tanaka, T. (Kyoto U.) ; Tantilian, G. (Aristotle U., Thessaloniki) ; Tasinato, G. (Swansea U.) ; Tattersall, O. (JAI, UK) ; Teukolsky, S. (Cornell U., Phys. Dept.) ; Tiec, A.L. (LUTH, Meudon) ; Theureau, G. (LPC2E, Orleans) ; Trodden, M. (Pennsylvania U.) ; Tolley, A. (Imperial Coll., London) ; Toubiana, A. (Paris, Inst. Astrophys. ; APC, Paris) ; Traykova, D. (JAI, UK) ; Tsokaros, A. (Illinois U., Urbana) ; Unal, C. (Minnesota U.) ; Unnikrishnan, C.S. (Tata Inst.) ; Vagenas, E.C. (Kuwait U.) ; Valageas, P. (IPhT, Saclay) ; Vallisneri, M. (Caltech, JPL) ; Van den Brand, J. (Nikhef, Amsterdam) ; Van den Broeck, C. (Nikhef, Amsterdam) ; van de Meent, M. (Potsdam, Max Planck Inst.) ; Vanhove, P. (IPhT, Saclay) ; Varma, V. (Caltech, JPL) ; Veitch, J. (Glasgow U.) ; Vercnocke, B. (Brussels U.) ; Verde, L. (ICC, Barcelona U.) ; Vernieri, D. (Lisbon U.) ; Vernizzi, F. (IPhT, Saclay) ; Vicente, R. (LUTH, Meudon) ; Vidotto, F. (Western Ontario U.) ; Visser, M. (Victoria U., Wellington) ; Vlah, Z. (Swansea U.) ; Vretinaris, S. (Aristotle U., Thessaloniki) ; Völkel, S. (Tubingen U. ; SISSA, Trieste) ; Wang, Q. (Perimeter Inst. Theor. Phys.) ; Wang, Yu-Tong (UCAS, KLVP, Beijing) ; Werner, M.C. (Kyoto U. (main)) ; Westernacher, J. (Arizona U.) ; Weygaert, R.v.d. (CERN ; U. Groningen, VSI) ; Wiltshire, D. (Canterbury U.) ; Wiseman, T. (Imperial Coll., London) ; Wolf, P. (SYRTE, Paris) ; Wu, K. (University Coll. London) ; Yamada, K. (Kyoto U.) ; Yang, H. (Perimeter Inst. Theor. Phys.) ; Yi, L. (Caltech, JPL) ; Yue, X. (Shanghai, Astron. Observ.) ; Yvon, D. (IRFU, Saclay) ; Zilhão, M. (LUTH, Meudon) ; Zimmerman, A. (Texas U.) ; Zumalacarregui, M. (Brobeck Assoc. ; IPhT, Saclay)

Publication 2020-08-31
Imprint 2020-01-27
Number of pages 22
Note 22 pages, 1 figure, to appear in General Relativity and Gravitation
In: Gen. Relativ. Gravit. 52 (2020) pp.8
DOI 10.1007/s10714-020-02691-1 (publication)
10.1007/s10714-020-02691-1. (publication)
Subject category gr-qc ; General Relativity and Cosmology
Accelerator/Facility, Experiment LISA
Abstract In this paper, which is of programmatic rather than quantitative nature, we aim to further delineate and sharpen the future potential of the LISA mission in the area of fundamental physics. Given the very broad range of topics that might be relevant to LISA, we present here a sample of what we view as particularly promising directions, based in part on the current research interests of the LISA scientific community in the area of fundamental physics. We organize these directions through a "science-first" approach that allows us to classify how LISA data can inform theoretical physics in a variety of areas. For each of these theoretical physics classes, we identify the sources that are currently expected to provide the principal contribution to our knowledge, and the areas that need further development. The classification presented here should not be thought of as cast in stone, but rather as a fluid framework that is amenable to change with the flow of new insights in theoretical physics.
Copyright/License publication: © Springer Science+Business Media, LLC, part of Springer Nature 2020
preprint: (License: arXiv nonexclusive-distrib 1.0)



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 Record created 2020-02-01, last modified 2024-11-13


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