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researcher

S. Zavatarelli

3 papers here

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

author position
  • middle author1

Across the 1 of 3 papers where every author was matched, so the position is known.

fields
  • nucl-ex2
  • physics.ins-det1
ORCID 0000-0002-5722-8896
same name
  • S. Zavatarelli — 153 papers, h 47
  • S. Zavatarelli — 6 papers
  • S. Zavatarelli — 2 papers
  • S. Zavatarelli — 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
20222025
most citedCharacterization of the LUNA neutron detector array for the measurement of the 13C(a,n)16O reaction

31 citations · 57 across the 3 of their papers we have counts for

collaborators

3 papers

nucl-ex2025★ 2 cited

Status and future directions for direct cross-section measurements of the 13C(a,n)16O reaction for astrophysics

L. Csedreki, Gy. Gyürky, D. Rapagnani +45

The 13C(a,n)16O reaction is the main neutron source of the s-process taking place in thermally pulsing AGB stars and it is one of the main candidate sources of neutrons for the i-p…

physics.ins-det2024★ 31 cited

Characterization of the LUNA neutron detector array for the measurement of the 13C(a,n)16O reaction

L. Csedreki, G. F. Ciani, J. Balibrea-Correa +46

We introduce the LUNA neutron detector array developed for the investigation of the 13C(a,n)16O reaction towards its astrophysical s-process Gamow peak in the low-background enviro…

nucl-ex2022★ 24 cited

First direct limit on the 334 keV resonance strength in the 22Ne(α,γ)26Mg reaction

D. Piatti, E. Masha, M. Aliotta +44

In stars, the fusion of 22Ne and 4He may produce either 25Mg, with the emission of a neutron, or 26Mg and a γ ray. At high temperature, the (α,n) channel domi…

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