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researcher

P. Beltrame

74 papers hereh-index 439.2k citations170 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • sole author1
  • middle author33

Across the 34 of 74 papers where every author was matched, so the position is known.

fields
  • hep-ex25
  • physics.ins-det22
  • astro-ph.CO12
  • astro-ph.IM9
  • hep-ph4
  • astro-ph.HE2
same name
  • P. Beltrame — 12 papers, h 2
  • P. Beltrame — 11 papers
  • P. Beltrame — 9 papers, h 11
  • P. Beltrame — 8 papers, h 9
  • P. Beltrame — 2 papers, h 3
  • P. Beltrame — 1 paper

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

activity
20052025
most citedResults from a search for dark matter in the complete LUX exposure

1.6k citations · 8.4k across the 73 of their papers we have counts for

collaborators
Showing 2021Show all

3 papers · 1 filter

physics.ins-det2021★ 12 cited

Projected sensitivity of the LUX-ZEPLIN (LZ) experiment to the two-neutrino and neutrinoless double beta decays of 134Xe

The LUX-ZEPLIN, Collaboration, : +194

The projected sensitivity of the LUX-ZEPLIN (LZ) experiment to two-neutrino and neutrinoless double beta decay of 134Xe is presented. LZ is a 10-tonne xenon time projection ch…

hep-ex2021★ 29 cited

Projected sensitivities of the LUX-ZEPLIN (LZ) experiment to new physics via low-energy electron recoils

The LZ Collaboration, D. S. Akerib, A. K. Al Musalhi +194

LUX-ZEPLIN (LZ) is a dark matter detector expected to obtain world-leading sensitivity to weakly interacting massive particles (WIMPs) interacting via nuclear recoils with a ~7-ton…

astro-ph.IM2021★ 8 cited

Enhancing the sensitivity of the LUX-ZEPLIN (LZ) dark matter experiment to low energy signals

D. S. Akerib, A. K. Al Musalhi, S. K. Alsum +184

Two-phase xenon detectors, such as that at the core of the forthcoming LZ dark matter experiment, use photomultiplier tubes to sense the primary (S1) and secondary (S2) scintillati…

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