pith. sign in

arxiv: 2001.09793 · v3 · pith:Z4QQSEFVnew · submitted 2020-01-27 · 🌀 gr-qc

Prospects for Fundamental Physics with LISA

Enrico Barausse , Emanuele Berti , Thomas Hertog , Scott A. Hughes , Philippe Jetzer , Paolo Pani , Thomas P. Sotiriou , Nicola Tamanini
show 313 more authors
Helvi Witek Kent Yagi Nicolas Yunes T. Abdelsalhin A. Achucarro K. V. Aelst N. Afshordi S. Akcay L. Annulli K. G. Arun I. Ayuso V. Baibhav T. Baker H. Bantilan T. Barreiro C. Barrera-Hinojosa N. Bartolo D. Baumann E. Belgacem E. Bellini N. Bellomo I. Ben-Dayan I. Bena R. Benkel E. Bergshoefs L. Bernard S. Bernuzzi D. Bertacca M. Besancon F. Beutler F. Beyer S. Bhagwat J. Bicak S. Biondini S. Bize D. Blas C. Boehmer K. Boller B. Bonga C. Bonvin P. Bosso G. Bozzola P. Brax M. Breitbach R. Brito M. Bruni B. Br\"ugmann H. Bulten A. Buonanno A. O. Burke L. M. Burko C. Burrage F. Cabral G. Calcagni C. Caprini A. C\'ardenas-Avenda\~no M. Celoria K. Chatziioannou D. Chernoff K. Clough A. Coates D. Comelli G. Comp\`ere D. Croon D. Cruces G. Cusin C. Dalang U. Danielsson S. Das S. Datta J. de Boer V. De Luca C. De Rham V. Desjacques K. Destounis F. Di Filippo A. Dima E. Dimastrogiovanni S. Dolan D. Doneva F. Duque R. Durrer W. East R. Easther M. Elley J. R. Ellis R. Emparan J.M. Ezquiaga M. Fairbairn S. Fairhurst H. F. Farmer M. R. Fasiello V. Ferrari P. G. Ferreira G. Ficarra P. Figueras S. Fisenko S. Foffa N. Franchini G. Franciolini K. Fransen J. Frauendiener N. Frusciante R. Fujita J. Gair A. Ganz P. Garcia J. Garcia-Bellido J. Garriga R. Geiger C. Geng L. \'A. Gergely C. Germani D. Gerosa S.B. Giddings E. Gourgoulhon P. Grandclement L. Graziani L. Gualtieri D. Haggard S. Haino R. Halburd W.-B. Han A. J. Hawken A. Hees I. S. Heng J. Hennig C. Herdeiro S. Hervik J. v. Holten C. J. D. Hoyle Y. Hu M. Hull T. Ikeda M. Isi A. Jenkins F. Juli\'e E. Kajfasz C. Kalaghatgi N. Kaloper M. Kamionkowski V. Karas S. Kastha Z. Keresztes L. Kidder T. Kimpson A. Klein S. Klioner K. Kokkotas H. Kolesova S. Kolkowitz J. Kopp K. Koyama N. V. Krishnendu J. A. V. Kroon M. Kunz O. Lahav A. Landragin R.N. Lang C. Le Poncin-Lafitte J. Lemos B. Li S. Liberati M. Liguori F. Lin G. Liu F.S.N. Lobo R. Loll L. Lombriser G. Lovelace R. P. Macedo E. Madge E. Maggio M. Maggiore S. Marassi P. Marcoccia C. Markakis W. Martens K. Martinovic C.J.A.P. Martins A. Maselli S. Mastrogiovanni S. Matarrese A. Matas N. E. Mavromatos A. Mazumdar P. D. Meerburg E. Megias J. Miller J. P. Mimoso L. Mittnacht M. M. Montero B. Moore P. Martin-Moruno I. Musco H. Nakano S. Nampalliwar G. Nardini A. Nielsen J. Nov\'ak N.J. Nunes M. Okounkova R. Oliveri F. Oppizzi G. Orlando N. Oshita G. Pappas V. Paschalidis H. Peiris M. Peloso S. Perkins V. Pettorino I. Pikovski L. Pilo J. Podolsky A. Pontzen S. Prabhat G. Pratten T. Prokopec M. Prouza H. Qi A. Raccanelli A. Rajantie L. Randall G. Raposo V. Raymond S. Renaux-Petel A. Ricciardone A. Riotto T. Robson D. Roest R. Rollo S. Rosofsky J. J. Ruan D. Rubiera-Garc\'ia M. Ruiz M. Rusu F. Sabatie N. Sago M. Sakellariadou I. D. Saltas L. Sberna B. Sathyaprakash M. Scheel P. Schmidt B. Schutz P. Schwaller L. Shao S. L. Shapiro D. Shoemaker A. d. Silva C. Simpson C. F. Sopuerta A. Spallicci B.A. Stefanek L. Stein N. Stergioulas M. Stott P. Sutton R. Svarc H. Tagoshi T. Tahamtan H. Takeda T. Tanaka G. Tantilian G. Tasinato O. Tattersall S. Teukolsky A. L. Tiec G. Theureau M. Trodden A. Tolley A. Toubiana D. Traykova A. Tsokaros C. Unal C. S. Unnikrishnan E. C. Vagenas P. Valageas M. Vallisneri J. Van den Brand C. Van den Broeck M. van de Meent P. Vanhove V. Varma J. Veitch B. Vercnocke L. Verde D. Vernieri F. Vernizzi R. Vicente F. Vidotto M. Visser Z. Vlah S. Vretinaris S. V\"olkel Q. Wang Yu-Tong Wang M. C. Werner J. Westernacher R. v. d. Weygaert D. Wiltshire T. Wiseman P. Wolf K. Wu K. Yamada H. Yang L. Yi X. Yue D. Yvon M. Zilh\~ao A. Zimmerman M. Zumalacarregui
This is my paper
classification 🌀 gr-qc
keywords physicslisafundamentaltheoreticalareaareasdirectionsfurther
0
0 comments X
read the original 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.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.

Forward citations

Cited by 14 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Detecting Chiral Gravitational Wave Background with a Dipole Pulsar Timing Array

    gr-qc 2026-04 unverdicted novelty 7.0

    A dipole pulsar timing array detects chiral nanohertz gravitational waves and extends PTA sensitivity into the microhertz regime.

  2. Black hole mergers beyond general relativity: a self-force approach

    gr-qc 2025-10 unverdicted novelty 7.0

    Self-force theory is extended to compute merger and ringdown waveforms in beyond-GR black hole binaries under the extreme mass-ratio approximation, with first calculations of self-force corrections to the merger waveform.

  3. Chiral Gravitational Wave Background from Audible Axion via Nieh-Yan Term

    hep-ph 2024-11 unverdicted novelty 7.0

    Axion-like fields coupled to the Nieh-Yan term generate a chiral GW background during radiation domination, with parameter space explored for detectability in PTA and space-based observatories.

  4. Parameter inference of millilensed gravitational waves using neural spline flows

    gr-qc 2025-05 conditional novelty 6.0

    Neural spline flows perform fast posterior inference on 11-dimensional millilensed GW parameters with accuracy comparable to dynesty for most quantities and a 3-day to 0.8-second speedup.

  5. Probing Kerr Symmetry Breaking with LISA Extreme-Mass-Ratio Inspirals

    gr-qc 2026-04 unverdicted novelty 5.0

    LISA EMRIs can constrain deviations from Kerr equatorial symmetry to 10^{-2} and axial symmetry to 10^{-3} using Analytic Kludge waveforms and Fisher analysis.

  6. Are Black Holes Fuzzballs? Probing Horizon-Scale Structure with LISA

    hep-th 2026-04 unverdicted novelty 5.0

    LISA can constrain non-axisymmetric mass quadrupole deformations at the 10^{-3} level and axisymmetric mass octupole deformations at the 10^{-2} level in EMRI signals to test fuzzball proposals.

  7. Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr

    gr-qc 2026-01 unverdicted novelty 5.0

    Numerical simulations benchmark the eikonal and post-Kerr approximations for quasinormal modes in deformed Kerr spacetimes, quantifying their errors relative to expected observational precision.

  8. Leading effective field theory corrections to the Kerr metric at all spins

    gr-qc 2025-12 unverdicted novelty 5.0

    Numerical solutions show that leading effective-field-theory corrections to the Kerr metric grow with spin and are largest near extremality.

  9. A multi-parameter expansion for the evolution of asymmetric binaries in astrophysical environments

    gr-qc 2025-07 unverdicted novelty 5.0

    A multi-parameter formalism is developed to describe asymmetric binaries in general matter distributions by perturbing around Schwarzschild and reducing metric and fluid perturbations to wave equations similar to the ...

  10. Gravitational Waves from Primordial Black Holes: Connecting Low-Frequency Scalar-Induced Signatures to High-Frequency Binary Mergers

    astro-ph.CO 2026-07 unverdicted novelty 4.0

    Establishes a model-independent link between scalar-induced GW backgrounds and PBH binary merger signals, including the mass-independent relation f_peak = 1.79 f_ISCO.

  11. Gravitational Waves from Post-Inflationary Magnetism: Direct and Scalar-Induced Contributions

    astro-ph.CO 2026-05 unverdicted novelty 4.0

    In a post-inflationary magnetogenesis scenario with time-dependent gauge couplings, magnetic anisotropic stress dominates peak GW amplitude while scalar-induced terms matter on larger scales, both showing f^3 infrared...

  12. Statistic threshold of distinguishing the environmental effects and modified theory of gravity with multiple massive black-hole binaries

    gr-qc 2025-06 unverdicted novelty 4.0

    The paper derives statistic thresholds to distinguish dynamical friction from dark matter spikes, extra dimension theory, and varying G theory using -4 PN order GW corrections in massive black hole binary inspirals ac...

  13. Waveform Modelling for the Laser Interferometer Space Antenna

    gr-qc 2023-11 unverdicted novelty 2.0

    A review of existing waveform models for LISA sources and the challenges that must still be overcome.

  14. Scalar induced gravitational waves review

    gr-qc 2021-09 unverdicted novelty 2.0

    A review that unifies analytical expressions for scalar-induced gravitational waves and emphasizes calculations for non-radiation-dominated cosmologies.