cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Awareness of Cervical Cancer Causes and Predeterminants of Likelihood to Screen Among Women in Haiti:
Creators: name: Calo, William A.
name: Gichane, Margaret W.
name: McCarthy, Schatzi H.
name: Beauvais, Harry A.
name: Walmer, Kathy A.
name: Boggan, Joel C.
name: Brewer, Noel T.
Publisher: name: The University of North Carolina at Chapel Hill University Libraries
Year: 2017

description: Cervical cancer is the leading cause of cancer deaths among women in Haiti. Given this high disease burden, we sought to better understand women's knowledge of its causes and the sociodemographic and health correlates of cervical cancer screening. Participants were 410 adult women presenting at clinics in Léogâne and Port-au-Prince, Haiti. We used bivariate and multivariate logic regression to identify correlates of Pap smear receipt. Only 29% of respondents had heard of human papillomavirus (HPV), whereas 98% were aware of cervical cancer. Of those aware of cervical cancer, 12% believed that sexually transmitted infections (STIs) cause it, and only 4% identified HPV infection as the cause. Women with a previous sexually transmitted infection were more likely to have had Pap smear (34% vs 71%, odds ratio = 3.45; 95% CI = 1.57-7.59). Screening was also more likely among women who were older than the age of 39 years, better educated, and employed (all p < .05). Almost all women (97%) were willing to undergo cervical cancer screening. This sample of Haitian women had limited awareness of HPV and cervical cancer causes; but when provided with health information, they saw the benefits of cancer screening. Future initiatives should provide health education messages, with efforts targeting young and at-risk women.
Fighting noise with noise in realistic quantum teleportation
Creators: name: Fortes, Raphael
name: Rigolin, Gustavo
Publisher: name: arXiv
Year: 2015
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We investigate how the efficiency of the quantum teleportation protocol is affected when the qubits involved in the protocol are subjected to noise or decoherence. We study all types of noise usually encountered in real world implementations of quantum communication protocols, namely, the bit flip, phase flip (phase damping), depolarizing, and amplitude damping noise. Several realistic scenarios are studied in which a part or all of the qubits employed in the execution of the quantum teleportation protocol are subjected to the same or different types of noise. We find noise scenarios not yet known in which more noise or less entanglement lead to more efficiency. Furthermore, we show that if noise is unavoidable it is better to subject the qubits to different noise channels in order to obtain an increase in the efficiency of the protocol.
description: 11 pages, 7 figures, RevTex4; v2: published version with new references
Musikleben im Oberamt Kirchheim/Teck im Spiegel der Lokalpresse 1832-1906
Creators: name: Eckstein, Susanne
Publisher: name: Universität Tübingen
Year: 2019
Subjects: subject: Musik , Geschichte , Württemberg , Alltagskultur , Musikleben , Kirchheim/Teck , Unterhaltungsmusik
subject: 780
subject: 900
subject: Musikpraxis
subject: Gesangvereine
subject: Musikkapellen
subject: Popularmusik
subject: 19. Jahrhundert

description: Diese chronologisch geordnete Quellensammlung umfasst Anzeigen, Meldungen, Konzertkritiken und Abbildungen aus den Lokalzeitungen des Oberamts Kirchheim/Teck von 1832 bis 1906 (vor allem Kirchheimer Wochenblatt und "Teckbote") mit Bezug auf das Musik- und Kulturleben; auch der zeitgeschichtliche Kontext ist berücksichtigt. Daraus entsteht ein facettenreiches Bild aller erdenklichen musikalischen Aktivitäten, gespiegelt in unterschiedlichsten medial vermittelten Informationen, von Instrumenten-Kleinanzeigen über Veranstaltungsanzeigen bis hin zu ausführlichen Konzertkritiken.
Deciphering the ultra-steep spectrum diffuse radio sources discovered in the cool-core cluster Abell~980
Creators: name: Salunkhe, Sameer
name: Paul, Surajit
name: Gopal-Krishna
name: Sonkamble, Satish
name: Bhagat, Shubham
Publisher: name: arXiv
Year: 2022
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: Clusters of galaxies are excellent laboratories for studying recurring nuclear activity in galactic nuclei since their hot gaseous medium can vastly prolong the detectability of their radio lobes via better confinement. We report here a multi-band study of the sparsely studied galaxy cluster Abell 980, based on our analysis of {\it{Chandra}} X-ray and the GMRT (150 and 325 MHz) and EVLA (1.5 GHz) radio archival data, revealing an unusually rich phenomenology. It is shown to be a quasi-relaxed cluster with a cool core ($T\sim4.2$ keV) surrounded by a hot and extensive intracluster medium (ICM) at $T\sim6.8$ keV. The radio emission shows a rich diversity, having (i) two large diffuse sources of ultra-steep spectrum (USS), extending to opposite extremities of the ICM, each associated with an X-ray brightness discontinuity (cold front), (ii) a bright radio-double of size $\sim55$ kpc coinciding with the central BCG, and (iii) a diffuse radio source, likely a mini-halo of size $\sim110$~kpc around the BCG which possesses a huge ellipsoidal stellar halo of extent $\sim 80$~kpc. The association of cold fronts with two highly aged (~ 260 Myr) USS sources in a cool-core cluster, makes it a very rare system. These USS sources are probably radio lobes from a previous episode of jet activity in the BCG, driven buoyantly towards the outskirts of the X-ray halo, thereby creating the cold fronts. A deeper radio image of this cluster may provide a rare opportunity to verify the recently proposed alternative model which explains radio mini-haloes as the aggregate radio emission from Type I supernovae occurring in the giant stellar halo extended across the cluster core.
description: 8 pages, 6 figures, Accepted for publication in A&A
How the Kurnool district in Andhra Pradesh, India, fought Corona
Creators: name: Dobe, Madhumita
name: Sahu, Monalisha
Publisher: name: South Eastern European Journal of Public Health (SEEJPH)
Year: 2020

description: Background: Kurnool, one of the four districts in the Rayalaseema region of the Indian state of Andhra Pradesh, emerged as a COVID-19 hotspot by mid-April 2020. Method: The authors compiled the publicly available information on different public health measures in Kurnool district and related them to the progression of COVID-19 from March to May 2020. Results: Two surges in pandemic progression of COVID-19 were recorded in Kurnool. The ini-tial upsurge in cases was attributed to return of people from other Indian states, along with return of participants of a religious congregation in Delhi, followed by in-migration of workers and truckers from other states and other districts of Andhra Pradesh, particularly from the state of Maharashtra (one of the worst affected states in India) and Chennai (the Koyambedu wholesale market - epicenter of the largest cluster of COVID-19 in Tamil Nadu). In a quick response to surging infections the state government launched operation ‘Kurnool Fights Corona’ to contain the outbreak. Kurnool had taken a targeted approach to testing, scaled up testing in areas with high case load, and conducted contact tracing for each positive case, along with requisitioning oxygenated beds in the district hospitals to meet the anticipated spurt in the number of positive cases. This combined approach paid rich dividends and from 26th April to May 9th, the growth curve flattened. Conclusion: Although the in migration of laborers and return of residents from other Indian states and abroad during the COVID-19 pandemic was a complex challenge, the timely actions of testing, tracing and isolation conducted by the district authorities in Kurnool greatly reduced transmission. Although this response assessment is based on a single district, the perspectives have revealed some important lessons regarding risk communication, preparedness and response for pandemics which will facilitate consolidation of the policy and program response to pandem-ics in future. Acknowledgement: Dr Sanjoy Sadhukhan (Professor, AIIH&PH) and District Authorities of Kurnool for their support. Conflicts of interest: None.
description: South Eastern European Journal of Public Health (SEEJPH), Volume XV, 2020
Prospects for Triple Gauge Coupling Measurements at Future Lepton Colliders and the 14 TeV LHC
Creators: name: Bian, Ligong
name: Shu, Jing
name: Zhang, Yongchao
Publisher: name: arXiv
Year: 2015
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The $WW$ production is the primary channel to directly probe the triple gauge couplings. We first analyze the $e^+ e^- \rightarrow W^+ W^-$ process at the future lepton collider, China's proposed Circular Electron-Positron Collider (CEPC). We use the five kinematical angles in this process to constrain the anomalous triple gauge couplings and relevant dimension six operators at the CEPC up to the order of magnitude of $10^{-4}$. The most sensible information is obtained from the distributions of the production scattering angle and the decay azimuthal angles. We also estimate constraints at the 14 TeV LHC, with both 300 fb$^{-1}$ and 3000 fb$^{-1}$ integrated luminosity from the leading lepton $p_T$ and azimuthal angle difference $Δϕ_{ll}$ distributions in the di-lepton channel. The constrain is somewhat weaker, up to the order of magnitude of $10^{-3}$. The limits on the triple gauge couplings are complementary to those on the electroweak precision observables and Higgs couplings. Our results show that the gap between sensitivities of the electroweak and triple gauge boson precision can be significantly decreased to less than one order of magnitude at the 14 TeV LHC, and that both the two sensitivities can be further improved at the CEPC.
description: 36 pages, 5 figures, 8 tables, version to appear in JHEP
High-Resolution M-band Spectroscopy of CO towards the Massive Young Stellar Binary W3 IRS5
Creators: name: Li, Jialu
name: Boogert, Adwin
name: Barr, Andrew G.
name: Tielens, Alexander G. G. M.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We present in this paper the results of high spectral resolution ($R$=88,100) spectroscopy at 4.7 $μ$m with iSHELL/IRTF of hot molecular gas close to the massive binary protostar W3 IRS5. The binary was spatially resolved and the spectra of the two sources (MIR1 and MIR2) were obtained simultaneously for the first time. Hundreds of $^{12}$CO $ν$=0-1, $ν$=1-2 lines, and $ν$=0-1 transitions of the isotopes of $^{12}$CO were detected in absorption, and are blue-shifted compared to the cloud velocity $v_{LSR}=-$38 km/s. We decompose and identify kinematic components from the velocity profiles, and apply rotation diagram and curve of growth analyses to determine their physical properties. Temperatures and column densities of the identified components range from 30$-$700 K and 10$^{21}-$10$^{22}$ cm$^{-2}$, respectively. Our curve of growth analyses consider two scenarios. One assumes a foreground slab with a partial covering factor, which well reproduces the absorption of most of the components. The other assumes a circumstellar disk with an outward decreasing temperature in the vertical direction, and reproduces the absorption of all the hot components. We attribute the physical origins of the identified components to the foreground envelope ($<$100 K), post-J-shock regions (200$-$300 K), and clumpy structures on the circumstellar disks ($\sim$600 K). We propose that the components with a J-shock origin are akin to water maser spots in the same region, and are complementing the physical information of water masers along the direction of their movements.
description: Accepted for publication in ApJ. 26 pages, 12 figures, and 9 tables. Comments are more than welcome!
National disaster preparedness and emergency response of nurses in Germany: An exploratory qualitative study
Creators: name: Grochtdreis, Thomas
name: Schröder-Bäck, Peter
name: Harenberg, Niels
name: Görres, Stefan
name: De Jong, Nynke
Publisher: name: South Eastern European Journal of Public Health (SEEJPH)
Year: 2020

description: Aim: This study aimed to explore the German nurses’ perceptions of their knowledge, roles and experience in the field of national preparedness and emergency response. Methods: An exploratory qualitative design was used with open-ended questions during semi-structured interviews with qualified nurses currently working in hospitals. The setting of the study consisted of wards of different hospitals in three northern federal states of Germany. The data analysis was done by summarizing analysis of the contents. From a convenient sample of n=31 hospitals, n=13 nurses were included in the study. Results: The median age of the participants was 45 years and 38% were female. Within the three professional socialization fields, knowledge, roles and experience, 17 themes were clustered. Conclusion: Within the themes of knowledge, role and experience in national disaster prepared-ness and emergency response, similarities and differences were explored in comparison to inter-national literature. Source of funding: This study did not receive any form of financial or other support. Acknowledgements: We would like to thank the nurses who participated in this study. We would also like to thank the nursing managers of the hospitals, the head of the departments and the head nurses for approaching their employees and colleagues. Conflict of interest: None declared
description: South Eastern European Journal of Public Health (SEEJPH), Volume XV, 2020
Multimodal Vulvar and Peripheral Sensitivity Among Women With Vulvodynia: A Case–Control Study
Creators: name: Gracely, Richard H.
name: Harlow, Sioban D.
name: Sen, Ananda
name: Reed, Barbara D.
name: Haefner, Hope K.
Publisher: name: The University of North Carolina at Chapel Hill University Libraries
Year: 2017

description: OBJECTIVE: To assess differences in vulvar and peripheral sensitivity between women with and without vulvodynia.

METHODS: Women with vulvodynia (n = 41) and age-matched controls (n = 43) seen in the outpatient setting were evaluated via surveys, clinical examination, and multimodal sensory testing (pressure, heat, cold, vibration, and electrical stimulation). The relationships between sensitivity to various sensory modalities and case/control status, as well as by vulvodynia subgroups, were assessed using logistic regression.

RESULTS: Women with vulvodynia were more sensitive to pressure and to electrical stimuli than were control women at the vulva (median, 22 vs 230 g and 0.495 vs 0.769 mA, respectively; P < 0.001 for each) and at the thumb (median, 2500 vs 4250 g and 0.578 vs 0.764 mA, respectively; P = 0.006 for pressure, P < 0.001 for electrical stimulation). Heat, cold, and vibration detection thresholds did not differ significantly between these groups (P > 0.025). Those reporting spontaneous pain versus provoked pain had greater pressure sensitivity to the thumb (median, 1850 vs 2690 g; P = 0.020) and greater electrical sensitivity at the introitus (0.450 vs 0.608 mA; P = 0.011), and those with primary versus secondary vulvodynia had substantially greater pressure sensitivity to the thumb (median, 2438 vs 3125 g, P = 0.004). However, having localized versus generalized vulvodynia was not associated with differences in pressure or electrical sensitivity.

CONCLUSIONS: Sensitivities to pressure and electrical stimuli are greater among vulvodynia cases than among controls and support 2 previously defined subgroups-those reporting spontaneous pain versus those whose pain only occurred when provoked, and those with primary versus secondary vulvodynia.
The health of the public: What has gone wrong?
Creators: name: Alderslade, Richard
name: Kokeny, Mihaly
name: Tsouros, Agis
Publisher: name: South Eastern European Journal of Public Health (SEEJPH)
Year: 2020

description: COVID-19, a new pandemic, has swept the world. How could this have happened? In theory the world should have been prepared, armed as it has been since 2005 with a new set of International Health Regulations with universal commitment by WHO Member States. Yet disaster has struck. The authors of this paper consider that fundamental rethinking is needed, with a new review of the post-World War 2 international system for global governance for health. Whilst WHO and its present and future actions will be scrutinized, the organization is fundamentally made up of 194 Member States, which must share the responsibility for ensuring better global health protection in the future. It is clear the world needs a more effective WHO, but it also needs countries to support and develop their public health infrastructure to face today’s more complex health challenges, which can only grow in scope and complexity over coming years. The paper proposes several key steps to achieve these goals. Conflict of interest: None declared.
description: South Eastern European Journal of Public Health (SEEJPH), Volume XV, 2020
Additional file 3 of ATM kinase inhibitor AZD0156 in combination with irinotecan and 5-fluorouracil in preclinical models of colorectal cancer
Creators: name: Davis, S. Lindsey
name: Hartman, Sarah J.
name: Bagby, Stacey M.
name: Schlaepfer, Marina
name: Yacob, Betelehem W.
name: Tse, Tonia
name: Simmons, Dennis M.
name: Diamond, Jennifer R.
name: Lieu, Christopher H.
name: Leal, Alexis D.
name: Cadogan, Elaine B.
name: Hughes, Gareth D.
name: Durant, Stephen T.
name: Messersmith, Wells A.
name: Pitts, Todd M.
Publisher: name: figshare
Year: 2022
Subjects: subject: Biochemistry
subject: Medicine
subject: Physiology
subject: FOS: Biological sciences
subject: Pharmacology
subject: Biotechnology
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences
subject: Cancer
subject: Hematology
subject: 60506 Virology

description: Additional file 3. ARRIVE guidelines checklist referencing details of animal experiments as outlined in the manuscript.
Discovery of gamma-ray pulsations of PSR J1835$-$3259B in the Globular Cluster NGC 6652
Creators: name: Zhang, Pengfei
name: Xing, Yi
name: Wang, Zhongxiang
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: Motivated by the newly discovery of a spin period 1.83\,ms pulsar J1835$-$3259B in the globular cluster (GC) NGC~6652, we analyze the gamma-ray data obtained with the Large Area Telescope (LAT) onboard {\it Fermi Gamma-ray Space Telescope (Fermi)} for the GC and detect the pulsations of this millisecond pulsar (MSP) at a 5.4$σ$ confidence level (the weighted H-test value is $\sim 41$). From timing analysis of the data, a pulse profile that is similar to the radio one is established. We thus consider that we have detected the \gr\ emission of the MSP, and discuss the implications. Based on our analysis results and different studies of the sources in the GC, the observed gamma-ray emission from the GC could mainly arise from this MSP, like the previous two cases the GCs NGC~6624 and NGC~6626. Assuming this is the case, the pulsar, at the GC's 9.46\,kpc distance and having a spin-down luminosity of $\leq 4.3\times 10^{35}$ erg s$^{-1}$, would have a gamma-ray luminosity of $\simeq (5.04\pm0.44)\times 10^{34}$ erg s$^{-1}$ and a gamma-ray efficiency of $\gtrsim 0.12$.
description: 5 pages, 2 figures, to appear in ApJL
Star Cluster Formation and Evolution in M101: An Investigation with the Legacy Extragalactic UV Survey
Creators: name: Linden, S. T.
name: Perez, G.
name: Calzetti, D.
name: Maji, S.
name: Messa, M.
name: Whitmore, B. C.
name: Chandar, R.
name: Adamo, A.
name: Grasha, K.
name: Cook, D. O.
name: Elmegreen, B. G.
name: Dale, D. A.
name: Sacchi, E.
name: Sabbi, E.
name: Grebel, E. K.
name: Smith, L.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We present Hubble Space Telescope WFC3/UVIS (F275W, F336W) and ACS/WFC optical (F435W, F555W, and F814W) observations of the nearby grand-design spiral galaxy M101 as part of the Legacy Extragalactic UV Survey (LEGUS). Compact sources detected in at least four bands were classified by both human experts and the convolutional neural network StarcNet. Human experts classified the 2,351 brightest sources, retrieving $N_{c} = 965$ star clusters. StarcNet, trained on LEGUS data not including M101, classified all 4,725 sources detected in four bands, retrieving $N_{c} = 2,270$ star clusters. The combined catalog represents the most complete census to date of compact star clusters in M101. We find that for the 2,351 sources with both a visual- and ML-classification StarcNet is able to reproduce the human classifications at high levels of accuracy ($\sim 80-90\%$), which is equivalent to the level of agreement between human classifiers in LEGUS. The derived cluster age distribution implies a disruption rate of $dN/dτ\propto τ^{-0.45 \pm 0.14}$ over $10^{7} < τ< 10^{8.5}$yr for cluster masses $\geq 10^{3.55} M_{\odot}$ for the central region of M101 and $dN/dτ\propto τ^{-0.02 \pm 0.15}$ for cluster masses $\geq 10^{3.38} M_{\odot}$ in the northwest region of the galaxy. The trends we recover are weaker than those of other nearby spirals (e.g. M51) and starbursts, consistent with the M101 environment having a lower-density interstellar medium, and providing evidence in favor of environmentally-dependent cluster disruption in the central, southeast, and northwest regions of M101.
description: 24 pages, 18 figures, 3 tables. Accepted for publication in the Astrophysical Journal
Socially responsible human resources management and stakeholders’ Health Promotion: A conceptual paper
Creators: name: Macassa, Gloria
name: Tomaselli, Gianpaolo
Publisher: name: South Eastern European Journal of Public Health (SEEJPH)
Year: 2020

description: The prime objective of this paper is to propose a new conceptual framework for how integrating corporate social responsibility (CSR) and human resources management (HRM) can impact on stakeholders’ health and wellbeing. The proposed framework argues that integrative socially responsible HRM (SR-HRM) policies coupled with public health literacy and integrative responsible leadership can play a significant role in shaping health behaviour change of internal stakeholders, which in turn can spill over to external stakeholders (family and proximate communities). From a health promotion and population health perspective, we see human resources (HR) as a leading partner in educating employees on the value of CSR and public health literacy programmes, and also as providing action plans on how to strategically and successfully implement these types of programmes. By helping to develop action plans to analyse CRS and public health literacy activities, HR professionals will be promoting both corporate citizenship and health behaviour change. Both of these are vital for developing a culture of social responsibility (and achieving the triple bottom line (TBL)) and sustainable population health promotion. Henceforth, SR-HRM policies and practices could help business organizations to contribute to the achievement of the United Nations’ Sustainable Development Goals (SDGs) and specifically Goals 3 and 8. This novel framework, which is especially pertinent to public health, has not yet been tested empirically. Hence, future studies are warranted to empirically test the theoretical framework using field data collection. Acknowledgements The authors would like to thank Dr Jesus Barrena-Martínez for his valuable comments and suggestions on the conceptual framework. GM is grateful for the support of the Department of Public Health and Sports Science at the University of Gävle, through the CSR-PhAM Programme and RELeSH project. Conflicts of interest: None declared.
description: South Eastern European Journal of Public Health (SEEJPH), Volume XV, 2020
Search for two-neutrino double electron capture on $^{124}$Xe with the XMASS-I detector
Creators: name: XMASS Collaboration
name: Abe, K.
name: Hiraide, K.
name: Ichimura, K.
name: Kishimoto, Y.
name: Kobayashi, K.
name: Kobayashi, M.
name: Moriyama, S.
name: Nakagawa, K.
name: Nakahata, M.
name: Norita, T.
name: Ogawa, H.
name: Sekiya, H.
name: Takachio, O.
name: Takeda, A.
name: Yamashita, M.
name: Yang, B. S.
name: Kim, N. Y.
name: Kim, Y. D.
name: Tasaka, S.
name: Liu, J.
name: Martens, K.
name: Suzuki, Y.
name: Fujita, R.
name: Hosokawa, K.
name: Miuchi, K.
name: Oka, N.
name: Onishi, Y.
name: Takeuchi, Y.
name: Kim, Y. H.
name: Lee, J. S.
name: Lee, K. B.
name: Lee, M. K.
name: Fukuda, Y.
name: Itow, Y.
name: Kegasa, R.
name: Kobayashi, K.
name: Masuda, K.
name: Takiya, H.
name: Uchida, H.
name: Nishijima, K.
name: Fujii, K.
name: Murayama, I.
name: Nakamura, S.
Publisher: name: arXiv
Year: 2015
Subjects: subject: Nuclear Experiment (nucl-ex)
subject: High Energy Physics - Experiment (hep-ex)
subject: Instrumentation and Detectors (physics.ins-det)
subject: FOS: Physical sciences

description: Double electron capture is a rare nuclear decay process in which two orbital electrons are captured simultaneously in the same nucleus. Measurement of its two-neutrino mode would provide a new reference for the calculation of nuclear matrix elements whereas observation of its neutrinoless mode would demonstrate lepton number violation. A search for two-neutrino double electron capture on $^{124}$Xe is performed using 165.9 days of data collected with the XMASS-I liquid xenon detector. No significant excess above background was observed and we set a lower limit on the half-life as $4.7 \times 10^{21}$ years at 90% confidence level. The obtained limit has ruled out parts of some theoretical expectations. We obtain a lower limit on the $^{126}$Xe two-neutrino double electron capture half-life of $4.3 \times 10^{21}$ years at 90% confidence level as well.
description: 6 pages, 3 figures, accepted for publication in Physics Letters B
Radio Emission from UV Cet: Auroral Emission from a Stellar Magnetosphere
Creators: name: Bastian, Timothy
name: Cotton, Bill
name: Hallinan, Gregg
Publisher: name: arXiv
Year: 2022
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: The archetypical flare star UV Cet was observed by MeerKAT on 5-6 October 2021. A large radio outburst with a duration of $\sim\!2$ hr was observed between 886-1682 MHz with a time resolution of 8s and a frequency resolution of 0.84 MHz, enabling sensitive dynamic spectra to be formed. The emission is characterized by three peaks containing a multitude of broadband arcs or partial arcs in the time-frequency domain. In general, the arcs are highly right-hand circularly polarized. During end of the third peak, brief bursts occur that are significantly elliptically polarized. We present a simple model that appears to be broadly consistent with the characteristics of the radio emission from UV Cet. Briefly, the stellar magnetic field is modeled as a dipole aligned with the rotational axis of the star. The radio emission mechanism is assumed to be due to the cyclotron maser instability where x-mode radiation near the electron gyrofrequency is amplified. While the elliptically polarized bursts may be intrinsic to the source, rather stringent limits are imposed on the plasma density in the source and along the propagation path. We suggest that the elliptically polarized radiation may instead be the result of reflection on an over-dense plasma structure at some distance from the source. Radio emission from UV~Cet shares both stellar and planetary attributes.
description: 29 pages, 10 figures
Additional file 1 of Nanoparticle-mediated selective Sfrp-1 silencing enhances bone density in osteoporotic mice
Creators: name: García-García, Patricia
name: Reyes, Ricardo
name: García-Sánchez, Daniel
name: Pérez-Campo, Flor María
name: Rodríguez-Rey, José Carlos
name: Évora, Carmen
name: Díaz-Rodríguez, Patricia
name: Delgado, Araceli
Publisher: name: figshare
Year: 2022
Subjects: subject: Biophysics
subject: Biochemistry
subject: Medicine
subject: Cell Biology
subject: Physiology
subject: FOS: Biological sciences
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Ecology
subject: Cancer

description: Additional file 1: Figure S1. Increase in the optimized NPs uptake after aptamer functionalization in murine MSC (C3H10T1/2) and fibroblasts (BALB/3T3). (*) denotes statistical significance to non-functionalized NPs (LPNPs) p < 0.05 (n = 5).
Painting new lines: Maximizing color difference in metro maps
Creators: name: Griffioen, Simone
name: Kiselev, Arthemy
Publisher: name: arXiv
Year: 2015
Subjects: subject: Optimization and Control (math.OC)
subject: Metric Geometry (math.MG)
subject: FOS: Mathematics
subject: 00A66, 65K10, 37C10, 37C50

description: Each metro line usually has its own color on the map. For obvious reasons, these colors should be maximally different. Suppose a new metro line is built. We now explain a strategy to choose the color or several colors for the new lines, making them as different as possible from both the old ones and each other. This is illustrated by using the Moscow metro map.
description: 9 pages, 4 figures, 3 tables
Angular Momentum Transport by Keplerian Turbulence in Liquid Metals
Creators: name: Vernet, Marlone
name: Fauve, Stephan
name: Gissinger, Christophe
Publisher: name: arXiv
Year: 2022
Subjects: subject: Fluid Dynamics (physics.flu-dyn)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Plasma Physics (physics.plasm-ph)
subject: FOS: Physical sciences

description: We report a laboratory study of the transport of angular momentum by a turbulent flow of an electrically conducting fluid confined in a thin disk. When the electromagnetic force applied to the liquid metal is large enough, the corresponding volume injection of angular momentum produces a turbulent flow characterized by a time-averaged Keplerian rotation rate $\barΩ\sim r^{-3/2}$. Two contributions to the local angular momentum transport are identified: one from the poloidal recirculation induced by the presence of boundaries, and the other from turbulent fluctuations in the bulk. The latter produces efficient angular momentum transport independent of the molecular viscosity of the fluid, and leads to Kraichnan's prediction $\text{Nu}_Ω\propto\sqrt{\text{Ta}}$. In this so-called ultimate regime, the experiment, therefore, provides a configuration analogous to accretion disks, allowing the prediction of accretion rates induced by Keplerian turbulence.
description: 6 pages, 5 figures, accepted in Phys. Rev. Lett
Tunable nonlinear graphene metasurfaces
Creators: name: Smirnova, Daria A.
name: Miroshnichenko, Andrey E.
name: Kivshar, Yuri S.
name: Khanikaev, Alexander B.
Publisher: name: arXiv
Year: 2015
Subjects: subject: Optics (physics.optics)
subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: We introduce the concept of nonlinear graphene metasurfaces employing the controllable interaction between a graphene layer and a planar metamaterial. Such hybrid metasurfaces support two types of subradiant resonant modes, asymmetric modes of structured metamaterial elements ("metamolecules") and graphene plasmons exhibiting strong mutual coupling and avoided dispersion crossing. High tunability of graphene plasmons facilitates strong interaction between the subradiant modes, modifying the spectral position and lifetime of the associated Fano resonances. We demonstrate that strong resonant interaction, combined with the subwavelength localization of plasmons, leads to the enhanced nonlinear response and high efficiency of the second-harmonic generation.
description: 6 pages, 5 figures
title: Making a Difference: Investing in Sustainable Health and Well-being for the People of Wales
Creators: name: Wales, Public Health
Publisher: name: South Eastern European Journal of Public Health
Year: 2017

description: The 'Making a Difference: Investing in Sustainable Health and Well-being for the People of Wales' report offers research evidence and expert opinion in support of preventing ill health and reducing inequalities to achieve a sustainable economy, thriving society and optimum health and well-being for the present and future generations in Wales.

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description: South Eastern European Journal of Public Health, Books
Diffusion-mediated  129 Xe gas depolarization in magnetic field gradients during continuous-flow optical pumping
Creators: name: Branca, Rosa Tamara
name: Burant, Alex
Publisher: name: The University of North Carolina at Chapel Hill University Libraries
Year: 2016

description: The production of large volumes of highly polarized noble gases like helium and xenon is vital to applications of magnetic resonance imaging and spectroscopy with hyperpolarized (HP) gas in humans. In the past ten years, (129)Xe has become the gas of choice due to its lower cost, higher availability, relatively high tissue solubility, and wide range of chemical shift values. Though near unity levels of xenon polarization have been achieved in-cell using stopped-flow Spin Exchange Optical Pumping (SEOP), these levels are currently unmatched by continuous-flow SEOP methods. Among the various mechanisms that cause xenon relaxation, such as persistent and transient xenon dimers, wall collisions, and interactions with oxygen, relaxation due to diffusion in magnetic field gradients, caused by rapidly changing magnetic field strength and direction, is often ignored. However, during continuous-flow SEOP production, magnetic field gradients may not have a negligible contribution, especially considering that this methodology requires the combined use of magnets with very different characteristics (low field for spin exchange optical pumping and high field for the reduction of xenon depolarization in the solid state during the freeze out phase) that, when placed together, inevitably create magnetic field gradients along the gas-flow-path. Here, a combination of finite element analysis and Monte Carlo simulations is used to determine the effect of such magnetic field gradients on xenon gas polarization with applications to a specific, continuous-flow hyperpolarization system.
Electron Quantization in Broken Atomic Wires
Creators: name: Do, Eui Hwan
name: Yeom, Han Woong
Publisher: name: arXiv
Year: 2015
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: We demonstrate using scanning tunneling microscopy and spectroscopy the electron quantization within metallic Au atomic wires self-assembled on a Si(111) surface and segmented by adatom impurities. The local electronic states of wire segments with a length up to 10 nm are investigated as terminated by two neighboring Si adatoms. One dimensional (1D) quantum well states are well resolved by their spatial distributions and the inverse-length-square dependence in their energies. The quantization also results in the quantum oscillation of the conductance at the Fermi level. These results deny the dopant role of the adatoms assumed for a long time but indicate their strong scattering nature. The present approach provides a new and convenient platform to investigate 1D quantum phenomena with atomic precision.
description: 5 pages, 4 figures
Intracluster magnetic filaments and an encounter with a radio jet
Creators: name: Rudnick, Lawrence
name: Bruggen, Marcus
name: Brunetti, Gianfranco
name: Cotton, William
name: Forman, William
name: Jones, Thomas W.
name: Nolting, Chris
name: Schellenberger, Gerrit
name: van Weeren, Reinout
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Thin synchrotron-emitting filaments are increasingly seen in the intracluster medium (ICM). We present the first example of a direct interaction between a magnetic filament, a radio jet, and a dense ICM clump in the poor cluster Abell 194. This enables the first exploration of the dynamics and possible histories of magnetic fields and cosmic rays in such filaments. Our observations are from the MeerKAT Galaxy Cluster Legacy Survey and the LOFAR Two Metre Sky Survey. Prominent 220 kpc long filaments extend east of radio galaxy 3C40B, with very faint extensions to 300 kpc, and show signs of interaction with its northern jet. They curve around a bend in the jet and intersect the jet in Faraday depth space. The X-ray surface brightness drops across the filaments; this suggests that the relativistic particles and fields contribute significantly to the pressure balance and evacuate the thermal plasma in a $\sim$35 kpc cylinder. We explore whether the relativistic electrons could have streamed along the filaments from 3C40B, and present a plausible alternative whereby magnetized filaments are a) generated by shear motions in the large-scale, post-merger ICM flow, b) stretched by interactions with the jet and flows in the ICM, amplifying the embedded magnetic fields, and c) perfused by re-energized relativistic electrons through betatron-type acceleration or diffusion of turbulently accelerated ICM cosmic ray electrons. We use the Faraday depth measurements to reconstruct some of the 3D structures of the filaments and of 3C40A and B.
description: Accepted for publication in ApJ. 32 pages, 28 figures. Each of the last four figures has a corresponding movie file (mpeg), available under the Ancillary Files associated with this preprint
Additional file 1 of Circulating Anti-Müllerian hormone in a cohort-study of women with severe obesity with and without polycystic ovary syndrome and the effect of a one-year weight loss intervention
Creators: name: Kataoka, Josefin
name: Larsson, Ingrid
name: Lindgren, Eva
name: Kindstrand, Li Oskarson
name: Schmidt, Johanna
name: Stener-Victorin, Elisabet
Publisher: name: figshare
Year: 2022
Subjects: subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Physiology
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Immunology
subject: FOS: Clinical medicine
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: Cancer
subject: Inorganic Chemistry

description: Supplementary Material 1
title: Global Population Health and Well-Being in the 21st Century: Toward New Paradigms, Policy and Practice
Creators: name: Behbod, Behrooz
name: George, Lueddeke R
Publisher: name: South Eastern European Journal of Public Health
Year: 2017

description: by George R Lueddeke, 476 p., 2016, Springer Publishing, New York, ISBN 978-082612767-9

Read: Introductory pages and chapter 1
description: South Eastern European Journal of Public Health, Books
title: Health: Systems – Lifestyle – Policies ; Forum for Public Health in Southeastern Europe Vol I
Creators: name: Burazeri, Genc
name: Kragelj, Lijana Zaletel
Publisher: name: South Eastern European Journal of Public Health
Year: 2017

description: A Handbook for Teachers, Researchers and Health Professionals (2nd edition)
 Editors: Genc Burazeri and Lijana Zaletel Kragelj
 Assistant editor: Kreshnik Petrela
 Lage 2013, 455 p., ISBN 978-3-89918-806-6
description: South Eastern European Journal of Public Health, Books
title: Health Investigation: Analysis – Planning – Evaluation ; Forum for Public Health in Southeastern Europe Vol II
Creators: name: Burazeri, Genc
name: Kragelj, Lijana Zaletel
Publisher: name: South Eastern European Journal of Public Health
Year: 2017

description: A Handbook for Teachers, Researchers and Health Professionals (2nd edition)
 Editors: Genc Burazeri and Lijana Zaletel Kragelj
 Assistant editor: Kreshnik Petrela and Herion Muja
 Lage 2013, 579 p., ISBN 978-3-89918-807-3
description: South Eastern European Journal of Public Health, Books
title: Modern Teaching – Distance Learning
Creators: name: ASPHER
Publisher: name: South Eastern European Journal of Public Health
Year: 2017

description: A Guide to online and blended Learning with Case Studies from Public Health
 Produced by the Working Group on Innovation and Good Practice in Public Health Education – ASPHER in cooperation with ASPHER members
 Lage 2013, 105 p., ISBN 978-3-89918-219-4
description: South Eastern European Journal of Public Health, Books
Knowledge and practice regarding bat-borne diseases among local residents in semi-urban area of central Thailand
Creators: name: Agari, Takahiro
Publisher: name: Chulalongkorn University Press
Year: 2018
Subjects: Bat-borne diseases
Knowledge and practice
Human-animal interface
Zoonosis
Thailand

description: Journal of Health Research, 32, Suppl.2, S177-S185
Simulated Photoevaporative Mass Loss from Hot Jupiters in 3D
Creators: name: Tripathi, Anjali
name: Kratter, Kaitlin M.
name: Murray-Clay, Ruth A.
name: Krumholz, Mark R.
Publisher: name: arXiv
Year: 2015
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: Ionizing stellar photons heat the upper regions of planetary atmospheres, driving atmospheric mass loss. Gas escaping from several hot, hydrogen-rich planets has been detected using UV and X-ray transmission spectroscopy. Because these planets are tidally locked, and thus asymmetrically irradiated, escaping gas is unlikely to be spherically symmetric. In this paper, we focus on the effects of asymmetric heating on local outflow structure. We use the Athena code for hydrodynamics to produce 3D simulations of hot Jupiter mass loss that jointly model wind launching and stellar heating via photoionization. Our fiducial planet is an inflated, hot Jupiter with radius $R_p=2.14 R_{\rm Jup}$ and mass $M_p = 0.53 M_{\rm Jup}$. We irradiate the initially neutral, atomic hydrogen atmosphere with 13.6 eV photons and compute the outflow's ionization structure. There are clear asymmetries in the atmospheric outflow, including a neutral shadow on the planet's nightside. Given an incident ionizing UV flux comparable to that of the Sun, we find a steady-state mass loss rate of ~$2\times10^{10}$ g s$^{-1}$. The total mass loss rate and the outflow substructure along the substellar ray show good agreement with earlier 1D models, for two different fluxes. Our 3D data cube can be used to generate the outflow's extinction spectrum during transit. As a proof of concept, we find absorption of stellar Lyman-alpha at Doppler-shifted velocities of up to $\pm 50$ km s$^{-1}$. Our work provides a starting point for further 3D models that can be used to predict observable signatures of hot Jupiter mass loss.
description: 16 pages, 15 figures, accepted for publication in ApJ. Replacement includes revised citations. Code is available for download and use from http://github.com/tripathi/Atmospheric-Athena
Inertial active Ornstein-Uhlenbeck particle in the presence of magnetic field
Creators: name: Muhsin, M
name: Sahoo, M
Publisher: name: arXiv
Year: 2022
Subjects: subject: Statistical Mechanics (cond-mat.stat-mech)
subject: FOS: Physical sciences

description: We consider an inertial active Ornstein-Uhlenbeck particle in an athermal bath. The particle is charged, constrained to move in a two-dimensional harmonic trap, and a magnetic field is applied perpendicular to the plane of motion. The steady state correlations and the mean square displacement are studied when the particle is confined as well as when it is set free from the trap. With the help of both numerical simulation and analytical calculations, we observe that inertia plays a crucial role in the dynamics in the presence of a magnetic field. In a highly viscous medium where the inertial effects are negligible, the magnetic field has no influence on the correlated behaviour of position as well as velocity. In the time asymptotic limit, the overall displacement of the confined harmonic particle gets enhanced by the presence of magnetic field and saturates for a stronger magnetic field. On the other hand, when the particle is set free, the overall displacement gets suppressed and approaches zero when strength of the field is very high. Interestingly, it is seen that in the time asymptotic limit, the confined harmonic particle behaves like a passive particle and becomes independent of the activity, especially in the presence of a very strong magnetic field. Similarly, for a free particle the mean square displacement in the long time limit becomes independent of activity even for a longer persistence of noise correlation in the dynamics.
description: Phys. Rev. E (Accepted), 9 pages, 6 figures
A phase field electro-chemo-mechanical formulation for predicting void evolution at the Li-electrolyte interface in all-solid-state batteries
Creators: name: Zhao, Y.
name: Wang, R.
name: Martínez-Pañeda, E.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: Computational Engineering, Finance, and Science (cs.CE)
subject: Applied Physics (physics.app-ph)
subject: Chemical Physics (physics.chem-ph)
subject: FOS: Physical sciences
subject: FOS: Computer and information sciences

description: We present a mechanistic theory for predicting void evolution in the Li metal electrode during the charge and discharge of all-solid-state battery cells. A phase field formulation is developed to model vacancy annihilation and nucleation, and to enable the tracking of the void-Li metal interface. This is coupled with a viscoplastic description of Li deformation, to capture creep effects, and a mass transfer formulation accounting for substitutional (bulk and surface) Li diffusion and current-driven flux. Moreover, we incorporate the interaction between the electrode and the solid electrolyte, resolving the coupled electro-chemical-mechanical problem in both domains. This enables predicting the electrolyte current distribution and thus the emergence of local current 'hot spots', which act as precursors for dendrite formation and cell death. The theoretical framework is numerically implemented, and single and multiple void case studies are carried out to predict the evolution of voids and current hot spots as a function of the applied pressure, material properties and charge (magnitude and cycle history). For both plating and stripping, insight is gained into the interplay between bulk diffusion, Li dissolution and deposition, creep, and the nucleation and annihilation of vacancies. The model is shown to capture the main experimental observations, including not only key features of electrolyte current and void morphology but also the sensitivity to the applied current, the role of pressure in increasing the electrode-electrolyte contact area, and the dominance of creep over vacancy diffusion.
Tidally synchronized solar dynamo: a rebuttal
Creators: name: Nataf, Henri-Claude
Publisher: name: arXiv
Year: 2022
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: The idea of a planetary origin for the solar cycle dates back to the nineteenth century. Despite unsurmounted problems, it is still advocated by some. Stefani, Giesecke, and Weier (2019) thus recently proposed a scenario based on this idea. A key argument they put forward is evidence that the $\sim$11 years-solar cycle is clocked. Their demonstration rests upon the computation of a ratio proposed by Dicke (1978) applied to the solar cycle time series of Schove (1955). I show that their demonstration is invalid, because the assumptions used by Schove to build his time series force a clocked behaviour. I also show that instabilities in a magnetized fluid can produce fluctuation time series that are close to being clocked.