Observed intensity of Persistent Lines of Neutral Hydrogen

In summary: The website does not specify how the intensity was observed, but the references seem to focus on calculations rather than observations.
  • #1
edguy99
Gold Member
450
28
The site http://physics.nist.gov/PhysRefData/Handbook/Tables/hydrogentable3.htm shows the intensity of various photon energy values from hydrogen. I was not able to see how this intensity was observed (ie. was it from a specific experiment, or does one simply look at the sun and count photons at this energy?). The references, from what I could see, seem to deal more with calculation of levels rather then calculating observed intensity.

To make the long question short: Why is the 2p3/2 to 1s1/2 (1215.66824 angstroms) transition twice the intensity of the 2p1/2 to 1s1/2 (1215.67364 angstroms) transition? Is it because the 3/2 has 4 states and the 1/2 only 2 states and we assume all the states are equally populated?

Another question: Why is the 2p to 1s transitions 5 times more likely then the 3p to 1s transition? ... what is the general rule for understanding the intensity column?
 
Physics news on Phys.org
  • #2
The intensity of the 2p3/2 to 1s1/2 transition is twice the intensity of the 2p1/2 to 1s1/2 transition because the former has four possible energy levels while the latter has only two. The general rule for understanding the intensity column is that the higher the number, the more likely it is that the transition will occur. For example, the 2p to 1s transitions are five times more likely than the 3p to 1s transitions because they involve more possible energy levels.
 

1. What is the Observed Intensity of Persistent Lines of Neutral Hydrogen?

The Observed Intensity of Persistent Lines of Neutral Hydrogen refers to the level of brightness or strength of the radiation emitted by neutral hydrogen atoms in space. This radiation is commonly observed using radio telescopes.

2. How is the Observed Intensity of Persistent Lines of Neutral Hydrogen measured?

The Observed Intensity of Persistent Lines of Neutral Hydrogen is measured using radio telescopes, which detect the radio waves emitted by neutral hydrogen atoms. These radio waves are then converted into a visual representation called a spectrum, which shows the intensity of the radiation at different wavelengths.

3. What causes variations in the Observed Intensity of Persistent Lines of Neutral Hydrogen?

The Observed Intensity of Persistent Lines of Neutral Hydrogen can vary due to a number of factors. These include the amount of neutral hydrogen present in a given region of space, the temperature and density of the gas, and the presence of nearby sources of radiation.

4. What can the Observed Intensity of Persistent Lines of Neutral Hydrogen tell us about the Universe?

The Observed Intensity of Persistent Lines of Neutral Hydrogen can provide valuable insights into the structure and evolution of the Universe. By studying the intensity of this radiation at different wavelengths, scientists can map out the distribution of neutral hydrogen and trace the history of star formation and galaxy formation.

5. How does the Observed Intensity of Persistent Lines of Neutral Hydrogen relate to dark matter?

The Observed Intensity of Persistent Lines of Neutral Hydrogen can help us indirectly study dark matter, which is a mysterious form of matter that does not emit or absorb light. By studying the distribution of neutral hydrogen gas, which is affected by the gravitational pull of dark matter, scientists can gain a better understanding of the role of dark matter in the Universe.

Similar threads

  • Quantum Physics
Replies
11
Views
1K
  • Quantum Physics
Replies
2
Views
978
Replies
2
Views
1K
  • Quantum Physics
Replies
18
Views
1K
Replies
8
Views
6K
Replies
0
Views
230
Replies
4
Views
4K
Replies
16
Views
1K
  • Other Physics Topics
2
Replies
56
Views
4K
  • Atomic and Condensed Matter
Replies
1
Views
3K
Back
Top