4,338 research outputs found
Balmer-Like Series for Baryon Resonances
The pole positions of various baryon resonances have been found to reveal a
well pronounced clustering, the so-called H"ohler cluster. In a previous work,
the H"ohler clusters have been shown to be identical to Lorentz multiplets of
the type (1/2+l', 1/2+l')*[(1/2,0)+(0,1/2)] with l' integer. Here we show that
the cluster positions are well described by means of a Balmer-series like
recursive mass formula.Comment: 5 pages LaTex, World Scientific style, two tables. A missing additive
factor of +1 on the rhs of Eq. (2) has been inserted and thereby a misprint,
not an error, correcte
Background estimation strategies in CMS
The simulation or data-driven estimations of the diverse background processes to top quark decays are a key activity to be performed with the first data. This document describes some of these strategies and the possible achievements with an integrated luminosity of 20 pbâ1
Simultaneous BeppoSAX and RXTE observations of the X-ray burst sources GX 3+1 and Ser X-1
We have obtained spectral and timing data on GX 3+1 and Ser X-1. Both sources
were observed simultaneously with BeppoSAX and RXTE. The RXTE data is used to
provide power spectra and colour-colour diagrams in order to constrain the
state (and thus track ) the sources are in. The BeppoSAX data provide
the broad-band spectra. The spectra of both sources are reasonably well-fit
using a model consisting of a disk-blackbody, a comptonized component and a Fe
line, absorbed by interstellar absorption. The electron temperature (kT) of the Comptonizing plasma is in both cases 2.5 keV. This implies
that no strong high-energy tail from the Comptonized component is present in
either of the sources. We discuss the similarities between these burst sources
and the luminous X-ray sources located in globular clusters. We find that the
spectral parameters of the comptonized component provide information about the
mass-accretion rate, which agrees well with estimates from the timing and
spectral variations.Comment: 8 pages, accepted by A&
A comparison of broad iron emission lines in archival data of neutron star low-mass X-ray binaries
Relativistic X-ray disk-lines have been found in multiple neutron star
low-mass X-ray binaries, in close analogy with black holes across the
mass-scale. These lines have tremendous diagnostic power and have been used to
constrain stellar radii and magnetic fields, often finding values that are
consistent with independent timing techniques. Here, we compare CCD-based data
from Suzaku with Fe K line profiles from archival data taken with gas-based
spectrometers. In general, we find good consistency between the gas-based line
profiles from EXOSAT, BeppoSAX and RXTE and the CCD data from Suzaku,
demonstrating that the broad profiles seen are intrinsic to the line and not
broad due to instrumental issues. However, we do find that when fitting with a
Gaussian line profile, the width of the Gaussian can depend on the continuum
model in instruments with low spectral resolution, though when the different
models fit equally well the line widths generally agree. We also demonstrate
that three BeppoSAX observations show evidence for asymmetric lines, with a
relativistic disk-line model providing a significantly better fit than a
Gaussian. We test this by using the posterior predictive p-value method, and
bootstrapping of the spectra to show that such deviations from a Gaussian are
unlikely to be observed by chance.Comment: 13 pages, 9 figures, accepted to Ap
Morphological analysis on the coherence of kHz QPOs
We take the recently published data of twin kHz quasi-period oscillations
(QPOs) in neutron star (NS) lowmass X-ray binaries (LMXBs) as the samples, and
investigate the morphology of the samples, which focuses on the quality factor,
peak frequency of kHz QPOs, and try to infer their physical mechanism. We
notice that: (1) The quality factors of upper kHz QPOs are low (2 ~ 20 in
general) and increase with the kHz QPO peak frequencies for both Z and Atoll
sources. (2) The distribution of quality factor versus frequency for the lower
kHz QPOs are quite different between Z and Atoll sources. For most Z source
samples, the quality factors of lower kHz QPOs are low (usually lower than 15)
and rise steadily with the peak frequencies except for Sco X-1, which drop
abruptly at the frequency of about 750 Hz. While for most Atoll sources, the
quality factors of lower kHz QPOs are very high (from 2 to 200) and usually
have a rising part, a maximum and an abrupt drop. (3) There are three Atoll
sources (4U 1728-34, 4U 1636-53 and 4U 1608-52) of displaying very high quality
factors for lower kHz QPOs. These three sources have been detected with the
spin frequencies and sidebands, in which the source with higher spin frequency
presents higher quality factor of lower kHz QPOs and lower difference between
sideband frequency and lower kHz QPO frequency.Comment: 8 pages, 8 figures, publishe
RXTE Studies of X-ray Spectral Variations with Accretion Rate in 4U 1915-05
We present the results of detailed spectral studies of the ultra-compact low
mass X-ray binary (LMXB) 4U 1915-05 carried out with the Rossi X-ray Timing
Explorer (RXTE) during 1996. 4U 1915-05 is an X-ray burster (XRB) known to
exhibit a ~199-day modulation in its 2--12 keV flux. Observations were
performed with the PCA and HEXTE instruments on RXTE at roughly one-month
intervals to sample this long-term period and study accretion rate-related
spectral changes. We obtain good fits with a model consisting of a blackbody
and an exponentially cut-off power law. The spectral parameters are strongly
correlated with both the broad-band (2--50 keV) luminosity and the position in
the color-color diagram, with the source moving from a low hard state to a high
soft state as the accretion rate increases. The blackbody component appears to
drive the spectral evolution. Our results are consistent with a geometry in
which the soft component arises from an optically thick boundary layer and the
hard component from an extended Comptonizing corona. Comparing our results with
those of a similar study of the brighter source 4U 1820-30 (Bloser et al.
2000), we find that the two ultra-compact LMXBs occupy similar spectral states
even though the transitions occur at very different total luminosities.Comment: 27 pages LaTeX, 8 figures, accepted to the Astrophysical Journa
Ultrafast light-induced response of photoactive yellow protein chromophore analogues
The fluorescence decays of several analogues of the photoactive yellow protein (PYP) chromophore in aqueous solution have been measured by femtosecond fluorescence up-conversion and the corresponding time-resolved fluorescence spectra have been reconstructed. The native chromophore of PYP is a thioester derivative of p-coumaric acid in its trans deprotonated form. Fluorescence kinetics are reported for a thioester phenyl analogue and for two analogues where the thioester group has been changed to amide and carboxylate groups. The kinetics are compared to those we previously reported for the analogues bearing ketone and ester groups. The fluorescence decays of the full series are found to lie in the 1â10 ps range depending on the electron-acceptor character of the substituent, in good agreement with the excited-state relaxation kinetics extracted from transient absorption measurements. Steady-state photolysis is also examined and found to depend strongly on the nature of the substituent. While it has been shown that the ultrafast light-induced response of the chromophore in PYP is controlled by the properties of the protein nanospace, the present results demonstrate that, in solution, the relaxation dynamics and pathway of the chromophore is controlled by its electron donorâacceptor structure: structures of stronger electron donorâacceptor character lead to faster decays and less photoisomerisation
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