|Date||September 29, 2017||Time||3:35 - 5:00 pm|
|Location||Baylor Sciences Building, Room A202|
The Gravitational Lensing Effect of Gravastars
General relativity has told us that the light could be bended by matter. In this way the actual position of the light source may be different from the observation. This kind of phenomenon is very similar to the effect of a lens so we just call it the gravitational lensing effect. I will give a brief review of the concept of the gravitational lensing effect to illustrate the basic ideas. Besides, I will also show some consequence from the analysis of the gravitational lensing by gravastars to make this physical procedure more vivid and explicit.
Reference: T. Kubo and N. Sakai, Phys. Rev. D 93, 084051 (2016)
New Measurement of Antineutrino Oscillation with the Full Detector Configuration at Daya Bay
The completion of the full construction of the Daya Bay Reactor Neutrino Experiment has resulted in a new measurement for electron antineutrino disappearance. Including the 404 days of data collected from October 2012 to November 2013 resulted in a total exposure of 6.9×105 GWth ton days, a 3.6 times increase over previous results. Moreover, improvements have limited variation to .2% between detectors, and reduced background by a factor of 2 in the farthest detectors. Direct prediction of the antineutrino signal in the far detectors based on the measurements in the near detectors explicitly minimized the dependence of the measurement on models of reactor antineutrino emission. As a result, the uncertainties in the estimates were halved. An analysis of the relative antineutrino rates and energy spectra between detectors gave uncertainties of sin22θ13 = 0.084±0.005 and |Δm2 ee| = (2.42±0.11)×10−3 eV2 in the three-neutrino framework.
Reference: F.P. An et al. (Daya Bay Collaboration), Phys. Rev. Lett. 115, 111802 (2015)
|Publisher||Department of Physics|
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