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
Master equation
(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|Equations governing time evolution of physical systems}} {{about||the master equation used in quantum physics|Lindblad equation|the master equations in Lagrangian gauge theory|Batalin–Vilkovisky formalism|the master theorem for analyzing algorithmic complexity|Master theorem (analysis of algorithms)}} {{More footnotes needed|date=June 2011}} In [[physics]], [[chemistry]], and related fields, '''master equations''' are used to describe the [[time evolution]] of a system that can be modeled as being in a [[probability|probabilistic]] combination of states at any given time, and the switching between states is determined by a [[transition rate matrix]]. The equations are a set of [[differential equations]] – over time – of the probabilities that the system occupies each of the different states. The name was proposed in 1940:<ref>{{Cite journal |last=Cohen |first=E. G. D. |date=July 1990 |title=George E. Uhlenbeck and statistical mechanics |url=https://pubs.aip.org/aapt/ajp/article/58/7/619-625/1043995 |journal=American Journal of Physics |language=en |volume=58 |issue=7 |pages=619–625 |doi=10.1119/1.16504 |bibcode=1990AmJPh..58..619C |issn=0002-9505|url-access=subscription }}</ref><ref>{{Cite journal |last1=Nordsieck |first1=A. |last2=Lamb |first2=W.E. |last3=Uhlenbeck |first3=G.E. |date=1940 |title=On the theory of cosmic-ray showers I: The Furry model and the fluctuation problem |url=https://www.sciencedirect.com/science/article/abs/pii/S0031891440901021 |journal=Physica |language=en |volume=7 |issue=4 |pages=344–360 |doi=10.1016/S0031-8914(40)90102-1|bibcode=1940Phy.....7..344N |hdl=2027.42/32597 |hdl-access=free }}</ref> {{Blockquote | text = ''When the probabilities of the elementary processes are known, one can write down a continuity equation for W, from which all other equations can be derived and which we will call therefore the "master” equation.'' | title = "On the theory of cosmic-ray showers I: The [[Wendell H. Furry|Furry]] model and the fluctuation problem" (1940) | author = Nordsieck, Lamb, and Uhlenbeck }}
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)