Precision Primordial 4^4He Measurement with CMB Experiments

Big bang nucleosynthesis (BBN) and the cosmic microwave background (CMB) are two major pillars of cosmology. Standard BBN accurately predicts the primordial light element abundances ($^4$He, D, $^3$He and $^7$Li), depending on one parameter, the baryon density. Light element observations are used as a baryometers. The CMB anisotropies also contain information about the content of the universe which allows an important consistency check on the Big Bang model. In addition CMB observations now have sufficient accuracy to not only determine the total baryon density, but also resolve its principal constituents, H and $^4$He. We present a global analysis of all recent CMB data, with special emphasis on the concordance with BBN theory and light element observations. We find $\Omega_{B}h^{2}=0.025+0.0019-0.0026$ and $Y_{p}=0.250+0.010-0.014$ (fraction of baryon mass as $^4$He) using CMB data alone, in agreement with $^4$He abundance observations. With this concordance established we show that the inclusion of BBN theory priors significantly reduces the volume of parameter space. In this case, we find $\Omega_{B}h^2=0.0244+0.00137-0.00284$ and $Y_p = 0.2493+0.0006-0.001$. We also find that the inclusion of deuterium abundance observations reduces the $Y_p$ and $\Omega_{B}h^2$ ranges by a factor of $\sim$2. Further light element observations and CMB anisotropy experiments will refine this concordance and sharpen BBN and the CMB as tools for precision cosmology.Comment: 7 pages, 3 color figures made minor changes to bring inline with journal versio

Horizontal Branch Stars: The Interplay between Observations and Theory, and Insights into the Formation of the Galaxy

We review HB stars in a broad astrophysical context, including both variable and non-variable stars. A reassessment of the Oosterhoff dichotomy is presented, which provides unprecedented detail regarding its origin and systematics. We show that the Oosterhoff dichotomy and the distribution of globular clusters (GCs) in the HB morphology-metallicity plane both exclude, with high statistical significance, the possibility that the Galactic halo may have formed from the accretion of dwarf galaxies resembling present-day Milky Way satellites such as Fornax, Sagittarius, and the LMC. A rediscussion of the second-parameter problem is presented. A technique is proposed to estimate the HB types of extragalactic GCs on the basis of integrated far-UV photometry. The relationship between the absolute V magnitude of the HB at the RR Lyrae level and metallicity, as obtained on the basis of trigonometric parallax measurements for the star RR Lyrae, is also revisited, giving a distance modulus to the LMC of (m-M)_0 = 18.44+/-0.11. RR Lyrae period change rates are studied. Finally, the conductive opacities used in evolutionary calculations of low-mass stars are investigated. [ABRIDGED]Comment: 56 pages, 22 figures. Invited review, to appear in Astrophysics and Space Scienc

Primordial Nucleosynthesis for the New Cosmology: Determining Uncertainties and Examining Concordance

Big bang nucleosynthesis (BBN) and the cosmic microwave background (CMB) have a long history together in the standard cosmology. The general concordance between the predicted and observed light element abundances provides a direct probe of the universal baryon density. Recent CMB anisotropy measurements, particularly the observations performed by the WMAP satellite, examine this concordance by independently measuring the cosmic baryon density. Key to this test of concordance is a quantitative understanding of the uncertainties in the BBN light element abundance predictions. These uncertainties are dominated by systematic errors in nuclear cross sections. We critically analyze the cross section data, producing representations that describe this data and its uncertainties, taking into account the correlations among data, and explicitly treating the systematic errors between data sets. Using these updated nuclear inputs, we compute the new BBN abundance predictions, and quantitatively examine their concordance with observations. Depending on what deuterium observations are adopted, one gets the following constraints on the baryon density: OmegaBh^2=0.0229\pm0.0013 or OmegaBh^2 = 0.0216^{+0.0020}_{-0.0021} at 68% confidence, fixing N_{\nu,eff}=3.0. Concerns over systematics in helium and lithium observations limit the confidence constraints based on this data provide. With new nuclear cross section data, light element abundance observations and the ever increasing resolution of the CMB anisotropy, tighter constraints can be placed on nuclear and particle astrophysics. ABRIDGEDComment: 54 pages, 20 figures, 5 tables v2: reflects PRD version minor changes to text and reference

Beyond induced mutants: using worms to study natural variation in genetic pathways

Induced mutants in the nematode Caenorhabditis elegans are used to study genetic pathways of processes ranging from aging to behavior. The effects of such mutations are usually analyzed in a single wildtype background: N2. However, studies in other species demonstrate that the phenotype(s) of induced mutations can vary widely depending on the genetic background. Moreover, induced mutations in one genetic background do not reveal the allelic effects that segregate in natural populations and contribute to phenotypic variation. Because other wildtype Caenorhabditis spp., including C. elegans, are now available, we review how current mapping resources and methodologies within and between species support the use of Caenorhabditis spp. for studying genetic variation, with a focus on pathways associated with human disease

Beyond induced mutants: using worms to study natural variation in genetic pathways

Induced mutants in the nematode Caenorhabditis elegans are used to study genetic pathways of processes ranging from aging to behavior. The effects of such mutations are usually analyzed in a single wildtype background: N2. However, studies in other species demonstrate that the phenotype(s) of induced mutations can vary widely depending on the genetic background. Moreover, induced mutations in one genetic background do not reveal the allelic effects that segregate in natural populations and contribute to phenotypic variation. Because other wildtype Caenorhabditis spp., including C. elegans, are now available, we review how current mapping resources and methodologies within and between species support the use of Caenorhabditis spp. for studying genetic variation, with a focus on pathways associated with human disease

Stop the Spin:The Role of Mindfulness Practices in Reducing Affect Spin

Affect spin refers to shifts in emotional states over time; it captures people's reactivity to affective events. Recent evidence suggests that affect spin has costs for both organizations and for employees, yet little is known about the antecedents of affect spin and possibilities to reduce it. The present study builds on existing research by examining mindfulness as an antecedent of affect spin in employees. Specifically, we hypothesized that mindfulness practice reduces affect spin over time. We also expected that levels of affect spin are positively related to emotional exhaustion and negatively to job satisfaction, both at the between- and the within-person level of analysis. Finally, we hypothesized that decreases in affect spin due to mindfulness practice are associated with lower levels of emotional exhaustion and higher levels of job satisfaction. To examine trajectories of affect spin over time, we tested our hypotheses in a randomized controlled mindfulness intervention study (with a wait-list control group; total N = 173 individuals) using experience sampling methods over the course of a month. Results revealed that mindfulness practice led to gradual decreases in affect spin over the course of the study. As expected, between-person differences in affect spin were positively related to emotional exhaustion and negatively to job satisfaction. However, affect spin was not related to well-being outcomes at the within-person level and decreases in affect spin over time were also not associated with levels of emotional exhaustion and job satisfaction

Worms under stress: C. elegans stress response and its relevance to complex human disease and aging

Many organisms have stress response pathways, components of which share homology with players in complex human disease pathways. Research on stress response in the nematode worm Caenorhabditis elegans has provided detailed insights into the genetic and molecular mechanisms underlying complex human diseases. In this review we focus on four different types of environmental stress responses – heat shock, oxidative stress, hypoxia, and osmotic stress – and on how these can be used to study the genetics of complex human diseases. All four types of responses involve the genetic machineries that underlie a number of complex human diseases such as cancer and neurodegenerative diseases, including Alzheimer's and Parkinson's. We highlight the types of stress response experiments required to detect the genes and pathways underlying human disease and suggest that studying stress biology in worms can be translated to understanding human disease and provide potential targets for drug discover

Stop the Spin: The Role of Mindfulness Practices in Reducing Affect Spin

Affect spin refers to shifts in emotional states over time; it captures people's reactivity to affective events. Recent evidence suggests that affect spin has costs for both organizations and for employees, yet little is known about the antecedents of affect spin and possibilities to reduce it. The present study builds on existing research by examining mindfulness as an antecedent of affect spin in employees. Specifically, we hypothesized that mindfulness practice reduces affect spin over time. We also expected that levels of affect spin are positively related to emotional exhaustion and negatively to job satisfaction, both at the between- and the within-person level of analysis. Finally, we hypothesized that decreases in affect spin due to mindfulness practice are associated with lower levels of emotional exhaustion and higher levels of job satisfaction. To examine trajectories of affect spin over time, we tested our hypotheses in a randomized controlled mindfulness intervention study (with a wait-list control group; total N = 173 individuals) using experience sampling methods over the course of a month. Results revealed that mindfulness practice led to gradual decreases in affect spin over the course of the study. As expected, between-person differences in affect spin were positively related to emotional exhaustion and negatively to job satisfaction. However, affect spin was not related to well-being outcomes at the within-person level and decreases in affect spin over time were also not associated with levels of emotional exhaustion and job satisfaction