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researcher

N. Fornengo

150 papers hereh-index 579.4k citations246 works total

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

author position
  • sole author10
  • first author20
  • middle author89
  • last author14

Across the 133 of 150 papers where every author was matched, so the position is known.

fields
  • hep-ph88
  • astro-ph.CO26
  • astro-ph.HE23
  • astro-ph12
  • astro-ph.GA1
same name
  • N. Fornengo — 4 papers, h 3
  • N. Fornengo — 2 papers

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
19932026
most citedMinimal Dark Matter

1k citations · 10k across the 146 of their papers we have counts for

collaborators
Showing 2009Show all

4 papers · 1 filter

astro-ph.CO2009★ 66 cited

Thermal Relics in Modified Cosmologies: Bounds on Evolution Histories of the Early Universe and Cosmological Boosts for PAMELA

R. Catena, N. Fornengo, M. Pato +2

Alternative cosmologies, based on extensions of General Relativity, predict modified thermal histories in the Early Universe during the pre Big Bang Nucleosynthesis (BBN) era, epoc…

hep-ph2009★ 65 cited

Relic neutralinos and the two dark matter candidate events of the CDMS II experiment

A. Bottino, F. Donato, N. Fornengo +1

The CDMS Collaboration has presented its results for the final exposure of the CDMS II experiment and reports that two candidate events for dark matter would survive after applicat…

hep-ph2009★ 43 cited

Investigating light neutralinos at neutrino telescopes

V. Niro, A. Bottino, N. Fornengo +1

We present a detailed analysis of the neutrino-induced muon signals coming from neutralino pair-annihilations inside the Sun and the Earth with particular emphasis for light neutra…

hep-ph2009★ 8 cited

Anti-Matter in Cosmic Rays : Backgrounds and Signals

Timur Delahaye, Pierre Brun, Fiorenza Donato +5

Recent PAMELA and ATIC data seem to indicate an excess in positron cosmic rays above approximately 10 GeV which might be due to galactic Dark Matter particle annihilation. However…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.