824 research outputs found
RAMPEX - a new spin experiment (presented for HELION97, 20-24 Jan 1997, Kobe, Japan)
RAMPEX - Russian-AMerican Polarization EXperiment - is dedicated to studies
of one-spin asymmetries which have twist-3 and also twist-2 origin, in hard and
semi-hard inclusive processes on the polarized propane-diol target. A special
consideration has been given for the prospects of using polarized 3He target.
The studies will be performed at the Serpukhov accelerator at 70 GeV/c (proton
beam) and 40 GeV/c (pi- beam).Comment: 8 pages, 1 figur
BCS - BEC crossover and quantum hydrodynamics in p-wave superfluids with a symmetry of the A1 - phase
We solve the Leggett equations for the BCS - BEC crossover in the three
dimension resonance p-wave superfluid with the symmetry of the A1 - phase. We
calculate the sound velocity, the normal density, and the specific heat for the
BCS-domain (\mu > 0), BEC-domain (\mu < 0), and close to important point \mu =
0 in 100% polarized case. We find the indications of quantum phase - transition
close to the point \mu(T = 0) = 0. Deep in the BCS and BEC-domains the
crossover ideas of Leggett and Nozieres, Schmitt-Rink work pretty well. We
discuss the spectrum of orbital waves, the paradox of intrinsic angular
momentum and complicated problem of chiral anomaly in the BCS A1 - phase at T =
0. We present two different approaches to a chiral anomaly: one based on
supersymmetric hydrodynamics, another one on the formal analogy with the Dirac
equation in quantum electrodynamics. We evaluate the damping of nodal fermions
due to different decay processes in superclean case at T = 0 and find that we
are in a ballistic regime \omega\tau >> 1. We propose to use aerogel or
nonmagnetic impurities to reach hydrodynamic regime \omega\tau<< 1 at T = 0. We
discuss the concept of the spectral flow and exact cancellations between
time-derivatives of anomalous and quasiparticle currents in the equation for
the total linear momentum conservation. We propose to derive and solve the
kinetic equation for the nodal quasiparticles both in the hydrodynamic and in
the ballistic regimes to demonstrate this cancellation explicitly. We briefly
discuss the role of the other residual interactions different from damping and
invite experimentalists to measure the spectrum and damping of orbital waves in
A-phase of 3He at low temperatures.Comment: 14 pages, 10 figure
On the chains of star complexes and superclouds in spiral arms
The relation is studied between occurrence of a regular chain of star
complexes and superclouds in a spiral arm, and other properties of the latter.
A regular string of star complexes is located in the north-western arm of M31;
they have about the same size 0.6 kpc with spacing of 1.1 kpc. Within the same
arm segment the regular magnetic field with the wavelength of 2.3 kpc was found
by Beck et al. (1989). We noted that this wavelength is twice as large as the
spacing between complexes and suggested that they were formed in result of
magneto-gravitational instability developed along the arm. In this NW arm, star
complexes are located inside the gas-dust lane, whilst in the south-western arm
of M31 the gas-dust lane is upstream of the bright and uniform stellar arm.
Earlier, evidence for the age gradient has been found in the SW arm. All these
are signatures of a spiral shock, which may be associated with unusually large
(for M31) pitch-angle of this SW arm segment. Such a shock may prevent the
formation of the regular magnetic field, which might explain the absence of
star complexes there. Anti-correlation between shock wave signatures and
presence of star complexes is observed in spiral arms of a few other galaxies.
Regular chains of star complexes and superclouds in spiral arms are rare, which
may imply that a rather specific mechanism is involved in their formation, and
the most probable one is the Parker-Jeans instability. The spiral pattern of
our Galaxy is briefly discussed; it may be of M101 type in the outer parts. The
regular bi-modal spacing of HI superclouds is found in Carina and Cygnus
(Outer) arms, which may be an indirect evidence for the regular magnetic field
along these arms.Comment: 20 pages, 12 figures, accepted for publication in MNRA
Quantum eigenstate tomography with qubit tunneling spectroscopy
Measurement of the energy eigenvalues (spectrum) of a multi-qubit system has
recently become possible by qubit tunneling spectroscopy (QTS). In the standard
QTS experiments, an incoherent probe qubit is strongly coupled to one of the
qubits of the system in such a way that its incoherent tunneling rate provides
information about the energy eigenvalues of the original (source) system. In
this paper, we generalize QTS by coupling the probe qubit to many source
qubits. We show that by properly choosing the couplings, one can perform
projective measurements of the source system energy eigenstates in an arbitrary
basis, thus performing quantum eigenstate tomography. As a practical example of
a limited tomography, we apply our scheme to probe the eigenstates of a kink in
a frustrated transverse Ising chain.Comment: 8 pages, 4 figure
On the Spiral Structure of the Milky Way Galaxy
We consider the possible pattern of the overall spiral structure of the
Galaxy, using data on the distribution of neutral (atomic), molecular, and
ionized hydrogen, on the base of the hypothesis of the spiral structure being
symmetric, i.e. the assumption that spiral arms are translated into each other
for a rotation around the galactic center by 180{\deg} (a two-arm pattern) or
by 90{\deg} (a four-arm pattern). We demonstrate that, for the inner region,
the observations are best represented with a four-arm scheme of the spiral
pattern, associated with all-Galaxy spiral density waves. The basic position is
that of the Carina arm, reliably determined from distances to HII regions and
from HI and H2 radial velocities. This pattern is continued in the quadrants
III and IV with weak outer HI arms; from their morphology, the Galaxy should be
considered an asymmetric multi-arm spiral. The kneed shape of the outer arms
that consist of straight segments can indicate that these arms are transient
formations that appeared due to a gravitational instability in the gas disk.
The distances between HI superclouds in the two arms that are the brightest in
neutral hydrogen, the Carina arm and the Cygnus (Outer) arm, concentrate to two
values, permitting to assume the presence of a regular magnetic field in these
arms.Comment: 21 pages, 14 fugures; accepted for publication in Astronomichesky
Journal (Astron. Rep.
- …