Movatterモバイル変換


[0]ホーム

URL:


Jump to content
WikipediaThe Free Encyclopedia
Search

Neutron flux

From Wikipedia, the free encyclopedia
Total distance traveled by neutrons within a volume over a time period

icon
This articleneeds additional citations forverification. Please helpimprove this article byadding citations to reliable sources. Unsourced material may be challenged and removed.
Find sources: "Neutron flux" – news ·newspapers ·books ·scholar ·JSTOR
(July 2008) (Learn how and when to remove this message)
Science withneutrons
Foundations
Neutron scattering
Other applications
Infrastructure
Neutron facilities

Theneutron flux is ascalar quantity used innuclear physics andnuclear reactor physics. It is the total distance travelled by all freeneutrons per unit time and volume.[1] Equivalently, it can be defined as the number of neutrons travelling through a small sphere of radiusR{\displaystyle R} in a time interval, divided by a maximal cross section of the sphere (thegreat disk area,πR2{\displaystyle \pi R^{2}}) and by the duration of the time interval.[2]: 82-83 Thedimension of neutron flux isL2T1{\displaystyle {\mathsf {L}}^{-2}{\mathsf {T}}^{-1}} and the usualunit is cm−2s−1 (reciprocalsquare centimetre timesreciprocal second).

Theneutron fluence is defined as the neutron fluxintegrated over a certain time period. So its dimension isL2{\displaystyle {\mathsf {L}}^{-2}} and its usual unit is cm−2 (reciprocal square centimetre). An older term used instead of cm−2 was "n.v.t." (neutrons, velocity, time).[3]

Natural neutron flux

[edit]

Neutron flux inasymptotic giant branchstars and insupernovae is responsible for most of the naturalnucleosynthesis producingelements heavier thaniron. In stars there is a relatively low neutron flux on the order of 105 to 1011 cm−2 s−1, resulting in nucleosynthesis by thes-process (slow neutron-capture process). By contrast, after a core-collapse supernova, there is an extremely high neutron flux, on the order of 1032 cm−2 s−1,[4] resulting in nucleosynthesis by ther-process (rapid neutron-capture process).

Earth atmospheric neutron flux, apparently from thunderstorms, can reach levels of 3·10−2 to 9·10+1 cm−2 s−1.[5][6] However, recent results[7] (considered invalid by the original investigators[8]) obtained with unshielded scintillation neutron detectors show a decrease in the neutron flux during thunderstorms. Recent research appears to support lightning generating 1013–1015 neutrons per discharge viaphotonuclear processes.[9]

Artificial neutron flux

[edit]
Further information:Neutron radiation

Artificial neutron flux refers to neutron flux which is man-made, either as byproducts from weapons or nuclear energy production or for a specific application such as from aresearch reactor or byspallation. A flow of neutrons is often used to initiate thefission of unstable large nuclei. One or more additional neutrons may cause a nucleus to become unstable, causing it to decay (split) to form more stable products. This effect is essential infission reactors andnuclear weapons.

Within a nuclear fission reactor, the neutron flux is the primary quantity measured to control the reaction inside. The flux shape is the term applied to the density or relative strength of the flux as it moves around the reactor. Typically the strongest neutron flux occurs in the middle of the reactor core, becoming lower toward the edges. The higher the neutron flux the greater the chance of a nuclear reaction occurring as there are more neutrons going through an area per unit time.

Reactor vessel wall neutron fluence

[edit]

Areactor vessel of a typical nuclear power plant (PWR) endures in 40 years (32 full reactor years) of operation approximately 6.5×1019 cm−2 (E > 1MeV) of neutron fluence.[10] Neutron flux causes reactor vessels to suffer fromneutron embrittlement and is a major problem with thermonuclear fusion likeITER and other magnetic confinement D-T reactors where fast (originally 14.06 MeV) neutrons damage equipment resulting in short equipment lifetime and huge costs and large volumes of radioactive waste streams.

See also

[edit]

References

[edit]
  1. ^Stamm'ler, Rudi J. J.; Abbate, Máximo Julio (1 July 1983).Methods of Steady-State Reactor Physics in Nuclear Design (1st ed.).Academic Press.ISBN 978-0-12-663320-7.LCCN 82072342.OCLC 9915614.OL 3512075M.
  2. ^Beckurts, Karl-Heinrich; Wirtz, Karl (1964)."5.1.1 Neutron Flux, Neutron Density, and Neutron Current".Neutron Physics. Translated by Dresner, L. (1st ed.).Springer-Verlag.ISBN 978-3-540-03096-6.LCCN 64025646.OCLC 569910840.OL 27986790M – viaInternet Archive.{{cite book}}:ISBN / Date incompatibility (help)
  3. ^M. F. Kaplan (August 1983).Nuclear Radiation and the Properties of Concrete(PDF). University of Cape Town. p. 2. Retrieved14 September 2022.
  4. ^Burbidge, E. Margaret; Burbidge, G. R.; Fowler, William A.; Hoyle, F. (October 1957)."Synthesis of the Elements in Stars".Reviews of Modern Physics.29 (4):548–650.Bibcode:1957RvMP...29..547B.doi:10.1103/RevModPhys.29.547.
  5. ^Gurevich, A. V.; Antonova, V. P. (2012). "Strong Flux of Low-Energy Neutrons Produced by Thunderstorms".Physical Review Letters.108 (12) 125001. American Physical Society.Bibcode:2012PhRvL.108l5001G.doi:10.1103/PhysRevLett.108.125001.PMID 22540588.
  6. ^Gurevich, A. V.; Almenova, A. M. (2016). "Observations of high-energy radiation during thunderstorms at Tien-Shan".Physical Review D.94 (2) 023003. American Physical Society.Bibcode:2016PhRvD..94b3003G.doi:10.1103/PhysRevD.94.023003.
  7. ^Alekseenko, V.; Arneodo, F.; Bruno, G.; Di Giovanni, A.; Fulgion, W.; Gromushkin, D.; Shchegolev, O.; Stenkin, Yu.; Stepanov, V.; Sulakov, V.; Yashin, I. (2015)."Decrease of Atmospheric Neutron Counts Observed during Thunderstorms".Physical Review Letters.114 (12) 125003. American Physical Society.Bibcode:2015PhRvL.114l5003A.doi:10.1103/PhysRevLett.114.125003.PMID 25860750. Archived fromthe original on 19 March 2024.
  8. ^Gurevich, A. V.; Ptitsyn, M. O. (2015). "Comment on "Decrease of Atmospheric Neutron Counts Observed during Thunderstorms"".Physical Review Letters.115 (12) 179501. American Physical Society.Bibcode:2015PhRvL.115q9501G.doi:10.1103/PhysRevLett.115.179501.PMID 26551144.
  9. ^Köhn, Christoph; Diniz, Gabriel; Harakeh, GMushin (2017)."Production mechanisms of leptons, photons, and hadrons and their possible feedback close to lightning leaders".Journal of Geophysical Research: Atmospheres.122 (2). American Geophysical Union: 1366.Bibcode:2017JGRD..122.1365K.doi:10.1002/2016JD025445.PMC 5349290.PMID 28357174.
  10. ^Nuclear Power Plant Borssele Reactor Pressure Vessel Safety Assessment, p. 29, 5.6 Neutron Fluence Calculation.
Fusion power, processes and devices
Core topics
Nuclear fusion
Processes,
methods
Confinement
type
Gravitational
Magnetic
Magneto-inertial
Inertial
Electrostatic
Other forms
Devices,
experiments
Magnetic
confinement
Tokamak
International
Americas
Asia,
Oceania
Europe
Stellarator
Americas
Asia,
Oceania
Europe
Levitated dipole
Pinch
RFP
Field-reversed
configuration
Colliding
Mirror
Magneto-inertial
Inertial
confinement
Laser
Americas
Asia
Europe
Non-laser
Retrieved from "https://en.wikipedia.org/w/index.php?title=Neutron_flux&oldid=1337408425"
Categories:
Hidden categories:

[8]ページ先頭

©2009-2026 Movatter.jp