Dppler and photoelectric effect

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SUMMARY

The discussion centers on the application of the Doppler effect and the photoelectric effect in astrophysics. It establishes that photons emitted from celestial bodies moving away from Earth will have reduced energy, as their observed frequency is lower than the required 5E14 Hz for inducing current in a device needing 600nm wavelength light. The conversation highlights the distinction between normal Doppler shifts and relativistic shifts, emphasizing that the actual frequency must be compared to expected values derived from atomic emission lines to accurately determine the source's characteristics.

PREREQUISITES
  • Doppler effect equations
  • Photoelectric effect principles
  • Lorentz transformation in physics
  • Atomic emission spectra analysis
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  • Study the implications of the Doppler effect on light and sound waves
  • Explore the principles of the photoelectric effect in different materials
  • Learn about the Lorentz transformation and its applications in astrophysics
  • Investigate spectral line analysis for identifying celestial objects
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Astrophysicists, physics students, and anyone interested in understanding the interaction of light with moving celestial bodies and the implications for energy transfer in astrophysical contexts.

Will
Doppler and photoelectric effect

When using the doppler effect equations to determine the speed of celestial objects, what happens to the energy of the photons? If a certain device required a 600nm wavelenth of light and frequency 5E14 Hz to induce current, would photons from a celestial body moving away from Earth and emitting this wavelength have sufficient energy to induce current, since observed f is less than 5E14 Hz and E=hf ?
I was curious as to how astrophysicists can distinguish between one lightsource traveling at v1 with frequency f1 and another with v2,f2 if the observed f is the same for both.
 
Last edited by a moderator:
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Greetings !
Originally posted by Will
I was curious as to how astrophysicists can
distinguish between one lightsource traveling
at v1 with frequency f1 and another with v2,f2
if the observed f is the same for both.
There are two types of shifts for light.
One is normal doppler and the other is
relativistic. The relativistic can only
be distinguished by comparing the
frequency to the one we would expect in
this case (based on expected materials,
compared atomic/molecular emmision lines
and so on). The normal doppler effect
is distinguished by comparing the energy
of the photon according to E = h * frequency
(the signs/smilies menu doesn't work for me,
sorry) to the actual reception frequency.

Live long and prosper.
 


Originally posted by drag
Greetings !

The normal doppler effect
is distinguished by comparing the energy
of the photon according to E = h * frequency
(the signs/smilies menu doesn't work for me,
sorry) to the actual reception frequency.

Live long and prosper.


So the energy equation uses what frequency, actual or observed?
 


Originally posted by Will
So the energy equation uses what frequency, actual or observed?

The actual frequency is the observed frequency.
 


Originally posted by Will
When using the doppler effect equations to determine the speed of celestial objects, what happens to the energy of the photons? If a certain device required a 600nm wavelenth of light and frequency 5E14 Hz to induce current, would photons from a celestial body moving away from Earth and emitting this wavelength have sufficient energy to induce current, since observed f is less than 5E14 Hz and E=hf ?
They would not. Energy depends on reference system.

Say, water will turn turbine falling from 100 m elevation, but it's energy vanishes if you place turbine at zero elevation and becomes negative if you move turbine higher. Bullet energy becomes zero in the co-moving with the bullet reference system.



I was curious as to how astrophysicists can distinguish between one lightsource traveling at v1 with frequency f1 and another with v2,f2 if the observed f is the same for both.

They can't. There is no way of figuring out "original" frequency of passing photon. Thus, they have to use additional information (say, about nature of source). For example, scientists are not exactly sure what was original temperature of CMBR when it was emitted. All they know is that at temperatures about T<(3-5)x1000 K hydrogen becomes transparent to radiation (with temperature T), so thery assume that this was the temperature of radiation (thus, of universe) at time of decoupling of CMBR from matter (hydrogen).
 
Last edited by a moderator:
Greetings !

Will, I'm terribly sorry !
I was somewhat confused myself and now
I apparently transferred my confusion to you.
But, as long as I admit my mistake and
fix it now, all is not lost ! :smile:

Anyway, The normal Doppler effect for light
is the same as for sound. As the source
moves towards/away from you the frequency of
the photons (EM waves) increases/decreases.

Now, when you "add" relativity you must
also use the Lorentz transformation.
The energy of a photon from such a source
will be higher for you than it is
for the source (in terms of the Lorentz
transformation at least).

Now, the Lorenz transformation only really
comes into play when the source is moving at
relativistic velocities. So, the normal
doppler shift is more significant before
you get to velocities close to the speed
of light (0.8 c +). What's important is that
the relativistic energy and hence frequency
increase of the photon occurs in any case -
no matter whether the source moves towards or
away from you.

The doppler shift is v/c.
The Lorentz transformation is 1/ sqrt(1 - sqr(v / c)).

How is the actual frequency discovered ?

Like I mentioned above it is done by comparing
spectral lines and looking for matches for the
type of materials and energy of reactions you
expect to be present at the source.
Fopr example, one well known frequency is
1.420 Gigahertz (hydrogen - which is abundant
in space - 90% of all normal matter) and it's
frequency shift from a the source can be used
to set the whole spectrum "right".

Another issue worth mentioning is the Universal
expansion. basically if you consider that
the Universe expands by about 65 km per Mega Parsec
per second then the photons traveling from the
source to you will also expand according to
the amount of time it took'em to reach you
(their frequency will decrease).
So, you have to account for that in your
calculations and spectral analyses of distant,
in astronomical terms, sources. Alternatively, this
can also be used to make a general estimate of
distance to the source.

Hope I helped this time. :wink:

Live long and prosper.
 

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