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Article title
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Abstract
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Keywords
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Introduction
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Parametrization of the astrophysical factor and temperature dependence of the D + 3He → p + 4He reaction reactivity in different approaches
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Group 1
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Group 2
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Parametrization of the astrophysical factor and temperature dependence on the D + 3He → p + 4He reaction rate based on the effective radius approximation
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Lawson criterion for different scenarios of using D-3He fuel in fusion reactors
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3He self-supply mode (δ = 1)
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Fully catalyzed D-D cycle
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Non-catalyzed D-D cycle for equimolar D-3He fuel (nD = 0.5n)
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Conclusions
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References
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Appendix 1
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