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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

  • Czech description

Classification

  • Type

    D - Article in proceedings

  • CEP classification

  • 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