16,636 research outputs found
Oblique triangular antiferromagnetic phase in CsCuCoCl
The spin-1/2 stacked triangular antiferromagnet CsCuCoCl with
undergoes two phase transitions at zero field. The
low-temperature phase is produced by the small amount of Co doping. In
order to investigate the magnetic structures of the two ordered phases, the
neutron elastic scattering experiments have been carried out for the sample
with . It is found that the intermediate phase is identical to
the ordered phase of CsCuCl, and that the low-temperature phase is an
oblique triangular antiferromagnetic phase in which the spins form a triangular
structure in a plane tilted from the basal plane. The tilting angle which is
42 at K decreases with increasing temperature, and becomes
zero at K. An off-diagonal exchange term is proposed as the
origin of the oblique phase.Comment: 6 pages, 7 figure
Differential equations for the cuspoid canonical integrals
Differential equations satisfied by the cuspoid canonical integrals I_n(a) are obtained for arbitrary values of n≥2, where n−1 is the codimension of the singularity and a=(ɑ_1,ɑ_2,...,ɑ_(n−1)). A set of linear coupled ordinary differential equations is derived for each step in the sequence I_n(0,0,...,0,0) →I_n(0,0,...,0,ɑ_(n−1)) →I_n(0,0,...,ɑ_(n−2),ɑ_(n−1)) →...→I_n(0,ɑ_2,...,ɑ_(n−2),ɑ_(n−1)) →I_n(ɑ_1,ɑ_2,...,ɑ_n−2,ɑ_(n−1)). The initial conditions for a given step are obtained from the solutions of the previous step. As examples of the formalism, the differential equations for n=2 (fold), n=3 (cusp), n=4 (swallowtail), and n=5 (butterfly) are given explicitly. In addition, iterative and algebraic methods are described for determining the parameters a that are required in the uniform asymptotic cuspoid approximation for oscillating integrals with many coalescing saddle points. The results in this paper unify and generalize previous researches on the properties of the cuspoid canonical integrals and their partial derivatives
Study of dopants for radiation-resistant silicon Final report
Radiation effects on electrical properties of both aluminum and lithium doped bulk silico
High-energy neutrino fluxes from AGN populations inferred from X-ray surveys
High-energy neutrinos and photons are complementary messengers, probing
violent astrophysical processes and structural evolution of the Universe. X-ray
and neutrino observations jointly constrain conditions in active galactic
nuclei (AGN) jets: their baryonic and leptonic contents, and particle
production efficiency. Testing two standard neutrino production models for
local source Cen A \citep{KT2008,BB2009}, we calculate the high-energy neutrino
spectra of single AGN sources and derive the flux of high-energy neutrinos
expected for the current epoch. Assuming that accretion determines both X-rays
and particle creation, our parametric scaling relations predict neutrino yield
in various AGN classes. We derive redshift-dependent number densities of each
class, from {\it Chandra} and {\it Swift}/BAT X-ray luminosity functions
\citep{SGB2008,ACS2009}. We integrate the neutrino spectrum expected from the
cumulative history of AGN (correcting for cosmological and source effects, e.g.
jet orientation and beaming). Both emission scenarios yield neutrino fluxes
well above limits set by {\it IceCube} (by -- at 1 PeV,
depending on the assumed jet models for neutrino production). This implies
that: (i) Cen A might not be a typical neutrino source as commonly assumed;
(ii) both neutrino production models overestimate the efficiency; (iii)
neutrino luminosity scales with accretion power differently among AGN classes
and hence does not follow X-ray luminosity universally; (iv) some AGN are
neutrino-quiet (e.g. below a power threshold for neutrino production); (v)
neutrino and X-ray emission have different duty cycles (e.g. jets alternate
between baryonic and leptonic flows); or (vi) some combination of the above.Comment: 16 pages, 6 figures, 3 tables, accepted for publication in MNRA
Compression of Atomic Phase Space Using an Asymmetric One-Way Barrier
We show how to construct asymmetric optical barriers for atoms. These
barriers can be used to compress phase space of a sample by creating a confined
region in space where atoms can accumulate with heating at the single photon
recoil level. We illustrate our method with a simple two-level model and then
show how it can be applied to more realistic multi-level atoms
Equivalence between Kaluza Klein modes of gravitinos and goldstinos in brane induced supersymmetry breaking
We identify the goldstino fields that give mass to the Kaluza Klein modes of
five dimensional supergravity, when supersymmetry breaking is induced by brane
effects. We then proof the four dimensional Equivalence Theorem that, in
renormalizable gauges, allows for the replacement of Kaluza Klein modes of
helicity gravitinos in terms of goldstinos. Finally we identify the
five dimensional renormalizable gauge fixing that leads to the Equivalence
Theorem.Comment: Final version published in JHEP. Typo corrected in eq. 2.
Damage coefficients in low resistivity silicon
Electron and proton damage coefficients are determined for low resistivity silicon based on minority-carrier lifetime measurements on bulk material and diffusion length measurements on solar cells. Irradiations were performed on bulk samples and cells fabricated from four types of boron-doped 0.1 ohm-cm silicon ingots, including the four possible combinations of high and low oxygen content and high and low dislocation density. Measurements were also made on higher resistivity boron-doped bulk samples and solar cells. Major observations and conclusions from the investigation are discussed
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