1,515 research outputs found
Distance, reddening and three dimensional structure of the SMC - I: Using RRab stars
We present a study of simultaneous determination of mean distance and
reddening to the Small Magellanic Cloud (SMC) using the two photometric band RR
Lyrae data. Currently available largest number of highly accurate and precise
light curve data of the fundamental mode RR Lyrae stars (RRab) with better
areal coverage released by the Optical Gravitational Lensing Experiment
(OGLE)-IV project observed in the two photometric bands were utilised
simultaneously in order to determine true distance and reddening independently
for each of the individual RRab stars. Different empirical and theoretical
calibrations leading to the determination of absolute magnitudes of RRab stars
in the two bands, and along with their mean magnitudes were utilised to
calculate the apparent distance moduli of each of these RRab stars in these two
bands. Decomposing the apparent distance moduli into true distance modulus and
reddening in each of these two bands, individual RRab distance and reddening
were estimated solving the two apparent distance moduli equations. Modeling the
observed distributions of the true distance moduli and reddenings of the SMC
RRab stars as Gaussian, the true mean distance modulus and mean reddening value
to the SMC were found to be {\bf mag and
mag, respectively. This corresponds to a distance of ~kpc to the SMC. The three dimensional distribution of the
SMC RRab stars was approximated as ellipsoid. Then using the principal axes
transformation method \citep{deb14} we find the axes ratios of the SMC:
with
and
.} These results are in agreement
with other recent independent previous studies using different tracers and
methodologies.Comment: 20 pages, 15 figures, Revised version resubmitted to MNRAS Main
Journal on October 22, 201
A Hybrid Profile-Gradient Approach for the Estimation of Surface Fluxes
The Monin--Obukhov similarity theory-based wind speed and potential
temperature profiles are inherently coupled to each other. We have developed
hybrid approaches to disentangle them, and as a direct consequence, the
estimation of Obukhov length (and associated turbulent fluxes) from either
wind-speed or temperature measurements becomes an effortless task.
Additionally, our approaches give rise to two easily measurable indices of
atmospheric stability. We compare these approaches with the traditional
gradient and profile methods that require both wind-speed and temperature
profile data. Using Monte-Carlo-type numerical experiments we demonstrate that,
if the input profiles are free of any random errors, the performance of the
proposed hybrid approaches is almost equivalent to the profile method and
better than the gradient method. However, the proposed hybrid approaches are
less competitive in comparison to their traditional counterparts in the
presence of random errors
Pseudo Fuzzy Set
Here a novel idea to handle imprecise or vague set viz. Pseudo fuzzy set has
been proposed. Pseudo fuzzy set is a triplet of element and its two membership
functions. Both the membership functions may or may not be dependent. The
hypothesis is that every positive sense has some negative sense. So, one
membership function has been considered as positive and another as negative.
Considering this concept, here the development of Pseudo fuzzy set and its
property along with Pseudo fuzzy numbers has been discussed
Finite Temperature Effects and Axion Cosmology
We investigate the impact of finite temperature effects on axions in the
context of cosmology. The temperature dependence of the decay constant is
modeled analogous to pions. For the two interesting cases considered here, we
find that the temperature effects do lead to changes relevant for detailed and
precise abundance and rate calculations. We also find that the axion decoupling
temperature starts showing large deviations for larger values of the axion
decay constant.Comment: 9 pages, 2 figure
Quantum aspects of antisymmetric tensor field with spontaneous Lorentz violation
We study the quantization of a simple model of antisymmetric tensor field
with spontaneous Lorentz violation in curved spacetime. We evaluate the 1-loop
corrections at first order of metric perturbation, using a general covariant
effective action approach. We revisit the issue of quantum equivalence, and
find that it holds for non-Lorentz-violating modes but breaks down for Lorentz
violating modes.Comment: 20 pages; minor corrections, text improvements, references added;
published versio
Preparations for detecting and characterizing gravitational-wave signals from binary black hole coalescences
We evaluate how well EOBNR waveforms, obtained from the effective one-body
formalism, perform in detecting gravitational wave (GW) signals from binary
black hole (BBH) coalescences modelled by numerical relativity (NR) groups
participating in the second edition of the numerical injection analysis
(NINJA-2). In this study, NINJA-2 NR-based signals that are available in the
public domain were injected in simulated Gaussian, stationary data prepared for
three LIGO-Virgo detectors with early Advanced LIGO sensitivities. Here we
studied only non-spinning BBH signals. A total of 2000 such signals from 20
NR-based signal families were injected in a two-month long data set. The
all-sky, all-time compact binary coalescence (CBC) search pipeline was run
along with an added coherent stage to search for those signals. We find that
the EOBNR templates are only slightly less efficient (by a few percent) in
detecting non-spinning NR-based signals than in detecting EOBNR injections. On
the other hand, the coherent stage improves the signal detectability by a few
percent over a coincident search
On Number Conservation of Non-uniform Cellular Automata
This paper studies the number conservation property of 1-dimensional
non-uniform cellular automata (CAs). In a non-uniform cellular automaton (CA),
different cells may follow different rules. The present work considers that the
cells follow Wolfram's CAs rules. A characterization tool, named Reachability
tree is used to discover the number conservation property of non-uniform CAs.
Then a decision algorithm is reported to conclude whether a given non-uniform
CA with cells is number conserving or not. Finally, a synthesis scheme is
developed to get an -cell number conserving non-uniform CA
Numerical Solution of Fuzzy Stochastic Differential Equation
In this paper an alternative approach to solve uncertain Stochastic
Differential Equation (SDE) is proposed. This uncertainty occurs due to the
involved parameters in system and these are considered as Triangular Fuzzy
Numbers (TFN). Here the proposed fuzzy arithmetic in [2] is used as a tool to
handle Fuzzy Stochastic Differential Equation (FSDE). In particular, a system
of Ito stochastic differential equations is analysed with fuzzy parameters.
Further exact and Euler Maruyama approximation methods with fuzzy values are
demonstrated and solved some standard SDE
Probing Low-x QCD With Very High Energy Prompt Muons
We explore the possibility of utilizing the prompt muon fluxes at very high
energies in order to discriminate various models/parametrizations of low-x QCD
behaviour of hadronic cross-sections relevant at such energies. We find that
the pair meter technique for measuring high energy prompt muons can be very
efficient in such an endeavor. As a by product, it allows to cleanly probe the
change in composition of the primary cosmic rays expected at high energies.Comment: 5 pages, 2 figure
Reversibility of d-State Finite Cellular Automata
This paper investigates reversibility properties of 1-dimensional
3-neighborhood d-state finite cellular automata (CAs) of length n under
periodic boundary condition. A tool named reachability tree has been developed
from de Bruijn graph which represents all possible reachable configurations of
an n-cell CA. This tool has been used to test reversibility of CAs. We have
identified a large set of reversible CAs using this tool by following some
greedy strategies.Comment: Copyright of Old City Publishin
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