Calculating Mean Thermal Wavelength for Relativistic Particles | Tutorial"

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To calculate the mean thermal wavelength for relativistic particles, different equations apply for massless and massive particles. For massless particles like photons, the equation is λ = hc/(π^(1/3) 2kT), while for massive particles, the thermal de Broglie wavelength is used. The discussion highlights the importance of the dispersion relation in deriving the thermal wavelength. A referenced paper by Z. Yan proposes a generalized equation for thermal wavelength applicable to all particles in n-dimensional space. Understanding these equations is crucial for accurate calculations in thermal physics.
shahrzad64
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hi
i want to calculate "mean thermal wavelenght for relativistic particles"for example for photon .
i don't khow how can i do it.
please help me.
thankyou.
 
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There are different (final) equations for massless particles than for massive particles. For massless particles, you use,
\lambda = \frac{hc}{\pi^{1/3} 2kT}
and for massive particles, you use the thermal de Broglie wavelength. In general, you can extract a thermal wavelength out of the dispersion relation for the particle.
 
Gokul43201 said:
There are different (final) equations for massless particles than for massive particles. For massless particles, you use,
\lambda = \frac{hc}{\pi^{1/3} 2kT}
and for massive particles, you use the thermal de Broglie wavelength. In general, you can extract a thermal wavelength out of the dispersion relation for the particle.

thankyou for your answer
i know this relation for phonon,but can you send for me relations ,that give this equetion .
in fact ,i don't khow how can i obtain this equation
thankyou
 
One answer is that it is simply defined this way, and needs no derivation, but that would not be an accurate statement. In fact, there is a paper that proposes a generalized equation for the thermal wavelength for all particles (living in n-dimensional space) with a power law dispersion relation.

Z. Yan, "General thermal wavelength and its applications", Eur. J. Phys. 21 (2000) 625
 
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