46,133 research outputs found
Star Formation and Relaxation in 379 Nearby Galaxy Clusters
We investigate the relationship between star formation (SF) and level of
relaxation in a sample of 379 galaxy clusters at z < 0.2. We use data from the
Sloan Digital Sky Survey to measure cluster membership and level of relaxation,
and to select star-forming galaxies based on mid-infrared emission detected
with the Wide-Field Infrared Survey Explorer. For galaxies with absolute
magnitudes M_r < -19.5, we find an inverse correlation between SF fraction and
cluster relaxation: as a cluster becomes less relaxed, its SF fraction
increases. Furthermore, in general, the subtracted SF fraction in all unrelaxed
clusters (0.117 +/- 0.003) is higher than that in all relaxed clusters (0.097
+/- 0.005). We verify the validity of our SF calculation methods and membership
criteria through analysis of previous work. Our results agree with previous
findings that a weak correlation exists between cluster SF and dynamical state,
possibly because unrelaxed clusters are less evolved relative to relaxed
clusters.Comment: 6 pages, 4 figures, accepted for publication in Ap
Predictors of disease-free and overall survival in retroperitoneal sarcomas: A modern 16-year multi-institutional study from the United States Sarcoma Collaboration (USSC)
Three path interference using nuclear magnetic resonance: a test of the consistency of Born's rule
The Born rule is at the foundation of quantum mechanics and transforms our
classical way of understanding probabilities by predicting that interference
occurs between pairs of independent paths of a single object. One consequence
of the Born rule is that three way (or three paths) quantum interference does
not exist. In order to test the consistency of the Born rule, we examine
detection probabilities in three path intereference using an ensemble of
spin-1/2 quantum registers in liquid state nuclear magnetic resonance (LSNMR).
As a measure of the consistency, we evaluate the ratio of three way
interference to two way interference. Our experiment bounded the ratio to the
order of , and hence it is consistent with Born's rule.Comment: 11 pages, 4 figures; Improved presentation of figures 1 and 4,
changes made in section 2 to better describe the experiment, minor changes
throughout, and added several reference
Radiation-reaction-induced evolution of circular orbits of particles around Kerr Black Holes
It is demonstrated that, in the adiabatic approximation, non-Equatorial
circular orbits of particles in the Kerr metric (i.e. orbits of constant
Boyer-Lindquist radius) remain circular under the influence of gravitational
radiation reaction. A brief discussion is given of conditions for breakdown of
adiabaticity and of whether slightly non-circular orbits are stable against the
growth of eccentricity.Comment: 23 pages. Revtex 3.0. Inquiries to [email protected]
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