Ladder Symmetry: The Necessary and Sufficient Condition for Vanishing Love Numbers

Fuente: arXiv
Saved in:
Bibliographic Details
Main Authors: Sharma, Chanchal, Roy, Shuvayu, Sarkar, Sudipta
Format: Preprint
Published: 2025
Subjects:
Online Access:
Tags: Add Tag
No Tags, Be the first to tag this record!
_version_ 1866918339311304704
author Sharma, Chanchal
Roy, Shuvayu
Sarkar, Sudipta
author_facet Sharma, Chanchal
Roy, Shuvayu
Sarkar, Sudipta
contents Black holes in four-dimensional, asymptotically flat general relativity have vanishing static tidal Love numbers (TLNs), a property tied to a hidden symmetry of the perturbation equations. Within the Konoplya-Rezzolla-Zhidenko (KRZ) parametrization, a subclass of spacetimes was previously shown to admit such Ladder symmetry, which enforces the absence of static scalar TLNs. In this work, we introduce parametric deformations to such Ladder-symmetric spacetimes and analyze the resultant linear tidal response. Using the parametrized formalism for TLNs, we show that any deviation from a Ladder-symmetric background leads to non-zero static scalar TLNs. This establishes Ladder symmetry as a necessary, as well as sufficient condition, for the vanishing of static TLNs in static, spherically symmetric black holes and in rotating black holes of the KRZ class.
format Preprint
id arxiv_https___arxiv_org_abs_2511_09670
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Ladder Symmetry: The Necessary and Sufficient Condition for Vanishing Love Numbers
Sharma, Chanchal
Roy, Shuvayu
Sarkar, Sudipta
General Relativity and Quantum Cosmology
High Energy Physics - Theory
Black holes in four-dimensional, asymptotically flat general relativity have vanishing static tidal Love numbers (TLNs), a property tied to a hidden symmetry of the perturbation equations. Within the Konoplya-Rezzolla-Zhidenko (KRZ) parametrization, a subclass of spacetimes was previously shown to admit such Ladder symmetry, which enforces the absence of static scalar TLNs. In this work, we introduce parametric deformations to such Ladder-symmetric spacetimes and analyze the resultant linear tidal response. Using the parametrized formalism for TLNs, we show that any deviation from a Ladder-symmetric background leads to non-zero static scalar TLNs. This establishes Ladder symmetry as a necessary, as well as sufficient condition, for the vanishing of static TLNs in static, spherically symmetric black holes and in rotating black holes of the KRZ class.
title Ladder Symmetry: The Necessary and Sufficient Condition for Vanishing Love Numbers
topic General Relativity and Quantum Cosmology
High Energy Physics - Theory
url https://arxiv.org/abs/2511.09670