Diagnosis of the building stock using Energy Performance Certificates for urban energy planning in Mediterranean compact cities. Case of study: The city of València in Spain.

[EN] This research aims to diagnose the energy performance of buildings in València and identify areas where energy efficiency can be improved. The energy performance results of all 129,487 EPCs in the city were mapped and compared to socioeconomic variables to gain insights into the reasons behind the results. The study reveals that the city¿s building stock has poor energy performance, attributed to the lack of building standards during the city¿s expansion in the 1960s and 1970s. The worst energy performances are observed in the peripheral districts, particularly in the city¿s northern half, where low-income and low-renting rates are common, resulting in reduced investment capacity for individuals to retrofit their homes. To promote quick dissemination of measures to retrofit households, they must be adequate, economical, and replicable, avoiding social, administrative, and economic barriers. The study highlights the importance of EPCs as an objective tool to diagnose the energy efficiency of a city¿s building stock. Policymakers can use the findings to identify areas that require improvements and evaluate the appropriate actions to improve the building stock¿s energy performance. This study presents significant potential to reduce buildings¿ energy demand and achieve climate goals through EPCs.This article is an extended and updated version of a paper originally presented at the 17th Conference on Sustainable Development of Energy, Water and Environment Systems (SDEWES 2022) held in Paphos, Cyprus, over the period 6th to 10th November 2022 (denoted then as paper SDEWES2022.00306 Assessment of Buildings¿ Energy Efficiency over the Years at a City-wide Level: the Case of Valencia). This project has received funding from the European Union¿s Horizon Europe research and innovation programme under Grant Agreement No. 101075582. The Spanish public administration partly supported this work under the grant PURPOSED project (ref: PID2021-128822OB-I00), financed by the Spanish State Investigation Agency. The Catedra ¿ de Transicion ¿ Energ¿etica Urbana (Las Naves-VCiE-UPV) also supported this work. Thanks to Mireia Roncero Tarazona for creating the maps in this article.Manso-Burgos, Á.; Ribó-Pérez, DG.; Van As, J.; Montagud- Montalvá, C.; Royo, R. (2023). Diagnosis of the building stock using Energy Performance Certificates for urban energy planning in Mediterranean compact cities. Case of study: The city of València in Spain. Energy Conversion and Management: X. 20:1-18. https://doi.org/10.1016/j.ecmx.2023.1004501182

Office Chit-Chat as a Social Ritual: The Uplifting Yet Distracting Effects of Daily Small Talk at Work

This is the author accepted manuscript. The final version is available from the Academy of Management via the DOI in this recordSmall talk—short, superficial, or trivial communication not core to task completion—is normative and ubiquitous in organizations. Although small talk comprises one-third of adults’ speech, its effects at work have been discounted. Integrating theories of interaction rituals and micro-role transitions, we explore how and why seemingly inconsequential conversations during the workday generate meaningful effects on employees’ experiences. In a sample of employed adults from a Northeast US University’s alumni database and LinkedIn (n = 151), we used an experience sampling method (ESM) to capture within-individual variation in small talk over three weeks. We also conducted a validation of our daily small talk measure with Masters students from a Northeastern US University (n = 73) and two samples of employed adults registered with Amazon Turk (n = 180 and n = 202). Results showed that, on one hand, small talk enhanced employees’ daily positive social emotions at work, which translated into heightened organizational citizenship behaviors (OCB) and well-being at the end of the workday; on the other hand, small talk disrupted employees’ ability to cognitively engage in their work, which compromised their OCB. Our results also showed higher levels of trait-level self-monitoring mitigated the negative effects of small talk on work engagement. Combined, results suggest that the polite, ritualistic, and formulaic nature of small talk is often uplifting yet distracting

Instantaneous shrinking and single point extinction for viscous Hamilton-Jacobi equations with fast diffusion

International audienceFor a large class of non-negative initial data, the solutions to the quasilinear viscous Hamilton-Jacobi equation $\partial_t u-\Delta_p u+|\nabla u|^q=0$ in $(0,\infty)\times\mathbb{R}^N$ are known to vanish identically after a finite time when $2N/(N+1) 0$, the positivity set of $u(t)$ is a bounded subset of $\mathbb{R}^N$ even if $u_0 > 0$ in $\mathbb{R}^N$. This decay condition on $u_0$ is also shown to be optimal by proving that the positivity set of any solution emanating from a positive initial condition decaying at a slower rate as $|x|\to\infty$ is the whole $\mathbb{R}^N$ for all times. The time evolution of the positivity set is also studied: on the one hand, it is included in a fixed ball for all times if it is initially bounded (\emph{localization}). On the other hand, it converges to a single point at the extinction time for a class of radially symmetric initial data, a phenomenon referred to as \emph{single point extinction}. This behavior is in sharp contrast with what happens when $q$ ranges in $[p-1,p/2)$ and $p\in (2N/(N+1),2]$ for which we show \emph{complete extinction}. Instantaneous shrinking and single point extinction take place in particular for the semilinear viscous Hamilton-Jacobi equation when $p=2$ and $q\in (0,1)$ and seem to have remained unnoticed

The quest for the solar g modes

Solar gravity modes (or g modes) -- oscillations of the solar interior for which buoyancy acts as the restoring force -- have the potential to provide unprecedented inference on the structure and dynamics of the solar core, inference that is not possible with the well observed acoustic modes (or p modes). The high amplitude of the g-mode eigenfunctions in the core and the evanesence of the modes in the convection zone make the modes particularly sensitive to the physical and dynamical conditions in the core. Owing to the existence of the convection zone, the g modes have very low amplitudes at photospheric levels, which makes the modes extremely hard to detect. In this paper, we review the current state of play regarding attempts to detect g modes. We review the theory of g modes, including theoretical estimation of the g-mode frequencies, amplitudes and damping rates. Then we go on to discuss the techniques that have been used to try to detect g modes. We review results in the literature, and finish by looking to the future, and the potential advances that can be made -- from both data and data-analysis perspectives -- to give unambiguous detections of individual g modes. The review ends by concluding that, at the time of writing, there is indeed a consensus amongst the authors that there is currently no undisputed detection of solar g modes.Comment: 71 pages, 18 figures, accepted by Astronomy and Astrophysics Revie

Building Thriving Workforces from the Top Down: A Call and Research Agenda for Organizations to Proactively Support Employee Well-Being

Organizational researchers studying well-being – as well as organizations themselves – often place much of the burden on employees to manage and preserve their own well-being. Missing from this discussion is how – from a human resources management (HRM) perspective – organizations and managers can directly and positively shape the well-being of their employees. The authors use this review to paint a picture of what organizations could be like if they valued people holistically and embraced the full experience of employees’ lives to promote well-being at work. In so doing, the authors tackle five challenges that managers may have to help their employees navigate, but to date have received more limited empirical and theoretical attention from an HRM perspective: (1) recovery at work; (2) women’s health; (3) concealable stigmas; (4) caregiving; and (5) coping with socio-environmental jolts. In each section, the authors highlight how past research has treated managerial or organizational support on these topics, and pave the way for where research needs to advance from an HRM perspective. The authors conclude with ideas for tackling these issues methodologically and analytically, highlighting ways to recruit and support more vulnerable samples that are encapsulated within these topics, as well as analytic approaches to study employee experiences more holistically. In sum, this review represents a call for organizations to now – more than ever – build thriving organizations

Effectiveness of a mobile smoking cessation service in reaching elderly smokers and predictors of quitting

<p>Abstract</p> <p>Background</p> <p>Different smoking cessation programmes have been developed in the last decade but utilization by the elderly is low. We evaluated a pilot mobile smoking cessation service for the Chinese elderly in Hong Kong and identified predictors of quitting.</p> <p>Methods</p> <p>The Mobile Smoking Cessation Programme (MSCP) targeted elderly smokers (aged 60 or above) and provided service in a place that was convenient to the elderly. Trained counsellors provided individual counselling and 4 week's free supply of nicotine replacement therapy (NRT). Follow up was arranged at 1 month by face-to-face and at 3 and 6 months by telephone plus urinary cotinine validation. A structured record sheet was used for data collection. The service was evaluated in terms of process, outcome and cost.</p> <p>Results</p> <p>102 governmental and non-governmental social service units and private residential homes for the elderly participated in the MSCP. We held 90 health talks with 3266 elderly (1140 smokers and 2126 non-smokers) attended. Of the 1140 smokers, 365 (32%) received intensive smoking cessation service. By intention-to-treat, the validated 7 day point prevalence quit rate was 20.3% (95% confidence interval: 16.2%–24.8%). Smoking less than 11 cigarettes per day and being adherent to NRT for 4 weeks or more were significant predictors of quitting. The average cost per contact was US$54 (smokers only); per smoker with counselling: US$168; per self-reported quitter: US$594; and per cotinine validated quitter: US$827.</p> <p>Conclusion</p> <p>This mobile smoking cessation programme was acceptable to elderly Chinese smokers, with quit rate comparable to other comprehensive programmes in the West. A mobile clinic is a promising model to reach the elderly and probably other hard to reach smokers.</p

HBV DNA suppression during entecavir treatment in previously treated children with chronic hepatitis B

The aim of this study was to assess HBV DNA suppression after 24 weeks of treatment with entecavir in previously treated children with CHB. Thirty children aged 5–17 years (25 males and 5 females) with CHB were treated with entecavir 0.5 or 1 mg daily. Twenty-two children were HBeAg-positive, eight were HBeAg-negative, and in eight HBV polymerase mutations were detected. After 24 weeks of treatment, mean and median HBV DNA levels and ALT activity were lower versus baseline, overall and in both subgroups. The overall median HBV DNA level decreased from 1.2 x 107 IU/mL to 3.3 x 102 IU/mL (p < 0.000004), in HBeAg-positive from 7.8x107 IU/mL to 6.3x103 IU/mL (p < 0.00004), and in HBeAg-negative from 2.5x104 IU/mL to 5.01x101 IU/mL (p < 0.03). The serum HBV DNA disappearance was observed in 7/8 (88%) HBeAg-negative and in 5/22 (23%) HBeAg-positive patients. The overall mean ALT activity decreased from 164+ 290 U/L to 34.1+ 18.9 U/L (p < 0.000007), in HBeAg-positive from 214+326 U/L to 38.59+19.2 U/L (p < 0.000074), and in HBeAg-negative from 27+14 U/L to 20+8 U/L (p < 0.03). Twenty-four weeks of treatment with entecavir results in suppression of HBV DNA in a substantial proportion of children previously treated ineffectively with CHB

LEMUR: Large European Module for solar Ultraviolet Research. European contribution to JAXA's Solar-C mission

Understanding the solar outer atmosphere requires concerted, simultaneous solar observations from the visible to the vacuum ultraviolet (VUV) and soft X-rays, at high spatial resolution (between 0.1" and 0.3"), at high temporal resolution (on the order of 10 s, i.e., the time scale of chromospheric dynamics), with a wide temperature coverage (0.01 MK to 20 MK, from the chromosphere to the flaring corona), and the capability of measuring magnetic fields through spectropolarimetry at visible and near-infrared wavelengths. Simultaneous spectroscopic measurements sampling the entire temperature range are particularly important. These requirements are fulfilled by the Japanese Solar-C mission (Plan B), composed of a spacecraft in a geosynchronous orbit with a payload providing a significant improvement of imaging and spectropolarimetric capabilities in the UV, visible, and near-infrared with respect to what is available today and foreseen in the near future. The Large European Module for solar Ultraviolet Research (LEMUR), described in this paper, is a large VUV telescope feeding a scientific payload of high-resolution imaging spectrographs and cameras. LEMUR consists of two major components: a VUV solar telescope with a 30 cm diameter mirror and a focal length of 3.6 m, and a focal-plane package composed of VUV spectrometers covering six carefully chosen wavelength ranges between 17 and 127 nm. The LEMUR slit covers 280" on the Sun with 0.14" per pixel sampling. In addition, LEMUR is capable of measuring mass flows velocities (line shifts) down to 2 km/s or better. LEMUR has been proposed to ESA as the European contribution to the Solar C mission.Comment: 35 pages, 14 figures. To appear on Experimental Astronom

Interaction Between Convection and Pulsation

This article reviews our current understanding of modelling convection dynamics in stars. Several semi-analytical time-dependent convection models have been proposed for pulsating one-dimensional stellar structures with different formulations for how the convective turbulent velocity field couples with the global stellar oscillations. In this review we put emphasis on two, widely used, time-dependent convection formulations for estimating pulsation properties in one-dimensional stellar models. Applications to pulsating stars are presented with results for oscillation properties, such as the effects of convection dynamics on the oscillation frequencies, or the stability of pulsation modes, in classical pulsators and in stars supporting solar-type oscillations.Comment: Invited review article for Living Reviews in Solar Physics. 88 pages, 14 figure