Ladder symmetries of black holes. Implications for love numbers and no-hair theorems
@article{Hui2022LadderSO, title={Ladder symmetries of black holes. Implications for love numbers and no-hair theorems}, author={Lam Hui and Austin Joyce and Riccardo Penco and Luca Santoni and Adam R. Solomon}, journal={Journal of Cosmology and Astroparticle Physics}, year={2022}, volume={2022} }
It is well known that asymptotically flat black holes in general relativity have a vanishing static, conservative tidal response. We show that this is a result of linearly realized symmetries governing static (spin 0,1,2) perturbations around black holes. The symmetries have a geometric origin: in the scalar case, they arise from the (E)AdS isometries of a dimensionally reduced black hole spacetime. Underlying the symmetries is a ladder structure which can be used to construct the full tower of…
7 Citations
Supergravity black holes, Love numbers, and harmonic coordinates
- PhysicsPhysical Review D
- 2022
To perform realistic tests of theories of gravity, we need to be able to look beyond general relativity and evaluate the consistency of alternative theories with observational data from, especially,…
Tidal deformability of dressed black holes and tests of ultralight bosons in extended mass ranges
- Physics
- 2021
The deformability of a compact object under the presence of a tidal perturbation is encoded in the tidal Love numbers (TLNs), which vanish for isolated black holes in vacuum. We show that the TLNs of…
Tidally induced multipole moments of a nonrotating black hole vanish to all post-Newtonian orders
- PhysicsPhysical Review D
- 2021
The tidal Love numbers of a black hole vanish, and this is often taken to imply that the hole’s tidally induced multipole moments vanish also. An obstacle to establishing a link between these…
Tidal response from scattering and the role of analytic continuation
- PhysicsPhysical Review D
- 2021
The tidal response of a compact object is a key gravitational-wave observable encoding information about its interior. This link is subtle due to the nonlinearities of general relativity. We show…
Hidden symmetry of the static response of black holes: Applications to Love numbers
- Physics
- 2022
We show that any static linear perturbations around a spherically symmetric black hole enjoys a set of conserved charges which forms a centrally extended Schrödinger algebra sh(1) = sl(2,R) ⋉H. The…
The post-Newtonian expansion in the effective theory of compact objects
- Physics
- 2022
: Using the effective field theory framework for extended objects, we build the effective theory of a binary system made up of the most general compact objects in a theory of gravity as general…
Effective actions for compact objects in an effective field theory of gravity
- Physics
- 2021
: Using the effective field theory framework for extended objects and the coset construction, we build the leading order effective action for the most general compact object allowed in an effective…
References
SHOWING 1-10 OF 84 REFERENCES
Conformal structure of the Schwarzschild black hole
- Physics
- 2012
We show that the scalar wave equation at low frequencies in the Schwarzschild geometry enjoys a hidden SL(2,R) invariance, which is not inherited from an underlying symmetry of the spacetime itself.…
On the vanishing of Love numbers for Kerr black holes
- Physics
- 2021
It was shown recently that the static tidal response coefficients, called Love numbers, vanish identically for Kerr black holes in four dimensions. In this work, we confirm this result and extend it…
Asymptotically flat black holes with scalar hair: a review
- Mathematics
- 2015
We consider the status of black hole (BH) solutions with nontrivial scalar fields but no gauge fields, in four-dimensional asymptotically flat spacetimes, reviewing both classical results and recent…
Black hole hair in generalized scalar-tensor gravity: An explicit example
- Physics
- 2014
In a recent paper we showed that in shift-symmetric Horndeski theory the scalar field is forced to obtain a nontrivial configuration in black hole spacetimes, unless a linear coupling with the…
No-hair theorem for Black Holes in Astrophysical Environments
- Physics
- 2015
According to the no-hair theorem, static black holes are described by a Schwarzschild spacetime provided there are no other sources of the gravitational field. This requirement, however, is in…
Mass Ladder Operators from Spacetime Conformal Symmetry
- Physics, Mathematics
- 2017
Ladder operators can be useful constructs, allowing for unique insight and intuition. In fact, they have played a special role in the development of quantum mechanics and field theory. Here, we…
Kerr black holes with scalar hair.
- PhysicsPhysical review letters
- 2014
We present a family of solutions of Einstein's gravity minimally coupled to a complex, massive scalar field, describing asymptotically flat, spinning black holes with scalar hair and a regular…
Near-horizon Carroll symmetry and black hole Love numbers
- Physics
- 2018
According to the black hole membrane paradigm, the black hole event horizon behaves like a 2+1 dimensional fluid. The fluid has nonzero momentum density but zero velocity. As a result, it does not…
Black hole stereotyping: induced gravito-static polarization
- Physics
- 2012
A bstractWe discuss the black hole effective action and define its static subsector. We determine the induced gravito-static polarization constants (electric Love numbers) of static black holes…
Tidal deformation and dissipation of rotating black holes
- PhysicsPhysical Review D
- 2021
We show that rotating black holes do not experience any tidal deformation when they are perturbed by a weak and adiabatic gravitational field. The tidal deformability of an object is quantified by…