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Prospects for fundamental physics with LISA

  • Invited Report: Introduction to Current Research
  • Published:
General Relativity and Gravitation Aims and scope Submit manuscript

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 fundamental physics directions. 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.

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Notes

  1. Theories with auxiliary fields manage to circumvent Lovelock theorem without introducing new dynamical degrees of freedom, but they have serious shortcomings [26,27,28,29].

  2. The term charge is used here loosely, to refer to a non-trivial configuration of some new field, as has become customary in the relevant literature.

  3. Technically speaking, the non-minimal coupling in the action is through the product of a pseudoscalar and the Pontryagin density and the action is parity invariant. The solutions exhibit parity violations.

  4. The well-motivated assumption that black holes should be uncharged could also be tested; see [93] for work in this direction.

  5. IMBHBs will also be detected at cosmological distances, but their existence is still debated nowadays and consequently no cosmological applications of this class of sources have ever been considered.

  6. A correction of N post-Newtonian, or NPN, order is one that is of \({{\mathcal {O}}}(v^{2N}/c^{2N})\) relative to the GR leading order term [249].

  7. The original ppE formalism also proposes a similar way to parameterize non-GR modifications in the ringdown phase [246].

  8. A term that scales as \((v/c)^{2N}\) is said to be of N PN order relative to its leading-order controlling factor.

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Acknowledgements

We would like to thank all of the attendees of the first, inaugural meeting of the Fundamental Physics Research Group in Florence for interesting and stimulating discussions and presentations. We would also like to thank the Galileo Galilei Institute for their hospitality during the organization of this meeting. E. Barausse, A. Dima, N. Franchini and S. Völkel acknowledge financial support provided under the European Union’s H2020 ERC Consolidator Grant “GRavity from Astrophysical to Microscopic Scales” Grant agreement No. GRAMS-815673. This work has also been supported by the European Union’s Horizon 2020 research and innovation program under the Marie Sklodowska-Curie Grant agreement No. 690904. The authors would like to acknowledge financial and networking support by the GWverse COST Action CA16104, “Black holes, gravitational waves and fundamental physics”; the European Research Council Starting Grant DarkGRA-757480 (“Unveiling the dark universe with gravitational waves”) and the Flemish Research Council through the Odysseus Grant G.0011.12. H. Witek acknowledges financial support provided by the Royal Society University Research Fellowship UF160547 and the Royal Society Research Grant RGF\(\backslash \)R1\(\backslash \)180073. S.A. Hughes’s work on LISA-related science is supported by NASA Grant No. 80NSSC18K1091. E. Berti is supported by NSF Grants No. PHY-1912550 and AST-1841358, NASA ATP Grants No. 17-ATP17-0225 and 19-ATP19-0051, and NSF-XSEDE Grant No. PHY-090003. N.Yunes acknowledges support from NSF grant PHY-1759615, and NASA Grants 80NSSC18K1352. K. Yagi acknowledges support from NSF Award PHY-1806776, a Sloan Foundation Research Fellowship, and the Ed Owens Fund. T. P. Sotiriou acknowledges partial support from the STFC Consolidated Grant No. ST/P000703/1.

Author information

Authors and Affiliations

  1. SISSA, Via Bonomea 265, 34136, Trieste, Italy

    Enrico Barausse

  2. INFN Sezione di Trieste, IFPU - Institute for Fundamental Physics of the Universe, Via Beirut 2, 34014, Trieste, Italy

    Enrico Barausse

  3. CNRS, UMR 7095, Institut d’Astrophysique de Paris, 98 bis Bd Arago, 75014, Paris, France

    Enrico Barausse

  4. Department of Physics and Astronomy, Johns Hopkins University, 3400 N. Charles Street, Baltimore, MD, 21218, USA

    Emanuele Berti

  5. Institute for Theoretical Physics, KU Leuven, Celestijnenlaan 200D, 3001, Leuven, Belgium

    Thomas Hertog

  6. Department of Physics, Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology, Cambridge, MA, 02139, USA

    Scott A. Hughes

  7. Physik-Institut, Universität Zürich, Winterthurerstrasse 190, 8057, Zurich, Switzerland

    Philippe Jetzer

  8. Dipartimento di Fisica, “Sapienza” Università di Roma and Sezione INFN Roma1, Piazzale Aldo Moro 5, 00185, Rome, Italy

    Paolo Pani

  9. School of Mathematical Sciences, School of Physics and Astronomy, University of Nottingham, University Park, Nottingham, NG7 2RD, UK

    Thomas P. Sotiriou

  10. Max-Planck-Institut für Gravitationsphysik, Albert-Einstein-Institut, Am Mühlenberg 1, 14476, Potsdam, Golm, Germany

    Nicola Tamanini

  11. Department of Physics, King’s College London, The Strand, London, WC2R 2LS, UK

    Helvi Witek

  12. Department of Physics, University of Illinois at Urbana-Champaign, Urbana, IL, 61801, USA

    Helvi Witek

  13. Department of Physics, University of Virginia, Charlottesville, VA, 22904, USA

    Kent Yagi

  14. Department of Physics, eXtreme Gravity Institute, Montana State University, Bozeman, MT, 59717, USA

    Nicolás Yunes

  15. University of Illinois at Urbana-Champaign, Urbana, IL, 61801, USA

    Nicolás Yunes

  16. Dipartimento di Fisica, “Sapienza” Università di Roma & Sezione INFN Roma1, Piazzale Aldo Moro 5, 00185, Roma, Italy

    T. Abdelsalhin, S. Bhagwat, R. Brito, V. Ferrari, L. Graziani, L. Gualtieri, E. Maggio, S. Marassi, A. Maselli, S. Prabhat & G. Raposo

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  24. Queen Mary University of London, London, UK

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  33. Department of Physics, Ariel University, Ariel, 40700, Israel

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  34. Institut de physique théorique, Université Paris Saclay, CEA, CNRS, 91191, Gif-sur-Yvette, France

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  39. Institute of Cosmology and Gravitation, University of Portsmouth, Burnaby Road, Portsmouth, PO1 3FX, UK

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  40. Department of Mathematics and Statistics, University of Otago, Dunedin, 9016, New Zealand

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  41. CEICO - Czech Academy of Sciences, Prague, Czechia

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    S. Biondini, P. D. Meerburg, D. Roest & R. v. d. Weygaert

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  45. Department of Mathematics, University College London, Gower Street, London, WC1E 6BT, UK

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  46. LISA NL Group, University of Twente, 7500, AE Enschede, The Netherlands

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  47. Theoretical Physics Group and Quantum Alberta, Department of Physics and Astronomy, University of Lethbridge, 4401 University Drive, Lethbridge, Alberta, T1K 3M4, Canada

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  48. Departments of Astronomy and Physics, University of Arizona, Tucson, Arizona, 85721, USA

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  50. LISA NL Group, Nikhef, The Netherlands

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  51. University of Edinburgh, Edinburgh, UK

    J. Gair & C. Simpson

  52. GGC Gravity Group, Georgia Gwinnett College, Lawrenceville, GA 30043, USA

    L. M. Burko

  53. Instituto de Estructura de la Materia - CSIC, Madrid, Spain

    G. Calcagni

  54. Institute for Theoretical Physics, University of Amsterdam, PO Box 94485, 1090GL, Amsterdam, The Netherlands

    J. de Boer

  55. INFN, Ferrara, Italy

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  56. Department of Physics, University of Illinois at Urbana-Champaign, Urbana, IL, 61820, USA

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  57. Jet Propulsion Laboratory, Caltech, USA

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  58. Cornell University, Ithaca, NY, USA

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  59. Theoretical Astrophysics, IAAT, University of Tübingen, 72076, Tübingen, Germany

    A. Coates, D. Doneva, K. Kokkotas & S. Völkel

  60. Université Libre de Bruxelles, CP 231, B-1050, Brussels, Belgium

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  61. Uppsala University, Uppsala, Sweden

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  62. Imperial College London, London, UK

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  63. Instituto Superior Tecnico, Lisboa, Portugal

    K. Destounis & F. Duque

  64. Case Western Reserve University, Cleveland, USA

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  65. University of Sheffield, Sheffield, UK

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  66. NZ Astrostatistics and GR, University of Auckland, Auckland, New Zealand

    R. Easther

  67. Cardiff University Gravity Exploration Institute, Cardiff, UK

    S. Fairhurst, C. Kalaghatgi, H. Qi, V. Raymond, B. Sathyaprakash, B. Schutz & P. Sutton

  68. Wilbur Wright College, Chicago, USA

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  69. Institute of Cosmology and Gravitation, University of Portsmouth, Portsmouth, UK

    M. R. Fasiello

  70. MSLU, Moscow, Russia

    S. Fisenko

  71. Japanese working group for LISA science, YITP, Kyoto University, Kyoto, Japan

    R. Fujita

  72. Taiwan Consortium for Gravitational Wave Research, National Tsing Hua University, Hsinchu City , Taiwan

    C. Geng

  73. Szeged Gravity Group, University of Szeged, Szeged, Hungary

    L. Á. Gergely & Z. Keresztes

  74. School of Physics and Astronomy and Institute for Gravitational Wave Astronomy, University of Birmingham, Birmingham, B15 2TT, UK

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  75. Haggard Research Group at McGill University, Montreal, Canada

    D. Haggard & J. J. Ruan

  76. Taiwan Consortium for Gravitational Wave Research, Academia Sinica, Taipei, Taiwan

    S. Haino

  77. Shanghai Astronomical Observatory, CAS, Shanghai, China

    W.-B. Han & X. Yue

  78. Aix Marseille Univ, CNRS/IN2P3, CPPM, Marseille, France

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  79. Glasgow LISA Science, University of Glasgow, Glasgow, UK

    I. S. Heng & J. Veitch

  80. University of Stavanger, Stavanger, Norway

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  81. Humboldt State University Gravitational Research Laboratory, Arcata, CA, USA

    C. J. D. Hoyle

  82. LIGO Laboratory, Massachusetts Institute of Technology, Cambridge, Massachusetts, 02139, USA

    M. Isi

  83. CENTRA, Departamento de Fisica, Instituto Superior Técnico - IST, Universidade de Lisboa - UL, Avenida Rovisco Pais 1, 1049-001, Lisboa, Portugal

    L. Annulli

  84. University of California, Davis, USA

    N. Kaloper

  85. Cornell University, Ithaca, USA

    L. Kidder & S. Teukolsky

  86. Lohrmann Observatory, Technische Universität Dresden, Dresden, Germany

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  87. University of Wisconsin, Madison, USA

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  88. Massachusetts Institute of Technology, Cambridge, USA

    R. N. Lang

  89. Taiwan Consortium for Gravitational Wave Research, National Taiwan Normal University, Taipei, Taiwan

    F. Lin

  90. Taiwan Consortium for Gravitational Wave Research, Tamkang University, New Taipei City, Taiwan

    G. Liu

  91. CSU Fullerton Gravitational-Wave Physics and Astronomy Center, Fullerton, USA

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  92. University of Granad, Granada, Spain

    E. Megias

  93. eXtreme Gravity Institute, Montana State University, Bozeman, USA

    B. Moore & T. Robson

  94. Complutense University of Madrid & IPARCOS, Madrid, Spain

    P. Martin-Moruno & D. Rubiera-García

  95. Japanese working group for LISA science, Ryukoku University, Kyoto, Japan

    H. Nakano

  96. Technical University of Liberec, Liberec, Czech Republic

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  97. Department of Physics, Aristotle University of Thessaloniki, Thessaloniki, Greece

    G. Pappas, N. Stergioulas, G. Tantilian & S. Vretinaris

  98. CAUP and IA-Porto, Porto, Portugal

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  125. Kavli Institute for Cosmological Physics, The University of Chicago, Chicago, USA

    J. M. Ezquiaga

  126. ESOC - European Space Operations Centre, D-64293, Darmstadt, Germany

    W. Martens

  127. Max Planck Institute for Gravitational Physics, Potsdam, Germany

    A. Buonanno & M. van de Meent

  128. SISSA, International School for Advanced Studies, Via Bonomea 265, 34136, Trieste, Italy

    F. Di Filippo, A. Dima, N. Franchini, S. Liberati & S. Völkel

  129. Laboratoire Astroparticule et Cosmologie, CNRS, Université Paris Diderot, 75013, Paris, France

    S. Mastrogiovanni

  130. CIDMA and Aveiro University, Aveiro, Portugal

    C. Herdeiro

  131. Victoria University of Wellington, Wellington, New Zealand

    M. Visser

  132. Physics Department, Technion, 3200003, Haifa, Israel

    V. Desjacques

  133. Center for Computational Astrophysics, Flatiron Institute, 162 5th Ave, New York, NY, 10010, USA

    K. Chatziioannou

  134. Department of Physics, University of California, Santa Barbara, CA, 93106, USA

    S. B. Giddings

  135. Institute for Theoretical Physics, KU Leuven, Celestijnenlaan 200D, B-3001, Leuven, Belgium

    K. Fransen

  136. School of Physics and Astronomy, University of Nottingham, Nottingham, NG7 2RD, UK

    C. Burrage

  137. Theoretical Physics Department, CERN, 1 Esplanade des Particules, CH-1211, Geneva 23, Switzerland

    A. Raccanelli

  138. INFN, Sezione di Padova, via Marzolo 8, I-35131, Padova, Italy

    A. Ricciardone

  139. Department of Applied Mathematics, The University of Western Ontario, N6A 5B7, Ontario, Canada

    A. Raccanelli & F. Vidotto

  140. Swansea University, Swansea, UK

    G. Tasinato

  141. Theoretical Physics Group, Department of Physics, Kuwait University, P.O. Box 5969, Safat, 13060, Kuwait

    E. C. Vagenas

  142. Departamento de Física and Instituto de Astrofísica e Ciências do Espaço, Faculdade de Ciências, Universidade de Lisboa, Edifício C8, Campo Grande, 1749-016, Lisbon, Portugal

    I. Ayuso

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Correspondence to Philippe Jetzer.

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Barausse, E., Berti, E., Hertog, T. et al. Prospects for fundamental physics with LISA. Gen Relativ Gravit 52, 81 (2020). https://doi.org/10.1007/s10714-020-02691-1

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