216 research outputs found
Molecular level study of hot water extracted green tea buried in soils - a proxy for labile soil organic matter
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Non-destructive optical measurement of relative phase between two Bose condensates
Full text linkWe study the interaction of light with two Bose condensates as an open
quantum system. The two overlapping condensates occupy two different Zeeman
sublevels and two driving light beams induce a coherent quantum tunneling
between the condensates. We derive the master equation for the system. It is
shown that stochastic simulations of the measurements of spontaneously
scattered photons establish the relative phase between two Bose condensates,
even though the condensates are initially in pure number states. These
measurements are non-destructive for the condensates, because only light is
scattered, but no atoms are removed from the system. Due to the macroscopic
quantum interference the detection rate of photons depends substantially on the
relative phase between the condensates. This may provide a way to distinguish,
whether the condensates are initially in number states or in coherent states.Comment: 26 pages, RevTex, 8 postscript figures, 1 MacBinary eps-figur
PTF10fqs: A Luminous Red Nova in the Spiral Galaxy Messier 99
Get PDFThe Palomar Transient Factory (PTF) is systematically charting the optical
transient and variable sky. A primary science driver of PTF is building a
complete inventory of transients in the local Universe (distance less than 200
Mpc). Here, we report the discovery of PTF10fqs, a transient in the luminosity
"gap" between novae and supernovae. Located on a spiral arm of Messier 99, PTF
10fqs has a peak luminosity of Mr = -12.3, red color (g-r = 1.0) and is slowly
evolving (decayed by 1 mag in 68 days). It has a spectrum dominated by
intermediate-width H (930 km/s) and narrow calcium emission lines. The
explosion signature (the light curve and spectra) is overall similar to thatof
M85OT2006-1, SN2008S, and NGC300OT. The origin of these events is shrouded in
mystery and controversy (and in some cases, in dust). PTF10fqs shows some
evidence of a broad feature (around 8600A) that may suggest very large
velocities (10,000 km/s) in this explosion. Ongoing surveys can be expected to
find a few such events per year. Sensitive spectroscopy, infrared monitoring
and statistics (e.g. disk versus bulge) will eventually make it possible for
astronomers to unravel the nature of these mysterious explosions.Comment: 12 pages, 12 figures, Replaced with published versio
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