• Media type: E-Article
  • Title: Sensitivity of multi-PMT optical modules in Antarctic ice to supernova neutrinos of MeV energy
  • Contributor: Lozano Mariscal, C. J.; Classen, L.; Unland Elorrieta, M. A.; Kappes, A.
  • imprint: Springer Science and Business Media LLC, 2021
  • Published in: The European Physical Journal C
  • Language: English
  • DOI: 10.1140/epjc/s10052-021-09809-y
  • ISSN: 1434-6044; 1434-6052
  • Keywords: Physics and Astronomy (miscellaneous) ; Engineering (miscellaneous)
  • Origination:
  • Footnote:
  • Description: <jats:title>Abstract</jats:title><jats:p>New optical sensors with a segmented photosensitive area are being developed for the next generation of neutrino telescopes at the South Pole. In addition to increasing sensitivity to high-energy astrophysical neutrinos, we show that this will also lead to a significant improvement in sensitivity to MeV neutrinos, such as those produced in core-collapse supernovae (CCSN). These low-energy neutrinos can provide a detailed picture of the events after stellar core collapse, testing our understanding of these violent explosions. We present studies on the event-based detection of MeV neutrinos with a segmented sensor and, for the first time, the potential of a corresponding detector in the deep ice at the South Pole for the detection of extra-galactic CCSN. We find that exploiting temporal coincidences between signals in different photocathode segments, a <jats:inline-formula><jats:alternatives><jats:tex-math>$$27\ \mathrm {M}_{\odot }$$</jats:tex-math><mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mrow> <mml:mn>27</mml:mn> <mml:mspace /> <mml:msub> <mml:mi>M</mml:mi> <mml:mo>⊙</mml:mo> </mml:msub> </mml:mrow> </mml:math></jats:alternatives></jats:inline-formula> progenitor mass CCSN can be detected up to a distance of 341 kpc with a false detection rate of <jats:inline-formula><jats:alternatives><jats:tex-math>$${0.01}\,\hbox {year}^{-1}$$</jats:tex-math><mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mrow> <mml:mrow> <mml:mn>0.01</mml:mn> </mml:mrow> <mml:mspace /> <mml:msup> <mml:mtext>year</mml:mtext> <mml:mrow> <mml:mo>-</mml:mo> <mml:mn>1</mml:mn> </mml:mrow> </mml:msup> </mml:mrow> </mml:math></jats:alternatives></jats:inline-formula> with a detector consisting of 10,000 sensors. Increasing the number of sensors to 20,000 and reducing the optical background by a factor of 70 expands the range such that a CCSN detection rate of 0.1 per year is achieved, while keeping the false detection rate at <jats:inline-formula><jats:alternatives><jats:tex-math>$${0.01}\,{\hbox {year}^{-1}}$$</jats:tex-math><mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mrow> <mml:mrow> <mml:mn>0.01</mml:mn> </mml:mrow> <mml:mspace /> <mml:msup> <mml:mtext>year</mml:mtext> <mml:mrow> <mml:mo>-</mml:mo> <mml:mn>1</mml:mn> </mml:mrow> </mml:msup> </mml:mrow> </mml:math></jats:alternatives></jats:inline-formula>.</jats:p>
  • Access State: Open Access