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M. Chianese

56 papers hereh-index 221.2k citations85 works total

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

author position
  • sole author7
  • first author22
  • middle author22
  • last author2

Across the 53 of 56 papers where every author was matched, so the position is known.

fields
  • hep-ph41
  • astro-ph.HE11
  • astro-ph.CO3
  • gr-qc1
same name
  • M. Chianese — 1 paper, h 1

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
20152026
most citedRadio Signal of Axion-Photon Conversion in Neutron Stars: A Ray Tracing Analysis

90 citations · 1.1k across the 52 of their papers we have counts for

collaborators
Showing 2016Show all

4 papers · 1 filter

hep-ph2016★ 36 cited

Dark Matter interpretation of low energy IceCube MESE excess

M. Chianese, G. Miele, S. Morisi

The 2-years MESE IceCube events show a slightly excess in the energy range 10-100 TeV with a maximum local statistical significance of 2.3σ, once a hard astrophysical power-law i…

hep-ph2016★ 40 cited

A Consistent Theory of Decaying Dark Matter Connecting IceCube to the Sesame Street

Marco Chianese, Alexander Merle

The high energy events observed at the IceCube Neutrino Observatory have triggered many investigations interpreting the highly energetic neutrinos detected as decay products of hea…

hep-ph2016★ 3 cited

IceCube PeV Neutrinos and Leptophilic Dark Matter

Marco Chianese

We analyze the scenario where the IceCube high energy neutrino events are explained in terms of an extraterrestrial flux due to two different components: a contribution coming from…

hep-ph2016★ 52 cited

Low energy IceCube data and a possible Dark Matter related excess

Marco Chianese, Gennaro Miele, Stefano Morisi +1

In this Letter we focus our attention on the IceCube events in the energy range between 60 and 100 TeV, which show an order 2-sigma excess with respect to a power-law with spectral…

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