8,121 research outputs found
Primordial Non-Gaussianity: Baryon Bias and Gravitational Collapse of Cosmic String Wakes
I compute the 3-D non-linear evolution of gas and dark matter fluids in the
neighbourhood of cosmic string wakes which are formed at high redshift
() for a ``realistic'' scenario of wake formation. These wakes
are the ones which stand out most prominently as cosmological sheets and are
expected to play a dominant r\^ole in the cosmic string model of structure
formation. Employing a high-resolution 3-D hydrodynamics code to evolve these
wakes until the present day yields results for the baryon bias generated in the
inner wake region. I find that today, wakes would be Mpc thick and
contain a 70% excess in the density of baryons over the dark matter density in
their centre. However, high density peaks in the wake region do not inherit a
baryon enhancement. I propose a mechanism for this erasure of the baryon excess
in spherically collapsed objects based on the geometry change around the
collapsing region. Further, I present heuristic arguments for the consequences
of this work for large scale structure in the cosmic string model and conclude
that the peculiarities of wake formation are unlikely to have significant
import on the discrepancy between power spectrum predictions and observations
in this model. If one invokes the nucleosynthesis bound on this
could be seen as strengthening the case against or for low Hubble
constants.Comment: 21 pages, 7 figures, 2 tables, prepared with the AASTeX package.
Minor modifications, results unchanged. ApJ in press, scheduled for Vol. 50
Gender Differences and Roles of Two Science Self-Efficacy Beliefs in Predicting Post-College Outcomes
The end of college is a key transition point when students prepare for the workforce or graduate school, and when competence beliefs that have been shaped throughout college play a particularly important role in decision-making processes. This study examined the roles of two competence beliefs, self-efficacy for scientific tasks and science academic self-efficacy, during the final year of college. A structural equation model was used to examine science research self-efficacy and science academic self-efficacy as predictors of post-graduation science career intentions and life satisfaction; prior achievement was also included as a predictor of competence beliefs and post-graduation outcomes. Findings indicated that both types of self-efficacy predicted career intentions and life satisfaction. To better understand the processes that contribute to gender gaps in certain science careers, gender differences in mean levels of self-efficacy and in the structural relations among the variables of interest were examined using multi-group analyses. Females reported lower academic self-efficacy, despite having similar levels of prior achievement and outcomes; structural relations also appeared to vary by gender. Results extend theoretical understanding of the roles of two distinct forms of self-efficacy and the potential mechanisms explaining gender gaps in science fields
Promoting Mental Health and Wellbeing with Men and Boys: What Works?
In May 2014 the Movember Foundation commissioned the Centre for Men’s Health, Leeds Beckett University, in collaboration with the Men’s Health Forum (England & Wales), to gather the current research evidence and practical (‘tacit’) knowledge about the core elements that make for successful work with boys and men around mental health promotion, early intervention and stigma reduction
Successful mental health promotion with men: evidence from 'tacit knowledge'
There remains significant concern about men’s mental health, particularly in terms of personal and societal barriers to help-seeking, negative coping mechanisms and high suicide rates. This paper presents findings from a multi-phase study looking at ‘what works’ in mental health promotion for men. Work here reports the collection and analysis of the tacit knowledge of those working within mental health promotion interventions for men. A ‘multiple hub and spoke’ approach was used to assist data collection. Thirteen key players, active in the men’s mental health field, half from the UK and half beyond, formed an Investigative Network collecting data, mainly through interviews, from wider geographical and professional community contexts where they had networks. The focus of data collection was on ‘what works’ in mental health promotion for men. Data was analysed using thematic analysis techniques. Findings suggest that settings which created safe male spaces acted to promote trust, reduce stigma and normalise men’s engagement in interventions. Embedding interventions within the communities of men being engaged, fully involving these men, and holding ‘male-positive’ values engendered familiarity and consolidated trust. Using ‘male-sensitive’ language and activity-based approaches allowed for positive expressions of emotions, facilitated social engagement, and provided a base for open communication. Appropriate partnerships were also seen as a necessary requirement for success and as crucial for maximising intervention impact. The importance of gender and ‘masculinity’ was apparent throughout these findings and taking time to understand gender could facilitate positive ways of working alongside men, increasing levels of engagement and successful outcomes
Molecular line CO (2→1) observations of ultraluminous IRAS galaxies
CO (J=2→1) observations of six ultraluminous IRAS galaxies are presented. Four of these galaxies have no previous CO J=2→1 data and two have no previous CO detections at all. Based on these observations, molecular hydrogen masses are estimated and range from 5x109 to 1.8x1010 M⊙. The present data follow the well established correlation that exists between the infrared luminosity LIR and the molecular mass content. The high values of the LIR/MH2 suggest either an increased star formation efficiency and / or an additional source of luminosity such as an active nucleus. The ratio R=(J=2→1)/(J=1→0) between the J=2→1 and 1→0 line temperatures, is examined next using our J=2→1 intensities and other published CO J=1→0 data. For Arp 220, Mrk 231, Mrk 273 R lies in the range 0.7 to 1.1; for IRAS 05189 the CO intensity and the ratio R were both found to have extremely low values. The low values of R≤1 found for all galaxies, suggest that the line profiles are dominated by emission coming from optically thick thermalized CO. Finally the line profiles are examined and compared to published models concerning the distribution and kinematics of the gas. Assuming that the CO is distributed in a disk as in normal spiral galaxies, then this region is probably concentrated towards the center of the galaxies
Recommended from our members
Scalable microaccordion mesh for deformable and stretchable metallic films
Elastically deformable materials can be created from rigids sheets through patterning appropriate meshes which can locally bend and flex. We demonstrate how micro-accordion patterns can be fabricated across large areas using three-beam interference lithography. Our resulting mesh induces a large and robust elasticity within any rigid material film. Gold coating the micro-accordion produces stretchable conducting films. Conductivity changes are negligible when the sample is stretched reversibly up to 30% and no major defects are introduced, in comparison to continuous sheets which quickly tear. Scaling analysis shows that our method is suited to further miniaturisation and large- scale fabrication of stretchable functional films. It thus opens routes to stretchable interconnects in electronic, photonic and sensing applications, as well as a wide variety of other deformable structures.We are grateful for funding from the Cambridge NanoDTC, ERC LINASS 320503 and UK EPSRC grants EP/G060649/1, EP/G037221/1, EP/L027151/1 and EP/L015978/1, as well as Nokia Research. RWB thanks Queens’ College Cambridge for financial support.This is the author accepted manuscript. The final version is available from APS via http://dx.doi.org/10.1103/PhysRevApplied.4.04400
A deep ATCA 20cm radio survey of the AKARI Deep Field South near the South Ecliptic Pole
The results of a deep 20 cm radio survey at 20 cm are reported of the AKARI
Deep Field South (ADF-S) near the South Ecliptic Pole (SEP), using the
Australia Telescope Compact Array telescope, ATCA. The survey has 1 sigma
detection limits ranging from 18.7--50 microJy per beam over an area of ~1.1 sq
degrees, and ~2.5 sq degrees to lower sensitivity. The observations, data
reduction and source count analysis are presented, along with a description of
the overall scientific objectives, and a catalogue containing 530 radio sources
detected with a resolution of 6.2" x 4.9". The derived differential source
counts show a pronounced excess of sources fainter than ~1 mJy, consistent with
an emerging population of star forming galaxies. Cross-correlating the radio
with AKARI sources and archival data we find 95 cross matches, with most
galaxies having optical R-magnitudes in the range 18-24 mag, and 52 components
lying within 1" of a radio position in at least one further catalogue (either
IR or optical). We have reported redshifts for a sub-sample of our catalogue
finding that they vary between galaxies in the local universe to those having
redshifts of up to 0.825. Associating the radio sources with the Spitzer
catalogue at 24 microns, we find 173 matches within one Spitzer pixel, of which
a small sample of the identifications are clearly radio loud compared to the
bulk of the galaxies. The radio luminosity plot and a colour-colour analysis
suggest that the majority of the radio sources are in fact luminous star
forming galaxies, rather than radio-loud AGN. There are additionally five cross
matches between ASTE or BLAST submillimetre galaxies and radio sources from
this survey, two of which are also detected at 90 microns, and 41 cross-matches
with submillimetre sources detected in the Herschel HerMES survey Public Data
release.Comment: MNRAS accepted and in press 9 July 2012: 28 pages, 15 Figures, 17
Table
The Feedback-Regulated Growth of Black Holes and Bulges through Gas Accretion and Starbursts in Cluster Central Dominant Galaxies
We present an analysis of the growth of black holes through accretion and
bulges through star formation in 33 galaxies at the centers of cooling flows.
Most of these systems show evidence of cavities in the intracluster medium
(ICM) inflated by radio jets emanating from their active galactic nuclei (AGN).
We present a new and extensive analysis of X-ray cavities in these systems. We
find that AGN are energetically able to balance radiative losses (cooling) from
the ICM in more than half of our sample. Using a subsample of 17 systems, we
examine the relationship between cooling and star formation. We find that the
star formation rates are approaching or are comparable to X-ray and far UV
limits on the rates of gas condensation onto the central galaxy. The remaining
radiative losses could be offset by AGN feedback. The vast gulf between
radiative losses and the sink of cooling material, which has been the primary
objection to cooling flows, has narrowed and, in some cases, is no longer a
serious issue. Using the cavity (jet) powers, we place strong lower limits on
the rate of growth of supermassive black holes in central galaxies, and we find
that they are growing at an average rate of ~ 0.1 solar masses per year, with
some systems growing as quickly as ~ 1 solar mass per year. We find a trend
between bulge growth (star formation) and black hole growth that is
approximately in accordance with the slope of the local (Magorrian) relation
between black hole and bulge mass. However, the large scatter in the trend
suggests that bulges and black holes do not always grow in lock step.
(Abridged)Comment: 17 pages, 6 figures, accepted to ApJ. Minor changes to text and
figure
- …