scholarly journals Overview on the Trojan Horse Method in nuclear astrophysics

2020 ◽  
Vol 1643 ◽  
pp. 012051
Author(s):  
L. Lamia ◽  
R.G. Pizzone ◽  
M. Mazzocco ◽  
S. Hayakawa ◽  
M. La Cognata ◽  
...  
2012 ◽  
Vol 54 (5-6) ◽  
pp. 745-753 ◽  
Author(s):  
A. Tumino ◽  
C. Spitaleri ◽  
S. Cherubini ◽  
M. Gulino ◽  
M. La Cognata ◽  
...  

2014 ◽  
Vol 569 ◽  
pp. 012018
Author(s):  
A Tumino ◽  
C Spitaleri ◽  
M La Cognata ◽  
L Lamia ◽  
R G Pizzone ◽  
...  

2007 ◽  
Vol 35 (1) ◽  
pp. 014008 ◽  
Author(s):  
S Romano ◽  
C Spitaleri ◽  
S Cherubini ◽  
V Crucillà ◽  
M Gulino ◽  
...  

2010 ◽  
Vol 834 (1-4) ◽  
pp. 639c-642c ◽  
Author(s):  
C. Spitaleri ◽  
S. Cherubini ◽  
M. La Cognata ◽  
L. Lamia ◽  
A. Mukhamedzhanov ◽  
...  

Author(s):  
Roberta Spartà ◽  
Giuseppe G. Rapisarda ◽  
Claudio Spitaleri ◽  
Marco La Cognata ◽  
Rosario G. Pizzone ◽  
...  

The Trojan Horse Method is an indirect method to measure reaction cross sections at energies of interest for nuclear astrophysics, exploiting the nuclei clustering properties. Here it is presented with its general features and detailed for the case of the ^22H(d,p)^33H and ^22H(d,n)^33He measurements, where interesting results for astrophysics and energy fusion power plants have been obtained.


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