General expression of chemical potential for Bose Einstein condensate in an anisotropic magnetic trap

2004 ◽  
Author(s):  
Shri-Prakash Tewari ◽  
Poonam Silotia ◽  
Aditya Saxena
Keyword(s):  
General Expression ◽  
Magnetic Trap ◽  
Chemical Potential ◽  
Einstein Condensate ◽  
Bose Einstein Condensate ◽  
Bose Einstein

Centrifugal effects in a Bose-Einstein condensate in the time-orbiting-potential magnetic trap

1997 ◽  
Vol 55 (1) ◽  
pp. 488-497 ◽  
Author(s):  
A. B. Kuklov ◽  
N. Chencinski ◽  
A. M. Levine ◽  
W. M. Schreiber ◽  
Joseph L. Birman
Keyword(s):  
Magnetic Trap ◽  
Einstein Condensate ◽  
Bose Einstein Condensate ◽  
Bose Einstein

scholarly journals Collective Excitations of a Bose-Einstein Condensate in a Magnetic Trap

1996 ◽  
Vol 77 (6) ◽  
pp. 988-991 ◽  
Author(s):  
M.-O. Mewes ◽  
M. R. Andrews ◽  
N. J. van Druten ◽  
D. M. Kurn ◽  
D. S. Durfee ◽  
...  
Keyword(s):  
Magnetic Trap ◽  
Einstein Condensate ◽  
Collective Excitations ◽  
Bose Einstein Condensate ◽  
Bose Einstein

scholarly journals Quantum dephasing of normal modes of a Bose-Einstein condensate in a magnetic trap

1997 ◽  
Vol 55 (5) ◽  
pp. R3307-R3310 ◽  
Author(s):  
A. B. Kuklov ◽  
N. Chencinski ◽  
A. M. Levine ◽  
W. M. Schreiber ◽  
Joseph L. Birman
Keyword(s):  
Magnetic Trap ◽  
Normal Modes ◽  
Einstein Condensate ◽  
Bose Einstein Condensate ◽  
Bose Einstein

scholarly journals Dark Matter as a Non-Relativistic Bose–Einstein Condensate with Massive Gravitons

Symmetry ◽  
2018 ◽  
Vol 10 (10) ◽  
pp. 520 ◽  
Author(s):  
Emma Kun ◽  
Zoltán Keresztes ◽  
Saurya Das ◽  
László Á. Gergely
Keyword(s):  
Dark Matter ◽  
Chemical Potential ◽  
Yukawa Potential ◽  
Scattering Length ◽  
Einstein Condensate ◽  
Graviton Mass ◽  
Bose Einstein Condensate ◽  
Upper Limits ◽  
Bose Einstein ◽  
Exponential Disk

We confront a non-relativistic Bose–Einstein Condensate (BEC) model of light bosons interacting gravitationally either through a Newtonian or a Yukawa potential with the observed rotational curves of 12 dwarf galaxies. The baryonic component is modeled as an axisymmetric exponential disk and its characteristics are derived from the surface luminosity profile of the galaxies. The purely baryonic fit is unsatisfactory, hence a dark matter component is clearly needed. The rotational curves of five galaxies could be explained with high confidence level by the BEC model. For these galaxies, we derive: (i) upper limits for the allowed graviton mass; and (ii) constraints on a velocity-type and a density-type quantity characterizing the BEC, both being expressed in terms of the BEC particle mass, scattering length and chemical potential. The upper limit for the graviton mass is of the order of 10 - 26 eV/c2, three orders of magnitude stronger than the limit derived from recent gravitational wave detections.

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