8,774 research outputs found
Characterisation and representation of non-dissipative electromagnetic medium with a double light cone
We study Maxwell's equations on a 4-manifold N with a medium that is
non-dissipative and has a linear and pointwise response. In this setting, the
medium can be represented by a suitable (2,2)-tensor on the 4-manifold N.
Moreover, in each cotangent space on N, the medium defines a Fresnel surface.
Essentially, the Fresnel surface is a tensorial analogue of the dispersion
equation that describes the response of the medium for signals in the geometric
optics limit. For example, in isotropic medium the Fresnel surface is at each
point a Lorentz light cone. In a recent paper, I. Lindell, A. Favaro and L.
Bergamin introduced a condition that constrains the polarisation for plane
waves. In this paper we show (under suitable assumptions) that a slight
strengthening of this condition gives a pointwise characterisation of all
medium tensors for which the Fresnel surface is the union of two distinct
Lorentz null cones. This is for example the behaviour of uniaxial medium like
calcite. Moreover, using the representation formulas from Lindell et al. we
obtain a closed form representation formula that pointwise parameterises all
medium tensors for which the Fresnel surface is the union of two distinct
Lorentz null cones. Both the characterisation and the representation formula
are tensorial and do not depend on local coordinates
Neural networks in geophysical applications
Neural networks are increasingly popular in geophysics.
Because they are universal approximators, these
tools can approximate any continuous function with an
arbitrary precision. Hence, they may yield important
contributions to finding solutions to a variety of geophysical applications.
However, knowledge of many methods and techniques
recently developed to increase the performance
and to facilitate the use of neural networks does not seem
to be widespread in the geophysical community. Therefore,
the power of these tools has not yet been explored to
their full extent. In this paper, techniques are described
for faster training, better overall performance, i.e., generalization,and the automatic estimation of network size
and architecture
Determination of electromagnetic medium from the Fresnel surface
We study Maxwell's equations on a 4-manifold where the electromagnetic medium
is described by an antisymmetric -tensor . In this setting,
the Tamm-Rubilar tensor density determines a polynomial surface of fourth order
in each cotangent space. This surface is called the Fresnel surface and acts as
a generalisation of the light-cone determined by a Lorentz metric; the Fresnel
surface parameterises electromagnetic wave-speed as a function of direction.
Favaro and Bergamin have recently proven that if has only a principal
part and if the Fresnel surface of coincides with the light cone for a
Lorentz metric , then is proportional to the Hodge star operator of
. That is, under additional assumptions, the Fresnel surface of
determines the conformal class of . The purpose of this paper is
twofold. First, we provide a new proof of this result using Gr\"obner bases.
Second, we describe a number of cases where the Fresnel surface does not
determine the conformal class of the original -tensor . For
example, if is invertible we show that and have
the same Fresnel surfaces.Comment: 23 pages, 1 figur
USDA Farm Programs: North Dakota Farmer Participation and Opinions
Agricultural and Food Policy,
Wigner Trajectory Characteristics in Phase Space and Field Theory
Exact characteristic trajectories are specified for the time-propagating
Wigner phase-space distribution function. They are especially simple---indeed,
classical---for the quantized simple harmonic oscillator, which serves as the
underpinning of the field theoretic Wigner functional formulation introduced.
Scalar field theory is thus reformulated in terms of distributions in field
phase space. Applications to duality transformations in field theory are
discussed.Comment: 9 pages, LaTex2
A restatement of the normal form theorem for area metrics
An area metric is a (0,4)-tensor with certain symmetries on a 4-manifold that
represent a non-dissipative linear electromagnetic medium. A recent result by
Schuller, Witte and Wohlfarth provides a pointwise normal form theorem for such
area metrics. This result is similar to the Jordan normal form theorem for
(1,1)-tensors, and the result shows that any area metric belongs to one of 23
metaclasses with explicit coordinate expressions for each metaclass. In this
paper we restate and prove this result for skewon-free (2,2)-tensors and show
that in general, each metaclasses has three different coordinate
representations, and each of metaclasses I, II, ..., VI, VII need only one
coordinate representation.Comment: Updated proof of Proposition A.2 (Claim 5). Fixed typo in Theorem 6
(Metaclass XXIII
Production and Decay of Double \u3ci\u3eL\u3c/i\u3e Vacancies in Argon and Phosphorus
Measurements have been made at two laboratories which indicate that the structure reported at 450-550eV in the electron spectrum from Ar+-Ar collisions by Ogurtsov, Flaks, and Avakyan is spurious. It is argued that the double L vacancies which they invoke to explain the structure are more likely to decay by the two-step Auger process L 2→LM2→M4 than by the one-step process L2→M3 suggested by these authors. Evidence supporting this is found in our electron spectra from P+-Ar collisions, where it is known from energy-loss and charge-state measurements that double L vacancies are produced in phosphorus
Electronic spectroscopy of FUV-irradiated diamondoids: A combined experimental and theoretical study
Irradiation with high energy photons (10.2 - 11.8 eV) was applied to small
diamondoids isolated in solid rare gas matrices at low temperature. The
photoproducts were traced via UV absorption spectroscopy. We found that upon
ionization the smallest of these species lose a peripheral H atom to form a
stable closed-shell cation. This process is also likely to occur under
astrophysical conditions for gas phase diamondoids and it opens the possibility
to detect diamond-like molecules using their rotational spectrum since the
dehydrogenated cations possess strong permanent dipole moments. The
lowest-energy electronic features of these species in the UV were found to be
rather broad, shifting to longer wavelengths with increasing molecular size.
Calculations using time-dependent density functional theory support our
experimental findings and extend the absorption curves further into the vacuum
ultraviolet. The complete sigma - sigma* spectrum displays surprisingly strong
similarities to meteoritic nanodiamonds containing 50 times more C atoms.Comment: 11 pages, 9 figures; published in The Astrophysical Journal;
corrected minor mistakes compared to the published pape
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