Jump to content
Main menu
Main menu
move to sidebar
hide
Navigation
Main page
Recent changes
Random page
Help about MediaWiki
Special pages
Niidae Wiki
Search
Search
Appearance
Create account
Log in
Personal tools
Create account
Log in
Pages for logged out editors
learn more
Contributions
Talk
Editing
Zeeman effect
(section)
Page
Discussion
English
Read
Edit
View history
Tools
Tools
move to sidebar
hide
Actions
Read
Edit
View history
General
What links here
Related changes
Page information
Appearance
move to sidebar
hide
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!
==Nomenclature== {{Anchor|anomalous}}Historically, one distinguishes between the '''normal''' and an '''anomalous Zeeman effect''' (discovered by [[Thomas Preston (scientist)|Thomas Preston]] in Dublin, Ireland<ref>{{cite journal |last1=Preston |first1=Thomas |title=Radiation phenomena in a strong magnetic field |journal=The Scientific Transactions of the Royal Dublin Society |date=1898 |volume=6 |pages=385–391 |url=https://babel.hathitrust.org/cgi/pt?id=mdp.39015035446916;view=1up;seq=481 |series=2nd series}}</ref>). The anomalous effect appears on transitions where the net [[Spin (physics)|spin]] of the [[electron]]s is non-zero. It was called "anomalous" because the electron spin had not yet been discovered, and so there was no good explanation for it at the time that Zeeman observed the effect. [[Wolfgang Pauli]] recalled that when asked by a colleague as to why he looked unhappy, he replied: "How can one look happy when he is thinking about the anomalous Zeeman effect?"<ref>"Niels Bohr's Times: In Physics, Philosophy, and Polity" By Abraham Pais, page 201.</ref> At higher magnetic field strength the effect ceases to be linear. At even higher field strengths, comparable to the strength of the atom's internal field, the electron coupling is disturbed and the spectral lines rearrange. This is called the [[#Strong field (Paschen–Back effect)|'''Paschen–Back effect''']]. In modern scientific literature, these terms are rarely used, with a tendency to use just the "Zeeman effect". Another rarely used obscure term is '''inverse Zeeman effect''',<ref>{{Cite book |edition = 4 |isbn = 978-0-07-256191-3 |last1 = Jenkins |first1 = Francis |last2 = White |first2 = Harvey |title = Fundamentals of Optics |date = 2001-12-03 |publisher = McGraw-Hill Education}}</ref> referring to the Zeeman effect in an absorption spectral line. A similar effect, splitting of the ''nuclear'' energy levels in the presence of a magnetic field, is referred to as the '''nuclear Zeeman effect'''.<ref>{{Cite book |doi = 10.1088/978-0-7503-6039-5ch7 |last = Dunlap |first = Richard A. |chapter = Hyperfine interactions—part III: the magnetic dipole interaction and the nuclear Zeeman effect |pages = 7-1–7-9 |title = The Mössbauer Effect |edition = 2 | publisher = IOP Publishing |accessdate = 2024-03-04 |year = 2023 |isbn = 978-0-7503-6039-5 |url = https://iopscience.iop.org/book/mono/978-0-7503-6039-5/chapter/bk978-0-7503-6039-5ch7}}</ref>
Summary:
Please note that all contributions to Niidae Wiki may be edited, altered, or removed by other contributors. If you do not want your writing to be edited mercilessly, then do not submit it here.
You are also promising us that you wrote this yourself, or copied it from a public domain or similar free resource (see
Encyclopedia:Copyrights
for details).
Do not submit copyrighted work without permission!
Cancel
Editing help
(opens in new window)
Search
Search
Editing
Zeeman effect
(section)
Add topic