34,301 research outputs found
Majorana Fermion Induced Resonant Andreev Reflection
We describe experimental signatures of Majorana fermion edge states, which
form at the interface between a superconductor and the surface of a topological
insulator. If a lead couples to the Majorana fermions through electron
tunneling, the Majorana fermions induce \textit{resonant} Andreev reflections
from the lead to the grounded superconductor. The linear tunneling conductance
is () if there is an even (odd) number of vortices in the
superconductor. Similar resonance occurs for tunneling into the zero mode in
the vortex core. We also study the current and noise of a two-lead device.Comment: 4 pages, 3 figures. Discussion on STM tunneling into the Majorana
zero mode in the vortex core is adde
Comparisons of soil suction induced by evapotranspiration and transpiration of S. <i>heptaphylla</i>
For a given evapotranspiration (ETr), both soil evaporation and plant transpiration (Tr) would induce soil suction. However, the relative contribution of these two processes to the amount of suction induced is not clear. The objective of this study is to quantify ETr- and Tr-induced suction by a selected tree species, Scheffllera heptaphylla, in silty sand. The relative contribution of transpiration and evaporation to the responses of suction is then explored based on observed differences in Tr- and ETr-induced suction. In total, 12 test boxes were used for testing: 10 for vegetated soil with different values of leaf area index (LAI) and root area index (RAI), while two were for bare soil as references. Each box was exposed to identical atmospheric conditions controlled in a plant room for monitoring suction responses over a week. Due to the additional effects of soil evaporation, ETr-induced suction could be 3%–47% higher than Tr-induced suction, depending on LAI. The significance of evaporation reduced substantially when LAI was higher, as relatively less radiant energy fell on the soil surface for evaporation. For a given LAI, the effects of evaporation were less significant at deeper depths within the root zone. The effects of RAI associated with root-water uptake upon transpiration were the dominant process of ETr affecting the suction responses.</jats:p
Supersolid phase in spin dimer XXZ systems under magnetic field
Using quantum Monte Carlo method, we study, under external magnetic fields,
the ground state phase diagram of the two-dimensional spin =1/2 dimer model
with an anisotropic intra-plane antiferromagnetic coupling. With the anisotropy
, a supersolid phase characterized by a non-uniform
bose condensate density that breaks translational symmetry is found. The rich
phase diagram also contains a checkerboard solid and two different types of
superfluid phase formed by and spin triplets, with finite
staggered magnetization in z-axis and in-plane direction, respectively. As we
show, the model can be realized as a consequence of including the next nearest
neighbor coupling among dimers and our results suggest that spin dimer systems
may be an ideal model system to study the supersolid phase.Comment: 4 pages, 5 figure
Probing the Galaxy I. The galactic structure towards the galactic pole
Observations of (B-V) colour distributions towards the galactic poles are
compared with those obtained from synthetic colour-magnitude diagrams to
determine the major constituents in the disc and spheroid. The disc is
described with four stellar sub-populations: the young, intermediate, old, and
thick disc populations, which have respectively scale heights of 100 pc, 250
pc, 0.5 kpc, and 1.0 kpc. The spheroid is described with stellar contributions
from the bulge and halo. The bulge is not well constrained with the data
analyzed in this study. A non-flattened power-law describes the observed
distributions at fainter magnitudes better than a deprojected R^{1/4}-law.
Details about the age, metallicity, and normalizations are listed in Table 1.
The star counts and the colour distributions from the stars in the intermediate
fields towards the galactic anti-centre are well described with the stellar
populations mentioned above. Arguments are given that the actual solar offset
is about 15 pc north from the galactic plane.Comment: 11 pages TeX, 4 separate pages with additional figures, accepted for
publication in A&
Selective Equal-Spin Andreev Reflections Induced by Majorana Fermions
In this work, we find that Majorana fermions induce selective equal spin
Andreev reflections (SESARs), in which incoming electrons with certain spin
polarization in the lead are reflected as counter propagating holes with the
same spin. The spin polarization direction of the electrons of this Andreev
reflected channel is selected by the Majorana fermions. Moreover, electrons
with opposite spin polarization are always reflected as electrons with
unchanged spin. As a result, the charge current in the lead is spin-polarized.
Therefore, a topological superconductor which supports Majorana fermions can be
used as a novel device to create fully spin-polarized currents in paramagnetic
leads. We point out that SESARs can also be used to detect Majorana fermions in
topological superconductors.Comment: 5 pages, 3 figures. Comments are welcome. Title changed to match
published versio
[CI], [CII] and CO emission lines as a probe for alpha variations at low and high redshifts
The offsets between the radial velocities of the rotational transitions of
carbon monoxide and the fine structure transitions of neutral and singly
ionized carbon are used to test the hypothetical variation of the fine
structure constant, alpha. From the analysis of the [CI] and [CII] fine
structure lines and low J rotational lines of 12CO and 13CO, emitted by the
dark cloud L1599B in the Milky Way disk, we find no evidence for fractional
changes in alpha at the level of || < 3*10^-7. For the
neighbour galaxy M33 a stringent limit on Delta alpha/alpha is set from
observations of three HII zones in [CII] and CO emission lines: || < 4*10^-7. Five systems over the redshift interval z = 5.7-6.4,
showing CO J=6-5, J=7-6 and [CII] emission, yield a limit on || < 1.3*10^-5. Thus, a combination of the [CI], [CII], and CO
emission lines turns out to be a powerful tool for probing the stability of the
fundamental physical constants over a wide range of redshifts not accessible to
optical spectral measurements.Comment: 10 pages, 3 figures, 5 tables. Accepted for publication in MNRA
The Ratio of Total to Selective Extinction Toward Baade's Window
We measure the ratio of total to selective extinction, R_{VI}=A_V/E(V-I),
toward Baade's Window by comparing the VIK colors of 132 Baade's Window G and K
giants from Tiede, Frogel, & Terndrup with the solar-neighborhood (V-I),(V-K)
relation from Bessell & Brett. We find R_{VI}=2.283 +/- 0.016, and show that
our measurement has no significant dependence on stellar type from G0 to K4.
Adjusting the Paczynski et al. determination of the centroid of the dereddened
Baade's Window clump for this revised value of , we find I_{0,RC}=14.43
and (V-I)_{0,RC}=1.058. This implies a distance to the Baade's Window clump of
d_{BW} = 8.63 +/- 0.16 kpc, where the error bar takes account of statistical
but not systematic uncertainties.Comment: 8 pages, 1 figure, submitted to Ap
Proximity fingerprint of s+- superconductivity
We suggest a straightforward and unambiguous test to identify possible
opposite signs of superconducting order parameter in different bands proposed
for iron-based superconductors (s+- state). We consider proximity effect in a
weakly coupled sandwich composed of a s+- superconductor and thin layer of
s-wave superconductor. In such system the s-wave order parameter is coupled
differently with different s+- gaps and it typically aligns with one of these
gaps. This forces the other s+- gap to be anti-aligned with the s-wave gap. In
such situation the aligned band induces a peak in the s-wave density of states
(DoS), while the anti-aligned band induces a dip. Observation of such
contact-induced negative feature in the s-wave DoS would provide a definite
proof for s+- superconductivity.Comment: 4 pages, one figur
- …