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Calculation of fusion rates at extremely low energies in laser plasmas

Published online by Cambridge University Press:  08 June 2011

D. Mascali ,
N. Gambino ,
S. Tudisco ,
A. Anzalone ,
A. Bonanno ,
S. Gammino  and
F. Musumeci
D. Mascali
Affiliation:
INFN - Laboratori Nazionali del Sud, via S. Sofia 62, 95123 Catania, Italy. email: [email protected] Universitá di Catania, Dpt. di Fisica e Astronomia & CSFNSM, Via S. Sofia 64, 95123 Catania, Italy
N. Gambino
Affiliation:
INFN - Laboratori Nazionali del Sud, via S. Sofia 62, 95123 Catania, Italy. email: [email protected] Universitá di Catania, Dpt. di Fisica e Astronomia & CSFNSM, Via S. Sofia 64, 95123 Catania, Italy
S. Tudisco
Affiliation:
INFN - Laboratori Nazionali del Sud, via S. Sofia 62, 95123 Catania, Italy. email: [email protected]
A. Anzalone
Affiliation:
INFN - Laboratori Nazionali del Sud, via S. Sofia 62, 95123 Catania, Italy. email: [email protected]
A. Bonanno
Affiliation:
INAF- Osservatorio Astrofisico di Catania, Via S. Sofia 78, 95123 Catania, Italy
S. Gammino
Affiliation:
INFN - Laboratori Nazionali del Sud, via S. Sofia 62, 95123 Catania, Italy. email: [email protected]
F. Musumeci
Affiliation:
INFN - Laboratori Nazionali del Sud, via S. Sofia 62, 95123 Catania, Italy. email: [email protected] Universitá di Catania, Dpt. di Fisica e Astronomia & CSFNSM, Via S. Sofia 64, 95123 Catania, Italy
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Abstract

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At temperatures and densities that are typical of plasmas produced by lasers pulses interacting with solid targets, at power intensities I > 1012W/cm2, the classical Debye screening factor in nuclear reactions becomes comparable with the one of the solar core. Preliminary calculations about the total number of fusion reactions have been performed following an hydrodynamical approach for the description of the plasma dynamics. This approach is propaedeutic for future measurements of D-D fusion reaction rates.

Keywords

plasmasnuclear reactionshydrodynamics
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 6 , Symposium S274: Advances in Plasma Astrophysics , September 2010 , pp. 44 - 47
Copyright
Copyright © International Astronomical Union 2011

References

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