Constraint logic programming: Difference between revisions
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The '''characteristic rotational temperature''' (θ<sub>R</sub> or θ<sub>rot</sub>) is commonly used in [[statistical thermodynamics]], to simplify the expression of the [[rotational partition function]] and the rotational contribution to molecular thermodynamic properties. It has units of [[temperature]] and is defined as<ref name=Atkins>P. Atkins and J. de Paula "Physical Chemistry", 9th edition (W.H. Freeman 2010), p.597</ref> | |||
<math>\theta _R=\frac{hc \bar B}{k_{B}}=\frac{\hbar ^{2}}{2k_{B}I}</math>, | |||
where B is the [[Rigid rotor#Quantum mechanical linear rigid rotor|rotational constant]], and <math>I</math> is a molecular [[moment of inertia]]. Also h is the [[Planck constant]], c is the [[speed of light]], ħ = h/2π is the [[reduced Planck constant]] and ''k<sub>B</sub>'' is the [[Boltzmann constant]]. | |||
The physical meaning of θ<sub>R</sub> is as an estimate of the temperature at which [[thermal energy]] (of the order of k<sub>B</sub>T) is comparable to the spacing between rotational energy levels (of the order of hcB). At about this temperature the population of excited rotational levels becomes important. Some typical values are 88 K for H<sub>2</sub>, 15.2 K for HCl and 0.561 K for CO<sub>2</sub>.<ref name=Atkins/> | |||
==References== | |||
{{reflist}} | |||
==See also== | |||
*[[Rotational spectroscopy]] | |||
*[[Vibrational temperature]] | |||
*[[Vibrational spectroscopy]] | |||
*[[Infrared spectroscopy]] | |||
*[[Spectroscopy]] | |||
{{DEFAULTSORT:Rotational Temperature}} | |||
[[Category:Atomic physics]] | |||
[[Category:Molecular physics]] | |||
Revision as of 21:03, 7 August 2013
The characteristic rotational temperature (θR or θrot) is commonly used in statistical thermodynamics, to simplify the expression of the rotational partition function and the rotational contribution to molecular thermodynamic properties. It has units of temperature and is defined as[1]
where B is the rotational constant, and is a molecular moment of inertia. Also h is the Planck constant, c is the speed of light, ħ = h/2π is the reduced Planck constant and kB is the Boltzmann constant.
The physical meaning of θR is as an estimate of the temperature at which thermal energy (of the order of kBT) is comparable to the spacing between rotational energy levels (of the order of hcB). At about this temperature the population of excited rotational levels becomes important. Some typical values are 88 K for H2, 15.2 K for HCl and 0.561 K for CO2.[1]
References
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