Low-energy d plus d fusion via the Trojan Horse Method

Kód výsledku v IS VaVaI

<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F61389005%3A_____%2F13%3A00398993" target="_blank" >RIV/61389005:_____/13:00398993 - isvavai.cz</a>

Výsledek na webu

<a href="http://dx.doi.org/10.1088/1742-6596/436/1/012073" target="_blank" >http://dx.doi.org/10.1088/1742-6596/436/1/012073</a>

DOI - Digital Object Identifier

<a href="http://dx.doi.org/10.1088/1742-6596/436/1/012073" target="_blank" >10.1088/1742-6596/436/1/012073</a>

Jazyk výsledku

angličtina

Název v původním jazyce

Low-energy d plus d fusion via the Trojan Horse Method

Popis výsledku v původním jazyce

he H-2(d,p)H-3 and H-2(d,n)He-3 reactions have been recently investigated from E-dd=1.5 MeV down to 2 keV, by means of the Trojan Horse Method (THM) applied to the Quasi Free He-3+d interaction at 18 MeV [1]. The knowledge of their fusion cross section at low energies is of interest for pure and applied physics. Both reactions belong to the network of processes to fuel the first inertial confinement fusion reactors in the range of kT= 1 to 30 keV. These energies overlap with the burning temperatures ofdeuterium in the Pre-main sequence of stellar evolution. They are key processes in the Standard Big Bang Nucleosynthesis (SBBN), in an energy region from 50 to 300 keV and experimental data at least up to 1 MeV are required for an accurate calculation ofthe reaction rate. Providing experimental data for both channels from a single experiment and over the entire energy range of interest is crucial for an accurate calculation of the reaction rates. This is what has been obtained from the

Název v anglickém jazyce

Low-energy d plus d fusion via the Trojan Horse Method

Popis výsledku anglicky

he H-2(d,p)H-3 and H-2(d,n)He-3 reactions have been recently investigated from E-dd=1.5 MeV down to 2 keV, by means of the Trojan Horse Method (THM) applied to the Quasi Free He-3+d interaction at 18 MeV [1]. The knowledge of their fusion cross section at low energies is of interest for pure and applied physics. Both reactions belong to the network of processes to fuel the first inertial confinement fusion reactors in the range of kT= 1 to 30 keV. These energies overlap with the burning temperatures ofdeuterium in the Pre-main sequence of stellar evolution. They are key processes in the Standard Big Bang Nucleosynthesis (SBBN), in an energy region from 50 to 300 keV and experimental data at least up to 1 MeV are required for an accurate calculation ofthe reaction rate. Providing experimental data for both channels from a single experiment and over the entire energy range of interest is crucial for an accurate calculation of the reaction rates. This is what has been obtained from the

Druh

D - Stať ve sborníku

CEP obor

BG - Jaderná, atomová a molekulová fyzika, urychlovače

OECD FORD obor

—

Projekt

—

Návaznosti

I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Rok uplatnění

2013

Kód důvěrnosti údajů

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

Název statě ve sborníku

Journal of physics: Conference series

ISBN

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ISSN

1742-6588

e-ISSN

—

Počet stran výsledku

5

Strana od-do

—

Název nakladatele

IOP Publishing

Místo vydání

Bristol

Místo konání akce

Debrecen

Datum konání akce

24. 9. 2012

Typ akce podle státní příslušnosti

WRD - Celosvětová akce

Kód UT WoS článku

000320267700072