10,296 research outputs found
Factorization in with elementary matrices when is the disk algebra and the Wiener algebra
Let be the polydisc algebra or the Wiener algebra. It is shown that the
group is generated by the subgroup of elementary matrices with all
diagonal entries and at most one nonzero off-diagonal entry. The result an
easy consequence of the deep result due to Ivarsson and Kutzschebauch (Ann. of
Math. 2012).Comment: 5 page
Projective freeness of algebras of real symmetric functions
Let D^n be the closed unit polydisk in C^n. Consider the ring C_r of
complex-valued continuous functions on D^n that are real symmetric, that is,
f(z)=(f(z^*))^* for all z in D^n. It is shown that C_r is projective free, that
is, finitely generated projective modules over C_r are free. We also show that
several subalgebras of the real symmetric polydisc algebra are projective free.Comment: 14 page
A summation method based on the Fourier series of periodic distributions and an example
A generalised summation method is considered based on the Fourier series of
periodic distributions. It is shown that where is the
-periodic distribution given by \begin{eqnarray*} \left\langle {\mathrm
P\mathrm f} {\displaystyle \frac{e^{it}}{(1+e^{it})^2}} ,\varphi \right\rangle
&=&
\lim_{\epsilon\searrow 0}
\left(
\int_{(-\delta,\pi-\epsilon)\cup(\pi+\epsilon,2\pi+\delta)}\frac{\varphi(t)
e^{it}}{(1+e^{it})^2}dt -\frac{\varphi(\pi)}{\tan (\epsilon/2)}\right)
\end{eqnarray*} with support
, where .
Applying the generalised summation method, we determine the sum of the
divergent series , and more generally for
.Comment: 31 pages, 5 figures (Typos corrected.
Noncoherence of the multiplier algebra of the Drury-Arveson space H^2_n for n>=3
Let H_n^2 denote the Drury-Arveson Hilbert space on the unit ball B_n in C^n,
and let M(H_n^2) be its multiplier algebra. We show that for n>=3, the ring
M(H_n^2) is not coherent.Comment: 10 page
Neutrino mass and dark energy constraints from redshift-space distortions
Cosmology in the near future promises a measurement of the sum of neutrino
masses, a fundamental Standard Model parameter, as well as
substantially-improved constraints on the dark energy. We use the shape of the
BOSS redshift-space galaxy power spectrum, in combination with CMB and
supernova data, to constrain the neutrino masses and the dark energy. Essential
to this calculation are several recent advances in non-linear cosmological
perturbation theory, including FFT methods, redshift space distortions, and
scale-dependent growth. Our 95% confidence upper bound of 180 meV on the sum of
masses degrades substantially to 540 meV when the dark energy equation of state
and its first derivative are also allowed to vary, representing a significant
challenge to current constraints. We also study the impact of additional galaxy
bias parameters, finding that a greater allowed range of scale-dependent bias
only slightly shifts the preferred neutrino mass value, weakens its upper bound
by about 20%, and has a negligible effect on the other cosmological parameters.Comment: Matches accepted version. Code available at
github.com/upadhye/redTim
Shannon's sampling theorem in a distributional setting
The classical Shannon sampling theorem states that a signal f with Fourier
transform F in L^2(R) having its support contained in (-\pi,\pi) can be
recovered from the sequence of samples (f(n))_{n in Z} via f(t)=\sum_{n in Z}
f(n) (sin(\pi (t -n)))/(\pi (t-n)) (t in R). In this article we prove a
generalization of this result under the assumption that F is a compactly
supported distribution with its support contained in (-\pi,\pi).Comment: This paper has been withdrawn by the author due to an error in a
claim about singular supports in the proo
On Isosceles Triangles and Related Problems in a Convex Polygon
Given any convex -gon, in this article, we: (i) prove that its vertices
can form at most isosceles trianges with two sides of
unit length and show that this bound is optimal in the first order, (ii)
conjecture that its vertices can form at most isosceles
triangles and prove this conjecture for a special group of convex -gons,
(iii) prove that its vertices can form at most regular
-gons for any integer and that this bound is optimal, and (iv)
provide a short proof that the sum of all the distances between its vertices is
at least and at most as
long as the convex -gon has unit perimeter
Parallel implementation of three-dimensional molecular dynamic simulation for laser-cluster interaction
The objective of this article is to report the parallel implementation of the
3D molecular dynamic simulation code for laser-cluster interactions. The
benchmarking of the code has been done by comparing the simulation results with
some of the experiments reported in the literature. Scaling laws for the
computational time is established by varying the number of processor cores and
number of macroparticles used. The capabilities of the code are highlighted by
implementing various diagnostic tools. To study the dynamics of the
laser-cluster interactions, the executable version of the code is available
from the author.Comment: 5 pages, 7 figure
Texture zeroes and discrete flavor symmetries in light and heavy Majorana neutrino mass matrices: a bottom-up approach
Texture zeroes in neutrino mass matrix may give us hints about the
symmetries involved in neutrino mass generation. We examine the viability of
such texture zeroes in a model independent way through a bottom-up approach.
Using constraints from the neutrino oscillation data, we develop an analytic
framework that can identify these symmetries and quantify deviations from them.
We analyze the textures of as well as those of , the mass matrix
of heavy Majorana neutrinos in the context of Type-I seesaw. We point out how
the viability of textures depends on the absolute neutrino mass scale, the
neutrino mass ordering and the mixing angle . We also examine the
compatibility of discrete flavor symmetries like -- exchange and
permutation with the current data. We show that the exchange
symmetry for can be satisfied for any value of the absolute neutrino
mass, but for to satisfy the symmetry, neutrino masses have to be
quasi-degenerate. On the other hand, both these symmetries are currently
allowed for for all values of absolute neutrino mass and both mass
orderings.Comment: 33 pages, minor revision in section-VI (A
On two natural extensions of Vinnicombe's metric: their noncoincidence yet equivalence on stabilizable plants over A_+
Let A_+ be the ring of Laplace transforms of complex Borel measures on R with
support in [0,+\infty) which do not have a singular nonatomic part. We compare
the nu-metric d_{A_+} for stabilizable plants over A_+ given in the article by
Ball and Sasane [2010], with yet another metric d_{H^\infty}|_{A_+}, namely the
one induced by the metric d_{H^\infty} for the set of stabilizable plants over
H^\infty given in teh article by Sasane in 2011. Both d_{A_+} and d_{H^\infty}
coincide with the classical Vinnicombe metric defined for rational transfer
functions, but we show here by means of an example that these two possible
extensions of the classical nu-metric for plants over A_+ do not coincide on
the set of stabilizable plants over A_+. We also prove that they nevertheless
give rise to the same topology on stabilizable plants over A_+, which in turn
coincides with the gap metric topology.Comment: 13 pages, 0 figure
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