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Einstein solid - Wikipedia

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Einstein solid The Einstein solid is a model of a solid based on two assumptions: Each atom in the lattice is an independent 3D quantum harmonic oscillator All atoms oscillate with the same frequency (contrast with the Debye model) While the assumption that a solid has independent oscillations is very accurate, these oscillations are sound waves or phonons, collective modes involving many atoms. In the Einstein model, however, each atom oscillates independently. Einstein was aware that getting the frequency of the actual oscillations would be difficult, but he nevertheless proposed this theory because it was a particularly clear demonstration that quantum mechanics could solve the specific heat problem in classical mechanics.[1]

Contents Historical impact Einstein's theory of specific heats Heat capacity (microcanonical ensemble) Heat capacity (canonical ensemble) See also References External links

Historical impact The original theory proposed by Einstein in 1907 has great historical relevance. The heat capacity of solids as predicted by the empirical Dulong–Petit law was required by classical mechanics, the specific heat of solids should be independent of temperature. But experiments at low temperatures showed that the heat capacity changes, going to zero at absolute zero. As the temperature goes up, the specific heat goes up until it approaches the Dulong and Petit prediction at high temperature. By employing Planck's quantization assumption, Einstein's theory accounted for the observed experimental trend for the first time. Together with the photoelectric effect, this became one of the most important pieces of evidence for the need of quantization. Einstein used the levels of the quantum mechanical oscillator many years before the advent of modern quantum mechanics.

Einstein's theory of specific heats In Einstein's model, the specific heat approaches zero exponentially fast at low temperatures. This is because all the oscillations have one common frequency. The correct behavior is found by quantizing the normal modes of the solid in the same way that Einstein suggested. Then the frequencies of the waves are not all the same, and the specific heat goes

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to zero as a

https://en.wikipedia.org/wiki/Einstein_solid

power law, which matches experiment. This modification is called the Debye model, which appeared in

1912. When Walther Nernst learned of Einstein's 1906 paper on specific heat,[2] he was so excited that he traveled all the way from Berlin to Zürich to meet with him.[3]

Heat capacity (microcanonical ensemble) The heat capacity of an object at constant volume V is defined through the internal energy U as

, the temperature of the system, can be found from the entropy

To find the entropy consider a solid made of

atoms, each of

which has 3 degrees of freedom. So there are

quantum

harmonic oscillators (hereafter SHOs for "Simple Harmonic Oscillators").

Heat capacity of an Einstein solid as a function of temperature. Experimental value of 3Nk is recovered at high temperatures.

Possible energies of an SHO are given by

or, in other words, the energy levels are evenly spaced and one can define a quantum of energy

which is the smallest and only amount by which the energy of an SHO is increased. Next, we must compute the multiplicity of the system. That is, compute the number of ways to distribute task becomes simpler if one thinks of distributing

or separating stacks of pebbles with

pebbles over

quanta of energy among

SHOs. This

boxes

partitions

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Einstein solid - Wikipedia

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or arranging pebbles and

partitions

The last picture is the most telling. The number of arrangements of arrangements of

pebbles and

partitions is

objects is

. So the number of possible

. However, if partition #3 and partition #5 trade

places, no one would notice. The same argument goes for quanta. To obtain the number of possible distinguishable arrangements one has to divide the total number of arrangements by the number of indistinguishable arrangements. There are

identical quanta arrangements, and

identical partition arrangements. Therefore, multiplicity of

the system is given by

which, as mentioned before, is the number of ways to deposit

quanta of energy into

oscillators. Entropy of the

system has the form

is a huge number—subtracting one from it has no overall effect whatsoever:

With the help of Stirling's approximation, entropy can be simplified:

Total energy of the solid is given by

since there are q energy quanta in total in the system in addition to the ground state energy of each oscillator. Some authors, such as Schroeder, omit this ground state energy in their definition of the total energy of an Einstein solid. We are now ready to compute the temperature

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Elimination of q between the two preceding formulas gives for U:

The first term is associated with zero point energy and does not contribute to specific heat. It will therefore be lost in the next step. Differentiating with respect to temperature to find

we obtain:

or

Although the Einstein model of the solid predicts the heat capacity accurately at high temperatures, it noticeably deviates from experimental values at low temperatures. See Debye model for how to calculate accurate low-temperature heat capacities.

Heat capacity (canonical ensemble) Heat capacity is obtained through the use of the canonical partition function of a simple harmonic oscillator (SHO).

where

substituting this into the partition function formula yields

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This is the partition function of one SHO. Because, statistically, heat capacity, energy, and entropy of the solid are equally distributed among its atoms (SHOs), we can work with this partition function to obtain those quantities and then simply multiply them by

to get the total. Next, let's compute the average energy of each oscillator

where

Therefore,

Heat capacity of one oscillator is then

Up to now, we calculated the heat capacity of a unique degree of freedom, which has been modeled as an SHO. The heat capacity of the entire solid is then given by three (for the three directional degree of freedom) times

, where the total number of degree of freedom of the solid is , the number of atoms in the solid. One thus obtains

which is algebraically identical to the formula derived in the previous section. The quantity

has the dimensions of temperature and is a characteristic property of a crystal. It is known as

the Einstein temperature.[4] Hence, the Einstein Crystal model predicts that the energy and heat capacities of a crystal are universal functions of the dimensionless ratio function of the ratio

. Similarly, the Debye model predicts a universal

.

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See also Kinetic theory of solids

References 1. Mandl, F. (1988) [1971]. Statistical Physics (2nd ed.). Chichester·New York·Brisbane·Toronto·Singapore: John Wiley & sons. ISBN 978-0471915331. 2. Einstein, Albert (1906). "Theorie der Strahlung und die Theorie der Spezifischen Wärme" (http://einsteinpapers.press.princeton.edu/vol2-trans/228) [Planck's theory of radiation and the theory of specific heat]. Annalen der Physik. 4. 22: 180–190, 800. Bibcode:1906AnP...327..180E (http://adsabs.harvard.edu /abs/1906AnP...327..180E). doi:10.1002/andp.19063270110 (https://doi.org/10.1002%2Fandp.19063270110). Retrieved 2016-03-18. 3. Stone, A. D. (2013). Einstein and the Quantum: The Quest of the Valiant Swabian (http://press.princeton.edu/titles /10068.html). Princeton University Press. p. 146. ISBN 978-0-691-13968-5. 4. Rogers, Donald (2005). Einstein's other theory: the Planck-Bose-Einstein theory of heat capacity. Princeton University Press. p. 73. ISBN 0-691-11826-4.

External links Zeleny, Enrique. "The Wolfram Demonstrations Project - Einstein Solid" (http://demonstrations.wolfram.com /EinsteinSolid/). Retrieved 2016-03-18.. Retrieved from "https://en.wikipedia.org/w/index.php?title=Einstein_solid&oldid=821008041"

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