Prospects for Fundamental Physics with LISA
arXiv:2001.09793 · doi:10.1007/s10714-020-02691-1
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.
22 pages, 1 figure, to appear in General Relativity and Gravitation
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- Non-Gaussianities and Primordial Black Holes
- Tensor spectrum of turbulence-sourced gravitational waves as a constraint on graviton mass
- Unraveling the CMB lack-of-correlation anomaly with the cosmological gravitational wave background
- Extreme mass ratio inspirals around topological stars
- Toward Second-Order Self-Force for Eccentric Extreme-Mass Ratio Inspirals in Schwarzschild Spacetime
- New model of spontaneous scalarization of black holes induced by curvature and matter
- Black-hole hair from vector dark matter accretion
- CLAP for modified gravity: scalar instabilities in binary black hole spacetimes
- Tidally-induced nonlinear resonances in EMRIs with an analogue model
- Multipolar Particles in Helically Symmetric Spacetimes
- Purely metric Horndeski theories and spontaneous curvaturization of black holes
- Analytical model of precessing binaries using post-Newtonian theory in the extreme mass-ratio limit I: General Formalism
- Chiral Gravitational Wave Background from Audible Axion via Nieh-Yan Term
- Spectral instability of horizonless compact objects within astrophysical environments
- The Impact of Dark Matter on Gravitational Wave Detection by Space-based Interferometers
- Probing Kalb-Ramond field with extreme mass ratio inspirals
- Gravitational wave energy momentum-tensor in reduced Horndeski theories
- Frequency-Domain Distribution of Astrophysical Gravitational-Wave Backgrounds
- Enhancement of small-scale induced gravitational waves from the soliton/oscillon domination
- Primordial gravitational waves and curvature perturbations induced energy density perturbation
- Korteweg-de Vries Integrals for Modified Black Hole Potentials: Instabilities and other Questions
- Log-periodic gravitational-wave background beyond Einstein gravity
- A multi-parameter expansion for the evolution of asymmetric binaries in astrophysical environments
- Epicyclic Frequencies for a Generic Ultracompact Object
- Observational and theoretical aspects of Superspinars
- Merging Black Holes: Assessing the Performance of Two Analytic Gravitational Waves Models
- Thermal evolution of dark matter and gravitational-wave production in the early universe from a symplectic glueball model
- Eccentric Pairs: Analytic Gravitational Waves from Binary Black Holes in Elliptic Orbits
- Conformal Unification in a Quiver Theory and Gravitational Waves
- Magnetogenesis from Sawtooth Coupling: Gravitational Wave Probe of Reheating
- Multi-parameter Tests of General Relativity Using Bayesian Parameter Estimation with Principal Component Analysis for LISA
- Dynamical Chameleon Neutron Stars: stability, radial oscillations and scalar radiation in spherical symmetry
- Ten years of extreme gravity tests of general theory of relativity with gravitational-wave observations
- Dynamical friction from scalar dark matter in the relativistic regime
- Co-evolution of Nuclear Star Clusters and Massive Black Holes: Extreme Mass-Ratio Inspirals
- Exploring Time Delay Interferometry Ranging as a Practical Ranging Approach in the Bayesian Framework
- Exploring black holes with multiple photon spheres by interferometric signatures
- Matter environments around black holes: geodesics, light rings, and ultracompact configurations
- Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr
- Rapid-turn inflation in supergravity is rare and tachyonic
- The landscape of massive black-hole spectroscopy with LISA and Einstein Telescope
- Gravitational waves from equatorially eccentric extreme mass ratio inspirals around swirling Kerr black holes
- Instability of the cosmological DBI-Galileon in the non-relativistic limit
- Quantum Physics in Space
- Test of the Statistical Isotropy of the Universe using Gravitational Waves
- Correlating Gravitational Wave and Gamma-ray Signals from Primordial Black Holes
- A Faster Growth of Perturbations in an Early Matter Dominated Epoch: Primordial Black Holes and Gravitational Waves
- Redshift factor and the small mass-ratio limit in binary black hole simulations
- Precisely computing bound orbits of spinning bodies around black holes I: General framework and results for nearly equatorial orbits
- The eye of the storm: A regular Kerr black hole
- Extreme mass-ratio inspirals as probes of scalar fields: eccentric equatorial orbits around Kerr black holes
- Resonances, black hole mimickers and the greenhouse effect: consequences for gravitational-wave physics
- Precisely computing bound orbits of spinning bodies around black holes II: Generic orbits
- 1PN effective binary Lagrangian for the gravity-Kalb-Ramond sector in the conservative regime
- Quantum gravity phenomenology and the blackbody radiation
- Parameter inference of millilensed gravitational waves using neural spline flows
- Bubble Nucleation from Boson Star Collapse
- Rising Tides: Analytic Modeling of Tidal Effects in Binary Neutron Star Mergers