Detection of Bosenovae with Quantum Sensors on Earth and in Space
In a broad class of theories, the accumulation of ultralight dark matter (ULDM) with particles of mass $10^{-22}~\textrm{eV} < m_{\phi} < 1~\textrm{eV}$ leads the to formation of long-lived bound states known as boson stars. When the ULDM exhibits self-interactions, prodigious bursts of energy...
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Main Authors: | , , , , |
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Format: | Journal Article |
Language: | English |
Published: |
28-06-2023
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Subjects: | |
Online Access: | Get full text |
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Summary: | In a broad class of theories, the accumulation of ultralight dark matter
(ULDM) with particles of mass $10^{-22}~\textrm{eV} < m_{\phi} < 1~\textrm{eV}$
leads the to formation of long-lived bound states known as boson stars. When
the ULDM exhibits self-interactions, prodigious bursts of energy carried by
relativistic bosons are released from collapsing boson stars in bosenova
explosions. We extensively explore the potential reach of terrestrial and
space-based experiments for detecting transient signatures of emitted
relativistic bursts of scalar particles, including ULDM coupled to photons,
electrons, and gluons, capturing a wide range of motivated theories. For the
scenario of relaxion ULDM, we demonstrate that upcoming experiments and
technology such as nuclear clocks as well as space-based interferometers will
be able to sensitively probe orders of magnitude in the ULDM coupling-mass
parameter space, challenging to study otherwise, by detecting signatures of
transient bosenova events. Our analysis can be readily extended to different
scenarios of relativistic scalar particle emission. |
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Bibliography: | IPMU23-0024, KEK-QUP-2023-0014, KEK-TH-2534, KEK-Cosmo-0316 |
DOI: | 10.48550/arxiv.2306.16468 |