21,465 research outputs found
The Effects of radial inflow of gas and galactic fountains on the chemical evolution of M31
Galactic fountains and radial gas flows are very important ingredients in
modeling the chemical evolution of galactic disks. Our aim here is to study the
effects of galactic fountains and radial gas flows in the chemical evolution of
the disk of M31. We adopt a ballistic method to study the effects of galactic
fountains on the chemical enrichment of the M31 disk. We find that the landing
coordinate for the fountains in M31 is no more than 1 kpc from the starting
point, thus producing negligible effect on the chemical evolution of the disk.
We find that the delay time in the enrichment process due to fountains is no
longer than 100 Myr and this timescale also produces negligible effects on the
results. Then, we compute the chemical evolution of the M31 disk with radial
gas flows produced by the infall of extragalactic material and fountains. We
find that a moderate inside-out formation of the disk coupled with radial flows
of variable speed can very well reproduce the observed gradient. We discuss
also the effects of other parameters such a threshold in the gas density for
star formation and an efficiency of star formation varying with the galactic
radius. We conclude that the most important physical processes in creating disk
gradients are the inside-out formation and the radial gas flows. More data on
abundance gradients both locally and at high redshift are necessary to confirm
this conclusion.Comment: Accepted by A&
Canonical Theory of 2+1 Gravity
Recently 2+1 dimensional gravity theory, especially has been
studied extensively. It was shown to be equivalent to the 2+1 Chern-Simon
theory and has been investigated to understand the black hole thermodynamics,
i.e. Hawking temperature and others. The purpose of this report is to
investigate the canonical formalism of the original 2+1 Einstein gravity theory
instead of the Chern-Simon theory. For the spherically symmetric space-time,
local conserved quantities(local mass and angular momentum) are introduced and
using them canonical quantum theory is defined. Constraints are imposed on
state vectors and solved analytically. The strategy to obtain the solution is
followed by our previous work.Comment: 6 pages, talk given at LLWI-2000: From Particles to Universe,
Alberta, 20-26 February 200
A small and light weight heat exchanger for on-board helium refrigerator
A small and light weight heat exchanger used for small helium refrigerator has been developed by Sumitomo Heavy Industries, Ltd. This heat exchanger is a laminated metal heat exchanger which consists of perforated aluminum metal plates and glassfiber reinforced plastic separators. The size is from 100 mm to 28 mm in diameter and about 300 mm in length. The weight is from 2.5 kg to 0.6 kg. Also it can be used between room temperature and liquid helium temperature. The thermal efficiency obtained has been more than 96%. The heat exchanger has been practically used for on-board helium refrigerator in Japanese National Railways' superconducting magnetic levitated trains
Charge dynamics in thermally and doping induced insulator-metal transitions of (Ti1-xVx)2O3
Charge dynamics of (Ti1-xVx)2O3 with x=0-0.06 has been investigated by
measurements of charge transport and optical conductivity spectra in a wide
temperature range of 2-600K with the focus on the thermally and doping induced
insulator-metal transitions (IMTs). The optical conductivity peaks for the
interband transitions in the 3d t2g manifold are observed in the both
insulating and metallic states, while their large variation (by ~0.4 eV) with
change of temperature and doping level scales with that of the Ti-Ti dimer bond
length, indicating the weakened singlet bond in the course of IMTs. The
thermally and V-doping induced IMTs are driven with the increase in carrier
density by band-crossing and hole-doping, respectively, in contrast to the
canonical IMT of correlated oxides accompanied by the whole collapse of the
Mott gap.Comment: 4 pages, 4 figure
Economic Evaluation of Catch Share Program: Rhode Island Fluke Fishery Sector Pilot Program
Catch share, sector allocation, fishery management, Demand and Price Analysis, Resource /Energy Economics and Policy, Q22, Q28,
Linear-response theory of the longitudinal spin Seebeck effect
We theoretically investigate the longitudinal spin Seebeck effect, in which
the spin current is injected from a ferromagnet into an attached nonmagnetic
metal in a direction parallel to the temperature gradient. Using the fact that
the phonon heat current flows intensely into the attached nonmagnetic metal in
this particular configuration, we show that the sign of the spin injection
signal in the longitudinal spin Seebeck effect can be opposite to that in the
conventional transverse spin Seebeck effect when the electron-phonon
interaction in the nonmagnetic metal is sufficiently large. Our linear-response
approach can explain the sign reversal of the spin injection signal recently
observed in the longitudinal spin Seebeck effect.Comment: Proc. of ICM 2012 (Accepted for publication in J. Korean Phys. Soc.),
typos correcte
Why current-carrying magnetic flux tubes gobble up plasma and become thin as a result
It is shown that if a current-carrying magnetic flux tube is bulged at its
axial midpoint z=0 and constricted at its axial endpoints z=+h,-h, then plasma
will be accelerated from z=+h,-h towards z=0 resulting in a situation similar
to two water jets pointed at each other. The ingested plasma convects embedded,
frozen-in toroidal magnetic flux from z=+h,-h to z=0. The counter-directed
flows collide and stagnate at z=0 and in so doing (i) convert their
translational kinetic energy into heat, (ii) increase the plasma density at
z~0, and (iii) increase the embedded toroidal flux density at z~0. The increase
in toroidal flux density at z~0 increases the toroidal field Bphi and hence
increases the magnetic pinch force at z~0 and so causes a reduction of the flux
tube radius at z~0. Thus, the flux tube develops an axially uniform
cross-section, a decreased volume, an increased density, and an increased
temperature. This model is proposed as a likely hypothesis for the
long-standing mystery of why solar coronal loops are observed to be axially
uniform, hot, and bright.Comment: to appear in Physics of Plasmas 24 pages, 5 figure
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