# Probing Dynamics of Boson Stars by Fast Radio Bursts and Gravitational Wave Detection

## TL;DR

This paper investigates the properties and detectability of boson stars with specific self-interactions, exploring their potential as dark matter candidates and how they can be distinguished through FRB lensing and gravitational wave signals.

## Contribution

It introduces new models of boson stars with Liouville and logarithmic potentials, analyzing their dynamics, constraints, and observational signatures.

## Key findings

- Boson stars with these potentials can be constrained by CMB and MACHO data.
- FRB lensing and GW detection can distinguish different boson star models.
- Allowed scalar particle mass ranges are derived based on observational constraints.

## Abstract

Boson stars may consist of a new type of light singlet scalar particles with nontrivial self-interactions, and may compose a fraction of the dark matter in the Universe. In this work, we study the dynamics of boson stars with Liouville and logarithmic scalar self-interaction potentials as benchmarks. We perform a numerical analysis as well as a semi-analytic study on how the compactness and the total mass will deviate from that of the usual boson stars formed with a quartic repulsive self-interaction. We apply the recently suggested Swampland conjecture to examine whether boson stars with such benchmark potentials belong to the Landscape of a quantum gravity. Using the mass constraint on the macroscopic compact halo object (MACHO) and the cold dark matter (CDM) isocurvature mode constraint from the cosmic microwave background (CMB), we derive the allowed mass range of scalar particles which compose the boson star. We further analyze applications of the lensing of fast radio bursts (FRBs) and the gravitational wave (GW) detection to probe the presence of such boson stars and constrain the parameter space of their corresponding models. We discuss how the two types of boson star potentials can be discriminated by the FRB and GW measurements.