The tidal gap: causality bound on exotic compact objects with applications in the solar and sub-solar mass range
Benedetta Russo, Alfredo Urbano

TL;DR
This paper explores the limits on tidal deformability of exotic compact objects imposed by causality, identifying a tidal gap from black holes, and discusses how certain boson stars could mimic black holes while having non-zero tidal deformability.
Contribution
It establishes a causality-based lower limit on tidal deformability, identifies a tidal gap between black holes and ECOs, and analyzes how boson stars could serve as black hole mimickers with non-zero tidal deformability.
Findings
Existence of a tidal gap between black holes and ECOs.
Potential for boson stars to mimic black holes with non-zero tidal deformability.
Lower bounds on tidal deformability influenced by causality and energy conditions.
Abstract
In this work, we highlight the existence of a lower limit on the tidal deformability parameter , determined by the requirement of relativistic causality. Additionally, by considering the upper bound set on compactness, we identify the region within the parameter space of compactness versus tidal deformability, where physically motivated exotic compact objects (ECOs) could potentially reside. Our analysis reveals the presence of a tidal gap between black holes, characterized by vanishing tidal deformability, and physically motivated ECOs. Prompted by this finding, we investigate the possibility that a population of maximally compact exotic objects, described by a linear equation of state (EoS), may simultaneously inhabit the lower mass gap and the sub-solar region, thus qualifying as (primordial) black hole mimickers while distinguishing themselves from the latter by their…
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Taxonomy
TopicsPulsars and Gravitational Waves Research · Black Holes and Theoretical Physics · Astrophysical Phenomena and Observations
