Home › Researcher directory › R. M. Bozza
R. M. Bozza
Affiliation : University of Naples Federico II · Istituto Nazionale di Fisica Nucleare, Sezione di Napoli
- 23Publications (affiliation in Italy)
Research profile
R. M. Bozza has 23 indexed publications (2023–2026). Their work appears mainly in “Journal of High Energy Physics”, “The European Physical Journal C” and “Journal of Cosmology and Astroparticle Physics”. Their most cited article, “Observation of an ultra-high-energy cosmic neutrino with KM3NeT” (2025), has been cited 146 times. 22 of these publications date from the last three years of activity. Their work is co-authored with at least 12 researchers, including institutions in France, Germany.
Is this you? Get your research seen
Create your free DzCademia profile and add your articles: they will show up more easily on Google and in AI assistants like ChatGPT, so more people can read and cite your work.
Create my free profile Add my publicationsPublications (23)
- Characterizing Candidate Blazar Counterparts of the Ultra-high-energy Event KM3-230213A
- On the Potential Galactic Origin of the Ultra-high-energy Event KM3-230213A
- Observation of an ultra-high-energy cosmic neutrino with KM3NeT
- Ultrahigh-Energy Event KM3-230213A within the Global Neutrino Landscape
- Author Correction: Observation of an ultra-high-energy cosmic neutrino with KM3NeT
- Search for quantum decoherence in neutrino oscillations with six detection units of KM3NeT/ORCA
- KM3NeT constraint on Lorentz-violating superluminal neutrino velocity
- Evaluation of the upgraded 3-inch Hamamatsu photomultiplier for the KM3NeT Neutrino Telescope
- Addendum: Measurement of neutrino oscillation parameters with the first six detection units of KM3NeT/ORCA
- Study of tau neutrinos and non-unitary neutrino mixing with the first six detection units of KM3NeT/ORCA
- Probing invisible neutrino decay with the first six detection units of KM3NeT/ORCA
- Measurement of the atmospheric $$\nu _{\mu }$$ flux with six detection units of KM3NeT/ORCA
- Astronomy potential of KM3NeT/ARCA
- Differential Sensitivity of the KM3NeT/ARCA detector to a diffuse neutrino flux and to point-like source emission: Exploring the case of the Starburst Galaxies
- Measurement of neutrino oscillation parameters with the first six detection units of KM3NeT/ORCA
- Atmospheric muons measured with the KM3NeT detectors in comparison with updated numeric predictions
- Search for neutrino emission from GRB 221009A using the KM3NeT ARCA and ORCA detectors
- Searches for neutrino counterparts of gravitational waves from the LIGO/Virgo third observing run with KM3NeT
- Prospects for combined analyses of hadronic emission from $$\gamma $$-ray sources in the Milky Way with CTA and KM3NeT
- The Power Board of the KM3NeT Digital Optical Module: Design, Upgrade, and Production
- KM3NeT real-time analysis framework
- Measurement of neutrino oscillation parameters with the first six detection units of KM3NeT/ORCA
- Embedded software of the KM3NeT central logic board
Publication venues
- Journal of High Energy Physics × 4
- The European Physical Journal C × 4
- Journal of Cosmology and Astroparticle Physics × 3
- Nature × 2
- The Astronomical Journal × 1
- The Astrophysical Journal × 1
Publications per year
- 20262
- 202510
- 202410
- 20231
Collaborations
Partner institutions : Istituto Nazionale di Fisica Nucleare, Laboratori Nazionali del Sud · Istituto Nazionale di Fisica Nucleare · Istituto Nazionale di Fisica Nucleare, Sezione di Bologna · University of Bologna · Istituto Nazionale di Fisica Nucleare, Sezione di Roma I
Co-authors’ countries : France · Germany
Co-authors
- Antonio Ambrosone
- F. Benfenati
- A. Capone
- S. Biagi
- T. Chiarusi
- B. Caiffi
- Riccardo Bruno
- A. De Benedittis
- Marouane Benhassi
- G. Cuttone
- R. Buompane
- Paolo Castaldi
Bibliographic data from OpenAlex (open database).
Why choose Dzcademia?
Profiles, articles and conference contributions: give your research a structured public presence. Integrated metadata help search engines and AI assistants identify your work and understand its references.
Comment with Google
Sign in with Google to comment directly on this page.