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D. Mercogliano

3 papers here

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

author position
  • middle author3

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

fields
  • nucl-ex3
ORCID 0009-0002-7265-8023
same name
  • D. Mercogliano — 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

most citedFirst direct measurement of the 64.5 keV resonance strength in 17O(p,γ)18F reaction

10 citations · 18 across the 3 of their papers we have counts for

collaborators

3 papers

nucl-ex2025

Improved direct measurement of low-energy resonances in the 21Ne(p,γ)22Na reaction

R. S. Sidhu, F. Casaburo, E. Masha +57

In the nova temperature range, 0.1 GK <T< 0.4 GK, several low-energy resonances dominate the 21Ne(p,γ)22Na reaction rate, which is currently affected by large uncer…

nucl-ex2025★ 8 cited

The 22Ne(α,n)25Mg reaction -- state of the art, astrophysics, and perspectives

Andreas Best, Philip Adsley, Ryan Amberger +11

One of the most important stellar neutron sources is the 22Ne(α,n)25Mg reaction, which gets activated both during the helium intershell burning in asymptotic giant bran…

nucl-ex2024★ 10 cited

First direct measurement of the 64.5 keV resonance strength in 17O(p,γ)18F reaction

R. M. Gesuè, G. F. Ciani, D. Piatti +50

The CNO cycle is one of the most important nuclear energy sources in stars. At temperatures of hydrostatic H-burning (20 MK < T < 80 MK) the 17O(p,γ)18F reaction ra…

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