Articles
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02/11/2014--
02/11/2014
Partial Hölder continuity for Q-valued energy minimizing maps
We consider multivalued maps between $\Omega \subset \mathbb{R}^N$ open ($N
\ge 2$) and a smooth, compact Riemannian manifold $\mathcal{N}$ locally
minimizing the Dirichlet energy. An interior partial H\"older regularity result
in the spirit of R. Schoen and K. Uhlenbeck is presented. Consequently a
minimizer is H\"older continuous outside a set of Hausdorff dimension at most
$N-3$. F. Almgren's original theory includes a global interior H\"older
continuity result if the minimizers are valued into some $\mathbb{R}^m$. It
cannot hold in general if the target is changed into a Riemannian manifold,
since it already fails for "classical" single valued harmonic maps.
Jonas Hirsch
01/11/2011--
08/09/2010
Semiclassical Gravity in the Far Field Limit of Stars, Black Holes, and Wormholes
Semiclassical gravity is investigated in a large class of asymptotically
flat, static, spherically symmetric spacetimes including those containing
static stars, black holes, and wormholes. Specifically the stress-energy
tensors of massless free spin 0 and spin 1/2 fields are computed to leading
order in the asymptotic regions of these spacetimes. This is done for spin 0
fields in Schwarzschild spacetime using a WKB approximation. It is done
numerically for the spin 1/2 field in Schwarzschild, extreme
Reissner-Nordstrom, and various wormhole spacetimes. And it is done by finding
analytic solutions to the leading order mode equations in a large class of
asymptotically flat static spherically symmetric spacetimes. Agreement is shown
between these various computational methods. It is found that for all of the
spacetimes considered, the energy density and pressure in the asymptotic region
are proportional to 1/r^5 to leading order. Furthermore, for the spin 1/2 field
and the conformally coupled scalar field, the stress-energy tensor depends only
on the leading order geometry in the far field limit. This is also true for the
minimally coupled scalar field for spacetimes containing either a static star
or a black hole, but not for spacetimes containing a wormhole.
Eric D. Carlson
Paul R. Anderson
Alessandro Fabbri
Serena Fagnocchi
William H. Hirsch
Sarah A. Klyap
11/23/2015--
11/23/2015
Femtosecond X-ray magnetic circular dichroism absorption spectroscopy at an X-ray free electron laser
X-ray magnetic circular dichroism spectroscopy using an X-ray free electron
laser is demonstrated with spectra over the Fe L$_{3,2}$-edges. This new
ultrafast time-resolved capability is then applied to a fluence-dependent study
of all-optical magnetic switching dynamics of Fe and Gd magnetic sublattices in
a GdFeCo thin film above its magnetization compensation temperature. At the
magnetic switching fuence, we corroborate the existence of a transient
ferromagnetic-like state. The timescales of the dynamics, however, are longer
than previously observed below the magnetization compensation temperature.
Above and below the switching fluence range, we observe secondary
demagnetization with about 5 ps timescales. This indicates that the spin
thermalization takes longer than 5 ps.
Daniel J. Higley
Konstantin Hirsch
Georgi L. Dakovski
Emmanuelle Jal
Edwin Yuan
Tianmin Liu
Alberto A. Lutman
James P. MacArthur
Elke Arenholz
Zhao Chen
Giacomo Coslovich
Peter Denes
Patrick W. Granitzka
Philip Hart
Matthias C. Hoffmann
John Joseph
Loïc Le Guyader
Ankush Mitra
Stefan Moeller
Hendrik Ohldag
Matthew Seaberg
Padraic Shafer
Joachim Stöhr
Arata Tsukamoto
Heinz-Dieter Nuhn
Alex H. Reid
Hermann A. Dürr
William F. Schlotter
06/27/2010--
05/26/2010
Hirsch index as a network centrality measure
We study the h Hirsch index as a local node centrality measure for complex
networks in general. The h index is compared with the Degree centrality (a
local measure), the Betweenness and Eigenvector centralities (two non-local
measures) in the case of a biological network (Yeast interaction
protein-protein network) and a linguistic network (Moby Thesaurus II) as test
environments. In both networks, the Hirsch index has poor correlation with
Betweenness centrality but correlates well with Eigenvector centrality,
specially for the more important nodes that are relevant for ranking purposes,
say in Search Machine Optimization. In the thesaurus network, the h index seems
even to outperform the Eigenvector centrality measure as evaluated by simple
linguistic criteria.
Monica G. Campiteli
Adriano J. Holanda
Paulo R. C. Soles
Leonardo H. D. Soares
Osame Kinouchi
09/29/2005--
08/03/2005
An index to quantify an individual's scientific research output
I propose the index $h$, defined as the number of papers with citation number
higher or equal to $h$, as a useful index to characterize the scientific output
of a researcher.
J. E. Hirsch
02/18/2014--
02/18/2014
Critique of Hirsch's citation index: a combinatorial Fermi problem
The h-index was introduced by the physicist J.E. Hirsch in 2005 as measure of
a researcher's productivity. We consider the "combinatorial Fermi problem" of
estimating h given the citation count. Using the Euler-Gauss identity for
integer partitions, we compute confidence intervals. An asymptotic theorem
about Durfee squares, due to E.R. Canfield-S. Corteel-C.D. Savage from 1998, is
reinterpreted as the rule of thumb h=0.54 x (citations)^{1/2}. We compare these
intervals and the rule of thumb to empirical data (primarily using
mathematicians).
Alexander Yong
01/26/2020--
01/26/2020
Superconductivity, what the H? The emperor has no clothes
A magnetic field H is expelled from the interior of a metal becoming
superconducting. Everybody thinks the phenomenon is perfectly well understood,
particularly scientists with the highest H-index think that. I don't. I will
explain why I believe that without Holes, conceptualized by Heisenberg in 1931
fifty years after Hall had first detected them in some metals, neither magnetic
field expulsion nor anything else about superconductivity can be understood. I
have been a Heretic in the field of superconductivity for over 30 years, and
believe that Hans' little story about the emperor perfectly captures the
essence of the situation. Here is (a highly condensed version of) the wHole
story.
J. E. Hirsch
04/07/2008--
04/07/2008
Searching for Hyper-Velocity Stars
We present our survey for subluminous hyper-velocity candidates, which has
been successfully initiated at the ESO NTT and the Calar Alto 3.5 m telescope.
A. Tillich
U. Heber
H. Hirsch
04/30/2010--
04/09/2010
Epitaxial ferromagnetic semiconductor GdN thin films on Si substrate
This paper has been withdrawn by the author
F. Natali
N. O. V. Plank
B. J. Ruck
H. J. Trodahl
F. Semond
S. Sorieul
L. Hirsch
03/29/2018--
03/29/2018
Term algebras of elementarily equivalent atom structures
We exhibit two relation algebra atom structures such that they are
elementarily equivalent but their term algebras are not. This answers Problem
14.19 in the book Hirsch, R. and Hodkinson, I., "Relation Algebras by Games",
North-Holland, 2002.
H. Andréka
I. Németi
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