1975
DOI: 10.1103/physrevb.11.1059
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Microscopic theory of surface excitations in superfluidHe4

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Cited by 39 publications
(12 citation statements)
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“…A good starting calculation for S(q ʈ ,) in the films is to use the Feynman theory of excitations 25 ͑generalized to the inhomogeneous geometry 26 ͒, where the elementary excitations are described by the ground state being modified by single density fluctuations. 22 Experience has shown that in spite of quantitative deficiencies, the qualitative features of the model are quite satisfactory.…”
Section: ͑22͒mentioning
confidence: 99%
“…A good starting calculation for S(q ʈ ,) in the films is to use the Feynman theory of excitations 25 ͑generalized to the inhomogeneous geometry 26 ͒, where the elementary excitations are described by the ground state being modified by single density fluctuations. 22 Experience has shown that in spite of quantitative deficiencies, the qualitative features of the model are quite satisfactory.…”
Section: ͑22͒mentioning
confidence: 99%
“…Similarly, a negative temperature fluctuation will induce a continual decrease in temperature. The surface energy contribution of the zero-point motion of the phonon modes is readily obtained from (56) and (14). We find = ---+ 2F(x)-2 log tanh (60) 8zr where x = 2,rrTa/hc.…”
Section: Of Phonons Is Includedmentioning
confidence: 96%
“…The probability density is thus of the same form as before, with b 2 rcTr/hc d)~(r, T)-~ -r2 sinh (IrTr/hc) (56) and so the kinetic energy term --(h2/4m)V2~p in the total energy again has the form of a repulsive interaction. The screening length hc/~'T is approximately 5.8/~ at 1 K. Inserting (56) into (14) and considering contributions from particle separations greater than 2a, we find that the finite-temperature phonon zero-point motion contribution to the bulk energy is (when 27rTR/hc >> 1) 2 R 3 /2~rTa\ AEv=-~(hcno)~a F~--~c ) (57) where 1 x ( x cosh x~…”
Section: Of Phonons Is Includedmentioning
confidence: 99%
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