Published April 15, 1997 | Version v1
Journal article

Systematic analysis of advanced fusion fuel in inertial fusion energy

  • 1. Institute of Nuclear Fusion, J. Gutierrez Abascal, 2 Madrid 28006 Spain (Spain)
  • 2. Soreq Nuclear Research Center (Israel)

Description

Aneutronic fusion reactions can be considered as the cleanest way to exploit nuclear energy. However, these reactions present in general two main drawbacks: - very high temperatures are needed to reach relevant values of their cross sections; - moderate (and even low) energy yield per reaction. This value is still lower if measured in relation to the Z number of the reacting particles. It is already known that bremsstrahlung overruns the plasma reheating by fusion born charged-particles in most of the advanced fuels. This is for instance the case for proton-boron-11 fusion in a stoichiometric plasma and is also so in lithium isotopes fusion reactions. In this paper, the use of deuterium-tritium seeding is suggested to allow to reach higher burnup fractions of advanced fuels, starting at a lower ignition temperature. Of course, neutron production increases as DT contents does. Nevertheless, the ratio of neutron production to energy generation is much lower in DT-advanced fuel mixtures than in pure DT plasmas. One of the main findings of this work is that some natural resources (as D and Li-7) can be burned-up in a catalytic regime for tritium. In this case, neither external tritium breeding nor tritium storage are needed, because the tritium inventory after the fusion burst is the same as before it. The fusion reactor can thus operate on a pure recycling of a small tritium inventory

Additional details

Identifiers

Publishing Information

Journal Title
AIP Conference Proceedings
Journal Volume
406
Journal Issue
1
Journal Page Range
p. 216-223
ISSN
0094-243X
CODEN
APCPCS

Conference

Title
13. international conference on laser interactions and related plasma phenomena
Dates
13-18 Apr 1997
Place
Monterey, CA (United States)

Optional Information

Notes
(c) 1997 American Institute of Physics.