17,660 research outputs found
The investigation of critical pressure burning of fuel droplets Annual report, 1 Jan. - 31 Dec. 1970
Experimental and theoretical results of critical pressure burning of fuel droplet
Three-dimensional power Doppler evaluation of cerebral vascular blood flow: A novel tool in the assessment of fetal growth restriction
Parrondo-like behavior in continuous-time random walks with memory
The Continuous-Time Random Walk (CTRW) formalism can be adapted to encompass
stochastic processes with memory. In this article we will show how the random
combination of two different unbiased CTRWs can give raise to a process with
clear drift, if one of them is a CTRW with memory. If one identifies the other
one as noise, the effect can be thought as a kind of stochastic resonance. The
ultimate origin of this phenomenon is the same of the Parrondo's paradox in
game theoryComment: 8 pages, 3 figures, revtex; enlarged and revised versio
Orally bioavailable glutamine antagonist prodrug JHU-083 penetrates mouse brain and suppresses the growth of MYC-driven medulloblastoma
Multi Spectural Flourescence Imager (MSFI)
Genetic transformation with in vivo reporter genes for fluorescent proteins can be performed on a variety of organisms to address fundamental biological questions. Model organisms that may utilize an ISS imager include unicellular organisms (Saccharomyces cerevisiae), plants (Arabidopsis thaliana), and invertebrates (Caenorhabditis elegans)
Minimal Brownian Ratchet: An Exactly Solvable Model
We develop an exactly-solvable three-state discrete-time minimal Brownian
ratchet (MBR), where the transition probabilities between states are
asymmetric. By solving the master equations we obtain the steady-state
probabilities. Generally the steady-state solution does not display detailed
balance, giving rise to an induced directional motion in the MBR. For a reduced
two-dimensional parameter space we find the null-curve on which the net current
vanishes and detailed balance holds. A system on this curve is said to be
balanced. On the null-curve, an additional source of external random noise is
introduced to show that a directional motion can be induced under the zero
overall driving force. We also indicate the off-balance behavior with biased
random noise.Comment: 4 pages, 4 figures, RevTex source, General solution added. To be
appeared in Phys. Rev. Let
Patterns and correlates of use of evidence-based interventions to control diabetes by local health departments across the USA
Coherent Radiation from Extensive Air Showers in the Ultra-High Frequency Band
Using detailed Monte Carlo simulations we have characterized the features of
the radio emission of inclined air showers in the Ultra-High Frequency band
(300 MHz - 3 GHz). The Fourier-spectrum of the radiation is shown to have a
sizable intensity well into the GHz frequency range. The emission is mainly due
to transverse currents induced by the geomagnetic field and to the excess
charge produced by the Askaryan effect. At these frequencies only a
significantly reduced volume of the shower around the axis contributes
coherently to the signal observed on the ground. The size of the coherently
emitting volume depends on frequency, shower geometry and observer position,
and is interpreted in terms of the relative time delays. At ground level, the
maximum emission at high frequencies is concentrated in an elliptical ring-like
region around the intersection of a Cherenkov cone with its vertex at shower
maximum and the ground. The frequency spectrum of inclined showers when
observed at positions that view shower maximum in the Cherenkov direction, is
shown to be in broad agreement with the pulses detected by the Antarctic
Impulsive Transient Antenna (ANITA) experiment, making the interpretation that
they are due to Ultra-High Energy Cosmic Ray atmospheric showers consistent
with our simulations. These results are also of great importance for
experiments aiming to detect molecular bremsstrahlung radiation in the GHz
range as they present an important background for its detection.Comment: 8 pages, 8 figure
PKSB1740-517: An ALMA view of the cold gas feeding a distant interacting young radio galaxy
Cold neutral gas is a key ingredient for growing the stellar and central
black hole mass in galaxies throughout cosmic history. We have used the Atacama
Large Millimetre Array (ALMA) to detect a rare example of redshifted
CO(2-1) absorption in PKS B1740-517, a young (
yr) and luminous ( erg s ) radio
galaxy at that is undergoing a tidal interaction with at least one
lower-mass companion. The coincident HI 21-cm and molecular absorption have
very similar line profiles and reveal a reservoir of cold gas ( M), likely distributed in a disc or ring within
a few kiloparsecs of the nucleus. A separate HI component is kinematically
distinct and has a very narrow line width ( km
s), consistent with a single diffuse cloud of cold (
K) atomic gas. The CO(2-1) absorption is not associated with this
component, which suggests that the cloud is either much smaller than 100 pc
along our sight-line and/or located in low-metallicity gas that was possibly
tidally stripped from the companion. We argue that the gas reservoir in PKS
B1740-517 may have accreted onto the host galaxy 50 Myr before the young
radio AGN was triggered, but has only recently reached the nucleus. This is
consistent with the paradigm that powerful luminous radio galaxies are
triggered by minor mergers and interactions with low-mass satellites and
represent a brief, possibly recurrent, active phase in the life cycle of
massive early type galaxies.Comment: 15 pages, 7 figures, accepted for publication in MNRA
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