7,805 research outputs found
Giant Microwave Absorption in Metallic Grains: Relaxation Mechanism
We show that the low frequency microwave absorption of an ensemble of small
metallic grains at low temperatures is dominated by a mesoscopic relaxation
mechanism. Giant positive magnetoresistance and very strong temperature
dependence of the microwave conductivity is predicted.Comment: 4 pages, REVTeX3+mutlticol+epsf, one EPS figur
Spitzer Constraints on the z=6.56 Galaxy Lensed by Abell 370
We report on Spitzer IRAC observations of the spectroscopically confirmed
z=6.56 lensed Ly-alpha emitting source HCM 6A which was found behind the
cluster Abell 370. Detection of the source at 3.6 and 4.5 microns,
corresponding to rest-frame optical emission, allows us to study the stellar
population of this primeval galaxy. The broadband flux density at 4.5 microns
is enhanced compared to the continuum at other wavelengths, likely due to the
presence of strong H-alpha in emission. The derived H-alpha line flux
corresponds to a star-formation rate of around 140 M_{sun}/yr, more than an
order of magnitude larger than estimates from the ultraviolet continuum and
Ly-alpha emission line. The dust extinction required to explain the discrepancy
is A_V of about 1 mag. The inference of dust at such high redshifts is
surprising and implies that the first epoch of star-formation in this galaxy
occurred at z~20.Comment: 11 pages, 3 figures, ApJ Letters in pres
Observations of Dense Molecular Gas in a Quasar Host Galaxy at z=6.42: Further Evidence for a Non-Linear Dense Gas - Star Formation Relation at Early Cosmic Times
We report a sensitive search for the HCN(J=2-1) emission line towards SDSS
J1148+5251 at z=6.42 with the VLA. HCN emission is a star formation indicator,
tracing dense molecular hydrogen gas (n(H2) >= 10^4 cm^-3) within star-forming
molecular clouds. No emission was detected in the deep interferometer maps of
J1148+5251. We derive a limit for the HCN line luminosity of L'(HCN) < 3.3 x
10^9 K km/s pc^2, corresponding to a HCN/CO luminosity ratio of L'(HCN)/L'(CO)
< 0.13. This limit is consistent with a fraction of dense molecular gas in
J1148+5251 within the range of nearby ultraluminous infrared galaxies (ULIRGs;
median value: L'(HCN)/L'(CO) = 0.17 {+0.05/-0.08}) and HCN-detected z>2
galaxies (0.17 {+0.09/-0.08}). The relationship between L'(HCN) and L(FIR) is
considered to be a measure for the efficiency at which stars form out of dense
gas. In the nearby universe, these quantities show a linear correlation, and
thus, a practically constant average ratio. In J1148+5251, we find
L(FIR)/L'(HCN) > 6600. This is significantly higher than the average ratios for
normal nearby spiral galaxies (L(FIR)/L'(HCN) = 580 {+510/-270}) and ULIRGs
(740 {+505/-50}), but consistent with a rising trend as indicated by other z>2
galaxies (predominantly quasars; 1525 {+1300/-475}). It is unlikely that this
rising trend can be accounted for by a contribution of AGN heating to L(FIR)
alone, and may hint at a higher median gas density and/or elevated
star-formation efficiency toward the more luminous high-redshift systems. There
is marginal evidence that the L(FIR)/L'(HCN) ratio in J1148+5251 may even
exceed the rising trend set by other z>2 galaxies; however, only future
facilities with very large collecting areas such as the SKA will offer the
sensitivity required to further investigate this question.Comment: 5 pages, 2 figures, 2 tables, to appear in ApJL (accepted October 24,
2007
Various features of quasiequilibrium sequences of binary neutron stars in general relativity
Quasiequilibrium sequences of binary neutron stars are numerically calculated
in the framework of the Isenberg-Wilson-Mathews (IWM) approximation of general
relativity. The results are presented for both rotation states of synchronized
spins and irrotational motion, the latter being considered as the realistic one
for binary neutron stars just prior to the merger. We assume a polytropic
equation of state and compute several evolutionary sequences of binary systems
composed of different-mass stars as well as identical-mass stars with adiabatic
indices gamma=2.5, 2.25, 2, and 1.8. From our results, we propose as a
conjecture that if the turning point of binding energy (and total angular
momentum) locating the innermost stable circular orbit (ISCO) is found in
Newtonian gravity for some value of the adiabatic index gamma_0, that of the
ADM mass (and total angular momentum) should exist in the IWM approximation of
general relativity for the same value of the adiabatic index.Comment: Text improved, some figures changed or deleted, new table, 38 pages,
31 figures, accepted for publication in Phys. Rev.
The Stellar Population of Lyman-alpha Emitting Galaxies at z ~ 5.7
We present a study of three Lyman-alpha emitting galaxies (LAEs), selected
via a narrow-band survey in the GOODS northern field, and spectroscopically
confirmed to have redshifts of z ~ 5.65. Using HST ACS and Spitzer IRAC data,
we constrain the rest-frame UV-to-optical spectral energy distributions (SEDs)
of the galaxies. Fitting stellar population synthesis models to the observed
SEDs, we find best-fit stellar populations with masses between ~ 10^9 - 10^10
M_sun and ages between ~ 5 - 100 Myr, assuming a simple starburst star
formation history. However, stellar populations as old as 700 Myr are
admissible if a constant star formation rate model is considered. Very deep
near-IR observations may help to narrow the range of allowed models by
providing extra constraints on the rest-frame UV spectral slope. Our
narrow-band selected objects and other IRAC-detected z ~ 6 i'-dropout galaxies
have similar 3.6 um magnitudes and z' - [3.6] colors, suggesting that they
posses stellar populations of similar masses and ages. This similarity may be
the result of a selection bias, since the IRAC-detected LAEs and i'-dropouts
probably only sample the bright end of the luminosity function. On the other
hand, our LAEs have blue i' - z' colors compared to the i'-dropouts, and would
have been missed by the i'-dropout selection criterion. A better understanding
of the overlap between the LAE and the i'-dropout populations is necessary in
order to constrain the properties of the overall high-redshift galaxy
population, such as the total stellar mass density at z ~ 6.Comment: 10 pages, 8 figures. Accepted for publication in Ap
Gravitational waves from black hole-neutron star binaries I: Classification of waveforms
Using our new numerical-relativity code SACRA, long-term simulations for
inspiral and merger of black hole (BH)-neutron star (NS) binaries are
performed, focusing particularly on gravitational waveforms. As the initial
conditions, BH-NS binaries in a quasiequilibrium state are prepared in a
modified version of the moving-puncture approach. The BH is modeled by a
nonspinning moving puncture and for the NS, a polytropic equation of state with
and the irrotational velocity field are employed. The mass ratio of
the BH to the NS, , is chosen in the range between 1.5
and 5. The compactness of the NS, defined by , is chosen to be between 0.145 and 0.178. For a large value of for
which the NS is not tidally disrupted and is simply swallowed by the BH,
gravitational waves are characterized by inspiral, merger, and ringdown
waveforms. In this case, the waveforms are qualitatively the same as that from
BH-BH binaries. For a sufficiently small value of Q \alt 2, the NS may be
tidally disrupted before it is swallowed by the BH. In this case, the amplitude
of the merger and ringdown waveforms is very low, and thus, gravitational waves
are characterized by the inspiral waveform and subsequent quick damping. The
difference in the merger and ringdown waveforms is clearly reflected in the
spectrum shape and in the "cut-off" frequency above which the spectrum
amplitude steeply decreases. When an NS is not tidally disrupted (e.g., for
Q=5), kick velocity, induced by asymmetric gravitational wave emission, agrees
approximately with that derived for the merger of BH-BH binaries, whereas for
the case that the tidal disruption occurs, the kick velocity is significantly
suppressed.Comment: 25 pages, 3 jpg figures, accepted for publication in PRD; erratum is
added on Jul 23. 201
The detection and photometric redshift determination of distant galaxies using SIRTF's Infrared Array Camera
We investigate the ability of the Space Infrared Telescope Facility's
Infrared Array Camera to detect distant (z ~ 3)galaxies and measure their
photometric redshifts. Our analysis shows that changing the original long
wavelength filter specifications provides significant improvements in
performance in this and other areas.Comment: 28 pages incl 12 figures; to appear in June 1999 PASP. Fig.12
replaced with corrected versio
Mechanical cleaning of graphene
Contamination of graphene due to residues from nanofabrication often
introduces background doping and reduces charge carrier mobility. For samples
of high electronic quality, post-lithography cleaning treatments are therefore
needed. We report that mechanical cleaning based on contact mode AFM removes
residues and significantly improves the electronic properties. A mechanically
cleaned dual-gated bilayer graphene transistor with hBN dielectrics exhibited a
mobility of ~36,000 cm2/Vs at low temperature.Comment: 4 pages, 4 figure
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