Gabe Hoshino

ORCID: 0000-0003-4864-3104
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About
Contact & Profiles
Research Areas
  • Dark Matter and Cosmic Phenomena
  • Random lasers and scattering media
  • Scientific Research and Discoveries
  • Particle physics theoretical and experimental studies
  • Cosmology and Gravitation Theories
  • Astrophysics and Cosmic Phenomena
  • Blind Source Separation Techniques
  • Superconducting and THz Device Technology
  • Orbital Angular Momentum in Optics
  • Atomic and Subatomic Physics Research

University of Chicago
2022-2025

Fermi National Accelerator Laboratory
2022

We introduce the Broadband Reflector Experiment for Axion Detection (BREAD) conceptual design and science program. This haloscope plans to search bosonic dark matter across [10^{-3},1] eV ([0.24, 240] THz) mass range. BREAD proposes a cylindrical metal barrel convert into photons, which novel parabolic reflector focuses onto photosensor. unique geometry enables enclosure in standard cryostats high-field solenoids, overcoming limitations of current dish antennas. A pilot 0.7 m^{2} experiment...

10.1103/physrevlett.128.131801 article EN Physical Review Letters 2022-03-28

We present first results from a dark photon matter search in the mass range 44 to 52 μeV (10.7-12.5 GHz) using room-temperature dish antenna setup called GigaBREAD. Dark converts ordinary photons on cylindrical metallic emission surface with area 0.5 m^{2} and is focused by novel parabolic reflector onto horn antenna. Signals are read out low-noise receiver system. A data taking run 24 days of does not show evidence for this range, excluding mixing parameters χ≳10^{-12} at 90% confidence...

10.1103/physrevlett.132.131004 article EN cc-by Physical Review Letters 2024-03-28

We report the first result from a dark photon matter search in mass range 78.62 to 83.95 μeV/c^{2} with dielectric haloscope prototype for madmax (Magnetized Disc and Mirror Axion eXperiment). Putative photons would convert detectable within stack consisting of three sapphire disks mirror. The emitted power this system is received by an antenna successively digitized using low-noise receiver. No significant signal attributable has been observed above expected background. Assuming unpolarized...

10.1103/physrevlett.134.151004 article EN cc-by Physical Review Letters 2025-04-18

We present the results from first axion-like particle search conducted using a dish antenna. The experiment was at room temperature and sensitive to particles in $44-52\,\mu\mathrm{eV}$ range ($10.7 - 12.5\,\mathrm{GHz}$). novel antenna geometry proposed by BREAD collaboration previously used conduct dark photon same mass range. To allow for sensitivity, placed $3.9\,\mathrm{T}$ solenoid magnet Argonne National Laboratory. In presence of magnetic field, matter converts photons conductive...

10.48550/arxiv.2501.17119 preprint EN arXiv (Cornell University) 2025-01-28

We present the results from first axionlike particle search conducted using a dish antenna. The experiment was at room temperature and sensitive to particles in <a:math xmlns:a="http://www.w3.org/1998/Math/MathML" display="inline"><a:mrow><a:mn>44</a:mn><a:mi>–</a:mi><a:mn>52</a:mn><a:mtext> </a:mtext><a:mtext> </a:mtext><a:mi mathvariant="normal">μ</a:mi><a:mi>eV</a:mi></a:mrow></a:math> range (10.7–12.5 GHz). novel antenna geometry proposed by BREAD Collaboration previously used conduct...

10.1103/physrevlett.134.171002 article EN cc-by Physical Review Letters 2025-04-30

We present first results from a dark photon matter search in the mass range 44 to 52 $\mu{\rm eV}$ ($10.7 - 12.5\,{\rm GHz}$) using room-temperature dish antenna setup called GigaBREAD. Dark converts ordinary photons on cylindrical metallic emission surface with area $0.5\,{\rm m}^2$ and is focused by novel parabolic reflector onto horn antenna. Signals are read out low-noise receiver system. A data taking run 24 days of does not show evidence for this range, excluding mixing parameters...

10.48550/arxiv.2310.13891 preprint EN cc-by arXiv (Cornell University) 2023-01-01
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