4.7 Article

Search for relativistic fractionally charged particles in space

Journal

PHYSICAL REVIEW D
Volume 106, Issue 6, Pages -

Publisher

AMER PHYSICAL SOC
DOI: 10.1103/PhysRevD.106.063026

Keywords

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Funding

  1. National Key Research and Development Program of China [2016YFA0400200]
  2. National Natural Science Foundation of China [11673021, U1738205, U1738208, U1738139, U1738135, 11705197, 11851302]
  3. Chinese Academy of Sciences [XDA15051100]
  4. Youth Innovation Promotion Association CAS [2021450]
  5. Outstanding Youth Science Foundation of NSFC [12022503]
  6. CAS Project for Young Scientists in Basic Research [YSBR-061]
  7. National Institute for Nuclear Physics (INFN) , Italy
  8. European Research Council (ERC) under the European Union [851103]
  9. Swiss National Science Foundation (SNSF) , Switzerland
  10. European Research Council (ERC) [851103] Funding Source: European Research Council (ERC)

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The existence of fractionally charged particles (FCPs) remains uncertain, but the search for FCPs is crucial for extensions of the Standard Model in particle physics. Previous searches were mostly conducted underground or at high altitudes, with limited searches in orbit. This study presents a five-year FCP search in space using the DAMPE satellite, demonstrating higher sensitivity than similar experiments.
More than a century after the performance of the oil drop experiment, the possible existence of fractionally charged particles (FCPs) still remains unsettled. The search for FCPs is crucial for some extensions of the Standard Model in particle physics. Most of the previously conducted searches for FCPs in cosmic rays were based on experiments underground or at high altitudes. However, there have been few searches for FCPs in cosmic rays carried out in orbit other than AMS-01 flown by a space shuttle and BESS by a balloon at the top of the atmosphere. In this study, we conduct an FCP search in space based on on -orbit data obtained using the Dark Matter Particle Explorer (DAMPE) satellite over a period of five years. Unlike underground experiments, which require an FCP energy of the order of hundreds of GeV, our FCP search starts at only a few GeV. An upper limit of 6.2 x 10-10 cm-2 sr-1 s-1 is obtained for the flux. Our results demonstrate that DAMPE exhibits higher sensitivity than experiments of similar types by three orders of magnitude that more stringently restricts the conditions for the existence of FCP in primary cosmic rays.

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