cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
title: ÐÐ½Ð°Ð»Ð¸Ð· Ð¸ Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ðµ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ Ñ Ð¾Ð½Ð¸Ð½Ð³Ð¾Ð²Ð°Ð½Ð¸Ñ Ð´Ð»Ð¸Ð½Ð½ÑÑ Ð¾ÑÐ²ÐµÑÑÑÐ¸Ð¹ Ð² Ð±ÑÐºÑÐ°Ñ ÑÐµÑÐ²Ð¾Ð¼Ð¾ÑÐ¾ÑÐ¾Ð²
title: Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð¼Ð°Ð³Ð¸ÑÑÑÐ°
titleType: Subtitle
Creators: name: ÐÐ¾ÑÐ¸Ð½ÐµÐ½ÐºÐ¾, ÐÐ°ÑÑÑ
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2018
Subjects: ÐÑÐ²ÐµÑÑÑÐ¸Ñ
Ð¡ÐµÑÐ²Ð¾Ð¼Ð¾ÑÐ¾ÑÑ
ÐÐ°Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸

description: Ð Ð°Ð±Ð¾ÑÐ° Ð¿Ð¾ÑÐ²ÑÑÐµÐ½Ð° Ð°Ð½Ð°Ð»Ð¸Ð·Ñ Ð¸ Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ñ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ ÑÐ¾Ð½Ð¸Ð½Ð³Ð¾Ð²Ð°Ð½Ð¸Ñ Ð´Ð»Ð¸Ð½Ð½ÑÑ Ð¾ÑÐ²ÐµÑÑÑÐ¸Ð¹ Ð² Ð±ÑÐºÑÐ°Ñ ÑÐµÑÐ²Ð¾Ð¼Ð¾ÑÐ¾ÑÐ¾Ð². Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ð° ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ñ Ð¸Ð·Ð³Ð¾ÑÐ¾Ð²Ð»ÐµÐ½Ð¸Ñ Ð´ÐµÑÐ°Ð»Ð¸ Â«ÐÑÐºÑÐ° Ð½ÐµÐ¿Ð¾Ð´Ð²Ð¸Ð¶Ð½Ð°ÑÂ» Ð½Ð° ÑÑÐ°Ð½ÐºÐµ Ñ Ð§ÐÐ£. ÐÐ°Ð³Ð¸ÑÑÐµÑÑÐºÐ°Ñ Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ñ ÑÐ²Ð»ÑÐµÑÑÑ ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑÐ½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐ¾Ð¹ Ð¸ ÑÐ¾ÑÑÐ¾Ð¸Ñ Ð¸Ð· ÑÑÐµÑ ÑÐ°Ð·Ð´ÐµÐ»Ð¾Ð²:
1. Ð¢ÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ°Ñ ÑÐ°ÑÑÑ;
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Cucinare un’altra Terra? Ecco la ricetta
Creators: Marco Malaspina
Publisher: name: Media Inaf
Year: 2015

La formula per creare un pianeta roccioso simile al nostro è più o meno sempre la stessa, anche al di fuori del Sistema solare. Lo mostrano i dati raccolti dallo strumento HARPS-N, installato alle Canarie sul Telescopio Nazionale Galileo dell’INAF
title: Nutritional and Economic Analysis of Small-Scale Agriculture in Imbabura, Ecuador
Creators: name: Erickson, Jake
Publisher: name: Utah State University
Year: 2013

description: Nutritional and Economic Analysis of Small-Scale Agriculture in Imbabura, Ecuador Intervention projects in the developing world normally aim to satisfy either the nutritional needs of a group, or advancing the economic stability, but not both. One of the many issues that may arise by narrowly focusing and creating an aid program is that although a group may be fed, they are not equipped to mitigate risks that will arise after project completion and thus continue or revert back to a malnourished state. A bridge is required to join the economic and nutritional programs to create aid interventions that are sustainable past the point of donor separation.
This paper proposes the creation of a linear program model to assess the effectiveness and sustainability of such intervention programs.
Investigating the effects of merging economic and nutrition interventions as pursued in this report required the first step to be the creation of economic information for a typical small-scale farm. The region of Cochas, Imbabura, Ecuador was selected as the study area in which data would be collected for a representative sample of production and living circumstances of a poor, rural, and small-scale farmer.
A comprehensive set of estimated cost and return (enterprise) budgets for small-scale agricultural crops that could be grown by the representative farm family used in this analysis was developed. This was accomplished via data collected in rural Ecuador by Jake Erickson, a Master's student in the department of Applied Economics at Utah State University. Of the supervisory committee, daily interaction occurred with Dr. DeeVon Bailey, project supervisor, and Dr. Ruby Ward, linear program specialist, whom were crucial in project completion. Various scenarios of the linear program were run with variations to the selection of nutritional requirements, off-farm income, and allowing food purchases off the family farm. Each of these scenarios was pursued as they mimic circumstances in which families may struggle to exist within the developing world. The results of each run are compared across the set of results to help understand what assumptions need to exist to validate an intervention's approach to improving the standard of living or nutrition of the world's poor, rural, small-scale farmers.
This model is a preliminary attempt at assessing the sustainability of merging common intervention approaches and it should be recognized that further development is needed to create a more encompassing model. Utilizing enterprise budgets, a linear programming model, and nutritional information, such as is done in this study, can help in planning rural development interventions as the income maximization and least-cost diet models are integrated into one within the resource and management constraints of the representative small-scale farm.
Ferromagnetic order in U(Rh,Co)Ge
Creators: name: Huy, N. T.
name: de Visser, A.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: We report the variation of ferromagnetic order in the pseudo-ternary compounds URh_{1-x}Co_{x}Ge (0 \leq x \leq 1). Magnetization and transport data taken on polycrystalline samples show that the Curie temperature T_{C} gradually increases with increasing Co content from a value of 9.5 K for URhGe to a maximum value of 20 K for x = 0.6 and then steadily decreases to 3 K for UCoGe. The magnetic interaction strength varies smoothly across the series. For all samples the electrical resistivity for T < T_{C} follows the behaviour ρ= ρ_{0} + AT^2. The A coefficient is dominated by scattering at spin waves and is strongly enhanced for x = 0 and 1.
description: 12 pages (4 figures), submitted to SSC
title: ÐÐ±ÑÐ°ÑÐµÐ½Ð¸Ðµ Ñ Ð¾ÑÑ Ð¾Ð´Ð°Ð¼Ð¸ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²Ð° Ð¸ Ð¿Ð¾ÑÑÐµÐ±Ð»ÐµÐ½Ð¸Ñ. ÐÐ¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ° ÑÑÐ°ÑÐ¸ÑÑÐ¸ÑÐµÑÐºÐ¾Ð¹ Ð¾ÑÑÐµÑÐ½Ð¾ÑÑÐ¸
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ
titleType: Subtitle
Creators: name: Ð¡ÐµÐ»Ð¸Ð²Ð°Ð½Ð¾Ð²Ð°, Ð¡Ð²ÐµÑÐ»Ð°Ð½Ð°
name: Ð§ÑÑÐ¾Ð², ÐÐ»ÐµÐºÑÐ°Ð½Ð´Ñ
Publisher: name: ÐÐÐÐÐ¢ÐÐ¥-ÐÐ ÐÐ¡Ð¡
Year: 2021
Subjects: ÐÑÑ Ð¾Ð´Ñ
ÑÑÐ°ÑÐ¸ÑÑÐ¸ÑÐµÑÐºÐ°Ñ Ð¾ÑÑÐµÑÐ½Ð¾ÑÑÑ
ÑÑÐµÐ±Ð½Ð¸ÐºÐ¸ Ð¸ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ñ Ð´Ð»Ñ Ð²ÑÐ·Ð¾Ð²

description: Ð ÑÑÐµÐ±Ð½Ð¾Ð¼ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ð¸ ÑÐ°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÑÑÑÑ Ð²Ð¾Ð¿ÑÐ¾ÑÑ, ÑÐ²ÑÐ·Ð°Ð½Ð½ÑÐµ Ñ ÑÑÐµÐ±Ð¾Ð²Ð°Ð½Ð¸ÑÐ¼Ð¸ Ðº Ð¿ÑÐ¸ÑÐ¾Ð´Ð¾Ð¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°ÑÐµÐ»ÑÐ¼, Ð² ÑÐ°ÑÑÐ¸ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ ÑÑÐ°ÑÐ¸ÑÑÐ¸ÑÐµÑÐºÐ¾Ð¹ Ð¾ÑÑÐµÑÐ½Ð¾ÑÑÐ¸ Ð¿Ð¾ ÑÐ¾ÑÐ¼Ðµ 2-Ð¢Ð (Ð¾ÑÑÐ¾Ð´Ñ), ÑÐ¾Ð´ÐµÑÐ¶Ð°ÑÐµÐ¹ ÑÐ²ÐµÐ´ÐµÐ½Ð¸Ñ Ð¾Ð± Ð¾Ð±ÑÐ°ÑÐµÐ½Ð¸Ð¸ Ñ Ð¾ÑÑÐ¾Ð´Ð°Ð¼Ð¸, Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð½ÑÐ¼Ð¸ Ð² ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐµ Ð¸Ñ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²ÐµÐ½Ð½Ð¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸, Ð´Ð»Ñ Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð² ÐºÐ¾Ð½ÑÑÐ¾Ð»Ð¸ÑÑÑÑÐ¸Ðµ Ð¾ÑÐ³Ð°Ð½Ñ. ÐÑÐµ Ð³Ð»Ð°Ð²Ñ ÑÑÐµÐ±Ð½Ð¾Ð³Ð¾ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ñ Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ñ Ð² ÑÐ¾Ð¾ÑÐ²ÐµÑÑÑÐ²Ð¸Ð¸ Ñ Ð´ÐµÐ¹ÑÑÐ²ÑÑÑÐ¸Ð¼ ÑÐµÐ´ÐµÑÐ°Ð»ÑÐ½ÑÐ¼ Ð¿ÑÐ¸ÑÐ¾Ð´Ð¾Ð¾ÑÑÐ°Ð½Ð½ÑÐ¼ Ð·Ð°ÐºÐ¾Ð½Ð¾Ð´Ð°ÑÐµÐ»ÑÑÑÐ²Ð¾Ð¼.
Ð£ÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ Ð¿ÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¾ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² Ð²ÑÐµÑ ÑÐ¾ÑÐ¼ Ð¾Ð±ÑÑÐµÐ½Ð¸Ñ Ð² ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ñ Ð²ÑÐ·Ð°Ñ Ð¸ Ð¼Ð¾Ð¶ÐµÑ Ð±ÑÑÑ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¾ Ð¿ÑÐ¸ Ð¸Ð·ÑÑÐµÐ½Ð¸Ð¸ Ð¸ Ð¿ÑÐµÐ¿Ð¾Ð´Ð°Ð²Ð°Ð½Ð¸Ð¸ ÑÐºÐ¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ñ, Ð³ÐµÐ¾ÑÐºÐ¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ñ Ð¸ Ð¿ÑÐ¸ÑÐ¾Ð´Ð¾Ð¾ÑÑÐ°Ð½Ð½ÑÑ Ð´Ð¸ÑÑÐ¸Ð¿Ð»Ð¸Ð½.
The impact of systematic uncertainties in stellar parameters on integrated spectra of stellar populations
Creators: name: Percival, Susan M.
name: Salaris, Maurizio
Publisher: name: arXiv
Year: 2009
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: In this paper we investigate a hitherto unexplored source of potentially significant error in stellar population synthesis (SPS) models, caused by systematic uncertainties associated with the three fundamental stellar atmospheric parameters; effective temperature T_eff, surface gravity g, and iron abundance [Fe/H]. All SPS models rely on calibrations of T_eff, logg and [Fe/H] scales, which are implicit in stellar models, isochrones and synthetic spectra, and are explicitly adopted for empirical spectral libraries. We assess the effect of a mismatch in scales between isochrones and spectral libraries (the two key components of SPS models) and quantify the effects on 23 commonly used diagnostic line indices. We find that typical systematic offsets of 100K in T_eff, 0.15 dex in [Fe/H] and/or 0.25 dex in logg significantly alter inferred absolute ages of simple stellar populations (SSPs) and that in some circumstances, relative ages also change. Offsets in T_eff, logg and [Fe/H] scales for a scaled-solar SSP produce deviations from the model which can mimic the effects of altering abundance ratios to non-scaled-solar chemical compositions, and could also be spuriously interpreted as evidence for a more complex population, especially when multiple-index or full-SED fitting methods are used. We stress that the behavior we find can potentially affect any SPS models, whether using full integrated spectra or fitting functions to determine line strengths. We present measured offsets in 23 diagnostic line indices and urge caution in the over-interpretation of line-index data for stellar populations.
description: 14 pages, including 4 figures and 3 tables. Accepted for publication in ApJ
title: Carrier Dynamics in InGaAs/GaAs Quantum Dots Excited by Femtosecond Laser Pulses
Creators: name: Chauhan, Kripa Nidhan
Publisher: name: Utah State University
Year: 2013

description: Ultrafast carrier dynamics studies have been carried out on samples with single layers of self-assembled In0.4Ga0.6As/GaAs quantum dots (QDs). Measurements were made using femtosecond degenerate pump-probe differential reflectivity with an 800-nm, 28-fs Ti-sapphire oscillator as the source. The QDs were grown via modified Stranski-Krastanov growth. This modified growth process consists of two steps: low-temperature growth and high-temperature annealing. Specifically, the InGaAs QD structures are fabricated on n-type GaAs(001) using molecular beam epitaxy. The InGaAs layer is deposited at 350-3700C followed by QD self assembly at 420-4900C. Finally, these QDs are capped with 10 nm or 100 nm of GaAs. The measured width and height of these QDs are typically 25 nm and 8 nm, respectively. Dots annealed at higher temperature have larger base area (width and length) and reduced height, as compared to those annealed at lower temperature. We have used a model consisting of a linear combination of an exponential decaying function to describe the carrier dynamics and fit the reflectivity data, revealing trends in the carrier capture and relaxation times associated with the InGaAs layer versus laser excitation level and QD morphology. Capture times are ~ 1 ps for the 100-nm capped samples, but slightly shorter for the 10-nm capped thin samples, indicating carrier transport plays a role in dynamics. The carrier dynamics in 10-nm capped samples are correlated with sample annealing temperature, indicating QD morphology affects carrier capture. Versus laser intensity, and thus carrier excitation level, the dynamics generally become slower, suggesting state filling is important in both the capture and relaxation of excited carriers in these samples.
Girocronologia stellare
Creators: Corrado Ruscica
Publisher: name: Media Inaf
Year: 2015

Al 225° meeting dell'AAS, che si sta svolgendo in questi giorni a Seattle, un gruppo di ricercatori guidati da Soren Meibom del CfA hanno presentato i risultati di un loro studio sull'applicazione di un metodo che permetterà di determinare in maniera più accurata l'età delle stelle. Si tratta di un nuovo, importante strumento di ricerca che gli astronomi potranno utilizzare non solo per studiare l’evoluzione delle stelle ma anche per identificare quei pianeti abbastanza evoluti dove potrebbero esistere forme di vita complesse.
title: Ð¢ÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ°Ñ ÑÐ¾Ð½ÐµÑÐ¸ÐºÐ° Ð°Ð½Ð³Ð»Ð¸Ð¹ÑÐºÐ¾Ð³Ð¾ ÑÐ·ÑÐºÐ°
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ
titleType: Subtitle
Creators: name: Ð¥ÑÑÐ½ÐµÐ½ÐºÐ¾Ð²Ð°, ÐÐ°ÑÐ¸Ð½Ð°
Publisher: name: ÐÐ·Ð´-Ð²Ð¾ ÐÐ¾Ð»Ð¸ÑÐµÑÐ½. ÑÐ½-ÑÐ°
Year: 2012
Subjects: Ð°Ð½Ð³Ð»Ð¸Ð¹ÑÐºÐ¸Ð¹ ÑÐ·ÑÐº
ÑÐ¾Ð½ÐµÑÐ¸ÐºÐ°
ÑÑÐµÐ±Ð½Ð¸ÐºÐ¸ Ð¸ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ñ Ð´Ð»Ñ Ð²ÑÐ·Ð¾Ð²

description: ÐÐ¾ÑÐ¾Ð±Ð¸Ðµ Â«Ð¢ÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ°Ñ ÑÐ¾Ð½ÐµÑÐ¸ÐºÐ° Ð°Ð½Ð³Ð»Ð¸Ð¹ÑÐºÐ¾Ð³Ð¾ ÑÐ·ÑÐºÐ°Â» Ð¿ÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¾ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² Ð¾ÑÐ½Ð¾Ð¹ Ð¸ Ð·Ð°Ð¾ÑÐ½Ð¾Ð¹ ÑÐ¾ÑÐ¼ Ð¾Ð±ÑÑÐµÐ½Ð¸Ñ. ÐÐ°ÑÐµÑÐ¸Ð°Ð» Ð½Ð°ÑÑÐ¾ÑÑÐµÐ³Ð¾ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ñ Ð¾ÑÐ²Ð°ÑÑÐ²Ð°ÐµÑ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ ÑÐ²Ð»ÐµÐ½Ð¸Ñ Ð·Ð²ÑÐºÐ¾Ð²Ð¾Ð³Ð¾ ÑÐ¾ÑÑÐ°Ð²Ð° ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð°Ð½Ð³Ð»Ð¸Ð¹ÑÐºÐ¾Ð³Ð¾ ÑÐ·ÑÐºÐ° Ð¸ ÑÐ¾Ð½ÐµÐ¼Ð½Ð¾Ð¹ ÑÑÑÑÐºÑÑÑÑ Ð°Ð½Ð³Ð»Ð¸Ð¹ÑÐºÐ¾Ð³Ð¾ ÑÐ»Ð¾Ð²Ð°, ÑÐ¾Ð¾ÑÐ½Ð¾ÑÐµÐ½Ð¸Ñ Ð·Ð²ÑÐºÐ¾Ð²ÑÑ Ð¸ Ð³ÑÐ°ÑÐ¸ÑÐµÑÐºÐ¸Ñ ÑÑÐµÐ´ÑÑÐ², Ð¾Ð¿Ð¸ÑÐ°Ð½Ð¸Ðµ ÑÐ»Ð¾Ð³Ð¾Ð²ÑÑ ÑÑÑÑÐºÑÑÑ, Ð°Ð½Ð³Ð»Ð¸Ð¹ÑÐºÐ¾Ð¹ Ð¿ÑÐ¾ÑÐ¾Ð´Ð¸Ð¸, Ð° ÑÐ°ÐºÐ¶Ðµ ÑÐ¾Ð½ÐµÑÐ¸ÑÐµÑÐºÐ¸Ñ Ð¿ÑÐ¾ÑÐµÑÑÐ¾Ð², Ð¿ÑÐ¾ÑÐµÐºÐ°ÑÑÐ¸Ñ Ð² Ð¿Ð¾ÑÐ¾ÐºÐµ Ð·Ð²ÑÑÐ°ÑÐµÐ¹ ÑÐµÑÐ¸. ÐÐ°ÑÐµÑÐ¸Ð°Ð»Ñ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ñ Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ñ Ð² Ð²Ð¸Ð´Ðµ 10 Ð»ÐµÐºÑÐ¸Ð¹, Ð²Ð¾Ð¿ÑÐ¾ÑÐ¾Ð² Ð½Ð° Ð¿Ð¾Ð²ÑÐ¾ÑÐµÐ½Ð¸Ðµ Ð¸Ð·ÑÑÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ð°, Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ¸Ñ Ð·Ð°Ð´Ð°Ð½Ð¸Ð¹ Ð¿Ð¾ ÐºÐ°Ð¶Ð´Ð¾Ð¹ ÑÐµÐ¼Ðµ, Ð¸ÑÐ¾Ð³Ð¾Ð²Ð¾Ð³Ð¾ ÑÐµÑÑÐ° Ñ ÐºÐ»ÑÑÐ°Ð¼Ð¸ Ð´Ð»Ñ ÑÐ°Ð¼Ð¾Ð¿ÑÐ¾Ð²ÐµÑÐºÐ¸ Ð¸ ÑÐ¿Ð¸ÑÐºÐ° ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´ÑÐµÐ¼Ð¾Ð¹ Ð»Ð¸ÑÐµÑÐ°ÑÑÑÑ.
description: ÐÐµÑÐ°ÑÐ°ÐµÑÑÑ Ð¿Ð¾ ÑÐµÑÐµÐ½Ð¸Ñ ÑÐµÐ´Ð°ÐºÑÐ¸Ð¾Ð½Ð½Ð¾-Ð¸Ð·Ð´Ð°ÑÐµÐ»ÑÑÐºÐ¾Ð³Ð¾ ÑÐ¾Ð²ÐµÑÐ° Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¾Ð³Ð¾ Ð³Ð¾ÑÑÐ´Ð°ÑÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑÐ°.
title: ÐÐµÑÐ¾Ð´Ñ Ð¿ÑÐ¾Ð´Ð²Ð¸Ð¶ÐµÐ½Ð¸Ñ Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»ÑÐ½Ð¾Ð³Ð¾ Ð±ÑÐµÐ½Ð´Ð° Ð² ÑÐ¾ÑÐ¸Ð°Ð»ÑÐ½ÑÑ Ð¼ÐµÐ´Ð¸Ð° (Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ ÐÐ Ð ÑÐ´Ð½Ð¸ÑÐµÐ½ÐºÐ¾ Ð. Ð.)
title: Ð¼Ð°Ð³Ð¸ÑÑÐµÑÑÐºÐ°Ñ Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ñ
titleType: Subtitle
Creators: name: Ð ÑÐ´Ð½Ð¸ÑÐµÐ½ÐºÐ¾, ÐÐºÐ°ÑÐµÑÐ¸Ð½Ð°
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2017
Subjects: Ð¼Ð°ÑÐºÐµÑÐ¸Ð½Ð³Ð¾Ð²ÑÐµ ÑÑÐµÐ´ÑÑÐ²Ð°
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description: ÐÐ±ÑÐµÐºÑÐ¾Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ²Ð»ÑÑÑÑÑ Ð¼ÐµÑÐ¾Ð´Ñ Ð¿ÑÐ¾Ð´Ð²Ð¸Ð¶ÐµÐ½Ð¸Ñ. Ð¦ÐµÐ»ÑÑ Ð²ÑÐ¿ÑÑÐºÐ½Ð¾Ð¹ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ ÑÐ²Ð»ÑÐµÑÑÑ Ð¿Ð¾Ð»ÑÑÐµÐ½Ð¸Ðµ Ð½Ð°Ð±Ð¾ÑÐ° ÑÑÑÐµÐºÑÐ¸Ð²Ð½ÑÑ Ð¼Ð°ÑÐºÐµÑÐ¸Ð½Ð³Ð¾Ð²ÑÑ ÑÑÐµÐ´ÑÑÐ² Ð´Ð»Ñ Ð¿ÑÐ¾Ð´Ð²Ð¸Ð¶ÐµÐ½Ð¸Ñ Ð»Ð¸ÑÐ½Ð¾Ð³Ð¾ Ð±ÑÐµÐ½Ð´Ð°. ÐÑÐ¾Ð´Ð²Ð¸Ð¶ÐµÐ½Ð¸Ðµ Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»ÑÐ½Ð¾Ð³Ð¾ Ð±ÑÐµÐ½Ð´Ð° - Ð¾ÑÐ½Ð¾ÑÐ¸ÑÐµÐ»ÑÐ½Ð¾ Ð½Ð¾Ð²Ð¾Ðµ Ð¿ÐµÑÑÐ¿ÐµÐºÑÐ¸Ð²Ð½Ð¾Ðµ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ Ð¡ÐÐ. ÐÐ° Ð´Ð°Ð½Ð½ÑÐ¹ Ð¼Ð¾Ð¼ÐµÐ½Ñ Ð¿Ð¾ÑÐ²Ð»ÑÐµÑÑÑ Ð¼Ð½Ð¾Ð¶ÐµÑÑÐ²Ð¾ ÑÐ¿Ð¾ÑÐ¾Ð±Ð¾Ð² Ð¼Ð¾Ð½ÐµÑÐ¸Ð·Ð¸ÑÐ¾Ð²Ð°ÑÑ Ð±Ð»Ð¾Ð³ÐµÑÑÐºÑÑ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÑ, ÑÑÐ¾ Ð¼Ð¾ÑÐ¸Ð²Ð¸ÑÑÐµÑ Ð»ÑÐ´ÐµÐ¹ ÑÐ°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÑÑ Ð±Ð»Ð¾Ð³ÑÑÐµÑÑ Ð½Ðµ ÐºÐ°Ðº ÑÐ¾Ð±Ð±Ð¸, Ð½Ð¾ ÐºÐ°Ðº Ð±Ð¸Ð·Ð½ÐµÑ. Ð ÑÑÐ¾Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ð¸ Ð°Ð²ÑÐ¾Ñ Ð¿ÑÐ¾Ð°Ð½Ð°Ð»Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð» ÑÐ¿ÐµÑÐ¸ÑÐ¸ÐºÑ Ð±Ð»Ð¾Ð³ÑÑÐµÑÑ Ð¸ Ð²ÑÐ±ÑÐ°Ð½Ð½Ð¾Ð¹ Ð¿Ð»Ð°ÑÑÐ¾ÑÐ¼Ñ ÑÐ¾ÑÐ¸Ð°Ð»ÑÐ½Ð¾Ð¹ Ð¼ÐµÐ´Ð¸Ð°, Ð¸Ð·ÑÑÐ¸Ð» ÑÑÐ½Ð¾Ðº Ð¸ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð» ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð°ÑÐ¸Ð¸ Ð¿Ð¾ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾Ð¼Ñ Ð¿ÑÐ¾Ð´Ð²Ð¸Ð¶ÐµÐ½Ð¸Ñ Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»ÑÐ½Ð¾Ð³Ð¾ Ð±ÑÐµÐ½Ð´Ð° Ð´Ð»Ñ ÑÐ¾Ð³Ð¾, ÑÑÐ¾Ð±Ñ ÑÐ²ÐµÐ»Ð¸ÑÐ¸ÑÑ Ð°ÑÐ´Ð¸ÑÐ¾ÑÐ¸Ñ Ð¸ Ð¿ÑÐ¸Ð²Ð»ÐµÑÑ Ð²Ð½Ð¸Ð¼Ð°Â­Ð½Ð¸Ðµ ÑÐµÐºÐ»Ð°Ð¼Ð¾Ð´Ð°ÑÐµÐ»ÐµÐ¹.
Oceani di altri mondi
Creators: Davide Coero Borga
Publisher: name: Media Inaf
Year: 2015

Una volta formatisi possono conservarsi anche per miliardi di anni: gli oceani su Super-Terre ed esopianeti sono una realtà. Purché l’irruenza di una vicina (troppo vicina) nana rossa non li faccia evaporare in poco tempo
The Stability and Dynamics of Planets in Tight Binary Systems
Creators: name: Saleh, Lamya
name: Rasio, Frederic
Publisher: name: arXiv
Year: 2009
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: Planets have been observed in tight binary systems with separations less than 20 AU. A likely formation scenario for such systems involves a dynamical capture, after which high relative inclinations are likely and may lead to Kozai oscillations. We numerically investigate the fate of an initially coplanar double-planet system in a class of binaries with separation ranging between $12 - 20 $ AU. Dynamical integrations of representative four-body systems are performed, each including a hot Jupiter and a second planet on a wider orbit. We find that, although such systems can remain stable at low relative inclinations ($\lesssim 40^\circ$), high relative inclinations are likely to lead to instabilities. This can be avoided if the planets are placed in a \emph{Kozai-stable zone} within which mutual gravitational perturbations can suppress the Kozai mechanism. We investigate the possibility of inducing Kozai oscillations in the inner orbit by a weak coupling mechanism between the planets in which the coplanarity is broken due to a differential nodal precession. Propagating perturbations from the stellar companion through a planetary system in this manner can have dramatic effects on the dynamical evolution of planetary systems, especially in tight binaries and can offer a reasonable explanation for eccentricity trends among planets observed in binary systems. We find that inducing such oscillations into the orbit of a hot Jupiter is more likely in tight binaries and an upper limit can be set on the binary separation above which these oscillations are not observed.
title: Facebooking for Social Support: An Experimental Test of Relational Regulation Theory
Creators: name: Knowles, Odessia
Publisher: name: Utah State University
Year: 2013

description: This study was conducted to examine social support in college student populations by way of the popular social networking website, Facebook. Relational regulation theory was used to drive the study as it posits that social support occurs when a person has conversations and/or shared activities with another individual with whom they identify as relationally meaningful. The conversation, activity, and individual are matters of personal taste; thus, this study examined whether Facebook was a good modality for this to occur. Participants were college students attending a predominately White university located in a semirural, western area of the United States. There were 122 participants across three experimental conditions. Data were collected in group format. Participants completed self-report measures, read news stories, completed puzzles as distractor tasks, and in some conditions interacted with their Facebook accounts. Results indicated that individuals receiving relational social support had a higher positive affect (M = 2.76) as compared to individuals who received no social support (M = 1.81) but were expecting it, and individuals who received nonrelational social support (M = 2.06). The difference between the no social support subgroup and the relational social support subgroup was significant, p = .012.
title: Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° ÐºÐ¾Ð¼Ð¿Ð¾Ð½ÐµÐ½ÑÐ° ÑÐ¸ÑÑÐµÐ¼Ñ Ð´Ð»Ñ ÑÐ°ÑÐ¿Ð¾Ð·Ð½Ð°Ð²Ð°Ð½Ð¸Ñ ÑÐ°ÑÑÐµÐ½Ð¸Ð¹
title: Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ°
titleType: Subtitle
Creators: name: Ð¥Ð°Ð·ÑÐ°Ñ, ÐÐ¸ÑÐ°Ð¸Ð»
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2018
Subjects: ÑÐ°ÑÐ¿Ð¾Ð·Ð½Ð°Ð²Ð°Ð½Ð¸Ðµ Ð¸Ð·Ð¾Ð±ÑÐ°Ð¶ÐµÐ½Ð¸Ð¹
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description: ÐÐ±ÑÐµÐºÑÐ¾Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ²Ð»ÑÑÑÑÑ Ð¼ÐµÑÐ¾Ð´Ñ ÑÐ°ÑÐ¿Ð¾Ð·Ð½Ð°Ð²Ð°Ð½Ð¸Ñ Ð¸Ð·Ð¾Ð±ÑÐ°Ð¶ÐµÐ½Ð¸Ð¹.
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Raorchestes cangyuanensis
Creators: name: Köhler, Gunther
name: Dost, Ole
name: Than, Ni Lar
name: Ohler, Annemarie
name: Charunrochana, Panupong Thammachoti
name: Chuaynkern, Yodchaiy
name: Chuaynkern, Chantip
name: Geiss, Katharina
Publisher: name: Zenodo
Year: 2025
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Amphibia
Anura
Rhacophoridae
Raorchestes
Raorchestes cangyuanensis

description: Raorchestes cangyuanensis
— Myanmar: Bago: Padaung Township, Nyaung Gyo village: CAS 239662; near airport: SMF 103268; Chin: Hakha Township, Hakha: CAS 233147–48, 233170–71; Falam Township, rd between Falam and Lei Zoe village: CAS 233268–69; Rakhine: Gwa Township, Gwa, Rakhine Yoma Elephant Wildlife Sanctuary: CAS 221942; Sagaing: Alaungdaw Kathapa National Park: CAS 221858–59; Hkamti Township, Htamanthi Wildlife Sanctuary, upper Nat E-Su stream: CAS 232280; Alaungdaw Kathapa National Park, Thaipeitsae (Log Cabin Camp): CAS 221679–81; Alaungdaw Kathapa National Park, tributary to Paya Chaung Creek: CAS 221857.
description: Published as part of Köhler, Gunther, Dost, Ole, Than, Ni Lar, Ohler, Annemarie, Charunrochana, Panupong Thammachoti, Chuaynkern, Yodchaiy, Chuaynkern, Chantip & Geiss, Katharina, 2025, A taxonomic revision of the genus Raorchestes in Myanmar and Thailand with the description of two new species from Myanmar (Amphibia, Anura, Rhacophoridae), pp. 47-81 in Zootaxa 5613 (1) on page 78, DOI: 10.11646/zootaxa.5613.1.2, http://zenodo.org/record/15216232
title: Ð¡Ð¸ÑÑÐµÐ¼Ñ Ð¸ÑÐºÑÑÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¸Ð½ÑÐµÐ»Ð»ÐµÐºÑÐ°. Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð±Ð°Ð· Ð·Ð½Ð°Ð½Ð¸Ð¹ Ð² Ð¸Ð½ÑÑÑÑÐ¼ÐµÐ½ÑÐ°Ð»ÑÐ½Ð¾Ð¹ ÑÑÐµÐ´Ðµ KAPPA
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ
titleType: Subtitle
Creators: name: ÐÐ°Ð²ÑÐ¸Ð»Ð¾Ð²Ð°, Ð¢Ð°ÑÑÑÐ½Ð°
Publisher: name: ÐÐ·Ð´-Ð²Ð¾ Ð¡ÐÐ±ÐÐÐ£
Year: 2004
Subjects: Ð­ÐºÑÐ¿ÐµÑÑÐ½ÑÐµ Ð¾ÑÐµÐ½ÐºÐ¸
ÐÑÐºÑÑÑÑÐ²ÐµÐ½Ð½ÑÐ¹ Ð¸Ð½ÑÐµÐ»Ð»ÐµÐºÑ

description: ÐÐ¾ÑÐ¾Ð±Ð¸Ðµ ÑÐ¾Ð¾ÑÐ²ÐµÑÑÑÐ²ÑÐµÑ Ð³Ð¾ÑÑÐ´Ð°ÑÑÑÐ²ÐµÐ½Ð½Ð¾Ð¼Ñ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°ÑÐµÐ»ÑÐ½Ð¾Ð¼Ñ ÑÑÐ°Ð½Ð´Ð°ÑÑÑ Ð´Ð¸ÑÑÐ¸Ð¿Ð»Ð¸Ð½Ñ Â«ÐÐ°Ð·Ñ Ð´Ð°Ð½Ð½ÑÑ Ð¸ Ð·Ð½Ð°Ð½Ð¸Ð¹Â». ÐÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ð¾ Ð¾Ð¿Ð¸ÑÐ°Ð½Ð¸Ðµ Ð¸Ð½ÑÐµÑÑÐµÐ¹ÑÐ° Ð¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°ÑÐµÐ»Ñ ÑÐ¸ÑÑÐµÐ¼Ñ ÐÐÐ Ð Ð (ÑÐ°ÑÑÑ 1); Ð¾Ð¿Ð¸ÑÐ°Ð½ ÑÐ¸Ð½ÑÐ°ÐºÑÐ¸Ñ Ð¸ ÑÐµÐ¼Ð°Ð½ÑÐ¸ÐºÐ° Ð²ÑÑÑÐ¾ÐµÐ½Ð½Ð¾Ð³Ð¾ ÑÐ·ÑÐºÐ° Ð´Ð»Ñ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ¸ Ð¿ÑÐ¸Ð»Ð¾Ð¶ÐµÐ½Ð¸Ð¹ KAL, Ð° ÑÐ°ÐºÐ¶Ðµ Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½ ÐºÑÐ°ÑÐºÐ¸Ð¹ ÑÐ¿ÑÐ°Ð²Ð¾ÑÐ½Ð¸Ðº Ð¿Ð¾ Ð²ÑÑÑÐ¾ÐµÐ½Ð½ÑÐ¼ ÑÑÐ½ÐºÑÐ¸ÑÐ¼ Ð¸ Ð¾Ð¿ÐµÑÐ°ÑÐ¸ÑÐ¼ ÑÐ·ÑÐºÐ° (ÑÐ°ÑÑÑ 2); Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ñ ÑÐ°Ð³Ð¸, Ð½ÐµÐ¾Ð±ÑÐ¾Ð´Ð¸Ð¼ÑÐµ Ð´Ð»Ñ ÑÐ¾Ð·Ð´Ð°Ð½Ð¸Ñ ÑÐºÑÐ¿ÐµÑÑÐ½Ð¾Ð¹ ÑÐ¸ÑÑÐµÐ¼Ñ Ñ Ð¿Ð¾Ð´ÑÐ¾Ð±Ð½ÑÐ¼Ð¸ Ð¿Ð¾ÑÑÐ½ÐµÐ½Ð¸ÑÐ¼Ð¸ (ÑÐ°ÑÑÑ 3); Ð¿ÑÐµÐ´Ð¾ÑÑÐ°Ð²Ð»ÐµÐ½ Ð¿ÑÐ¸Ð¼ÐµÑ Ð¿Ð¾ÑÑÑÐ¾ÐµÐ½Ð¸Ñ ÑÐºÑÐ¿ÐµÑÑÐ½Ð¾Ð¹ ÑÐ¸ÑÑÐµÐ¼Ñ (ÑÐ°ÑÑÑ 4). ÐÐ¾ÑÐ¾Ð±Ð¸Ðµ Ð¿ÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¾ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð², Ð¾Ð±ÑÑÐ°ÑÑÐ¸ÑÑÑ Ð¿Ð¾ ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾ÑÑÐ¸ Â«ÐÐ²ÑÐ¾Ð¼Ð°ÑÐ¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ð½ÑÐµ ÑÐ¸ÑÑÐµÐ¼Ñ Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸ÑÂ», Ð° ÑÐ°ÐºÐ¶Ðµ Ð¼Ð¾Ð¶ÐµÑ Ð±ÑÑÑ Ð¿Ð¾Ð»ÐµÐ·Ð½Ð¾ ÑÑÑÐ´ÐµÐ½ÑÐ°Ð¼ Ð¸ Ð°ÑÐ¿Ð¸ÑÐ°Ð½ÑÐ°Ð¼ Ð´ÑÑÐ³Ð¸Ñ ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾ÑÑÐµÐ¹, Ð·Ð°Ð½Ð¸Ð¼Ð°ÑÑÐ¸ÑÑÑ Ð¸Ð·ÑÑÐµÐ½Ð¸ÐµÐ¼, Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸ÐµÐ¼ Ð¸Ð»Ð¸ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ¾Ð¹ Ð¿Ð¾Ð´ÑÐ¾Ð´Ð¾Ð², Ð¸ÑÐ¿Ð¾Ð»ÑÐ·ÑÑÑÐ¸ÑÑÑ Ð¿ÑÐ¸ Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ð¸ ÑÐºÑÐ¿ÐµÑÑÐ½ÑÑ ÑÐ¸ÑÑÐµÐ¼.
description: ÐÐµÑÐ°ÑÐ°ÐµÑÑÑ Ð¿Ð¾ ÑÐµÑÐµÐ½Ð¸Ñ ÑÐµÐ´Ð°ÐºÑÐ¸Ð¾Ð½Ð½Ð¾-Ð¸Ð·Ð´Ð°ÑÐµÐ»ÑÑÐºÐ¾Ð³Ð¾ ÑÐ¾Ð²ÐµÑÐ° Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¾Ð³Ð¾ Ð³Ð¾ÑÑÐ´Ð°ÑÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑÐ°.
Erste Verurteilung von Frauenordinationsgegnern in Finnland durch ein weltliches Gericht
Creators: name: Wenz, Armin
Publisher: name: Lutherische Beiträge
Year: 1970

description: Lutherische Beiträge, Bd. 13 Nr. 2 (2008): Lutherische Beiträge, Band 13, Heft 2
Seattle, al via il «Super Bowl» dell’astronomia
Creators: Marco Malaspina
Publisher: name: Media Inaf
Year: 2015

Quasi duemila presentazioni scientifiche in quattro giorni – fra talk, poster e conferenze plenarie – nel programma del 225esimo meeting dell’American Astronomical Society. Da oggi a venerdì 8 gennaio, una ricca rassegna di novità in ambito astrofisico, cosmologico e tecnologico che Media INAF seguirà sul posto
Upper tails for counting objects in randomly induced subhypergraphs and rooted random graphs
Creators: name: Janson, Svante
name: Rucinski, Andrzej
Publisher: name: arXiv
Year: 2009
Subjects: subject: Probability (math.PR)
subject: Combinatorics (math.CO)
subject: FOS: Mathematics
subject: 60C05; 05C80, 05C65

description: General upper tail estimates are given for counting edges in a random induced subhypergraph of a fixed hypergraph H, with an easy proof by estimating the moments. As an application we consider the numbers of arithmetic progressions and Schur triples in random subsets of integers. In the second part of the paper we return to the subgraph counts in random graphs and provide upper tail estimates in the rooted case.
description: 15 pages
Theory of resonant photon drag in monolayer graphene
Creators: name: Entin, M. V.
name: Magarill, L. I.
name: Shepelyansky, D. L.
Publisher: name: arXiv
Year: 2010
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: Photon drag current in monolayer graphene with degenerate electron gas is studied under interband excitation near the threshold of fundamental transitions. Two main mechanisms generate an emergence of electron current. Non-resonant drag effect (NDE) results from direct transfer of in-plane photon momentum ${\bf q}$ to electron and dependence of matrix elements of transitions on ${\bf q}$. Resonant drag effect (RDE) originates from ${\bf q}$-dependent selection of transitions due to a sharp form of the Fermi distribution in energy. The drag current essentially depends on the polarization of radiation and, in general, is not parallel to ${\bf q}$. The perpendicular current component appears if the in-plain electric field is tilted towards ${\bf q}$. The RDE has no smallness connected with $q$ and exists in a narrow region of photon frequency $ω$: $|\hbarω-2ε_F|< \hbar sq$, where $s$ is the electron velocity.
description: 5 pages, 4 figures
title: Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° ÑÐ¸ÑÑÐµÐ¼Ñ ÑÐ¸Ð»ÑÑÑÐ°ÑÐ¸Ð¸ ÑÐ¾ÑÐ¾-ÐºÐ¾Ð½ÑÐµÐ½ÑÐ° Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ðµ Ð½ÐµÐ¹ÑÐ¾Ð½Ð½ÑÑ ÑÐµÑÐµÐ¹
title: Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð¼Ð°Ð³Ð¸ÑÑÑÐ°
titleType: Subtitle
Creators: name: ÐÐµÐ¼ÐµÐ½ÑÑÐµÐ², ÐÐ»ÐµÐºÑÐµÐ¹
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2018
Subjects: ÐÐ½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¾Ð½Ð½ÑÐµ ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸Ð¸
ÐÑÐºÑÑÑÑÐ²ÐµÐ½Ð½ÑÐ¹ Ð¸Ð½ÑÐµÐ»Ð»ÐµÐºÑ
ÐÐµÐ¹ÑÐ¾Ð½Ð½ÑÐµ ÑÐµÑÐ¸
Ð Ð°ÑÐ¿Ð¾Ð·Ð½Ð°Ð²Ð°Ð½Ð¸Ðµ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²
Ð¼Ð°ÑÐ¸Ð½Ð½Ð¾Ðµ Ð¾Ð±ÑÑÐµÐ½Ð¸Ðµ
Ð¸ÑÐºÑÑÑÑÐ²ÐµÐ½Ð½ÑÐµ Ð½ÐµÐ¹ÑÐ¾Ð½Ð½ÑÐµ ÑÐµÑÐ¸
ÐºÐ»Ð°ÑÑÐ¸ÑÐ¸ÐºÐ°ÑÐ¸Ñ Ð¸Ð·Ð¾Ð±ÑÐ°Ð¶ÐµÐ½Ð¸Ð¹

description: Ð Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ Ð¸Ð·Ð»Ð¾Ð¶ÐµÐ½ Ð¿Ð¾Ð´ÑÐ¾Ð´ Ð¸ Ð°Ð»Ð³Ð¾ÑÐ¸ÑÐ¼ Ðº Ð¿Ð¾ÑÑÑÐ¾ÐµÐ½Ð¸Ñ ÐºÐ»Ð°ÑÑÐ¸ÑÐ¸ÐºÐ°ÑÐ¾ÑÐ° Ð¸Ð·Ð¾Ð±ÑÐ°Ð¶ÐµÐ½Ð¸Ð¹ Ñ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸ÐµÐ¼ Ð¸ÑÐºÑÑÑÑÐ²ÐµÐ½Ð½ÑÑ Ð½ÐµÐ¹ÑÐ¾Ð½Ð½ÑÑ ÑÐµÑÐµÐ¹.
ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÑÑÐµÑÑÐ²ÑÑÑÐ¸Ñ Ð°Ð½Ð°Ð»Ð¾Ð³Ð¾Ð². ÐÐ·ÑÑÐµÐ½Ð° ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ñ Ð¾Ð±ÑÑÐµÐ½Ð¸Ñ Ð¸ÑÐºÑÑÑÑÐ²ÐµÐ½Ð½Ð¾Ð¹ Ð½ÐµÐ¹ÑÐ¾Ð½Ð½Ð¾Ð¹ ÑÐµÑÐ¸. Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ð° ÑÐ¸ÑÑÐµÐ¼Ð°, Ð¿Ð¾Ð·Ð²Ð¾Ð»ÑÑÑÐ°Ñ ÐºÐ»Ð°ÑÑÐ¸ÑÐ¸ÑÐ¸ÑÐ¾Ð²Ð°ÑÑ Ð¸Ð·Ð¾Ð±ÑÐ°Ð¶ÐµÐ½Ð¸Ñ Ð¿Ð¾ Ð·Ð°ÑÐ°Ð½ÐµÐµ Ð·Ð°Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð½Ð¾Ð¼Ñ ÐºÐ»Ð°ÑÑÑ.
Two-loop electroweak fermionic corrections to sin^2 theta_{eff}^{b anti-b}
Creators: name: Awramik, M.
name: Czakon, M.
name: Freitas, A.
name: Kniehl, B. A.
Publisher: name: arXiv
Year: 2008
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We present the first calculation of the two-loop electroweak fermionic correction to the flavour-dependent effective weak-mixing angle for bottom quarks, sin^2 theta_{eff}^{b anti-b}. For the evaluation of the missing two-loop vertex diagrams, two methods are employed, one based on a semi-numerical Bernstein-Tkachov algorithm and the second on asymptotic expansions in the large top-quark mass. A third method based on dispersion relations is used for checking the basic loop integrals. We find that for small Higgs-boson mass values, M_H ~ 100 GeV, the correction is sizable, of order O(10^{-4}).
description: 17 pages, 2 figures, references added, accepted for publication in Nucl. Phys. B
title: Mule Deer and Wildlife Crossings in Utah, USA
Creators: name: Schwender, Megan
Publisher: name: Utah State University
Year: 2013

description: Wildlife-vehicle collisions (WVCs) negatively impact wildlife populations and create dangerous driving situations for motorists. In Utah, USA, mule deer (Odocoileus hemionus) encounter a variety of hazards as they attempt to cross highways and interstates, some of which are 8 lanes wide. Agencies have sought to mitigate the risks posed to drivers and mule deer by building crossing structures for wildlife. The objectives of this study were to evaluate the effectiveness of crossing structures in Utah to safely pass mule deer under highways and to determine the variables that best explain mule deer passage use. From 2008 - 2011 we used 26 camera traps to measure levels of mule deer use of 9 culverts and 4 bridges in Utah. We tested for relationships between mule deer structure use and a variety of structural and landscape attributes at each site, including 2 time variables: time since the structure was built and time each structure was monitored by our camera traps. We also developed and tested a new equation (window ratio) that measured culvert openness to approaching mule deer. In the single variable regression models, mule deer structure use was positively correlated with short culverts and coarse scale shrub cover, and negatively correlated with fine scale grass cover. In the multivariate model, structure use was positively correlated with days monitored and elevation and short culverts. Although the new window ratio did not emerge as the most important predictor for mule deer crossing use, it was more effective at predicting mule deer culvert use than the often referenced openness factor. Our results indicated that 12 of the 13 crossing structures studied effectively facilitate the movement of mule deer in Utah; however some were used far more than others. We suggest that older crossing structures built with the shortest dimensions possible, with attached wildlife-exclusion fencing, and in shrubby habitat will be most effective at passing a high volume of mule deer under Utah highways.
title: Ð¢ÑÑÐ±Ð¾Ð²Ð°Ð»ÑÐ½ÑÐ¹ Ð´Ð²Ð¸Ð³Ð°ÑÐµÐ»Ñ Ð¼Ð¾ÑÐ½Ð¾ÑÑÑÑ 1500 ÐºÐÑ.
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: Ð¡Ð°ÑÐ¾Ð½Ð¾Ð², ÐÐ»ÐµÐºÑÐ°Ð½Ð´Ñ
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2016
Subjects: ÑÑÑÐ±Ð¾Ð²Ð°Ð»ÑÐ½ÑÐ¹ Ð´Ð²Ð¸Ð³Ð°ÑÐµÐ»Ñ
Ð°Ð²Ð¸Ð°ÑÐ¸Ð¾Ð½Ð½ÑÐ¹ Ð´Ð²Ð¸Ð³Ð°ÑÐµÐ»Ñ
Ð¾ÑÐµÐ²Ð¾Ð¹ ÐºÐ¾Ð¼Ð¿ÑÐµÑÑÐ¾Ñ
Ð¿ÑÑÐ¼Ð¾ÑÐ¾ÑÐ½Ð°Ñ ÐºÐ°Ð¼ÐµÑÐ° ÑÐ³Ð¾ÑÐ°Ð½Ð¸Ñ

description: Ð¦ÐµÐ»ÑÑ Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ ÑÐ²Ð»ÑÐµÑÑÑ ÑÐ¾Ð·Ð´Ð°Ð½Ð¸Ðµ ÑÑÑÐ±Ð¾Ð²Ð°Ð»ÑÐ½Ð¾Ð³Ð¾ Ð´Ð²Ð¸Ð³Ð°ÑÐµÐ»Ñ Ð¼Ð¾ÑÐ½Ð¾ÑÑÑ 1500 ÐºÐÑ. Ð ÑÐ¾Ð¾ÑÐ²ÐµÑÑÑÐ²Ð¸Ðµ Ñ ÑÐºÐ°Ð·Ð°Ð½Ð½Ð¾Ð¹ ÑÐµÐ»ÑÑ Ð² ÑÐ°Ð±Ð¾ÑÐµ Ð¿Ð¾ÑÑÐ°Ð²Ð»ÐµÐ½Ñ Ð¸ ÑÐµÑÐµÐ½Ñ ÑÐ»ÐµÐ´ÑÑÑÐ¸Ðµ Ð·Ð°Ð´Ð°ÑÐ¸: ÑÐ¾ÑÑÐ°Ð²Ð»ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸ÑÐ¸ÑÐµÑÐºÐ¸Ð¹ Ð¾Ð±Ð·Ð¾Ñ ÑÑÑÐ±Ð¾Ð²Ð°Ð»ÑÐ½ÑÑ Ð´Ð²Ð¸Ð³Ð°ÑÐµÐ»ÐµÐ¹; Ð¿ÑÐ¾Ð¸Ð·Ð²ÐµÐ´ÐµÐ½ ÑÐ°ÑÑÐµÑ ÑÐ·Ð»Ð¾Ð² Ð´Ð²Ð¸Ð³Ð°ÑÐµÐ»Ñ Ñ ÑÐµÐ»ÑÑ Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ñ Ð¼Ð¾ÑÐ½Ð¾ÑÑÐ¸; Ñ Ð¿Ð¾Ð¼Ð¾ÑÑÑ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ñ OPTI Ð±ÑÐ»Ð¸ Ð¾Ð¿ÑÐ¸Ð¼Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ñ ÑÑÑÐ±Ð¸Ð½Ñ (ÑÐ²Ð¾Ð±Ð¾Ð´Ð½Ð°Ñ ÑÑÑÐ±Ð¸Ð½Ñ Ð¸ ÑÑÑÐ±Ð¸Ð½Ð° ÐºÐ¾Ð¼Ð¿ÑÐµÑÑÐ¾ÑÐ°); Ð±ÑÐ»Ð° Ð¿ÑÐ¾Ð¸Ð·Ð²ÐµÐ´ÐµÐ½Ð° ÑÐ°Ð±Ð¾ÑÐ° Ð¿Ð¾ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¸ ÑÐµÐ¼Ð¾Ð½ÑÐ° ÑÐ°Ð±Ð¾ÑÐ¸Ñ Ð»Ð¾Ð¿Ð°ÑÐ¾Ðº ÑÑÑÐ¿ÐµÐ½ÐµÐ¹ ÑÐ¾ÑÐ¾ÑÐ° ÐºÐ¾Ð¼Ð¿ÑÐµÑÑÐ¾ÑÐ°; Ð¿ÑÐ¾Ð¸Ð·Ð²ÐµÐ´ÐµÐ½ ÑÐ°ÑÑÐµÑ Ð´Ð¸ÑÐºÐ° Ð¿Ð¾ÑÐ»ÐµÐ´Ð½ÐµÐ¹ ÑÑÑÐ¿ÐµÐ½Ð¸ ÑÐ²Ð¾Ð±Ð¾Ð´Ð½Ð¾Ð¹ ÑÑÑÐ±Ð¸Ð½Ñ Ð½Ð° Ð¿ÑÐ¾ÑÐ½Ð¾ÑÑÑ. ÐÐ¾Ð»ÑÑÐµÐ½Ð½ÑÐµ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÑ Ð¿Ð¾Ð·Ð²Ð¾Ð»Ð¸Ð»Ð¸ Ð¿Ð¾Ð²ÑÑÐ¸ÑÑ Ð¼Ð¾ÑÐ½Ð¾ÑÑÑ ÑÑÑÐ±Ð¾Ð²Ð°Ð»ÑÐ½Ð¾Ð³Ð¾ Ð´Ð²Ð¸Ð³Ð°ÑÐµÐ»Ñ.
Magnetic ordering in EuRh2As2 studied by x-ray resonant magnetic scattering
Creators: name: Nandi, S.
name: Kreyssig, A.
name: Lee, Y.
name: Singh, Yogesh
name: Kim, J. W.
name: Johnston, D. C.
name: Harmon, B. N.
name: Goldman, A. I.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: Superconductivity (cond-mat.supr-con)
subject: FOS: Physical sciences

description: Element-specific x-ray resonant magnetic scattering investigations were performed to determine the magnetic structure of Eu in EuRh2As2. In the temperature range from 46 K down to 6 K, an incommensurate antiferromagnetic (ICM)structure with a temperature dependent propagation vector (0 0 0.9) coexists with a commensurate antiferromagnetic (CM) structure. Angular-dependent measurements of the magnetic intensity indicate that the magnetic moments lie in the tetragonal basal plane and are ferromagnetically aligned within the a-b plane for both magnetic structures. The ICM structure is a spiral-like magnetic structure with a turn angle of 162 deg between adjacent Eu planes. In the CM structure, this angle is 180 deg. These results are consistent with band-structure calculations which indicate a strong sensitivity of the magnetic configuration on the Eu valence.
description: 5 pages, 5 figures (technical problem with abstract corrected, no other changes)
Cosmic Evolution of Star Formation In SDSS Quasar Hosts Since z=1
Creators: name: Shi, Yong
name: Rieke, George H.
name: Ogle, Patrick
name: Jiang, Linhua
name: Diamond-Stanic, Aleksandar M.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We present Spitzer IRS observations of a complete sample of 57 SDSS type-1 quasars at z~1. Aromatic features at 6.2 and/or 7.7 um are detected in about half of the sample and show profiles similar to those seen in normal galaxies at both low- and high-redshift, indicating a star-formation origin for the features. Based on the ratio of aromatic to star-formation IR (SFIR) luminosities for normal star-forming galaxies at z~1, we have constructed the SFIR luminosity function (LF) of z~1 quasars. As we found earlier for low-redshift PG quasars, these z~1 quasars show a flatter SFIR LF than do z~1 field galaxies, implying the quasar host galaxy population has on average a higher SFR than the field galaxies do. As measured from their SFIR LF, individual quasar hosts have on average LIRG-level SFRs, which mainly arise in the circumnuclear regions. By comparing with similar measurements of low-redshift PG quasars, we find that the comoving SFIR luminosity density in quasar hosts shows a much larger increase with redshift than that in field galaxies. The behavior is consistent with pure density evolution since the average SFR and the average SFR/BH-accretion-rate in quasar hosts show little evolution with redshift. For individual quasars, we have found a correlation between the aromatic-based SFR and the luminosity of the nuclear radiation, consistent with predictions of some theoretical models. We propose that type 1 quasars reside in a distinct galaxy population that shows elliptical morphology but that harbors a significant fraction of intermediate-age stars and is experiencing intense circumnuclear star formation.
description: Accepted for publication in ApJ, 20 pages, 11 figures
title: Ð¡ÑÐ°Ð²Ð½Ð¸ÑÐµÐ»ÑÐ½ÑÐ¹ Ð°Ð½Ð°Ð»Ð¸Ð· Ð´Ð»Ð¸Ð½ ÑÐµÐ»Ð¾Ð¼ÐµÑ Ñ Ð»Ð¸Ñ, ÑÑÐ°ÑÑÐ²ÑÑÑÐ¸Ñ Ð² ÑÐ½Ð¸ÑÑÐ¾Ð¶ÐµÐ½Ð¸Ð¸ Ð²ÑÐµÐ´Ð½ÑÑ Ð²ÐµÑÐµÑÑÐ², ÑÐ°Ð·Ð»Ð¸ÑÐ°ÑÑÐ¸Ñ ÑÑ Ð¿Ð¾Ð» Ð°Ð»Ð»ÐµÐ»ÑÐ¼ Ð³ÐµÐ½Ð¾Ð² ÑÑÐ°Ð½ÑÐ¿Ð¾ÑÑÐµÑÐ° ÑÐµÑÐ¾ÑÐ¾Ð½Ð¸Ð½Ð° 5-htt
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ¾ÑÑÑÐº, ÐÐ¼Ð¸ÑÑÐ¸Ð¹
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2017
Subjects: ÐÐµÐ¹ÑÐ¾Ð½Ñ
ÑÐµÑÐ¾ÑÐ¾Ð½Ð¸Ð½Ð¾Ð²ÑÐµ ÑÐµÑÐµÐ¿ÑÐ¾ÑÑ
ÑÐµÐ»Ð¾Ð¼ÐµÑÑ
Ð¿Ð¾Ð»Ð¸Ð¼Ð¾ÑÑÐ½ÑÐ¹ ÑÑÐ°ÑÑÐ¾Ðº

description: Ð¡ÐµÑÐ¾ÑÐ¾Ð½Ð¸Ð½Ð¾Ð²ÑÐ¹ ÑÑÐ°Ð½ÑÐ¿Ð¾ÑÑÐµÑ (5HTT) ÑÐ²Ð»ÑÐµÑÑÑ ÑÑÐ°Ð½ÑÐ¼ÐµÐ¼Ð±ÑÐ°Ð½Ð½ÑÐ¼ Ð±ÐµÐ»ÐºÐ¾Ð¼, Ð¾ÑÐ²ÐµÑÐ°ÑÑÐ¸Ð¼ Ð·Ð° Ð¾Ð±ÑÐ°ÑÐ½ÑÐ¹ ÑÑÐ°Ð½ÑÐ¿Ð¾ÑÑ ÑÐµÑÐ¾ÑÐ¾Ð½Ð¸Ð½Ð° Ð¸Ð· ÑÐ¸Ð½Ð¾Ð¿ÑÐ¸ÑÐµÑÐºÐ¾Ð¹ ÑÐµÐ»Ð¸ Ð² Ð¿ÑÐµÑÐ¸Ð½Ð°Ð¿ÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð½ÐµÐ¹ÑÐ¾Ð½Ñ. ÐÐ°Ð½Ð½ÑÐ¹ Ð±ÐµÐ»Ð¾Ðº ÑÐºÑÐ¿ÑÐµÑÑÐ¸ÑÑÐµÑÑÑ Ð² Ð¼Ð¾Ð·Ð³Ðµ Ð¸ ÑÑÐ¾Ð¼Ð±Ð¾ÑÐ¸ÑÐ°Ñ. Ð Ð¿ÑÐ¾Ð¼Ð¾ÑÐ¾ÑÐ½Ð¾Ð¹ Ð¾Ð±Ð»Ð°ÑÑÐ¸ Ð³ÐµÐ½Ð° 5HTT Ð½Ð°Ð¹Ð´ÐµÐ½ ÑÑÐ½ÐºÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½Ð¾ Ð·Ð½Ð°ÑÐ¸Ð¼ÑÐ¹ Ð¿Ð¾Ð»Ð¸Ð¼Ð¾ÑÑÐ½ÑÐ¹ ÑÑÐ°ÑÑÐ¾Ðº HTTLPR ÑÐ¸Ð¿Ð° Ð²ÑÑÐ°Ð²ÐºÐ°/Ð´ÐµÐ»ÐµÑÐ¸Ñ, ÑÐ°ÑÐ°ÐºÑÐµÑÐ¸Ð·ÑÑÑÐ¸Ð¹ÑÑ Ð½Ð°Ð»Ð¸ÑÐ¸ÐµÐ¼ Ð¸Ð»Ð¸ Ð¾ÑÑÑÑÑÑÐ²Ð¸ÐµÐ¼ ÑÑÐ°Ð³Ð¼ÐµÐ½ÑÐ° ÐÐÐ Ð´Ð»Ð¸Ð½Ð¾Ð¹ 44 Ð¿.Ð½. Ð ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐµ Ð¿Ð¾Ð»ÑÑÐ°ÑÑÑÑ Ð´Ð²Ð° Ð°Ð»Ð»ÐµÐ»Ñ - Ð´Ð»Ð¸Ð½Ð½ÑÐ¹ (L) c Ð½Ð°Ð»Ð¸ÑÐ¸ÐµÐ¼ Ð¸ ÐºÐ¾ÑÐ¾ÑÐºÐ¸Ð¹ (S) c Ð¾ÑÑÑÑÑÑÐ²Ð¸ÐµÐ¼ Ð²ÑÑÐ°Ð²ÐºÐ¸.Ð ÑÐ¾Ð´Ðµ ÑÐ°Ð±Ð¾ÑÑ, Ð¼Ñ ÑÑÐ°Ð²Ð½Ð¸Ð»Ð¸ ÑÐ°ÑÐ¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð¸Ðµ Ð³ÐµÐ½Ð¾ÑÐ¸Ð¿Ð¾Ð² ÑÑÐµÐ´Ð¸ Ð¼ÑÐ¶ÑÐ¸Ð½ Ð¸ Ð¶ÐµÐ½ÑÐ¸Ð½ Ð¸ Ð¾Ð±Ð½Ð°ÑÑÐ¶Ð¸Ð»Ð¸ Ð·Ð½Ð°ÑÐ¸Ð¼ÑÐµ ÑÐ°Ð·Ð»Ð¸ÑÐ¸Ñ: Ð³ÐµÐ½Ð¾ÑÐ¸Ð¿ Ð2Ð2 ÑÐ°ÑÐµ Ð²ÑÑÑÐµÑÐ°ÐµÑÑÑ Ñ Ð¼ÑÐ¶ÑÐ¸Ð½, Ð° ÑÑÐµÐ´Ð¸ Ð¶ÐµÐ½ÑÐ¸Ð½ Ð¿ÑÐµÐ¾Ð±Ð»Ð°Ð´Ð°ÑÑ Ð³ÐµÑÐµÑÐ¾Ð·Ð¸Ð³Ð¾ÑÑ Ð1Ð2.Ð¢Ð°Ðº Ð¶Ðµ, Ð½Ð°Ð±Ð»ÑÐ´Ð°Ñ Ð·Ð° Ð´Ð»Ð¸Ð½Ð°Ð¼Ð¸ ÑÐµÐ»Ð¾Ð¼ÐµÑ, Ð¼Ñ Ð¾Ð±Ð½Ð°ÑÑÐ¶Ð¸Ð»Ð¸, ÑÑÐ¾ Ñ Ð¼ÑÐ¶ÑÐ¸Ð½ Ñ Ð³ÐµÐ½Ð¾ÑÐ¸Ð¿Ð¾Ð¼ Ð1Ð1 ÑÐµÐ»Ð¾Ð¼ÐµÑÑ ÐºÐ¾ÑÐ¾ÑÐµ, ÑÐµÐ¼ Ñ Ð¼ÑÐ¶ÑÐ¸Ð½ Ñ Ð´Ð²ÑÐ¼Ñ Ð´ÑÑÐ³Ð¸Ð¼Ð¸ Ð³ÐµÐ½Ð¾ÑÐ¸Ð¿Ð°Ð¼Ð¸, Ð¾Ð´Ð½Ð°ÐºÐ¾ ÑÑÐ¸ ÑÐ°Ð·Ð»Ð¸ÑÐ¸Ñ Ð±ÑÐ»Ð¸ Ð½Ðµ Ð´Ð¾ÑÑÐ¾Ð²ÐµÑÐ½Ñ.ÐÑÐ¸ Ð°Ð½Ð°Ð»Ð¸Ð·Ðµ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐ¾Ð², Ð¿Ð¾ÑÑÑÐ¾Ð¸Ð»Ð¸ Ð¼Ð¾Ð´ÐµÐ»Ñ Ð¼Ð½Ð¾Ð¶ÐµÑÑÐ²ÐµÐ½Ð½Ð¾Ðµ ÑÐµÐ³ÑÐµÑÑÐ¸Ð¸, ÐºÐ¾ÑÐ¾ÑÐ°Ñ ÑÑÐ¸ÑÑÐ²Ð°Ð»Ð° Ð½Ðµ ÑÐ¾Ð»ÑÐºÐ¾ Ð³ÐµÐ½Ð¾ÑÐ¸Ð¿ Ð¸ Ð¿Ð¾Ð», Ð° ÑÐ°ÐºÐ¶Ðµ Ð²Ð¾Ð·ÑÐ°ÑÑ Ð¸ Ð²Ð·Ð°Ð¸Ð¼Ð¾Ð´ÐµÐ¹ÑÑÐ²Ð¸Ðµ Ð³ÐµÐ½Ð¾ÑÐ¸Ð¿Ð° Ñ Ð²Ð¾Ð·ÑÐ°ÑÑÐ¾Ð¼, Ð¼Ñ ÑÐ²Ð¸Ð´ÐµÐ»Ð¸ Ð·Ð°Ð²Ð¸ÑÐ¸Ð¼Ð¾ÑÑÑ Ð´Ð»Ð¸Ð½Ñ ÑÐµÐ»Ð¾Ð¼ÐµÑ Ð¾Ñ Ð³ÐµÐ½Ð¾ÑÐ¸Ð¿Ð° Ð2Ð2 Ñ Ð¼ÑÐ¶ÑÐ¸Ð½ Ð¿Ð¾ Ð¼ÐµÑÐµ ÑÐ²ÐµÐ»Ð¸ÑÐµÐ½Ð¸Ñ Ð²Ð¾Ð·ÑÐ°ÑÑÐ°. Ð¢Ð¾ ÐµÑÑÑ ÑÐ¾Ð³Ð»Ð°ÑÐ½Ð¾ ÑÑÐ¾Ð¹ Ð¼Ð¾Ð´ÐµÐ»Ð¸ Ð´Ð»Ð¸Ð½Ð° ÑÐµÐ»Ð¾Ð¼ÐµÑ Ñ Ð¼ÑÐ¶ÑÐ¸Ð½ Ñ Ð³ÐµÐ½Ð¾ÑÐ¸Ð¿Ð¾Ð¼ Ð2Ð2 Ð´Ð¾ÑÑÐ¾Ð²ÐµÑÐ½Ð¾ Ð±Ð¾Ð»ÑÑÐµ.
Position-dependent exact-exchange energy for slabs and semi-infinite jellium
Creators: name: Horowitz, C. M.
name: Constantin, L. A.
name: Proetto, C. R.
name: Pitarke, J. M.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Other Condensed Matter (cond-mat.other)
subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: The position-dependent exact-exchange energy per particle $\varepsilon_x(z)$ (defined as the interaction between a given electron at $z$ and its exact-exchange hole) at metal surfaces is investigated, by using either jellium slabs or the semi-infinite (SI) jellium model. For jellium slabs, we prove analytically and numerically that in the vacuum region far away from the surface $\varepsilon_{x}^{\text{Slab}}(z \to \infty) \to - e^{2}/2z$, {\it independent} of the bulk electron density, which is exactly half the corresponding exact-exchange potential $V_{x}(z \to \infty) \to - e^2/z$ [Phys. Rev. Lett. {\bf 97}, 026802 (2006)] of density-functional theory, as occurs in the case of finite systems. The fitting of $\varepsilon_{x}^{\text{Slab}}(z)$ to a physically motivated image-like expression is feasible, but the resulting location of the image plane shows strong finite-size oscillations every time a slab discrete energy level becomes occupied. For a semi-infinite jellium, the asymptotic behavior of $\varepsilon_{x}^{\text{SI}}(z)$ is somehow different. As in the case of jellium slabs $\varepsilon_{x}^{\text{SI}}(z \to \infty)$ has an image-like behavior of the form $\propto - e^2/z$, but now with a density-dependent coefficient that in general differs from the slab universal coefficient 1/2. Our numerical estimates for this coefficient agree with two previous analytical estimates for the same. For an arbitrary finite thickness of a jellium slab, we find that the asymptotic limits of $\varepsilon_{x}^{\text{Slab}}(z)$ and $\varepsilon_{x}^{\text{SI}}(z)$ only coincide in the low-density limit ($r_s \to \infty$), where the density-dependent coefficient of the semi-infinite jellium approaches the slab {\it universal} coefficient 1/2.
description: 26 pages, 7 figures, to appear in Phys. Rev. B
Dynamically generated resonances from the vector octet-baryon octet interaction
Creators: name: Oset, E.
name: Ramos, A.
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: We study the interaction of vector mesons with the octet of stable baryons in the framework of the local hidden gauge formalism using a coupled channels unitary approach. We examine the scattering amplitudes and their poles, which can be associated to known J^P=1/2^-,3/2^- baryon resonances, in some cases, or give predictions in other ones. The formalism employed produces doublets of degenerate J^P=1/2^-,3/2^- states, a pattern which is observed experimentally in several cases. The findings of this work should also be useful to guide present experimental programs searching for new resonances, in particular in the strange sector where the current information is very poor.
description: 21 pages, 4 figures
Fig. S1: The ethanolic UV-absorption spectra of zero order of DOB [A], TROX [B] and HQ [C] ; Fig. S2: The pH Effect on the native fluorescence intensity of TROX , DOB and HQ.; Fig. S3: Different surfactant effect on the native fluorescence intensity of TROX , DOB and HQ; Fig. S4: First approach application for the determination of DOB in spiked human plasma
Creators: name: M. M. Tolba
name: Salim, M. M.
name: El-Awady, M.
Publisher: name: The Royal Society
Year: 2021
Subjects: subject: 30203 Inorganic Green Chemistry
subject: FOS: Chemical sciences
subject: 30504 Organic Green Chemistry
subject: 30606 Structural Chemistry and Spectroscopy
subject: 30799 Theoretical and Computational Chemistry not elsewhere classified

description: In the present study, we conducted two facile and highly sensitive spectrofluorimetric approaches in order to quantify the vasoprotective agents; troxerutin (TROX) and calcium dobesilate (DOB) in the presence of hydroquinone (HQ) (as a highly toxic impurity and potential degradation product of DOB) in commercial formulations and human plasma. The first approach relies simply on using ethanol as an eco-friendly solvent for the estimation of DOB at 345 nm after being excited at 305 nm. The linearity was carefully investigated between DOB concentration and the relative fluorescence intensity in the range of 0.05–0.8 µg ml−1. Due to the high method simplicity and sensitivity, applying the first approach to quality control analysis and spiked human plasma samples with mean % recoveries 100.74 ± 3.71 adds another merit. The second approach involved rapid conventional fluorimetric estimation of ethanolic TROX solution in TROX/DOB combined dosage forms at 455/350 nm (emission/excitation) with a linear calibration chart covering the range of 0.1–1.2 µg ml−1. Moreover, the second approach involved a comprehensive study in a trial to solve the problem of superposition of DOB and HQ graph adopting the first derivative synchronous fluorimetric mechanism in ethanol at Δλ = 60 nm. Therefore, DOB was measured at 286 and 323 nm, while HQ could be quantitated at 301 nm. Beer's–Lambert law has complied over the ranges of 0.1–1.0 µg ml−1 and 0.02–0.4 µg ml−1 for DOB and HQ, respectively. Guidelines adopted by the International Council of Harmonization (ICH) were used to validate the target approaches. The developed methods are more convenient for routine quality control laboratory instead of the time-consuming and sophisticated reported techniques. Moreover, different aspects of evaluating the greenness of the proposed approaches were conducted to have a complete image of their environmental impact.
Definition, Grundlage, Ermöglichung und Grenzen von Kirchengemeinschaft
Creators: name: Slenczka, Reinhard
Publisher: name: Lutherische Beiträge
Year: 1970

description: Lutherische Beiträge, Bd. 13 Nr. 2 (2008): Lutherische Beiträge, Band 13, Heft 2
title: Student Engagement in LDS Seminaries
Creators: name: Aardema, Thomas P
Publisher: name: Utah State University
Year: 2013

description: This qualitative study examined student engagement in seminaries of The Church of Jesus Christ of Latter-day Saints (LDS). This study sought to answer the following question: "What are seminary teachers, who have been identified by content experts as having high levels of student engagement, doing to generate high levels of student engagement in their classrooms?" Ten LDS Seminary teachers were selected as participants for this study. The findings from this study were organized around the concepts of: competence, school membership, clarity of purpose, fairness, personal support, caring, authentic work, extrinsic reward, intrinsic interests, sense of ownership, connection to real-world application, and fun. The findings from this study suggest that there are 48 strategies that the 10 participants used to generate student engagement in their classrooms.