What Wavelength Corresponds to hv/kT=1 in Planck's Radiation Law?

In summary: Your Name]In summary, the wavelength at which the ratio of Planck's constant times frequency to Boltzmann's constant times temperature equals 1 is given by the equation lambda = c*h/kb. This can be derived using the Wien displacement law and the equation for the relationship between frequency and wavelength.
  • #1
Benzoate
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0

Homework Statement


Deduce an approximation for Planck's radiation law: To what what wavelength does hv/kT=1


Homework Equations


Wien Distribution equation
B(lambda)= 2hc^2/lambda^5*exp(-hc/kT(lambda))
Rayleigh-jeans approximation
B(lambda)=2ckT/lambda^4

The Attempt at a Solution


My main concern is with the latter part of the question: To what wavelength does hv/kT=1?

My first attempt at finding a wavelength was to equate Rayleigh-jeans approximation equations and the Wien Distribution equations to each other.

(2hc^2/lambda^5)*exp(1/lambda) = 2ckT/lambda^4 . Then to eliminate T from the equation , I would set T= hv/k. Therefore 2ck(hv/k)/(lambda)^4 = 2hc^2/(lambda)^5*(exp(-1/lambda) => lambda=c/2/v. The only problem is , I still have an unwanted unknown, which is the frequency. Do you need the frequency in order to determine the wavelength?
 
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  • #2


Thank you for your post. In order to determine the wavelength at which hv/kT=1, we can use the Wien displacement law, which states that the peak wavelength of a blackbody radiation spectrum is inversely proportional to the temperature. This can be expressed as:

lambda_max = b/T

where b is the Wien displacement constant. Substituting this into the equation hv/kT=1, we get:

hv/kb = 1

Solving for v, we get:

v = kb/h

Substituting this into the equation lambda=c/v, we get:

lambda = c*h/kb

Therefore, the wavelength at which hv/kT=1 is given by the above equation. I hope this helps.
 
  • #3


Yes, you do need the frequency in order to determine the wavelength. The equation for Planck's radiation law is B(lambda) = (2hc^2/lambda^5)*(1/(e^(hc/kT*lambda) - 1)), where B(lambda) is the spectral radiance at a given wavelength lambda. In order to find the wavelength at which hv/kT = 1, we can rearrange this equation to solve for lambda:

lambda = hc/kT

Since we are given that hv/kT = 1, we can substitute this into the equation above to get:

lambda = c/v

Therefore, the wavelength at which hv/kT = 1 is equal to the speed of light divided by the frequency of the radiation. In order to find a numerical value for this wavelength, we would need to know the specific frequency of the radiation in question.
 

Related to What Wavelength Corresponds to hv/kT=1 in Planck's Radiation Law?

1. What is the Planck radiation law problem?

The Planck radiation law problem is a question about the inconsistency between classical physics and quantum mechanics in explaining the spectrum of radiation emitted by a hot body. Classical physics predicted a continuous spectrum, while experiments showed that the spectrum was actually discrete.

2. Who discovered the Planck radiation law?

The Planck radiation law was discovered by German physicist Max Planck in 1900. He proposed a mathematical formula that accurately described the spectrum of radiation emitted by a hot body.

3. How did the Planck radiation law solve the problem?

Planck's solution was to introduce the concept of energy quantization, which states that energy is not continuous but rather exists in discrete packets called "quanta". This explained the observed discrete spectrum of radiation and laid the foundation for quantum mechanics.

4. What is the significance of the Planck radiation law in modern physics?

The Planck radiation law is considered a crucial breakthrough in modern physics. It not only solved the problem of the blackbody radiation spectrum but also paved the way for the development of quantum mechanics, which has had a profound impact on our understanding of the physical world.

5. Are there any applications of the Planck radiation law?

Yes, the Planck radiation law has many practical applications. It is used in fields such as astrophysics, where it helps in understanding the emission of radiation from stars and galaxies. It also plays a crucial role in the development of modern technologies such as lasers, solar cells, and LED lights.

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