Characteristic frequency of the magnetic radiation of spinor condensates
Zhibing Li, Chengguang Bao
Abstract
The magnetic radiation of the fully-condensed states of 23Na condensates have been studied. A narrow characteristic spectral line with a wave length proportional to N(-2/5) (N is the number of particles) and with a probability of transition proportional to N(17/5) emitted (absorbed) by the condensate was found. It implies that short wave radiation with a huge probability of transition can be obtained if numerous atoms are trapped. A new technique developed by the authors, namely, the analytical forms of the fractional parentage coefficients, was used to calculate analytically the matrix elements between the total spin-states.
Create a lesson
Related papers
Coexistence of Multiple Distinct Corner-State Classes via Nearest-Neighbor Couplings Alone
Luhong Su, Dongyi Wang, Shenglong Guo et al.
Non-Hermitian Two-Kink Control of Corner States in Twisted Chern Bilayers
Xiao-Ming Zhao, Su-Peng Kou
Revealing New Leakage Paths in GAAFETs using Predictive First-Principles Simulations
Denis Mamaluy, Juan P. Mendez, Coleman Cariker et al.
Ultrafast laser-stimulated field emission from a metal: a non-equilibrium Green's functions approach
Luciano Jacopo D'Onofrio, Adolfo Avella, Martin Eckstein
Three-dimensional dopant distribution from a single, out-of-focus spectroscopic image
Michael Deimetry, Timothy Petersen, Matthew Weyland et al.
A nonclassical law of the wall in superfluid helium-4
Mikai Hulse, Musfequs Salehin, Sosuke Inui et al.