4,387 research outputs found
Propagation of Vortex Electron Wave Functions in a Magnetic Field
The physics of coherent beams of photons carrying axial orbital angular
momentum (OAM) is well understood and such beams, sometimes known as vortex
beams, have found applications in optics and microscopy. Recently electron
beams carrying very large values of axial OAM have been generated. In the
absence of coupling to an external electromagnetic field the propagation of
such vortex electron beams is virtually identical mathematically to that of
vortex photon beams propagating in a medium with a homogeneous index of
refraction. But when coupled to an external electromagnetic field the
propagation of vortex electron beams is distinctly different from photons. Here
we use the exact path integral solution to Schrodingers equation to examine the
time evolution of an electron wave function carrying axial OAM. Interestingly
we find that the nonzero OAM wave function can be obtained from the zero OAM
wave function, in the case considered here, simply by multipling it by an
appropriate time and position dependent prefactor. Hence adding OAM and
propagating can in this case be replaced by first propagating then adding OAM.
Also, the results shown provide an explicit illustration of the fact that the
gyromagnetic ratio for OAM is unity. We also propose a novel version of the
Bohm-Aharonov effect using vortex electron beams.Comment: 14 pages, 2 figures, submitted to Phys Rev
Charge breaking bounds in the Zee model
We study the possibility that charge breaking minima occur in the Zee model.
We reach very different conclusions from those attained in simpler, two Higgs
doublet models, and the reason for this is traced back to the existence of
cubic terms in the potential. A scan of the Zee model's parameter space shows
that CB is restricted to a narrow region of values of the parameters
Fully self-consistent calculations of nuclear Schiff moments
We calculate the Schiff moments of the nuclei 199Hg and 211Ra in completely
self-consistent odd-nucleus mean-field theory by modifying the
Hartree-Fock-Bogoliubov code HFODD. We allow for arbitrary shape deformation,
and include the effects of nucleon dipole moments alongside those of a
CP-violating pion-exchange nucleon-nucleon interaction. The results for 199Hg
differ significantly from those of previous calculations when the CP-violating
interaction is of isovector character.Comment: 7 pages, 2 figure
Charmonia from Lattice QCD
Recent lattice QCD results on charmonium properties are reviewed. I comment
on molecules and hybrid states as well as on future studies of states near
strong decay thresholds.Comment: 8 pages, 5 figures, Invited talk presented at ``Charm 2006'',
Beijing, 5-7 June 200
Aspects of Neutrino Mass Matrices
After an Introduction briefly describing the rise and fall of the three-zero
texture of the Zee model, we discuss still-allowed two-zero textures for the
Majorana three-neutrino mass matrix. Finally, a model with two right-handed
neutrinos and two Dirac texture zeros is described (FGY model) which can relate
CP violation in leptogenesis to CP violation in long-baseline neutrino
oscillations.Comment: 9 pages latex. Talk at Coral Gables 2003. Added reference
A Search for Low Surface Brightness Structure Around Compact Narrow Emission Line Galaxies
As the most extreme members of the rapidly evolving faint blue galaxy
population at intermediate redshift, the compact narrow emission line galaxies
(CNELGs) are intrinsically luminous (-22 < M_B < -18) with narrow emission
linewidths (30 < \sigma < 125 km/s). Their nature is heavily debated: they may
be low-mass starbursting galaxies that will fade to present-day dwarf galaxies
or bursts of star formation temporarily dominating the flux of more massive
galaxies, possibly related to in situ bulge formation or the formation of cores
of galaxies. We present deep, high-quality (~0.6 - 0.8 arcsec) images with CFHT
of 27 CNELGs. One galaxy shows clear evidence for a tidal tail; the others are
not unambiguously embedded in galactic disks. Approximately 55% of the CNELGS
have sizes consistent with local dwarfs of small-to-intermediate sizes, while
45% have sizes consistent with large dwarfs or disks galaxies. At least 4
CNELGs cannot harbor substantial underlying disk material; they are
low-luminosity galaxies at the present epoch (M_B > -18). Conversely, 15 are
not blue enough to fade to low-luminosity dwarfs (M_B > -15.2). The majority of
the CNELGs are consistent with progenitors of intermediate-luminosity dwarfs
and low-luminosity spiral galaxies with small disks. CNELGs are a heterogeneous
progenitor population with significant fractions (up to 44%) capable of fading
into today's faint dwarfs (M_B > -15.2), while 15 to 85% may only experience an
apparently extremely compact CNELG phase at intermediate redshift but remain
more luminous galaxies at the present epoch.Comment: 16 pages, 14 figures, emulateapj, published in Ap
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