Mean Frequency and Frequency Spread of a Laser Pulse

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SUMMARY

The discussion focuses on calculating the mean frequency and frequency spread (∆ν) of a laser pulse operating at a wavelength of 400 nm and producing a 1 femtosecond pulse. The mean frequency is derived using the formula \(\bar{\nu} = \frac{c}{\bar{\lambda}}\), resulting in \(\bar{\nu} = 7.5 \times 10^{14}\) Hz, while the frequency spread is approximated to be \(\Delta \nu \sim 10^{15}\) Hz based on a coherence time (\(\tau_c\)) of \(10^{-15}\) s. The discussion emphasizes the importance of understanding statistical distributions of wavelengths and the use of approximations in calculations, particularly when assuming a uniform distribution of wavelengths.

PREREQUISITES
  • Understanding of laser physics and pulse duration
  • Familiarity with the coherence time concept in optics
  • Knowledge of statistical distributions, particularly Gaussian and uniform distributions
  • Proficiency in applying the time-energy uncertainty relation
NEXT STEPS
  • Explore the implications of coherence time on laser performance
  • Learn about the statistical properties of laser pulse wavelengths
  • Investigate the time-energy uncertainty principle in quantum mechanics
  • Study advanced laser pulse shaping techniques and their applications
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Students and professionals in physics, particularly those focused on optics and laser technology, as well as researchers analyzing atomic and molecular states using high temporal resolution laser probes.

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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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