Articles
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05/02/2006--
05/02/2006
Algebraic Topology of Calabi-Yau Threefolds in Toric Varieties
We compute the integral homology (including torsion), the topological
K-theory, and the Hodge structure on cohomology of Calabi-Yau threefold
hypersurfaces and complete intersections in Gorenstein toric Fano varieties.
The methods are purely topological.
Charles F. Doran
John W. Morgan
03/03/2013--
03/03/2013
Algebraic vector bundles on punctured affine spaces and smooth quadrics
We construct examples of non-isomorphic algebraic vector bundles on the
punctured affine space with isomorphic pullbacks to the smooth quadric.
Brent Doran
Jun Yu
04/27/2006--
02/07/2003
CMBEASY:: an Object Oriented Code for the Cosmic Microwave Background
We have ported the cmbfast package to the C++ programming language to produce
cmbeasy, an object oriented code for the cosmic microwave background. The code
is available at www.cmbeasy.org. We sketch the design of the new code,
emphasizing the benefits of object orientation in cosmology, which allow for
simple substitution of different cosmological models and gauges. Both gauge
invariant perturbations and quintessence support has been added to the code.
For ease of use, as well as for instruction, a graphical user interface is
available.
Michael Doran
04/26/2005--
11/22/2004
Can we test Dark Energy with Running Fundamental Constants ?
We investigate a link between the running of the fine structure constant
$\alpha$ and a time evolving scalar dark energy field. Employing a versatile
parameterization for the equation of state, we exhaustively cover the space of
dark energy models. Under the assumption that the change in $\alpha$ is to
first order given by the evolution of the Quintessence field, we show that
current Oklo, Quasi Stellar Objects and Equivalence Principle observations
restrict the model parameters considerably stronger than observations of the
Cosmic Microwave Background, Large Scale Structure and Supernovae Ia combined.
Michael Doran
01/20/2005--
01/20/2005
Testing Dark Energy and Light Particles via Black Hole Evaporation at Colliders
We show that collider experiments have the potential to exclude a light
scalar field as well as generic models of modified gravity as dark energy
candidates. Our mechanism uses the spectrum radiated by black holes and can
equally well be applied to determine the number of light degrees of freedom. We
obtain the grey body factors for massive scalar particles and calculate the
total emissivity. While the Large Hadron Collider (LHC) may not get to the
desired accuracy, the measurement is within reach of next generation colliders.
Michael Doran
Joerg Jaeckel
08/04/2005--
08/04/2005
Observational constraints on the dark energy density evolution
We constrain the evolution of the dark energy density from Cosmic Microwave
Background, Large Scale Structure and Supernovae Ia measurements. While
Supernovae Ia are most sensitive to the equation of state $w_0$ of dark energy
today, the Cosmic Microwave Background and Large Scale Structure data best
constrains the dark energy evolution at earlier times. For the parametrization
used in our models, we find $w_0 < -0.8$ and the dark energy fraction at very
high redshift $\Omega_{early} < 0.03$ at 95 per cent confidence level.
Michael Doran
Khamphee Karwan
Christof Wetterich
04/16/2008--
03/19/2007
Boundary sources in the Doran - Lobo - Crawford spacetime
We take a null hypersurface (the causal horizon) generated by a congruence of
null geodesics as the boundary of the Doran-Lobo-Crawford spacetime, to be the
place where the Brown-York quasilocal energy is located. The components of the
outer and inner stress tensors are computed and shown to depend on time and on
the impact parameter $b$ of the test particle trajectory. The surface energy
density $\sigma$ on the boundary is given by the same expression as that
obtained previously for the energy stored on a Rindler horizon.
Hristu Culetu
12/31/1998--
12/31/1998
Picard-Fuchs Uniformization: Modularity of the Mirror Map and Mirror-Moonshine
Motivated by a conjecture of Lian and Yau concerning the mirror map in string
theory, we determine when the mirror map q-series of certain elliptic curve and
K3 surface families are Hauptmoduln (genus zero modular functions). Our
geometric criterion for modularity characterizes orbifold uniformization
properties of their Picard-Fuchs equations, effectively demystifying the
mirror-moonshine phenomenon. A longer, more comprehensive treatment of these
results will appear shortly.
Charles F. Doran
04/04/2004--
04/04/2004
Moduli Space of Cubic Surfaces as Ball Quotient via Hypergeometric Functions
We describe hypergeometric functions of Deligne-Mostow type for open subsets
of the configuration space of six points on P^2, induced from those for seven
points on P^1. The seven point ball quotient example DM(2^5,1^2) does not
appear on Mostow's original list, but does appear on Thurston's corrected
version. We show that DM(2^5,1^2) is a finite cover of the moduli space of
cubic surfaces M_C endowed with the ball quotient structure G_C\B^4 of Allcock,
Carlson, and Toledo. This answers a question of Allcock about the
commensurability of G_C with the monodromy groups of Deligne-Mostow
hypergeometric functions.
Brent R. Doran
09/26/2005--
09/26/2005
Spacetime algebra and electron physics
This paper surveys the application of geometric algebra to the physics of
electrons. It first appeared in 1996 and is reproduced here with only minor
modifications. Subjects covered include non-relativistic and relativistic
spinors, the Dirac equation, operators and monogenics, the Hydrogen atom,
propagators and scattering theory, spin precession, tunnelling times, spin
measurement, multiparticle quantum mechanics, relativistic multiparticle wave
equations, and semiclassical mechanics.
C. J. L. Doran
A. N. Lasenby
S. F. Gull
S. Somaroo
A. D. Challinor
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