1.1 The Photon Veto Detectors - NA62
As we have described, the way light interacts with atoms is by exerting tugs on the positively charged nuclei and the negatively charged electrons. The tugs ...
Single Atoms on Demand for Cavity QED ExperimentsWe have shown that the radiation pressure exerted by thermal photons is a very efficient source of decoherence, although the corresponding energy damping effect ... Quantum Physics of Light-Matter InteractionsThe liquid crystal can independently change the polarizations in the |D and |A modes, thereby controlling the diagonal (TD) and antidiagonal (TA) transmissions ... Chapter 2, Quantum aspects of light and matter - Boston UniversityFor example, when light passes through matter it exerts forces on the charges, setting them in motion, and delivering momentum to the medium. Since this is ... Arbitrary remote control of photon polarizations for quantum ...In this case, Tsp = TD rather than Tsp = TK and typical turbu- lent velocity contributions to TD will put a 30?120 K floor on measurements of Tsp (see Sect. Electromagnetic Momentum - Reed CollegeThe chapter is divided into five sections which describe the dependence of the TD photon penetration depth on each parameter of interest, i.e., absorption ... STATISTICS OF PHOTON PENETRATION DEPTH IN A TWO ...This inequality defines a range vD of velocities (called the velocity capture range) over which the atomic motion is most effectively damped by Doppler cooling. New Mechanisms for Laser CoolingQuantum Electrodynamical Time-Dependent Density. Functional Theory. Recently, the field of quantum electrodynamics (QED) has gained increas-. Quantum Electrodynamical Time-Dependent Density Functional ...The counterpropagating wave gets closer to resonance and exerts a stronger radiation pres- sure force than the copropagating wave which gets far- ther from ... Manipulating atoms with photons* - Physical Review JournalsWe study radiation pressure due to Ly? line photons, obtaining and exploring analytical expressions for the force-multiplier, MF(NH, ... the cosmic fluidThe typical total power is P = 4 W. For these parameters the trap depth equals |U0| = 3 mK and the photon scattering rate is 32 photons/s. To transfer atoms ... Photon-photon physics at the LHC and laser beam experiments ...particles exert a pressure as well. Friedman I with p??? p+ 3P. 2. Page 2 ... photons in the tail of the thermal distribution can can still ionize. Basics of AstrophysicsThe interest is that the photon-photon interactions happen at unprecedented energies (a few TeV per nucleon pairs) where the quantum ...
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