1,337 research outputs found
Work-related psychological health and psychological type among lead elders within the Newfrontiers network of churches in the United Kingdom
Building on a series of recent studies concerned with assessing work-related psychological health and psychological type among various groups of church leaders, this study reports new data provided by 134 Lead Elders within the Newfrontiers network of churches in the United Kingdom who completed the Francis Psychological Type Scales (FPTS) together with the two scales of the Francis Burnout Inventory (FBI) concerned with emotional exhaustion and satisfaction in ministry. Compared with other groups of church leaders, Lead Elders within the Newfrontiers network of churches reported lower levels of emotional exhaustion and higher levels of satisfaction in ministry. Compared with other groups of church leaders, there was a higher proportion of extraverts among Lead Elders within the Newfrontiers network of churches. There was only a weak association between psychological type and burnout
Clergy work-related satisfactions in parochial ministry: the influence of personality and churchmanship
The aim of this study was to test several hypotheses that clergy work-related satisfaction could be better explained by a multidimensional rather than a unidimensional model. A sample of 1071 male stipendiary parochial clergy in the Church of England completed the Clergy Role Inventory, together with the short-form Revised Eysenck Personality Questionnaire. Factor analysis of the Clergy Role Inventory identified five separate clergy roles: Religious Instruction, Administration, Statutory Duties (conducting marriages and funerals), Pastoral Care, and Role Extension (including extra-parochial activities). Respondents also provided an indication of their predispositions on the catholic-evangelical and liberal-conservative dimensions. The significant associations of the satisfactions derived from each of the roles with the demographic, personality, and churchmanship variables were numerous, varied, and, with few exceptions, small in magnitude. Separate hierarchical regressions for each of the five roles indicated that the proportion of total variance explained by churchmanship was, in general, at least as great as that explained by personality, and was greater for three roles: Religious Instruction, Statutory Duties, and Role Extension. It was concluded that clergy satisfactions derived from different roles are not uniform and that churchmanship is at least as important as personality in accounting for clergy work satisfaction
Radiation in Lorentz violating electrodynamics
Synchrotron radiation is analyzed in the classical effective Lorentz
invariance violating model of Myers-Pospelov. Within the full far-field
approximation we compute the electric and magnetic fields, the angular
distribution of the power spectrum and the total emitted power in the m-th
harmonic, as well as the polarization. We find the appearance of rather
unexpected and large amplifying factors, which go together with the otherwise
negligible naive expansion parameter. This opens up the possibility of further
exploring Lorentz invariance violations by synchrotron radiation measurements
in astrophysical sources where these amplifying factors are important.Comment: Presented at the Second Mexican Meeting on Theoretical and
Experimental Physics, El Colegio Nacional, Mexico City, 6-10 September 200
Coronal X-Ray Emission from the Stellar Companions to Transiently Accreting Black Holes
Observations of soft X-ray transients (SXTs) in quiescence have found that
the binaries harboring black holes are fainter than those that contain a
neutron star. Narayan and collaborators postulated that the faint X-ray
emission from black hole binaries was powered by an advection dominated
accretion flow (ADAF). We explore an alternative explanation for the quiescent
X-ray emission from the black hole systems: coronal emission from the rapidly
rotating optical companion. This is commonly observed and well studied in other
tidally locked binaries, such as the RS CVns. We show that two of the three
X-ray detected black hole binaries (A0620-00 and GRO J1655-40) exhibit X-ray
fluxes entirely consistent with coronal emission. The X-ray spectra of these
objects should be best fit with thermal Raymond-Smith models rich in lines when
coronal emission predominates. One black hole system (V404 Cyg) is too X-ray
bright to be explained as coronal emission. The quiescent X-ray emission from
the neutron star binaries is far too bright for coronal emission. It might be
that all SXT's have variable accretion rates in quiescence and that the basal
quiescent X-ray flux is set by either coronal emission from the companion or --
when present -- by thermal emission from the neutron star. We also show that
the lithium abundances in the black hole systems are comparable to those in the
RS CVns, reducing the need for production mechanisms that involve the compact
object.Comment: ApJ, accepted (v541; Oct 1, 2000); Changes to figures and tables,
minor modifications to text. Uses emulateapj.sty. 14 pages, 3 figure
XMM-Newton observations of two black hole X-ray transients in quiescence
We report on XMM-Newton observations of GRO J1655-40 and GRS 1009-45, which
are two black hole X-ray transients currently in their quiescent phase. GRO
J1655-40 was detected with a 0.5 - 10 keV luminosity of 5.9 10^{31} erg/s. This
luminosity is comparable to a previous Chandra measurement, but ten times lower
than the 1996 ASCA value, most likely obtained when the source was not yet in a
true quiescent state. Unfortunately, XMM-Newton failed to detect GRS 1009-45. A
stringent upper limit of 8.9 10^{30} erg/s was derived by combining data from
the EPIC-MOS and PN cameras.
The X-ray spectrum of GRO J1655-40 is very hard as it can be fitted with a
power law model of photon index ~ 1.3 +/- 0.4. Similarly hard spectra have been
observed from other systems; these rule out coronal emission from the secondary
or disk flares as the origin of the observed X-rays. On the other hand, our
observations are consistent with the predictions of the disc instability model
in the case that the accretion flow forms an advection dominated accretion flow
(ADAF) at distances less than a fraction ~ 0.1 - 0.3) of the circularization
radius. This distance corresponds to the greatest extent of the ADAF that is
thought to be possible.Comment: 6 pages, 4 figures. Submitted to Astronomy and Astrophysic
Neutron rich matter, neutron stars, and their crusts
Neutron rich matter is at the heart of many fundamental questions in Nuclear
Physics and Astrophysics. What are the high density phases of QCD? Where did
the chemical elements come from? What is the structure of many compact and
energetic objects in the heavens, and what determines their electromagnetic,
neutrino, and gravitational-wave radiations? Moreover, neutron rich matter is
being studied with an extraordinary variety of new tools such as Facility for
Rare Isotope Beams (FRIB) and the Laser Interferometer Gravitational Wave
Observatory (LIGO). We describe the Lead Radius Experiment (PREX) that is using
parity violation to measure the neutron radius in 208Pb. This has important
implications for neutron stars and their crusts. Using large scale molecular
dynamics, we model the formation of solids in both white dwarfs and neutron
stars. We find neutron star crust to be the strongest material known, some 10
billion times stronger than steel. It can support mountains on rotating neutron
stars large enough to generate detectable gravitational waves. Finally, we
describe a new equation of state for supernova and neutron star merger
simulations based on the Virial expansion at low densities, and large scale
relativistic mean field calculations.Comment: 10 pages, 2 figures, Plenary talk International Nuclear Physics
Conference 2010, Vancouver, C
The X-ray spectrum of a disk illuminated by ions
The X-ray spectrum from a cool disk embedded in an ion supported torus is
computed. The interaction of the hot ions with the disk increases the hard
X-ray luminosity of the system}. A surface layer of the disk is heated by the
protons from the torus. The Comptonized spectrum produced by this layer has a
shape that depends only weakly on the incident energy flux and the distance
from the accreting compact object. It consists of a `blue bump' of
unComptonized soft photons and a flat high energy tail, reminiscent of the
observed spectra. The hard tail becomes flatter as the thermalization depth in
the cool disk is increased. Further evidence for ion illumination are the Li
abundance in the secondaries of low mass X-ray binaries and the 450 keV lines
sometimes seen in black-hole transient spectra.Comment: 7p, to appear in Monthly Notice
No Persistent Pulsations in Aql X-1 as it Fades into Quiescence
We searched for coherent X-ray pulsations from Aql X-1 in a series of RXTE
observations taken shortly after a recent outburst. During the course of these
observations, Aql X-1 passes through an apparent ``propeller'' phase as its
luminosity fades to its quiescent value. No pulsations were detected, and we
place upper limits (ranging from 0.52% to 9.0%) on the fractional RMS amplitude
of any periodic signal contained in the various data sets searched. This result
has implications for the geometry of the system, if the quiescent luminosity is
due to continued low-level accretion. Alternatively, our result supports the
idea that the quiescent luminosity may be due to thermal emission.Comment: 27 pages, 1 figure; ApJ, accepte
Virtual Compton scattering and the generalized polarizabilities of the proton at Q(2)=0.92 and 1.76 GeV2
Virtual Compton scattering (VCS) on the proton has been studied at the Jefferson Laboratory using the exclusive photon electroproduction reaction ep -\u3e ep gamma. This paper gives a detailed account of the analysis which has led to the determination of the structure functions P-LL - P-TT/epsilon and P-LT and the electric and magnetic generalized polarizabilities (GPs) alpha(E) (Q(2)) and beta(M) (Q(2)) at values of the four-momentum transfer squared Q(2) = 0.92 and 1.76 GeV2. These data, together with the results of VCS experiments at lower momenta, help building a coherent picture of the electric and magnetic GPs of the proton over the full measured Q(2) range and point to their nontrivial behavior
Virtual Compton scattering and neutral pion electroproduction in the resonance region up to the deep inelastic region at backward angles
We have made the first measurements of the virtual Compton scattering (VCS) process via the H(e, e\u27p). exclusive reaction in the nucleon resonance region, at backward angles. Results are presented for the W-dependence at fixed Q(2) = 1 GeV(2) and for the Q(2) dependence at fixed W near 1.5 GeV. The VCS data show resonant structures in the first and second resonance regions. The observed Q(2) dependence is smooth. The measured ratio of H(e, e\u27p). to H(e, e\u27p) pi(0) cross sections emphasizes the different sensitivity of these two reactions to the various nucleon resonances. Finally, when compared to real Compton scattering (RCS) at high energy and large angles, our VCS data at the highest W (1.8-1.9 GeV) show a striking Q(2) independence, which may suggest a transition to a perturbative scattering mechanism at the quark level
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