Clustering and alpha-capture reaction rates from first-principle structure calculations for nucleosynthesis
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F61389005%3A_____%2F18%3A00499251" target="_blank" >RIV/61389005:_____/18:00499251 - isvavai.cz</a>
Result on the web
<a href="http://dx.doi.org/10.1063/1.5078832" target="_blank" >http://dx.doi.org/10.1063/1.5078832</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1063/1.5078832" target="_blank" >10.1063/1.5078832</a>
Alternative languages
Result language
angličtina
Original language name
Clustering and alpha-capture reaction rates from first-principle structure calculations for nucleosynthesis
Original language description
We outline a new formalism that begins with first-principles structure calculations to describe alpha-clustering, and ultimately leads to a description of alpha-capture reaction rates and impacts on abundance patterns from x-ray burst (XRB) nucle-osynthesis. We utilize a symmetry-adapted basis, which allows us to extend traditional ab initio calculations into the larger model spaces needed for the development of collectivity and clustering in nuclei. In particular, the use of symplectic symmetry allows us to describe spatially expansive states in nuclei - including the Hoyle state of 12C, its 2+ excitation, and B(E2) transitions - with only one or a few basis configurations. For narrow resonances, coupling to the continuum is weak and the number of competing channels is greatly reduced, so most of the physics of the system is described through the overlap of a wave function for the complete A-particle system, computed with a single symplectic configuration (consisting of several hundreds of basis states), and a cluster basis for a single cluster partitioning. This proves to be a very powerful tool for estimating spectroscopic amplitudes, decay widths, and nuclear reaction rates, with the ability to push toward nuclear reactions involving exotic nuclei that cannot currently be measured. We show preliminary results for the 16O(α, γ)20Ne reaction rate, and consider the implications for abundance patterns determined from XRB nucleosynthesis simulations.
Czech name
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Czech description
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Classification
Type
D - Article in proceedings
CEP classification
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OECD FORD branch
10301 - Atomic, molecular and chemical physics (physics of atoms and molecules including collision, interaction with radiation, magnetic resonances, Mössbauer effect)
Result continuities
Project
<a href="/en/project/GA16-16772S" target="_blank" >GA16-16772S: Development of symmetry-guided methods for first principle modeling of medium-mass atomic nuclei</a><br>
Continuities
P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)
Others
Publication year
2018
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Data specific for result type
Article name in the collection
AIP Conference Proceedings
ISBN
978-0-73541-764-9
ISSN
0094-243X
e-ISSN
—
Number of pages
6
Pages from-to
020013
Publisher name
AIP Publishing
Place of publication
Melville
Event location
Texas
Event date
May 13, 2018
Type of event by nationality
WRD - Celosvětová akce
UT code for WoS article
000468354600012