TY - JOUR
T1 - Planck distribution of phonons in a bose-einstein condensate
AU - Schley, R.
AU - Berkovitz, A.
AU - Rinott, S.
AU - Shammass, I.
AU - Blumkin, A.
AU - Jeff, Steinhauer
N1 - Israel Science FoundationWe thank N. Pavloff, L. I. Glazman, L. P. Pitaevskii, G. V. Shlyapnikov, R. J. Rivers, I. Zapata, R. Pugatch, D. Podolsky, J. R. Anglin, B. Damski, W. H. Zurek, E. Polturak, Y. Kafri, and B. Shapiro for helpful conversations. This work was supported by the Israel Science Foundation.
PY - 2013/7/29
Y1 - 2013/7/29
N2 - The Planck distribution of photons emitted by a blackbody led to the development of quantum theory. An analogous distribution of phonons should exist in a Bose-Einstein condensate. We observe this Planck distribution of thermal phonons in a 3D condensate. This observation provides an important confirmation of the basic nature of the condensate's quantized excitations. In contrast to the bunching effect, the density fluctuations are seen to increase with increasing temperature. This is due to the nonconservation of the number of phonons. In the case of rapid cooling, the phonon temperature is out of equilibrium with the surrounding thermal cloud. In this case, a Bose-Einstein condensate is not as cold as previously thought. These measurements are enabled by our in situ k-space technique.
AB - The Planck distribution of photons emitted by a blackbody led to the development of quantum theory. An analogous distribution of phonons should exist in a Bose-Einstein condensate. We observe this Planck distribution of thermal phonons in a 3D condensate. This observation provides an important confirmation of the basic nature of the condensate's quantized excitations. In contrast to the bunching effect, the density fluctuations are seen to increase with increasing temperature. This is due to the nonconservation of the number of phonons. In the case of rapid cooling, the phonon temperature is out of equilibrium with the surrounding thermal cloud. In this case, a Bose-Einstein condensate is not as cold as previously thought. These measurements are enabled by our in situ k-space technique.
UR - http://www.scopus.com/inward/record.url?scp=84881493652&partnerID=8YFLogxK
U2 - 10.1103/PhysRevLett.111.055301
DO - 10.1103/PhysRevLett.111.055301
M3 - مقالة
SN - 0031-9007
VL - 111
JO - Physical Review Letters
JF - Physical Review Letters
IS - 5
M1 - 055301
ER -