Hydrogen Spectra: Lyman, Balmer, Paschen, Brackett Series

In summary: There is a correlation between energy and radiation in the atomic model, however it is not in a simple way that correlates with temperature. The atomic model describes how radiation is emitted from an atom and it does not follow the simple rule that higher energy photons are emitted at higher temperatures.
  • #1
Hydr0matic
197
1
Let me see if I got this straight... The hydrogen spectra consists of a couple of series - Lyman, Balmer, Paschen, Brackett, etc - which all corresponds to a certain energy transition - Lyman (n>1 -> n=1), Balmer (n>2 -> n=2).. and so on... correct ?
And since n=1 is the ground state, a hydrogen atom in a low energy state will mainly emit lines in the Lyman series, right ?

Isn't it strange that the highest energy photons are emitted at the lowest energy state ?

Exactly what lines are emitted given a certain temperature (or energy state) ? I've been under the impression that all series are emitted seperately, i.e. all lines of a specific series (and only those lines) are emitted at a certain temperature. Is this true ? Or are all alfa-lines (in each series) emitted together, or perhaps just lines within a certain scope, e.g. 1000nm-2000nm ?

If the entire lyman series is emitted at a lower energy state than say the alfa-line in Balmer, does this mean that the transition from say n=100 -> n=1 is more likely to happen than the transition from n=3 -> n=2 ?
i.e. given a certain energy state, are all transitions in a lower series always more likely than any in a higher series ?
 
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  • #2
Isn't it strange that the highest energy photons are emitted at the lowest energy state ?
You sound confused. As you had stated just before, the highest energy photons result from transitions to the ground state. Therefore the energy differences would be the largest.
 
  • #3
Oh :smile: .. by "lowest energy state" I meant the general state of the hydrogen, the temperature, if you will ...

Anything else unclear, perhaps ? let me know ...
 
  • #4
Hydr0matic said:
Oh :smile: .. by "lowest energy state" I meant the general state of the hydrogen, the temperature, if you will ...

Anything else unclear, perhaps ? let me know ...

Hydr0,
AFAIK the electron's energy level in a hydrogen atom does not correspond in a simple way to temperature

a box of hydrogen gas at some temperature will have H2 molecules whizzing around at different speeds----the higher the temp the higher the average speed---and there will be some collisions too. the collisions could transfer energy to the electrons and put them in higher states.


in a simplified picture of the electron energy states, if you pick the right unit and the right energy to be the reference level (the zero on an energy scale is an arbitrary choice you make) then the energy levels are:

-1, -1/4, -1/9, -1/16

you can see the lowest is -1 and they get higher and higher as the electron's orbit absorbs more energy.

and then it can jump down
if it jumps from -1/4 down to -1 then it emits
3/4 of a unit of energy

or if it jumps down from -1/16 to -1/4 then it emits 3/16 units of energy

these are nice units of energy called Rydberg units IIRC
a rydberg unit is 13.6 eV which is about the same as 2 x 10-18 joules

that is, I guess, 2 "attojoules"

anyway you can see if it emits 3/16 of a unit by jumping down to the lower state then you can tell the photon energy in eevee if you want
by multiplying 3/16 by 13.6
 
  • #5
marcus said:
AFAIK the electron's energy level in a hydrogen atom does not correspond in a simple way to temperature
I understand... But there is some relationship isn't there ? I'm basing this assumption on the behaviour of most radiators. Hydrogen isn't even a good radiator, but it is, none the less, a radiator... right ? :smile: .. And I believe we can generally say that, the radiation from a certain piece (or volume) of matter reflects it's temperature, in some way. An extremely hot gas radiates more than a cold gas, and the same goes for any solid.

But the question concerning hydrogen is if there's a wavelength relationship as well - i.e. a perfect radiator will emit higher energy photons at higher temperatures, and lower respectively. Hydrogen on the other hand not only behaves unlike most other radiators, but it appears to behave the opposite !

This isn't a question concerning hydrogen actually, but rather the atomic model. It's seems rather contradictory to me that either
1. there's no correlation between the energy in a single atom and the energy in the entire system of atoms... or
2. the correlation is the opposite of the one described by Planck, i.e. the higher energy in the system, the lower energy photons emitted.

I know Nr 1 isn't true for solids like metalls and such, that follow the Planck law... which is another thing I'm not clear about by the way. If the atomic model doesn't incorporate the Planck law, why do metalls follow it ? What exactly is the source of the radiation in glowing metall ?

I'm guessing there's a big chance I've probably misunderstood something here though :wink: ..
 
  • #6
Hydr0 I have to go out so someone else will
have to respond but remember
a gas of H2 molecules is different from an isolated H atom

the molecules have a lot of other ways to absorb energy
they whiz around they collide they bounce off the walls they
tumble end over end
they can even do a springy action between the two atoms
if the temperature is high enough

at no matter what temp
the most occupied atom state is the ground state
when some accident happens and bumps the electron up in to
a higher state then it quicky radiates off the energy and falls back
to the ground state

the thermal radiation, following Planck curve, must come from
many other things besides the single atom electron state hopping

so discrete spectrum of H atom is different from continuous thermal spectrum

have to go
 
  • #7
marcus said:
at no matter what temp
the most occupied atom state is the ground state
when some accident happens and bumps the electron up in to
a higher state then it quicky radiates off the energy and falls back
to the ground state
marcus said:
so discrete spectrum of H atom is different from continuous thermal spectrum
Yes, I know, but how can't there be any connection between them if the source is one and the same ? (Maybe not true for hydrogen but definitely for metals). ... The radiation curve of iron for example follows Plancks law very nicely, but how is this explained if the radiation really consist of photons radiated (mainly) from the atoms ?
Like you said, at no matter what temp, electrons fall down to ground state emitting higher energy photons.


marcus said:
the molecules have a lot of other ways to absorb energy
they whiz around they collide they bounce off the walls they
tumble end over end
they can even do a springy action between the two atoms
if the temperature is high enough
This is exactly my point. The atomic system isn't isolated from it's surroundings, and in no way is it a "stationary unit". Atoms basically bump around ALL the time, and when they do it's the electrons and protons that interact. So how could the systems not be correlated ?
 
  • #8
Anyone want to continue this discussion with me ?
 
  • #9
Planck's blackbody law *doesn't* apply to a single Hydrogen atom. The blackbody radiation curve arises when you do a statistical analysis of lots and lots of atoms, the most simple case is when you have rectangular prism cavity with a vacuum inside and you just consider the atoms in the walls (as classical harmonic oscillators).

Most of the derivation of the blackbody curve is actually electromagnetism, because it involves finding the energy density of the resonant cavity modes. The "Planck hypothesis", the oh-so-famous origin of h, states that the energy is absorbed or emitted in lumps of hf, and in particular the *average* energy of all the oscillators at frequency f will be:

[tex] E_{av} = \frac{hf}{e^{\frac{hf}{k_{B}T}}-1} [/tex]

where k_B is the Boltzmann constant and T is the temperature of the blackbody. This average is calculated using Boltzmann statistics.

The quantum harmonic oscillator analysis shows that the hypothesis about energy coming in lumps of hf is correct. Since we used harmonic oscillators, not real atoms, there isn't really a connection to atomic energy levels that you are asking about. An analysis using a cavity made of a particular element would probably be *very* difficult.

Can someone with more experience than me make some corrections to this post? It's been a while since I've done the blackbody derivation, and I've never seen it done using atomic energy levels...
 
  • #10
Thnx for replying :)

My point is this:
Kane O'Donnell said:
there isn't really a connection to atomic energy levels that you are asking about.
.. take iron for example. When heating iron it first starts glowing red, then there's a hint of orange, then yellow, then white.. and at last a hint of blue. Analysing the intensity/wavelength relationship in the radiation as a function of temperature would reveal a Planck-like curve. And YET, the same radiation would produce very discrete lines in a spectrometer.
How can photons emitted by atoms follow Plancks' law if there's no connection to atomic energy levels ?
 
  • #11
Well, in the example you give, you *wouldn't* get a very discrete spectrum, because having a gazillion atoms close together causes the energy levels to split into a gazillion finely spaced levels clustered around each of the discrete spectrum. This is a consequence of the exclusion principle. Instead of seeing energy levels, you see energy bands. In a metal such as iron, the bands overlap to a certain extent so you will in fact have a pseudocontinuous spectrum.

This is what I mean by statistical - you get a gazillion atoms together and the emission spectrum of the bulk object is *not* just an amplified version of the emission spectrum for a single atom.

So your intuition is sort of right, but you can't apply single-atom physics directly to a blackbody situation because of the exclusion principle. The energy band phenomena is studied extensively in semiconductor theory and there are plenty of websites explaining it. Try HyperPhysics for a simple explanation.

http://hyperphysics.phy-astr.gsu.edu/hbase/solids/fermi.html

Cheerio!

Kane O'Donnell
 
  • #12
Thnx again, but you're sort of missing my point. Never mind the degree of discreteness in the spectrum, the radiation producing the pseudocontinuous spectrum is still mainly emitted by the atoms, right ? Even though the energy levels split within the atoms the photons are still emitted by the atoms, right ?

So why do these photons follow Planck's law ?

Here's the iron spectrum: http://www.webelements.com/webelements/elements/text/Fe/econ.html

The tiny (I guess) bulk of iron that produced this spectrum would follow Planck's law, even though the radiation obviously originates from energy transitions within the atoms.

How is this possible ? According to everybody, blackbodies have nothing to do with atomic energy levels.
 
  • #13
Hydr0matic said:
Thnx again, but you're sort of missing my point. Never mind the degree of discreteness in the spectrum, the radiation producing the pseudocontinuous spectrum is still mainly emitted by the atoms, right ? Even though the energy levels split within the atoms the photons are still emitted by the atoms, right ?

So why do these photons follow Planck's law ?

Here's the iron spectrum: http://www.webelements.com/webelements/elements/text/Fe/econ.html

The tiny (I guess) bulk of iron that produced this spectrum would follow Planck's law, even though the radiation obviously originates from energy transitions within the atoms.

How is this possible ? According to everybody, blackbodies have nothing to do with atomic energy levels.

You have to understand that the iron block is a black body containing iron atoms that absorb/emit following their discrete spectrum (em field in a given volume).
When you heat your iron block, you have a black body at a given temperature with the known continuous spectrum of the black body. In superpostion, you have the iron atomes that can absorb emit/energy on the discrete spectrum.

Seratend.

Seratend.
 
  • #14
thnx seratend, but I don't see if or how your reply answered my question. Seems you just stated what we already know.
 
  • #15
Hydr0matic said:
thnx seratend, but I don't see if or how your reply answered my question. Seems you just stated what we already know.
Your question:
Hydr0matic said:
The tiny (I guess) bulk of iron that produced this spectrum would follow Planck's law, even though the radiation obviously originates from energy transitions within the atoms.

How is this possible ? According to everybody, blackbodies have nothing to do with atomic energy levels.

I have tried to answer quickly to your question.
If you have a piece of iron, you can model it, in a first approximation as an *empty* box that contains the em field (as you stated above: it has "nothing to do with atomic energy levels", just with boundaries of the box and the input energy given to the box). The radiation spectrum of this box is the well-known continuous black body radiation that depends on the temperature of this box (the external energy given to this box).
Now, inside this box, you have iron atoms that may emit/absorb the continuous black body radiation (simplified model: we assume each iron atom is independent). Therefore, iron atoms can only absorb/release energy on a discrete spectrum (your "atomic energy levels").
If you assume (the model) that this is the only possible way the "independent" iron atoms may interact with the em field of the black box, your piece of iron will radiate all the frequencies of the black body (energy conservation, in a steady state).
Now, you may add the possibility for the iron atoms to release the absorbed energy frequencies through other means (for example phonons). In this case, the external black body spectrum will have (almost) missing frequencies that follows the iron atomic energy levels (i.e. an iron atom absorb a photon then it releases the photon energy through a phonon => the black body radiation loses this photon).
You are free to complicate the model in order to take into account other phenomena.

Seratend.
 

FAQ: Hydrogen Spectra: Lyman, Balmer, Paschen, Brackett Series

What is the significance of the Lyman, Balmer, Paschen, and Brackett series in hydrogen spectra?

The Lyman, Balmer, Paschen, and Brackett series are specific patterns of spectral lines that are observed in the emission or absorption spectra of hydrogen. These series correspond to different energy levels that electrons can transition between within a hydrogen atom.

How are the Lyman, Balmer, Paschen, and Brackett series related to each other?

The Lyman series represents transitions to the ground state (n=1), the Balmer series represents transitions to the first excited state (n=2), the Paschen series represents transitions to the second excited state (n=3), and the Brackett series represents transitions to the third excited state (n=4). As the energy levels increase, the spectral lines are closer together, resulting in the different series overlapping.

Why are the Lyman, Balmer, Paschen, and Brackett series important in astronomy?

The Lyman, Balmer, Paschen, and Brackett series are important in astronomy because they provide valuable information about the composition and physical conditions of celestial objects. By analyzing the spectral lines in the emission or absorption spectra, scientists can determine the chemical composition, temperature, and density of stars, galaxies, and other astronomical objects.

How do the Lyman, Balmer, Paschen, and Brackett series support the Bohr model of the atom?

The Bohr model of the atom states that electrons exist in specific energy levels and can transition between these levels by absorbing or emitting photons of specific energies. The Lyman, Balmer, Paschen, and Brackett series correspond to the different energy levels of the hydrogen atom, providing evidence for the validity of the Bohr model.

Can the Lyman, Balmer, Paschen, and Brackett series be observed in other elements?

While the Lyman, Balmer, Paschen, and Brackett series are specific to hydrogen, other elements also exhibit similar spectral series. For example, helium has a series similar to the Balmer series, and other elements have their own unique series. However, the energy levels and wavelengths of the lines will be different for each element.

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