1,714 research outputs found
Hamilton-Jacobi Method and Gravitation
Studying the behaviour of a quantum field in a classical, curved, spacetime
is an extraordinary task which nobody is able to take on at present time.
Independently by the fact that such problem is not likely to be solved soon,
still we possess the instruments to perform exact predictions in special,
highly symmetric, conditions. Aim of the present contribution is to show how it
is possible to extract quantitative information about a variety of physical
phenomena in very general situations by virtue of the so-called Hamilton-Jacobi
method. In particular, we shall prove the agreement of such semi-classical
method with exact results of quantum field theoretic calculations.Comment: To appear in the proceedings of "Cosmology, the Quantum Vacuum, and
Zeta Functions": A workshop with a celebration of Emilio Elizalde's Sixtieth
birthday, Bellaterra, Barcelona, Spain, 8-10 Mar 201
Detectability of Exoplanetary Transits from Radial Velocity Surveys
Of the known transiting extra-solar planets, a few have been detected through
photometric follow-up observations of radial velocity planets. Perhaps the best
known of these is the transiting exoplanet HD 209458b. For hot Jupiters
(periods less than ~5 days), the a priori information that 10% of these planets
will transit their parent star due to the geometric transit probability leads
to an estimate of the expected transit yields from radial velocity surveys. The
radial velocity information can be used to construct an effective photometric
follow-up strategy which will provide optimal detection of possible transits.
Since the planet-harbouring stars are already known in this case, one is only
limited by the photometric precision achieveable by the chosen
telescope/instrument. The radial velocity modelling code presented here
automatically produces a transit ephemeris for each planet dataset fitted by
the program. Since the transit duration is brief compared with the fitted
period, we calculate the maximum window for obtaining photometric transit
observations after the radial velocity data have been obtained, generalising
for eccentric orbits. We discuss a typically employed survey strategy which may
contribute to a possible radial velocity bias against detection of the very hot
Jupiters which have dominated the transit discoveries. Finally, we describe how
these methods can be applied to current and future radial velocity surveys.Comment: 11 pages, 8 figures, accepted for publication in MNRAS, minor
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LinkMind: Link Optimization in Swarming Mobile Sensor Networks
A swarming mobile sensor network is comprised of a swarm of wirelessly connected mobile robots equipped with various sensors. Such a network can be applied in an uncertain environment for services such as cooperative navigation and exploration, object identification and information gathering. One of the most advantageous properties of the swarming wireless sensor network is that mobile nodes can work cooperatively to organize an ad-hoc network and optimize the network link capacity to maximize the transmission of gathered data from a source to a target. This paper describes a new method of link optimization of swarming mobile sensor networks. The new method is based on combination of the artificial potential force guaranteeing connectivities of the mobile sensor nodes and the max-flow min-cut theorem of graph theory ensuring optimization of the network link capacity. The developed algorithm is demonstrated and evaluated in simulation
On the Eccentricity Distribution of Short-Period Single-Planet Systems
We apply standard Markov chain Monte Carlo (MCMC) analysis techniques for 50
short- period, single-planet systems discovered with radial velocity technique.
We develop a new method for accessing the significance of a non-zero orbital
eccentricity, namely {\Gamma} analysis, which combines frequentist bootstrap
approach with Bayesian analysis of each simulated data set. We find the
eccentricity estimations from {\Gamma} analysis are generally consistent with
results from both standard MCMC analysis and previous references. The {\Gamma}
method is particular useful for assessing the significance of small
eccentricities. Our results suggest that the current sample size is
insufficient to draw robust conclusions about the roles of tidal interaction
and perturbations in shaping the eccentricity distribution of short-period
single-planet systems. We use a Bayesian population analysis to show that a
mixture of analytical distributions is a good approximation of the underlying
eccentricity distribution. For short-period planets, we find the most probable
values of parameters in the analytical functions given the observed
eccentricities. These analytical functions can be used in theoretical
investigations or as priors for the eccentricity distribution when analyzing
short-period planets. As the measurement precision improves and sample size
increases, the method can be applied to more complex parametrizations for the
underlying distribution of eccentricity for extrasolar planetary systems.Comment: 13 pages, 11 figures, 4 tables, accepted by MNRA
The First Extrasolar Planet Discovered with a New Generation High Throughput Doppler Instrument
We report the detection of the first extrasolar planet, ET-1 (HD 102195b),
using the Exoplanet Tracker (ET), a new generation Doppler instrument. The
planet orbits HD 102195, a young star with solar metallicity that may be part
of the local association. The planet imparts radial velocity variability to the
star with a semiamplitude of m s and a period of 4.11 days.
The planetary minimum mass () is .Comment: 42 pages, 11 figures and 5 tables, Accepted for publication in Ap
Emission from the D1D5 CFT: Higher Twists
We study a certain class of nonextremal D1D5 geometries and their ergoregion
emission. Using a detailed CFT computation and the formalism developed in
arXiv:0906.2015 [hep-th], we compute the full spectrum and rate of emission
from the geometries and find exact agreement with the gravity answer.
Previously, only part of the spectrum had been reproduced using a CFT
description. We close with a discussion of the context and significance of the
calculation.Comment: 39 pages, 6 figures, late
Excitations in the deformed D1D5 CFT
We perform some simple computations for the first order deformation of the
D1D5 CFT off its orbifold point. It had been shown earlier that under this
deformation the vacuum state changes to a squeezed state (with the further
action of a supercharge). We now start with states containing one or two
initial quanta and write down the corresponding states obtained under the
action of deformation operator. The result is relevant to the evolution of an
initial excitation in the CFT dual to the near extremal D1D5 black hole: when a
left and a right moving excitation collide in the CFT, the deformation operator
spreads their energy over a larger number of quanta, thus evolving the state
towards the infrared.Comment: 26 pages, Latex, 4 figure
Deforming the D1D5 CFT away from the orbifold point
The D1D5 brane bound state is believed to have an `orbifold point' in its
moduli space which is the analogue of the free Yang Mills theory for the D3
brane bound state. The supergravity geometry generated by D1 and D5 branes is
described by a different point in moduli space, and in moving towards this
point we have to deform the CFT by a marginal operator: the `twist' which links
together two copies of the CFT. In this paper we find the effect of this
deformation operator on the simplest physical state of the CFT -- the Ramond
vacuum. The twist deformation leads to a final state that is populated by pairs
of excitations like those in a squeezed state. We find the coefficients
characterizing the distribution of these particle pairs (for both bosons and
fermions) and thus write this final state in closed form.Comment: 30 pages, 4 figures, Late
Isolation of a wide range of minerals from a thermally treated plant: Equisetum arvense, a Mare’s tale
Silica is the second most abundant biomineral being exceeded in nature only by biogenic CaCO3. Many land plants (such as rice, cereals, cucumber, etc.) deposit silica in significant amounts to reinforce their tissues and as a systematic response to pathogen attack. One of the most ancient species of living vascular plants, Equisetum arvense is also able to take up and accumulate silica in all parts of the plant. Numerous methods have been developed for elimination of the organic material and/or metal ions present in plant material to isolate biogenic silica. However, depending on the chemical and/or physical treatment applied to branch or stem from Equisetum arvense; other mineral forms such glass-type materials (i.e. CaSiO3), salts (i.e. KCl) or luminescent materials can also be isolated from the plant material. In the current contribution, we show the chemical and/or thermal routes that lead to the formation of a number of different mineral types in addition to biogenic silica
The Unified First law in "Cosmic Triad" Vector Field Scenario
In this letter, we try to apply the unified first law to the "cosmic triad"
vector field scenario both in the minimal coupling case and in the
non-minimalcoupling case. After transferring the non-minimally coupling action
in Jordan frame to Einstein frame, the correct dynamical equation (Friedmann
equation) is gotten in a thermal equilibrium process by using the already
existing entropy while the entropy in the non-minimal coupled "cosmic triad"
scenario has not been derived. And after transferring the variables back to
Jordan frame, the corresponding Friedmann equation is demonstrated to be
correct. For complete arguments, we also calculate the related Misner-Sharp
energy in Jordan and Einstein frames.Comment: 19 pages, no figure
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