Nuclear reaction cross sections at astrophysical energies are key parameters for understanding the primordial universe and the further synthesis of the elements. The Trojan Horse Method (THM) is particularly suitable for their investigation since it makes it possible to overcome the Coulomb barrier and to suppress the electron screening effects in the two-body entrance channel. The method was already applied for a number of astrophysically relevant reactions and accurate descriptions can be found in [1-4].

Nuclear reaction cross sections at astrophysical energies are key parameters for understanding the primordial universe and the further synthesis of the elements. The Trojan Horse Method (THM) is particularly suitable for their investigation since it makes it possible to overcome the Coulomb barrier and to suppress the electron screening effects in the two-body entrance channel. The method was already applied for a number of astrophysically relevant reactions and accurate descriptions can be found in [1-4].

The Trojan-Horse Method applied to the Li-6(p,alpha)He-3 reaction down to astrophysical energies

CHERUBINI, SILVIO;MUSUMARRA, Agatino;ROMANO, Stefano;
2004

Abstract

Nuclear reaction cross sections at astrophysical energies are key parameters for understanding the primordial universe and the further synthesis of the elements. The Trojan Horse Method (THM) is particularly suitable for their investigation since it makes it possible to overcome the Coulomb barrier and to suppress the electron screening effects in the two-body entrance channel. The method was already applied for a number of astrophysically relevant reactions and accurate descriptions can be found in [1-4].
Nuclear reaction cross sections at astrophysical energies are key parameters for understanding the primordial universe and the further synthesis of the elements. The Trojan Horse Method (THM) is particularly suitable for their investigation since it makes it possible to overcome the Coulomb barrier and to suppress the electron screening effects in the two-body entrance channel. The method was already applied for a number of astrophysically relevant reactions and accurate descriptions can be found in [1-4].
File in questo prodotto:
File Dimensione Formato  
160_NPA_2004_Tumino.pdf

non disponibili

Tipologia: Versione Editoriale (PDF)
Dimensione 254 kB
Formato Adobe PDF
254 kB Adobe PDF   Visualizza/Apri

I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.

Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/20.500.11769/14854
Citazioni
  • ???jsp.display-item.citation.pmc??? ND
  • Scopus ND
  • ???jsp.display-item.citation.isi??? 4
social impact