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I. Dafinei

133 papers hereh-index 5421.8k citations419 works total

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

author position
  • first author1
  • middle author81

Across the 82 of 133 papers where every author was matched, so the position is known.

fields
  • physics.ins-det69
  • nucl-ex48
  • hep-ex7
  • hep-ph4
  • astro-ph.CO2
  • astro-ph.HE1
same name
  • I. Dafinei — 5 papers
  • I. Dafinei — 1 paper
  • I. Dafinei — 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
20092026
most citedFirst Results from CUORE: A Search for Lepton Number Violation via 0νββ Decay of 130Te

271 citations · 4k across the 129 of their papers we have counts for

collaborators
Showing hep-phShow all

4 papers · 1 filter

hep-ph2026

Cosmic Ray Boosted Dark Matter in COSINUS: Modeling and Constraints

G. Angloher, M. R. Bharadwaj, A. Böhmer +41

Direct detection of nuclear recoils due to sub-GeV dark matter is challenging because of the small kinetic energy of the light dark matter particles. Although limits down to a few…

hep-ph2026

Neutrino NSI in archaeological Pb

D. Alloni, G. Benato, P. Carniti +47

Dark matter direct detection experiments can observe solar neutrinos via coherent elastic neutrino-nucleus scattering, making it possible to test new physics in the neutrino sector…

hep-ph2025★ 1 cited

Defect Formation in NaI Crystals: A Novel Pathway to Dark Matter Detection

G. Angloher, M. R. Bharadwaj, A. Böhmer +44

Sodium iodide (NaI) is a widely used scintillator in direct dark matter searches. In particular, NaI-based cryogenic scintillating calorimeters have emerged as promising candidates…

hep-ph2025

COSINUS model-independent sensitivity to the DAMA/LIBRA dark matter signal

G. Angloher, M. R. Bharadwaj, A. Böhmer +40

COSINUS is a dark matter direct detection experiment using NaI crystals as cryogenic scintillating calorimeters. If no signal is observed, this will constrain the dark matter scatt…

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