Smoking Cessation Programs for LGBTI People: A Systematic Review of Content and Effect

Despite widespread evidence of smoking’s harms to health, rising costs of tobacco products, and the visibility of public health interventions aimed at tobacco users, tobacco use remains high among lesbian women, gay men, bisexual people and transgender people (LGBT ) internationally, with US data showing at least double the smoking rates of the general population. [1-5] Although anecdotal evidence suggests similar rates internationally, no formal smoking data exist for intersex people, representing an important area for research.[6] There are many reasons why LGBT people may begin or continue smoking. Commonly cited reasons include minority stress due to the effects of discrimination, harassment, and violence; lack of social support; and fear of weight gain.[7,8] The NSW Tobacco Strategy 2012-17 stresses the importance of promoting smoking cessation and assistance to priority groups, i.e. those with high smoking prevalence.[9] Similarly to LGBT communities internationally, 30% of Australia’s LGB people smoke compared to 16% of the general population.[10-13] While smoking rates have declined among heterosexual people, the 2013 National Drug Strategy Household Survey shows no significant change among LGB people since 2010.[10] There is little specific Australian data regarding smoking rates amongst trans people, but one study in 2006 reported smoking rates of 44% of trans men and 35% of trans women.[14] Applying existing public health interventions to marginalised populations without modifying, piloting, and evaluating them may lead to further inequalities. In 2014, ACON received a Cancer Institute NSW Evidence to Practice Grant to develop a smoking cessation intervention to address the high and stable smoking rate among sexual minority women in Australia. The current review is intended to guide development of that intervention and promote future research on smoking cessation interventions for LGBT people.The production of this report would not have been possible without the financial support from an Evidence to Practice grant provided by the Cancer Institute NSW – Australia’s first state-wide, government-funded cancer control agency, funding from ACON Health – New South Wales’s leading health promotion organisation specialising in HIV prevention, HIV support, and lesbian, gay, bisexual, transgender and intersex (LGBTI) health, and in-kind support from the School of Public, University of Sydney

World History: Cultures, States, and Societies to 1500

Editor\u27s Description: World History: Cultures, States, and Societies to 1500 offers a comprehensive introduction to the history of humankind from prehistory to 1500. Authored by six USG faculty members with advance degrees in History, this textbook offers up-to-date original scholarship. It covers such cultures, states, and societies as Ancient Mesopotamia, Ancient Israel, Dynastic Egypt, India’s Classical Age, the Dynasties of China, Archaic Greece, the Roman Empire, Islam, Medieval Africa, the Americas, and the Khanates of Central Asia. It includes 350 high-quality images and maps, chronologies, and learning questions to help guide student learning. Its digital nature allows students to follow links to applicable sources and videos, expanding their educational experience beyond the textbook. It provides a new and free alternative to traditional textbooks, making World History an invaluable resource in our modern age of technology and advancement. Ancillary resources for this textbook were created under a Round 18 Continuous Improvement Grant.https://oer.galileo.usg.edu/history-textbooks/1001/thumbnail.jp

GRB 000911: Evidence for an Associated Supernova?

We present photometric and spectroscopic observations of the late afterglow of GRB 000911. We detect a moderately significant re-brightening in the R, I and J lightcurves, associated with a sizable reddening of the spectrum. This can be explained through the presence of an underlying supernova, outshining the afterglow ~ 30 days after the burst event

Estimating Redshifts for Long Gamma-Ray Bursts

We are constructing a program to estimate the redshifts for GRBs from the original Swift light curves and spectra, aiming to get redshifts for the Swift bursts \textit{without} spectroscopic or photometric redshifts. We derive the luminosity indicators from the light curves and spectra of each burst, including the lag time between low and high photon energy light curves, the variability of the light curve, the peak energy of the spectrum, the number of peaks in the light curve, and the minimum rise time of the peaks. These luminosity indicators can each be related directly to the luminosity, and we combine their independent luminosities into one weighted average. Then with our combined luminosity value, the observed burst peak brightness, and the concordance redshift-distance relation, we can derive the redshift for each burst. In this paper, we test the accuracy of our method on 107 bursts with known spectroscopic redshift. The reduced $\chi^2$ of our best redshifts ($z_{best}$) compared with known spectroscopic redshifts ($z_{spec}$) is 0.86, and the average value of $log_{10}(z_{best}/z_{spec})$ is 0.01, with this indicating that our error bars are good and our estimates are not biased. The RMS scatter of $log_{10}(z_{best}/z_{spec})$ is 0.26. For Swift bursts measured over a relatively narrow energy band, the uncertainty in determining the peak energy is one of the main restrictions on our accuracy. Although the accuracy of our $z_{best}$ values are not as good as that of spectroscopic redshifts, it is very useful for demographic studies, as our sample is nearly complete and the redshifts do not have the severe selection effects associated with optical spectroscopy.Comment: The Astrophysical Journal accepte

The short GRB070707 afterglow and its very faint host galaxy

We present the results from an ESO/VLT campaign aimed at studying the afterglow properties of the short/hard gamma ray burst GRB 070707. Observations were carried out at ten different epochs from ~0.5 to ~80 days after the event. The optical flux decayed steeply with a power-law decay index greater than 3, later levelling off at R~27.3 mag; this is likely the emission level of the host galaxy, the faintest yet detected for a short GRB. Spectroscopic observations did not reveal any line features/edges that could unambiguously pinpoint the GRB redshift, but set a limit z < 3.6. In the range of allowed redshifts, the host has a low luminosity, comparable to that of long-duration GRBs. The existence of such faint host galaxies suggests caution when associating short GRBs with bright, offset galaxies, where the true host might just be too dim for detection. The steepness of the decay of the optical afterglow of GRB 070707 challenges external shock models for the optical afterglow of short/hard GRBs. We argue that this behaviour might results from prolonged activity of the central engine or require alternative scenarios.Comment: 6 pages, 5 figures, accepted by A&

Absence of trapped surfaces and singularities in cylindrical collapse

The gravitational collapse of an infinite cylindrical thin shell of generic matter in an otherwise empty spacetime is considered. We show that geometries admitting two hypersurface orthogonal Killing vectors cannot contain trapped surfaces in the vacuum portion of spacetime causally available to geodesic timelike observers. At asymptotic future null infinity, however, congruences of outgoing radial null geodesics become marginally trapped, due to convergence induced by shear caused by the interaction of a transverse wave component with the geodesics. The matter shell itself is shown to be always free of trapped surfaces, for this class of geometries. Finally, two simplified matter models are analytically examined. For one model, the weak energy condition is shown to be a necessary condition for collapse to halt; for the second case, it is a sufficient condition for collapse to be able to halt.Comment: 26 pages, revtex4, 1 eps figure; matches version to appear in Phys. Rev. D (in press

Event horizons and apparent horizons in spherically symmetric geometries

Spherical configurations that are very massive must be surrounded by apparent horizons. These in turn, when placed outside a collapsing body, must propagate outward with a velocity equal to the velocity of radially outgoing photons. That proves, within the framework of (1+3) formalism and without resorting to the Birkhoff theorem, that apparent horizons coincide with event horizons.Comment: 5 pages, plainte

Numerical Approaches to Spacetime Singularities

This Living Review updates a previous version which its itself an update of a review article. Numerical exploration of the properties of singularities could, in principle, yield detailed understanding of their nature in physically realistic cases. Examples of numerical investigations into the formation of naked singularities, critical behavior in collapse, passage through the Cauchy horizon, chaos of the Mixmaster singularity, and singularities in spatially inhomogeneous cosmologies are discussed.Comment: 51 pages, 6 figures may be found in online version: Living Rev. Relativity 2002-1 at www.livingreviews.or