2,160 research outputs found
Results of a Search for Paraphotons with Intense X-ray Beams at SPring-8
A search for paraphotons, or hidden U(1) gauge bosons, is performed using an
intense X-ray beamline at SPring--8. "Light Shining through a Wall" technique
is used in this search. No excess of events above background is observed. A
stringent constraint is obtained on the photon--paraphoton mixing angle, for .Comment: 10 pages, 4 figure
Cosmological constant and time delay
The effect of the cosmological constant on the time delay caused by an
isolated spherical mass is calculated without using the lens equation and
compared to a recent observational bound on the time delay of the lensed quasar
SDSS J1004+4112.Comment: 8 pages, 1 figur
Search for Photon-Photon Elastic Scattering in the X-ray Region
We report the first results of a search for real photon-photon scattering
using X rays. A novel system is developed to split and collide X-ray pulses by
applying interferometric techniques. A total of pulses (each
containing about photons) from an X-ray Free-Electron Laser are
injected into the system. No scattered events are observed, and an upper limit
of (95% C.L.) is obtained on the
photon-photon elastic scattering cross section at 6.5 keV
The Sloan Digital Sky Survey Quasar Lens Search. V. Final Catalog from the Seventh Data Release
We present the final statistical sample of lensed quasars from the Sloan
Digital Sky Survey (SDSS) Quasar Lens Search (SQLS). The well-defined
statistical lens sample consists of 26 lensed quasars brighter than i=19.1 and
in the redshift range of 0.6<z<2.2 selected from 50,836 spectroscopically
confirmed quasars in the SDSS Data Release 7 (DR7), where we restrict the image
separation range to 1"<\theta<20" and the i-band magnitude differences in two
image lenses to be smaller than 1.25 mag. The SDSS DR7 quasar catalog also
contains 36 additional lenses identified with various techniques. In addition
to these lensed quasars, we have identified 81 pairs of quasars from follow-up
spectroscopy, 26 of which are physically associated binary quasars. The
statistical lens sample covers a wide range of image separations, redshifts,
and magnitudes, and therefore is suitable for systematic studies of
cosmological parameters and surveys of the structure and evolution of galaxies
and quasars.Comment: 42 pages, 2 figures, 6 tables, accepted for publication in AJ; see
http://www-utap.phys.s.u-tokyo.ac.jp/~sdss/sqls/ for supplemental informatio
The Sloan Digital Sky Survey Quasar Lens Search. VI. Constraints on Dark Energy and the Evolution of Massive Galaxies
We present a statistical analysis of the final lens sample from the Sloan
Digital Sky Survey Quasar Lens Search (SQLS). The number distribution of a
complete subsample of 19 lensed quasars selected from 50,836 source quasars is
compared with theoretical expectations, with particular attention to the
selection function. Assuming that the velocity function of galaxies does not
evolve with redshift, the SQLS sample constrains the cosmological constant to
\Omega_\Lambda=0.79^{+0.06}_{-0.07}(stat.)^{+0.06}_{-0.06}(syst.) for a flat
universe. The dark energy equation of state is found to be consistent with w=-1
when the SQLS is combined with constraints from baryon acoustic oscillation
(BAO) measurements or results from the Wilkinson Microwave Anisotropy Probe
(WMAP). We also obtain simultaneous constraints on cosmological parameters and
redshift evolution of the galaxy velocity function, finding no evidence for
redshift evolution at z<1 in any combinations of constraints. For instance,
number density evolution quantified as \nu_n=d\ln\phi_*/d\ln(1+z) and the
velocity dispersion evolution \nu_\sigma=d\ln\sigma_*/d\ln(1+z) are constrained
to \nu_n=1.06^{+1.36}_{-1.39}(stat.)^{+0.33}_{-0.64}(syst.) and
\nu_\sigma=-0.05^{+0.19}_{-0.16}(stat.)^{+0.03}_{-0.03}(syst.) respectively
when the SQLS result is combined with BAO and WMAP for flat models with a
cosmological constant. We find that a significant amount of dark energy is
preferred even after fully marginalizing over the galaxy evolution parameters.
Thus the statistics of lensed quasars robustly confirm the accelerated cosmic
expansion.Comment: 44 pages, 12 figures, 4 tables, accepted for publication in A
The Chandra view of the Largest Quasar Lens SDSS J1029+2623
We present results from Chandra observations of the cluster lens SDSS
J1029+2623 at z_l=0.58, which is a gravitationally lensed quasar with the
largest known image separation. We clearly detect X-ray emission both from the
lensing cluster and the three lensed quasar images. The cluster has an X-ray
temperature of kT = 8.1 (+2.0, -1.2) keV and bolometric luminosity of L_X =
9.6e44 erg s^-1. Its surface brightness is centered near one of the brightest
cluster galaxies, and it is elongated East-West. We identify a subpeak
North-West of the main peak, which is suggestive of an ongoing merger. Even so,
the X-ray mass inferred from the hydrostatic equilibrium assumption appears to
be consistent with the lensing mass from the Einstein radius of the system. We
find significant absorption in the soft X-ray spectrum of the faintest quasar
image, which can be caused by an intervening material at either the lens or
source redshift. The X-ray flux ratios between the quasar images (after
correcting for absorption) are in reasonable agreement with those at optical
and radio wavelengths, and all the flux ratios are inconsistent with those
predicted by simple mass models. This implies that microlensing effect is not
significant for this system and dark matter substructure is mainly responsible
for the anomalous flux ratios.Comment: 35 pages, 8 figures. Accepted for publication in Ap
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