All

What are you looking for?

All
Projects
Results
Organizations

Quick search

  • Projects supported by TA ČR
  • Excellent projects
  • Projects with the highest public support
  • Current projects

Smart search

  • That is how I find a specific +word
  • That is how I leave the -word out of the results
  • “That is how I can find the whole phrase”

Asymptotic normalization coefficients from the Ne-20(He-3, d)Na-21 reaction and astrophysical factor for Ne-20(p,gamma)Na-21

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F61389005%3A_____%2F06%3A00032224" target="_blank" >RIV/61389005:_____/06:00032224 - isvavai.cz</a>

  • Result on the web

  • DOI - Digital Object Identifier

Alternative languages

  • Result language

    angličtina

  • Original language name

    Asymptotic normalization coefficients from the Ne-20(He-3, d)Na-21 reaction and astrophysical factor for Ne-20(p,gamma)Na-21

  • Original language description

    The Ne-20(p,gamma)Na-21 reaction rate at stellar energies is dominated by capture to the ground state through the tail of a subthreshold resonance state at an excitation energy of 2425 keV in Na-21. Both resonant and direct capture contribute to the reaction rate while direct captures to other bound states are negligible. The overall normalization of direct capture to the subthreshold state is determined by the asymptotic normalization coefficient (ANC). Simultaneously this ANC determines the proton partial width of the subthreshold resonance state. To determine the ANC, the Ne-20(He-3,d)Na-21 proton transfer reaction has been measured, at an incident energy of 25.83 MeV. Angular distributions for proton transfer to the ground and first three excited states were measured, and ANCs were then extracted from comparison with distorted-wave Born approximation calculations. Using these ANCs, we calculated the astrophysical factor for Ne-20(p,gamma)Na-21.

  • Czech name

    Asymptotické normalizační koeficienty z reakce 20Ne(3He, d)21Na a astrofyzikální faktor pro 20Ne(p, gamma)21Na

  • Czech description

    Z naměřených úhlových rozložení byly pomocí výpočtů DWBA určeny ANC. Analýza potvrdila, že je důležitý pouze rezonanční a nerezonanční záchyt jdoucí přes podprahový stav 2 425 keV v 21Na.

Classification

  • Type

    J<sub>x</sub> - Unclassified - Peer-reviewed scientific article (Jimp, Jsc and Jost)

  • CEP classification

    BG - Nuclear, atomic and molecular physics, accelerators

  • OECD FORD branch

Result continuities

  • Project

    Result was created during the realization of more than one project. More information in the Projects tab.

  • Continuities

    P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)<br>Z - Vyzkumny zamer (s odkazem do CEZ)

Others

  • Publication year

    2006

  • Confidentiality

    S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Data specific for result type

  • Name of the periodical

    Physical Review. C

  • ISSN

    0556-2813

  • e-ISSN

  • Volume of the periodical

    73

  • Issue of the periodical within the volume

    3

  • Country of publishing house

    US - UNITED STATES

  • Number of pages

    1

  • Pages from-to

    035806

  • UT code for WoS article

  • EID of the result in the Scopus database