Are 'soft' policy instruments effective? The link between environmental management systems and the environmental performance of companies

Based on the analysis of a large dataset on the environmental performance of European companies in selected industrial sectors, the paper examines the question of whether the presence of an environmental management system (EMS) has a positive impact on the ecoefficiency of companies. It begins with a review of current evidence about the link between EMS and environmental performance, finding that despite much research into EMS there is still very little quantitative research on their actual environmental outcome. The second part of the paper uses three different statistical methods to assess whether companies and production sites with EMS perform better than those without and whether performance improves after an EMS has been introduced. Identifying only a weak link between EMS and eco-efficiency, the authors propose a number of possible explanations and warn against an overly-positive view of EMS as an autonomous driver of environmental performance.environmental management systems, environmental performance, eco-efficiency

The Relationship Between Social Support and Self-Advocacy in College Students with Disabilities

This study explored the connection between social support and self-advocacy in college students with disabilities. The College Students with Disabilities Campus Climate Survey (Lombardi, Gerdes, & Murray, 2011) was used to gather data from undergraduate students at a midsize western private university. Social support was found to be a significant predictor of self-advocacy in college students with disabilities. Peer support, family support, and faculty teaching practices made up the construct of social support. Peer support and faculty teaching practices were found to be significant predictors of student self-advocacy. Family support was not found to be significant. The data was examined for group differences between genders, disability types, and disability status (high incidence disabilities versus low incidence disabilities). No significant group differences were found. These findings suggest helping students build social support will increase their level of self-advocacy, which in turn may increase academic success

E_{10} Symmetry in One-dimensional Supergravity

We consider dimensional reduction of the eleven-dimensional supergravity to less than four dimensions. The three-dimensional $E_{8(+8)}/SO(16)$ nonlinear sigma model is derived by direct dimensional reduction from eleven dimensions. In two dimensions we explicitly check that the Matzner-Misner-type $SL(2,R)$ symmetry, together with the $E_8$, satisfies the generating relations of $E_9$ under the generalized Geroch compatibility (hypersurface-orthogonality) condition. We further show that an extra $SL(2,R)$ symmetry, which is newly present upon reduction to one dimension, extends the symmetry algebra to a real form of $E_{10}$. The new $SL(2,R)$ acts on certain plane wave solutions propagating at the speed of light. To show that this $SL(2,R)$ cannot be expressed in terms of the old $E_9$ but truly enlarges the symmetry, we compactify the final two dimensions on a two-torus and confirm that it changes the conformal structure of this two-torus.Comment: 33 pages, 3 figures. The action of the Chevalley generators of SL(2,R)_8 is corrected. Commutativity of SL(2,R)_0 and SL(2,R)_8 is checked in detail. The generalized Geroch compatibility (hypersurface-orthogonality) condition is derive

Digital Cavities and Their Potential Applications

The concept of a digital cavity is presented. The functionality of a tunable radio-frequency/microwave cavity with unrestricted Q-factor is implemented. The theoretical aspects of the cavity and its potential applications in high resolution spectroscopy and synchronization of clocks together with examples in signal processing and data acquisition are discussed

What produces the extended LINER-type emission in the NUGA galaxy NGC 5850?

(Abridged) The role of low ionization nuclear emission region (LINER) galaxies within the picture of active galactic nuclei (AGN) has been controversial. It is still not clear whether they host an AGN in a low accretion mode, or whether they are not active at all but dominated by alternative ionization mechanisms, namely shocks, winds/outflows, or photoionization by a post asymptotic giant branch (p-AGB) stellar population. The detection of extended LINER-like emission was often taken as evidence of ionization by stellar components but this has not been undisputed. We performed optical integral field spectroscopic observations on the central approx. 4 kpc of NGC 5850 using VIMOS at the VLT, which provides spatially-resolved spectra for the gas emission and the stellar continuum. We derive and analyse emission line and kinematic maps. We find the central few kpc of NGC 5850 to be dominated by extended LINER-like emission. The emission-line ratios that are sensitive to the ionization parameter increase with radial distance to the nucleus. Therefore, the extended LINER-like emission in NGC 5850 is dominated by ionization from distributed ionization sources, probably by stars on the p-AGB. The LINER-like region is surrounded by emission that is classed as 'composite', likely due to a mixture of a LINER-like ionization pattern and photoionization by low-level star formation. Two star-forming regions are present in the 21"x19" field of view. One of them is located approximately in the ring surrounding the kinematically decoupled core. The second one is close to the nucleus and is the origin of a region of decreased emission line ratios oriented radially outwards. We find the interstellar gas to have areas of steep velocity gradients and a complex kinematic morphology, probably caused by the lopsided (m=1) distribution of the gas. The inflow of gas toward the center appears possible.Comment: 18 pages, 17 figures, 2 tables, accepted by 'Astronomy and Astrophysics

Detection of gravitational waves in circular particle accelerators II. Response analysis and parameter estimation using synthetic data

We simulate the response of a Storage Ring Gravitational-wave Observatory (SRGO) to astrophysical gravitational waves (GWs), numerically obtaining its sensitivity curve, parameter degeneracies, and optimal choices of some controllable experiment parameters. We also generate synthetic noisy GW data and use Markov Chain Monte Carlo (MCMC) methods to perform parameter estimation of the source properties. With this, we show that a single SRGO could potentially localize the GW source in the sky using Earth's rotation. Then, we study the source sky localization area, mass and distance estimation errors as functions of noise, data sampling rate, and observing time. Finally, we discuss, along with its implications, the capacity of an SRGO to detect and constrain the parameters of millihertz (mHz) GW events.Comment: This manuscript is the sequel to Phys. Rev. D 102, 122006 (2020) or arXiv:2012.00529. This manuscript will be submitted for review and publication to Physical Review D (PRD). 21 pages, 10 figure