What is the expression for the spectrum of a hot gas with Doppler broadening?

Click For Summary
SUMMARY

The discussion focuses on deriving the expression for the spectrum of a hot gas exhibiting Doppler broadening due to thermal motion. It is established that the emitted wavelengths form a spectrum influenced by the velocities of gas molecules, with red shifts for molecules moving away and blue shifts for those moving towards the observer. The key formula derived is dP/df = Pt >< dv/df >< fr(v), where Pt represents the total power emitted, fr(v) is the Maxwell-Boltzmann distribution for the radial component of speed, and v(f) is the inverse function relating Doppler frequency to radial velocity.

PREREQUISITES
  • Understanding of Doppler effect in physics
  • Familiarity with Maxwell-Boltzmann distribution
  • Knowledge of thermal motion in gases
  • Basic principles of spectral analysis
NEXT STEPS
  • Study the derivation of the Maxwell-Boltzmann distribution in detail
  • Explore the mathematical formulation of the Doppler effect
  • Learn about spectral broadening mechanisms in astrophysics
  • Investigate applications of Doppler broadening in spectroscopy
USEFUL FOR

Physicists, astrophysicists, and students studying thermodynamics and spectroscopy who are interested in understanding the spectral characteristics of hot gases and the effects of thermal motion on emitted radiation.

broegger
Messages
257
Reaction score
0
Hi,

A very hot gas is enclosed in an oven with a small window. The gas molecules emits radiation at a characteristic wavelength. I assume that because of the thermal motion of the molecules the emitted wavelengths will form a spectrum of some kind (Doppler broadening.) I am trying to derive an expression for this spectrum, but I don't know how... Any hints?

Thanks.
 
Physics news on Phys.org
Yes. There would be no Doppler broadening for molecules moving parallel to the plane of the window. Molecules moving away would have red shift, and molecules moving toward the window would have a blue shift. The higher the temperature, the greater the range of velocities.

Maxwell-Boltzmann distribution - http://hyperphysics.phy-astr.gsu.edu/hbase/kinetic/kintem.html#c2
 
Like Astronuc said, you know the Doppler shift as a function of atomic velocity, and you know the distribution for atomic velocities. It's basically a change of variables.
 
I tried to perform the calculation of the spectrum.
I got the spectrum dP/df (power emitted each frequency unit):

dP/df = Pt >< dv/df >< fr(v)

Pt is the total power emitted by the gas, fr(v) is the Maxwell distribution regarding the radial component of speed (component in observer's direction), and v(f) is the inverse of f(v) which gives the doppler frequency as a function of the radial velocity.
 

Similar threads

  • · Replies 5 ·
Replies
5
Views
2K
Replies
1
Views
4K
  • · Replies 3 ·
Replies
3
Views
3K
  • · Replies 5 ·
Replies
5
Views
2K
  • · Replies 1 ·
Replies
1
Views
2K
  • · Replies 4 ·
Replies
4
Views
3K
  • · Replies 27 ·
Replies
27
Views
5K
  • · Replies 6 ·
Replies
6
Views
3K
  • · Replies 23 ·
Replies
23
Views
3K
  • · Replies 1 ·
Replies
1
Views
1K