We present a new bound on the ultralight axion (ULA) dark matter mass m_{a}, using the Lyman-alpha forest to look for suppressed cosmic structure growth: a 95% lower limit m_{a}>2×10^{-20} eV. This strongly disfavors (>99.7% credibility) the canonical ULA with 10^{-22} eV
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http://dx.doi.org/10.1103/PhysRevLett.126.071302 DOI Listing Publication Analysis
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Phys Rev Lett
November 2024
School of Physics, The University of Sydney, Sydney, New South Wales 2006, Australia.
Nat Commun
January 2024
School of Physics and State Key Laboratory of Nuclear Physics and Technology, Peking University, 100871, Beijing, China.
Ultralight dark photons and axions are well-motivated hypothetical dark matter candidates. Both dark photon dark matter and axion dark matter can resonantly convert into electromagnetic waves in the solar corona when their mass is equal to the solar plasma frequency. The resultant electromagnetic waves appear as monochromatic signals within the radio-frequency range with an energy equal to the dark matter mass, which can be detected via radio telescopes for solar observations.
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September 2023
Duke Quantum Center, Duke University, Durham, NC, 27701, USA.
Ultralight axion-like particles are well-motivated relics that might compose the cosmological dark matter and source anomalous time-dependent magnetic fields. We report on terrestrial bounds from the Noble And Alkali Spin Detectors for Ultralight Coherent darK matter (NASDUCK) collaboration on the coupling of axion-like particles to neutrons and protons. The detector uses nuclei of noble-gas and alkali-metal atoms and operates in the Spin-Exchange Relaxation-Free (SERF) regime, achieving high sensitivity to axion-like dark matter fields.
View Article and Find Full Text PDFPhys Rev Lett
February 2022
High Energy Theory Group, Physics Department, Brookhaven National Laboratory, Upton, New York 11973, USA.
The formation of ultrarare supermassive black holes (SMBHs), with masses of O(10^{9} M_{⊙}), in the first billion years of the Universe remains an open question in astrophysics. At the same time, ultralight dark matter (DM) with mass in the vicinity of O(10^{-20} eV) has been motivated by small scale DM distributions. Though this type of DM is constrained by various astrophysical considerations, certain observations could be pointing to modest evidence for it.
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February 2022
Department of Physics of Complex Systems, Weizmann Institute of Science, Rehovot 76100, Israel.
Dark matter is one of the greatest mysteries in physics. It interacts via gravity and composes most of our universe, but its elementary composition is unknown. We search for nongravitational interactions of axion-like dark matter with atomic spins using a precision quantum detector.
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