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학술연구/단체지원/교육 등 연구자 활동을 지속하도록 DBpia가 지원하고 있어요.
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연구자들이 자신의 연구와 전문성을 널리 알리고, 새로운 협력의 기회를 만들 수 있는 네트워킹 공간이에요.
논문 기본 정보
- 자료유형
- 학술저널
- 저자정보
- 발행연도
- 2017.1
- 수록면
- 1,199 - 1,210 (12page)
이용수
초록· 키워드
오류제보하기
A new in-line method for sampling neutrons emitted in (α,n) reactions based on alpha particle source information has been developed for continuous-energy Monte Carlo simulations. The new method uses a continuous-slowing-down model coupled with (α,n) cross section data to precompute the expected neutron yield over the alpha particle lifetime. This eliminates the complexity and computational cost associated with explicit charged particle transport. When combined with an integrated alpha particle decay source sampling capability, the proposed method provides an efficient and accurate method for sampling (α,n) neutrons based solely on nuclide inventories in the problem, with no additional user input required. Results from several example calculations show that the proposed method reproduces the (α,n) neutron yields and energy spectra from reference experiments and calculations.
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등록된 정보가 없습니다.
참고문헌 (27)
참고문헌 신청
/ 2002 / COG User's Manual, UCRL-TM-202590 / Lawrence Livermore National Laboratory
A. Ferrari / 2011 / FLUKA: A Multi-Particle Transport Code, Version 2011
B. Lu / 1993 / Chord-length distribution function for two-phase random media / Phys. Rev. E 47 : 2950 ~ 2953
C. Kalbach / 1981 / Phenomenology of continuum angular distributions: I. Systematics and Parametrization / Phys. Rev. C 23 : 112 ~ 123
C. Kalbach / 1988 / Systematics of continuum angular distributions : extensions to higher energies / Phys. Rev. C 37 : 2350 ~ 2370
A. Ferrari / 2011 / FLUKA: A Multi-Particle Transport Code, Version 2011
B. Lu / 1993 / Chord-length distribution function for two-phase random media / Phys. Rev. E 47 : 2950 ~ 2953
C. Kalbach / 1981 / Phenomenology of continuum angular distributions: I. Systematics and Parametrization / Phys. Rev. C 23 : 112 ~ 123
C. Kalbach / 1988 / Systematics of continuum angular distributions : extensions to higher energies / Phys. Rev. C 37 : 2350 ~ 2370
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