Open main menu
Home
Random
Recent changes
Special pages
Community portal
Preferences
About Wikipedia
Disclaimers
Incubator escapee wiki
Search
User menu
Talk
Dark mode
Contributions
Create account
Log in
Editing
Prompt neutron
(section)
Warning:
You are not logged in. Your IP address will be publicly visible if you make any edits. If you
log in
or
create an account
, your edits will be attributed to your username, along with other benefits.
Anti-spam check. Do
not
fill this in!
{{Short description|Immediate emission of neutrons after nuclear fission}} [[File:Gabab4ff2 hr.jpg|thumb|Diagram of a fission event; the prompt neutrons are emitted in the yellow area, after between 10<sup>β18</sup> and 10<sup>β14</sup> seconds.]] In [[nuclear engineering]], a '''prompt neutron''' is a [[neutron]] immediately emitted ([[neutron emission]]) by a [[nuclear fission]] event, as opposed to a [[delayed neutron|delayed neutron decay]] which can occur within the same context, emitted after [[beta decay]] of one of the [[fission product]]s anytime from a few milliseconds to a few minutes later. Prompt neutrons emerge from the fission of an unstable [[fissionable]] or [[fissile]] heavy nucleus almost instantaneously. There are different definitions for how long it takes for a prompt neutron to emerge. For example, the [[United States Department of Energy]] defines a prompt neutron as a neutron born from fission within 10<sup>β13</sup> seconds after the fission event.<ref>{{Citation|contribution=DOE Fundamentals Handbook - Nuclear Physics and Reactor Theory|title=DOE Fundamentals Handbook - Nuclear Physics and Reactor Theory|contribution-url=https://www.navsea.navy.mil/Portals/103/Documents/NNPTC/Physics/doe_phys_nuc.pdf|page=29 (p. 133 of .pdf format)|series=DOE-HDBK-1019/1-93|date=January 1993 |publisher=[[U.S. Department of Energy]]}}</ref> The U.S. [[Nuclear Regulatory Commission]] defines a prompt neutron as a neutron emerging from fission within 10<sup>β14</sup> seconds.<ref>{{Citation|first=John T.|last=Mihalczo |title=Radiation Detection From Fission|contribution=Radiation Detection From Fission|contribution-url=http://www.ornl.gov/~webworks/cppr/y2004/rpt/121589.pdf?origin=publication_detail|page=1 (p. 11 of .pdf format)|series=ORNL/TM-2004/234|date=November 19, 2004|publisher=[[Oak Ridge National Laboratory]]}}</ref> This emission is controlled by the [[nuclear force]] and is extremely fast. By contrast, so-called delayed neutrons are delayed by the time delay associated with beta decay (mediated by the [[Weak interaction|weak force]]) to the precursor excited nuclide, after which neutron emission happens on a prompt time scale (i.e., almost immediately).
Edit summary
(Briefly describe your changes)
By publishing changes, you agree to the
Terms of Use
, and you irrevocably agree to release your contribution under the
CC BY-SA 4.0 License
and the
GFDL
. You agree that a hyperlink or URL is sufficient attribution under the Creative Commons license.
Cancel
Editing help
(opens in new window)