Indirect Approach To The H-2(d,p)H-3 Reaction Study

R. Sparta; R. G. Pizzone; C. Spitaleri; M. Aliotta; V. Burjan; S. Cherubini; V. Crucilla; M. Gulino; Z. Hons; G. Kiss; V. Kroha; M. La Cognata; L. Lamia; M. McCleskey; J. Mrazek; S. M. R. Puglia; G. G. Rapisarda; S. Romano; M. L. Sergi; L. Trache; A. Tumino

Indirect Approach To The H-2(d,p)H-3 Reaction Study

R. Sparta, R. G. Pizzone, C. Spitaleri, M. Aliotta, V. Burjan, S. Cherubini, V. Crucilla, M. Gulino, Z. Hons, G. Kiss, V. Kroha, M. La Cognata, L. Lamia, M. McCleskey, J. Mrazek, S. M. R. Puglia, G. G. Rapisarda, S. Romano, M. L. Sergi, L. TracheA. Tumino

School of Physics and Astronomy

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

Abstract / Description of output

In order to understand primordial and stellar nucleosynthesis, we have studied H-2(d,p)H-3 reaction at 0.4 MeV down to astrophysical energies. Knowledge of its S-factor is interesting also to plan reactions for fusion reactors to produce energy. The H-2(d,p)H-3 reaction has been studied through the Trojan Horse Method applied to the three-body reaction H-2(He-3,pt)H, at beam energy of 17 MeV. Once selection of protons and tritons detected in coincidence and the selection of quasi-free events, the obtained S-factor is compared with direct measurements. Such data are in agreement with the direct ones and a pole invariance test has been obtained comparing the present results with another H-2(d,p)H-3 THM measurements, where a different spectator particle was employed.

Original language	English
Title of host publication	EXOTIC NUCLEI AND NUCLEAR - PARTICLE ASTROPHYSICS III: FROM NUCLEI TO STARS
Editors	L Trache, S Stoica, A Smirnov
Place of Publication	MELVILLE
Publisher	American Institute of Physics
Pages	420-424
Number of pages	5
ISBN (Print)	978-0-7354-0859-3
Publication status	Published - 2010
Event	Carpathian Summer School of Physics Conference - Sinaia Duration: 20 Jun 2010 → 3 Jul 2010

Conference

Conference	Carpathian Summer School of Physics Conference
City	Sinaia
Period	20/06/10 → 3/07/10

Keywords / Materials (for Non-textual outputs)

Nuclear Astrophysics
Trojan Horse
H-2(d,p)H-3
Big Bang Nucleosynthesis

Cite this

Sparta, R., Pizzone, R. G., Spitaleri, C., Aliotta, M., Burjan, V., Cherubini, S., Crucilla, V., Gulino, M., Hons, Z., Kiss, G., Kroha, V., La Cognata, M., Lamia, L., McCleskey, M., Mrazek, J., Puglia, S. M. R., Rapisarda, G. G., Romano, S., Sergi, M. L., ... Tumino, A. (2010). Indirect Approach To The H-2(d,p)H-3 Reaction Study. In L. Trache, S. Stoica, & A. Smirnov (Eds.), EXOTIC NUCLEI AND NUCLEAR - PARTICLE ASTROPHYSICS III: FROM NUCLEI TO STARS (pp. 420-424). American Institute of Physics.

@inproceedings{c09aef5cbc664c8eaf3a702d13067456,

title = "Indirect Approach To The H-2(d,p)H-3 Reaction Study",

abstract = "In order to understand primordial and stellar nucleosynthesis, we have studied H-2(d,p)H-3 reaction at 0.4 MeV down to astrophysical energies. Knowledge of its S-factor is interesting also to plan reactions for fusion reactors to produce energy. The H-2(d,p)H-3 reaction has been studied through the Trojan Horse Method applied to the three-body reaction H-2(He-3,pt)H, at beam energy of 17 MeV. Once selection of protons and tritons detected in coincidence and the selection of quasi-free events, the obtained S-factor is compared with direct measurements. Such data are in agreement with the direct ones and a pole invariance test has been obtained comparing the present results with another H-2(d,p)H-3 THM measurements, where a different spectator particle was employed.",

keywords = "Nuclear Astrophysics, Trojan Horse, H-2(d,p)H-3, Big Bang Nucleosynthesis",

author = "R. Sparta and Pizzone, {R. G.} and C. Spitaleri and M. Aliotta and V. Burjan and S. Cherubini and V. Crucilla and M. Gulino and Z. Hons and G. Kiss and V. Kroha and {La Cognata}, M. and L. Lamia and M. McCleskey and J. Mrazek and Puglia, {S. M. R.} and Rapisarda, {G. G.} and S. Romano and Sergi, {M. L.} and L. Trache and A. Tumino",

year = "2010",

language = "English",

isbn = "978-0-7354-0859-3",

pages = "420--424",

editor = "L Trache and S Stoica and A Smirnov",

booktitle = "EXOTIC NUCLEI AND NUCLEAR - PARTICLE ASTROPHYSICS III: FROM NUCLEI TO STARS",

publisher = "American Institute of Physics",

note = "Carpathian Summer School of Physics Conference ; Conference date: 20-06-2010 Through 03-07-2010",

}

Sparta, R, Pizzone, RG, Spitaleri, C, Aliotta, M, Burjan, V, Cherubini, S, Crucilla, V, Gulino, M, Hons, Z, Kiss, G, Kroha, V, La Cognata, M, Lamia, L, McCleskey, M, Mrazek, J, Puglia, SMR, Rapisarda, GG, Romano, S, Sergi, ML, Trache, L & Tumino, A 2010, Indirect Approach To The H-2(d,p)H-3 Reaction Study. in L Trache, S Stoica & A Smirnov (eds), EXOTIC NUCLEI AND NUCLEAR - PARTICLE ASTROPHYSICS III: FROM NUCLEI TO STARS. American Institute of Physics, MELVILLE, pp. 420-424, Carpathian Summer School of Physics Conference, Sinaia, 20/06/10.

TY - GEN

T1 - Indirect Approach To The H-2(d,p)H-3 Reaction Study

AU - Sparta, R.

AU - Pizzone, R. G.

AU - Spitaleri, C.

AU - Aliotta, M.

AU - Burjan, V.

AU - Cherubini, S.

AU - Crucilla, V.

AU - Gulino, M.

AU - Hons, Z.

AU - Kiss, G.

AU - Kroha, V.

AU - La Cognata, M.

AU - Lamia, L.

AU - McCleskey, M.

AU - Mrazek, J.

AU - Puglia, S. M. R.

AU - Rapisarda, G. G.

AU - Romano, S.

AU - Sergi, M. L.

AU - Trache, L.

AU - Tumino, A.

PY - 2010

Y1 - 2010

N2 - In order to understand primordial and stellar nucleosynthesis, we have studied H-2(d,p)H-3 reaction at 0.4 MeV down to astrophysical energies. Knowledge of its S-factor is interesting also to plan reactions for fusion reactors to produce energy. The H-2(d,p)H-3 reaction has been studied through the Trojan Horse Method applied to the three-body reaction H-2(He-3,pt)H, at beam energy of 17 MeV. Once selection of protons and tritons detected in coincidence and the selection of quasi-free events, the obtained S-factor is compared with direct measurements. Such data are in agreement with the direct ones and a pole invariance test has been obtained comparing the present results with another H-2(d,p)H-3 THM measurements, where a different spectator particle was employed.

AB - In order to understand primordial and stellar nucleosynthesis, we have studied H-2(d,p)H-3 reaction at 0.4 MeV down to astrophysical energies. Knowledge of its S-factor is interesting also to plan reactions for fusion reactors to produce energy. The H-2(d,p)H-3 reaction has been studied through the Trojan Horse Method applied to the three-body reaction H-2(He-3,pt)H, at beam energy of 17 MeV. Once selection of protons and tritons detected in coincidence and the selection of quasi-free events, the obtained S-factor is compared with direct measurements. Such data are in agreement with the direct ones and a pole invariance test has been obtained comparing the present results with another H-2(d,p)H-3 THM measurements, where a different spectator particle was employed.

KW - Nuclear Astrophysics

KW - Trojan Horse

KW - H-2(d,p)H-3

KW - Big Bang Nucleosynthesis

M3 - Conference contribution

SN - 978-0-7354-0859-3

SP - 420

EP - 424

BT - EXOTIC NUCLEI AND NUCLEAR - PARTICLE ASTROPHYSICS III: FROM NUCLEI TO STARS

A2 - Trache, L

A2 - Stoica, S

A2 - Smirnov, A

PB - American Institute of Physics

CY - MELVILLE

T2 - Carpathian Summer School of Physics Conference

Y2 - 20 June 2010 through 3 July 2010

ER -

Indirect Approach To The H-2(d,p)H-3 Reaction Study

Abstract / Description of output

Conference

Keywords / Materials (for Non-textual outputs)

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Cite this