61,182 research outputs found
Design considerations for a HE-3 refrigerator for space applications
The low temperature provided by He-3 refrigerators (0.3 to 3 K) have useful space applications. However, the low temperatures and the low surface tension of He-3 require special design considerations. The considerations include the need for small pores to contain the liquid in a matrix; the effects of bubble nucleation and growth; and the effects of the thermal conductivity within the matrix. These design considerations are discussed and a possible confinement system is analyzed
Observations of 8-amu/unit charge ion cyclotron whistlers
Ion cyclotron whistler in very low frequency noise observations with Injun 5 satellit
Correlation of bow shock plasma wave turbulence with solar wind parameters
The r.m.s. field strengths of electrostatic and electromagnetic turbulence in the earth's bow shock, measured in the frequency range 20 Hz to 200 kHz with IMP-6 satellite, are found to correlate with specific solar wind parameters measured upstream of the bow shock
Emergent Nesting of the Fermi Surface from Local-Moment Description of Iron-Pnictide High-Tc Superconductors
We uncover the low-energy spectrum of a t-J model for electrons on a square
lattice of spin-1 iron atoms with 3dxz and 3dyz orbital character by applying
Schwinger-boson-slave-fermion mean-field theory and by exact diagonalization of
one hole roaming over a 4 x 4 x 2 lattice. Hopping matrix elements are set to
produce hole bands centered at zero two-dimensional (2D) momentum in the
free-electron limit. Holes can propagate coherently in the t-J model below a
threshold Hund coupling when long-range antiferromagnetic order across the d+ =
3d(x+iy)z and d- = 3d(x-iy)z orbitals is established by magnetic frustration
that is off-diagonal in the orbital indices. This leads to two hole-pocket
Fermi surfaces centered at zero 2D momentum. Proximity to a commensurate
spin-density wave (cSDW) that exists above the threshold Hund coupling results
in emergent Fermi surface pockets about cSDW momenta at a quantum critical
point (QCP). This motivates the introduction of a new Gutzwiller wavefunction
for a cSDW metal state. Study of the spin-fluctuation spectrum at cSDW momenta
indicates that the dispersion of the nested band of one-particle states that
emerges is electron-type. Increasing Hund coupling past the QCP can push the
hole-pocket Fermi surfaces centered at zero 2D momentum below the Fermi energy
level, in agreement with recent determinations of the electronic structure of
mono-layer iron-selenide superconductors.Comment: 41 pages, 12 figures, published versio
Does the proton-to-electron mass ratio vary in the course of cosmological evolution?
The possible cosmological variation of the proton-to-electron mass ratio was
estimated by measuring the H_2 wavelengths in the high-resolution spectrum of
the quasar Q~0347-382. Our analysis yielded an estimate for the possible
deviation of \mu value in the past, 10 Gyr ago: for the unweighted value
; for the weighted value Since the significance of the both
results does not exceed 3, further observations are needed to increase
the statistical significance. In any case, this result may be considered as the
most stringent estimate on an upper limit of a possible variation of \mu (95%
C.L.): This value serves as an
effective tool for selection of models determining a relation between possible
cosmological deviations of the fine-structure constant \alpha and the
elementary particle masses (m, m, etc.).Comment: 6 pages, 1 figure. Talk presented at the JENAM 2002 Workshop on
Varying Fundamental Constants, Porto, 4th September 2002. To be published in
the Conference Proceeding
Macroscopic Phase Coherence of Defective Vortex Lattices in Two Dimensions
The superfluid density is calculated theoretically for incompressible vortex
lattices in two dimensions that have isolated dislocations quenched in by a
random arrangement of pinned vortices. The latter are assumed to be sparse and
to be fixed to material defects. It is shown that the pinned vortices act to
confine a single dislocation of the vortex lattice along its glide plane.
Plastic creep of the two-dimensional vortex lattice is thereby impeded, and
macroscopic phase coherence results at low temperature in the limit of a dilute
concentration of quenched-in dislocations.Comment: 18 pages, 1 figure, 1 table, new title, submitted to Physical Review
On the heating of source of the Orion KL hot core
We present images of the J=10-9 rotational lines of HC3N in the vibrationally
excited levels 1v7, 1v6 and 1v5 of the hot core (HC) in Orion KL. The images
show that the spatial distribution and the size emission from the 1v7 and 1v5
levels are different. While the J=10-9 1v7 line has a size of 4''x 6'' and
peaks 1.1'' NE of the 3 mm continuum peak, the J=10--9 1v5 line emission is
unresolved (<3'') and peaks 1.3'' south of the 3 mm peak. This is a clear
indication that the HC is composed of condensations with very different
temperatures (170 K for the 1v7 peak and K for the 1v5 peak). The
temperature derived from the 1v7 and 1v5 lines increases with the projected
distance to the suspected main heating source I. Projection effects along the
line of sight could explain the temperature gradient as produced by source I.
However, the large luminosity required for source I, >5 10^5 Lsolar, to explain
the 1v5 line suggests that external heating by this source may not dominate the
heating of the HC. Simple model calculations of the vibrationally excited
emission indicate that the HC can be internally heated by a source with a
luminosity of 10^5 Lsolar, located 1.2'' SW of the 1v5 line peak (1.8'' south
of source I). We also report the first detection of high-velocity gas from
vibrationally excited HC3N emission. Based on excitation arguments we conclude
that the main heating source is also driving the molecular outflow. We
speculate that all the data presented in this letter and the IR images are
consistent with a young massive protostar embedded in an edge-on disk.Comment: 13 pages, 3 figures, To be published in Ap.J. Letter
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