Effective Magnetic Field in Ground-State Hydrogen Atom?

Click For Summary
SUMMARY

The discussion focuses on the effective magnetic field (B) experienced by the electron in a ground-state hydrogen atom, which is influenced by the proton's magnetic field. The energy levels of the electron are determined by its magnetic moment (μ) orientation relative to B, resulting in spin up (higher energy) and spin down (lower energy) states. The photon emitted during a spin-flip transition has a wavelength of 21 cm, significant for astronomical observations of hydrogen gas. The effective magnitude of B can be calculated using the equation E=Bμ, with considerations for relativistic effects such as Thomas precession.

PREREQUISITES
  • Understanding of quantum mechanics principles, specifically energy levels in atoms.
  • Familiarity with magnetic moments and their role in atomic physics.
  • Knowledge of the Thomas precession effect in relativistic quantum theory.
  • Ability to apply equations related to energy and magnetic fields, such as E=Bμ.
NEXT STEPS
  • Study the derivation of the magnetic moment (μ) for the electron in hydrogen atoms.
  • Research the implications of Thomas precession in quantum mechanics.
  • Explore the significance of 21 cm radiation in astrophysics and its detection methods.
  • Learn about the relationship between energy levels and magnetic fields in atomic systems.
USEFUL FOR

Students and professionals in physics, particularly those specializing in atomic physics, quantum mechanics, and astrophysics, will benefit from this discussion.

hvthvt
Messages
42
Reaction score
0

Homework Statement



A hydrogen atom in its ground state actually has two possible, closely spaced energy levels because
the electron is in the magnetic field B of the proton (the nucleus). Accordingly, an energy is associated
with the orientation of the electron's magnetic moment (μ) relative to B, and the electron is said to be
either spin up (higher energy) or spin down (lower energy) in that field. If the electron is excited to
the higher-energy level, it can de-excite by spin-flipping and emitting a photon. The wavelength
associated with that photon is 21 cm. (Such a process occurs extensively in the Milky Way galaxy,
and reception of the 21 cm radiation by radio telescopes reveals where hydrogen gas lies between
stars.) What is the effective magnitude of B as experienced by the electron in the ground-state
hydrogen atom?


Homework Equations



E=Bμ
B(total)= B(int) + B(ext)
E=hf

The Attempt at a Solution


I determined the energy with the wavelength given. However, I do not know how to tackle the effective magnitude of B .. The groundstate of an hydrogen atom => 13.6 eV
How can I determine μ? Or do I not need it?
 
Physics news on Phys.org
Of course, you need the magnetic moment of the electron. There's a caveat when doing this. Look at a textbook on atomic physics under the key work "Thomas precession". It's a huge relativistic effect (factor of 2) which you wouldn't expect when thinking within naive non-relativistic QT!
 

Similar threads

  • · Replies 2 ·
Replies
2
Views
2K
  • · Replies 11 ·
Replies
11
Views
3K
Replies
4
Views
2K
  • · Replies 22 ·
Replies
22
Views
4K
Replies
3
Views
2K
  • · Replies 2 ·
Replies
2
Views
2K
  • · Replies 22 ·
Replies
22
Views
3K
Replies
2
Views
2K
Replies
18
Views
4K
Replies
1
Views
2K