Nuclear structure constraints on nucleosynthesis

Lídia S. Ferreira; Pooja Siwach; P. Arumugam; Enrico Maglione

doi:10.1393/ncc/i2024-24055-6

Nuclear structure constraints on nucleosynthesis

Lídia S. Ferreira
, Pooja Siwach
, P. Arumugam
, Enrico Maglione

Research output: Contribution to journal › Article › peer-review

Abstract

Nuclear structure properties of proton rich nuclei at the limits of stability are an importance input for nuclear astrophysics models. The theoretical interpretation of the experimental decay data of these nuclei, makes possible the assignment of nuclear levels, and proton separation energies, crucial to understand how the rp process for the formation of the elements flows, and how it ends.

Original language	English (US)
Article number	55
Journal	Nuovo Cimento della Societa Italiana di Fisica C
Volume	47
Issue number	2
DOIs	https://doi.org/10.1393/ncc/i2024-24055-6
State	Published - Mar 2024
Externally published	Yes

ASJC Scopus subject areas

Astronomy and Astrophysics
Physics and Astronomy (miscellaneous)

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10.1393/ncc/i2024-24055-6

Cite this

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title = "Nuclear structure constraints on nucleosynthesis",

abstract = "Nuclear structure properties of proton rich nuclei at the limits of stability are an importance input for nuclear astrophysics models. The theoretical interpretation of the experimental decay data of these nuclei, makes possible the assignment of nuclear levels, and proton separation energies, crucial to understand how the rp process for the formation of the elements flows, and how it ends.",

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AU - Arumugam, P.

AU - Maglione, Enrico

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N2 - Nuclear structure properties of proton rich nuclei at the limits of stability are an importance input for nuclear astrophysics models. The theoretical interpretation of the experimental decay data of these nuclei, makes possible the assignment of nuclear levels, and proton separation energies, crucial to understand how the rp process for the formation of the elements flows, and how it ends.

AB - Nuclear structure properties of proton rich nuclei at the limits of stability are an importance input for nuclear astrophysics models. The theoretical interpretation of the experimental decay data of these nuclei, makes possible the assignment of nuclear levels, and proton separation energies, crucial to understand how the rp process for the formation of the elements flows, and how it ends.

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U2 - 10.1393/ncc/i2024-24055-6

DO - 10.1393/ncc/i2024-24055-6

M3 - Article

AN - SCOPUS:85190528869

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VL - 47

JO - Nuovo Cimento della Societa Italiana di Fisica C

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Nuclear structure constraints on nucleosynthesis

Abstract

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