Search for MeV-Scale Axionlike Particles and Dark Photons with PandaX-4T.

Phys Rev Lett

School of Physics and Astronomy, Shanghai Jiao Tong University, Key Laboratory for Particle Astrophysics and Cosmology (MoE), Shanghai Key Laboratory for Particle Physics and Cosmology, Shanghai 200240, China.

Published: February 2025

Axionlike particles (ALPs) and dark photons (DPs) are viable dark matter particle candidates. We have searched for possible ALP/DP signals in the PandaX-4T liquid xenon detector using 440  kg·yr of data. A binned likelihood fit is constructed to search for possible mono-energetic peaks induced by the absorption processes between ALPs/DPs and atomic electrons of xenon. A detailed temporal model of decays associated with xenon isotopes is introduced to constrain the number of background events. No signal excess over background expectations is observed, and we have established the most stringent exclusion limits for most ALP/DP masses across the range of 150  keV/c^{2} to 1  MeV/c^{2}. The improvement is particularly significant within the mass range of 150-400  keV/c^{2}, with the average factor of 3.5 compared to previous results.

Download full-text PDF

Source
http://dx.doi.org/10.1103/PhysRevLett.134.071004DOI Listing

Publication Analysis

Top Keywords

axionlike particles
8
dark photons
8
search mev-scale
4
mev-scale axionlike
4
particles dark
4
photons pandax-4t
4
pandax-4t axionlike
4
particles alps
4
alps dark
4
photons dps
4

Similar Publications

Search for MeV-Scale Axionlike Particles and Dark Photons with PandaX-4T.

Phys Rev Lett

February 2025

School of Physics and Astronomy, Shanghai Jiao Tong University, Key Laboratory for Particle Astrophysics and Cosmology (MoE), Shanghai Key Laboratory for Particle Physics and Cosmology, Shanghai 200240, China.

Axionlike particles (ALPs) and dark photons (DPs) are viable dark matter particle candidates. We have searched for possible ALP/DP signals in the PandaX-4T liquid xenon detector using 440  kg·yr of data. A binned likelihood fit is constructed to search for possible mono-energetic peaks induced by the absorption processes between ALPs/DPs and atomic electrons of xenon.

View Article and Find Full Text PDF

Hunting Dark Matter Lines in the Infrared Background with the James Webb Space Telescope.

Phys Rev Lett

February 2025

University of Chicago, Fermi National Accelerator Laboratory, Theoretical Astrophysics Department, Batavia, Illinois 60510, USA and , Kavli Institute for Cosmological Physics, Chicago, Illinois 60637, USA.

Dark matter particles with a mass around 1 eV can decay into near-infrared photons. Utilizing available public blank sky observations from the NIRSpec IFU on the James Webb Space Telescope (JWST), we search for a narrow emission line due to decaying dark matter and derive leading constraints in the mass range 0.8-3 eV on the decay rate to photons, and more specifically, on the axion-photon coupling for the case of axionlike particles.

View Article and Find Full Text PDF

First Result for Dark Matter Search by WINERED.

Phys Rev Lett

February 2025

Kyoto Sangyo University Motoyama, Laboratory of Infrared High-resolution Spectroscopy, Koyama Astronomical Observatory, Kamigamo, Kita-ku, Kyoto 603-8555, Japan.

The identity of dark matter has been a mystery in astronomy, cosmology, and particle theory for about a century. We present the first dark matter search with a high-dispersion spectrograph by using WINERED at the 6.5 m Magellan Clay telescope to measure the photons from the dark matter decays.

View Article and Find Full Text PDF

We present new exclusion bounds obtained at the European X-Ray Free Electron Laser facility (EuXFEL) on axionlike particles in the mass range 10^{-3}  eV≲m_{a}≲10^{4}  eV. Our experiment exploits the Primakoff effect via which photons can, in the presence of a strong external electric field, decay into axions, which then convert back into photons after passing through an opaque wall. While similar searches have been performed previously at a third-generation synchrotron [Yamaji et al.

View Article and Find Full Text PDF

Exploring New Physics with PandaX-4T Low Energy Electronic Recoil Data.

Phys Rev Lett

January 2025

Shanghai Jiao Tong University, School of Physics and Astronomy, Key Laboratory for Particle Astrophysics and Cosmology (MoE), Shanghai Key Laboratory for Particle Physics and Cosmology, Shanghai 200240, China.

New particles beyond the standard model of particle physics, such as axions, can be effectively searched through their interactions with electrons. We use the large liquid xenon detector PandaX-4T to search for novel electronic recoil signals induced by solar axions, neutrinos with anomalous magnetic moment, axionlike particles, dark photons, and light fermionic dark matter. A detailed background model is established using the latest datasets with 1.

View Article and Find Full Text PDF

Want AI Summaries of new PubMed Abstracts delivered to your In-box?

Enter search terms and have AI summaries delivered each week - change queries or unsubscribe any time!