The (18)O(p, alpha)(15)N reaction is of primary importance to pin down the uncertainties affecting present-day models of asymptotic giant branch stars. An indirect measurement of the low-energy region of the (18)O(p, alpha)(15)N reaction has been performed by means of the Trojan Horse Method. We discuss why the plane wave approximation is justified by evaluating what changes the more correct DWBA approach introduces.
DWBA momentum distribution and its effect on THM
LAMIA, LIVIO;Pizzone R. G;Sergi M. L;
2010-01-01
Abstract
The (18)O(p, alpha)(15)N reaction is of primary importance to pin down the uncertainties affecting present-day models of asymptotic giant branch stars. An indirect measurement of the low-energy region of the (18)O(p, alpha)(15)N reaction has been performed by means of the Trojan Horse Method. We discuss why the plane wave approximation is justified by evaluating what changes the more correct DWBA approach introduces.File in questo prodotto:
File | Dimensione | Formato | |
---|---|---|---|
c38_lacognata_nn2009.pdf
solo gestori archivio
Tipologia:
Versione Editoriale (PDF)
Licenza:
NON PUBBLICO - Accesso privato/ristretto
Dimensione
340.53 kB
Formato
Adobe PDF
|
340.53 kB | Adobe PDF | Visualizza/Apri |
I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.