Mean Frequency and Frequency Spread of a Laser Pulse

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Homework Help Overview

The problem involves calculating the mean frequency and frequency spread of a laser pulse operating at a wavelength of 400 nm and producing a 1 femtosecond pulse. The context is within the field of optics and quantum mechanics, particularly focusing on the behavior of light and its interaction with atomic and molecular states.

Discussion Character

  • Exploratory, Conceptual clarification, Mathematical reasoning

Approaches and Questions Raised

  • The original poster attempts to find the mean frequency using a relationship involving the speed of light and wavelength but questions the validity of their approach due to the statistical nature of the wavelengths in the pulse. They express uncertainty about how to proceed without knowing the distribution of wavelengths.
  • Some participants suggest simplifying assumptions, such as treating the pulse as symmetric and using the time-energy uncertainty relation to establish a lower bound on the frequency spread.
  • Others explore the implications of using approximations in the context of probability distributions, discussing the uniform distribution of wavelengths and how it affects the mean value calculations.

Discussion Status

Contextual Notes

Participants note the lack of specific details in the problem statement, which may influence the assumptions they can make about the distribution of wavelengths. The coherence time is also mentioned as a critical factor in determining the frequency spread.

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Homework Statement


Laser probes are being used to examine the states of atoms and molecules at high temporal resolution. A laser operating at a wavelength of 400 nm produces a 1 femtosecond pulse. Compute the mean frequency and frequency spread, ∆ν, of this laser pulse.

Homework Equations


c = f \lambda, \ \Delta \nu \sim \frac{1}{\tau_c}, \ \text{where} \ \tau_c \ \text{is the coherence time.}
3. The Attempt at a Solution [/B]
At first glance, I decided to find the mean frequency using \bar{\nu} = \frac{c}{\bar{\lambda}}. After further consideration, I don't think this necessarily correct since if we think of the wavelengths present in the pulse as following a statistical distribution with ##\mathbb{E}(\lambda) = 400## nm, then by Jensen's inequality, we would have \mathbb{E}\left(\frac{c}{\lambda}\right) = \mathbb{E}(\nu) \geq \frac{c}{\mathbb{E}(\lambda)}. I.e I expect the mean frequency ##\bar{\nu}## to be greater than ##\frac{c}{\bar{\lambda}}.##

I am not sure how to proceed, as I can't compute the exact mean frequency without knowing the distribution of the wavelengths, and I have only found a lower bound for the mean frequency. I could assume that the wavelength is gaussian distributed, but I'd also need to specify the variance of the wavelength in that case.

I took the coherence time ##\tau_c## to be ##10^{-15}## s, so I expect the frequency spread to approximately be ##\Delta \nu \sim 10^{15} ## Hz. Using ##\bar{\nu} = \frac{c}{\bar{\lambda}}##, I get ##\bar{\nu} = 7.5 \times 10^{14}##, which is less than the spread, meaning that according to this calculation, the minimum frequency is ##0##.
 
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I think you are overthinking the problem. From the lack of details given in the problem statement, the appears to be a simple introductory exercise, so you can take the pulse to be symmetric around its peak frequency and to be transform-limited and thus use the time-energy uncertainty relation to get a lower bound on the frequency spread.
 
While you are correct that E[1/X] is not 1/E[X], it's an OK approximation to use when the associated probability distribution is narrow, as you're supposed to assume here.
 
RPinPA said:
While you are correct that E[1/X] is not 1/E[X], it's an OK approximation to use when the associated probability distribution is narrow, as you're supposed to assume here.

It's a good thing to know when you're using an approximation and how good the approximation is. So I explored that a little. Let's assume for simplicity in the calculation that ##\lambda \sim U[a, b]##, that ##\lambda## is uniformly distributed between some values ##a## and ##b##, and we'll define a fractional width ##\epsilon## by ##b = a(1 + \epsilon)##.

So ##b - a = a\epsilon## and ##b + a = a(2 + \epsilon)##.

Clearly the mean value of ##\lambda## is halfway between a and b, ##E[\lambda] = \frac{b + a}{2} = a(1 + \frac{\epsilon}{2})##.

Now what is ##E[1/\lambda]##?

$$E \left [\frac{1}{\lambda} \right ] = \frac{1}{b - a} \int_a^b \frac{d\lambda}{\lambda} = \frac{\ln(b) - \ln(a)}{b-a} = \frac{\ln(b/a)}{b - a} \\
= \frac{\ln(1 + \epsilon)}{a\epsilon} = \frac{1}{a \epsilon} \left (\epsilon - \frac{\epsilon^2}{2} + \frac{\epsilon^3}{3} - \frac{\epsilon^4}{4} + ...\right )\\
= \frac{1}{a} \left (1 - \frac{\epsilon}{2} + \frac{\epsilon^2}{3} - \frac{\epsilon^3}{4} + ... \right )$$
For comparison,
$$\frac {1}{E[\lambda]} = \frac{1}{a} \frac{1}{1 + \frac{\epsilon}{2}} \\
= \frac{1}{a} \left (1 - \frac{\epsilon}{2} + \frac{\epsilon^2}{4} - \frac{\epsilon^3}{8} + ... \right )$$
So as you can see, they are the same to first order in ##\epsilon##. If ##\epsilon^2## is a lot smaller than ##\epsilon## (as it would be for, say, ##\epsilon < 0.01##) then these expressions are approximately the same.
 

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