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257 - M. Egorov , A. Fix 2014
Coherent photoproduction of two neutral pions on the deuteron and ^3He is calculated. The isoscalar and isovector parts of the elementary photoproduction amplitude was determined by fitting the measured total cross section on protons and neutrons. Th e dependence of the cross section on the isospin of the target nucleus is discussed.
We use collective oscillations of a two-component Bose-Einstein condensate (2CBEC) of Rb atoms prepared in the internal states $ket{1}equivket{F=1, m_F=-1}$ and $ket{2}equivket{F=2, m_F=1}$ for the precision measurement of the interspecies scattering length $a_{12}$ with a relative uncertainty of $1.6times 10^{-4}$. We show that in a cigar-shaped trap the three-dimensional (3D) dynamics of a component with a small relative population can be conveniently described by a one-dimensional (1D) Schr{o}dinger equation for an effective harmonic oscillator. The frequency of the collective oscillations is defined by the axial trap frequency and the ratio $a_{12}/a_{11}$, where $a_{11}$ is the intra-species scattering length of a highly populated component 1, and is largely decoupled from the scattering length $a_{22}$, the total atom number and loss terms. By fitting numerical simulations of the coupled Gross-Pitaevskii equations to the recorded temporal evolution of the axial width we obtain the value $a_{12}=98.006(16),a_0$, where $a_0$ is the Bohr radius. Our reported value is in a reasonable agreement with the theoretical prediction $a_{12}=98.13(10),a_0$ but deviates significantly from the previously measured value $a_{12}=97.66,a_0$ cite{Mertes07} which is commonly used in the characterisation of spin dynamics in degenerate Rb atoms. Using Ramsey interferometry of the 2CBEC we measure the scattering length $a_{22}=95.44(7),a_0$ which also deviates from the previously reported value $a_{22}=95.0,a_0$ cite{Mertes07}. We characterise two-body losses for the component 2 and obtain the loss coefficients ${gamma_{12}=1.51(18)times10^{-14} textrm{cm}^3/textrm{s}}$ and ${gamma_{22}=8.1(3)times10^{-14} textrm{cm}^3/textrm{s}}$.
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