cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
The Stellar Chemical Abundances of Simulated Massive Galaxies at $z = 2$
Creators: name: Kim, Jee-Ho
name: Belli, Sirio
name: Weinberger, Rainer
Publisher: name: arXiv
Year: 2022
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We analyze the stellar abundances of massive galaxies ($\log M_\ast/M_\odot>10.5$) at $z=2$ in the IllustrisTNG simulation with the goal of guiding the interpretation of current and future observations, particularly from the James Webb Space Telescope. We find that the effective size, $R_e$, of galaxies strongly affects the abundance measurements: both [Mg/H] and [Fe/H] are anti-correlated with $R_e$, while the relative abundance [Mg/Fe] slightly increases with $R_e$. The $α$ enhancement as tracked by [Mg/Fe] traces the formation timescale of a galaxy weakly, and mostly depends on $R_e$. Aperture effects are important: measuring the stellar abundances within 1~kpc instead of within $R_e$ can make a large difference. These results are all due to a nearly universal, steeply declining stellar abundance profile that does not scale with galaxy size -- small galaxies appear metal-rich because their stars live in the inner part of the profile where abundances are high. The slope of this profile is mostly set by the gas-phase abundance profile and not substantially modified by stellar age gradients. The gas-phase abundance profile, in turn, is determined by the strong radial dependence of the gas fraction and star formation efficiency. We develop a simple model to describe the chemical enrichment, in which each radial bin of a galaxy is treated as an independent closed-box system. This model reproduces the gas-phase abundance profile of simulated galaxies, but not the detailed distribution of their stellar abundances, for which gas and/or metal transport are likely needed.
description: 16 pages, 12+2 figures, accepted for publication in MNRAS
Additional file 1 of The global prevalence of parasites in non-biting flies as vectors: a systematic review and meta-analysis
Creators: name: Liu, Yufeng
name: Chen, Yuancai
name: Wang, Nanhao
name: Qin, Huikai
name: Zhang, Longxian
name: Zhang, Sumei
Publisher: name: figshare
Year: 2023
Subjects: subject: Physical Sciences not elsewhere classified
subject: Microbiology
subject: FOS: Biological sciences
subject: Environmental Sciences not elsewhere classified
subject: Ecology
subject: Science Policy

description: Additional file 1: Table S1. PRISMA checklist.
Experimental Determination of Entanglement for Arbitrary Pure States
Creators: name: Fei, Shao-Ming
name: Zhao, Ming-Jing
name: Chen, Kai
name: Wang, Zhi-Xi
Publisher: name: arXiv
Year: 2009
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We present a way of experimentally determining the concurrence in terms of the expectation values of local observables for arbitrary multipartite pure states. In stead of the joint measurements on two copies of a state in the experiment for two-qubit systems [S. P. Walborn et al. Nature (London)440, 20(2006)], we only need one copy of the state in every measurement for any arbitrary dimensional multipartite systems, avoiding the preparation of twin states or the imperfect copy of the state.
description: 6 pages
System Integration of ATLAS ITK Pixel DCS ASICs
Creators: name: Qamesh, A.
name: Ahmad, R.
name: Ecker, D.
name: Fischer, T.
name: Karagounis, M.
name: Kind, P.
name: Kersten, S.
name: Krawutschke, T.
name: Schreiter, L.
name: Zeitnitz, C.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Instrumentation and Detectors (physics.ins-det)
subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: During the ATLAS phase II upgrade, the tracking system of the ATLAS experiment will be replaced by an all-silicon detector called the inner tracker (ITK) with a pixel detector as the most inner part. The monitoring data of the new system will be aggregated from an on-detector ASIC called Monitoring Of Pixel System (MOPS) and sent to the Detector Control System(DCS) using a new interface called MOPS-HUB. The hardware components of the MOPS-HUB, firmware specifications for the FPGA of MOPS-HUB and its integration plan will be presented. In addition, an irradiation plan for the new system will be introduced.
title: ÐÐ°Ð·Ð° Ð¿Ð¾ Ð¿ÑÐµÐ´ÑÐºÐ¿Ð»ÑÐ°ÑÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐµ Ð°Ð²ÑÐ¾Ð¼Ð¾Ð±Ð¸Ð»ÐµÐ¹
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ¸Ð»ÐµÑÐºÐ¾, 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: Ð¾Ð±ÐµÐºÑ
ÑÐ°ÑÑÐµÑ
ÑÑÐ½Ð´Ð°Ð¼ÐµÐ½Ñ

description: Ð Ð´Ð¸Ð¿Ð»Ð¾Ð¼Ðµ Ð±ÑÐ»Ð¾ ÑÐ¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¾ Ð¿Ð¾Ð¼ÐµÑÐµÐ½Ð¸Ðµ Ð´Ð»Ñ ÑÐµÐ¼Ð¾Ð½ÑÐ°, ÑÑÐ°Ð½ÐµÐ½Ð¸Ñ Ð¸ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐµ Ð°Ð²ÑÐ¾Ð¼Ð¾Ð±Ð¸Ð»ÐµÐ¹ Ð´Ð»Ñ Ð¸Ð·ÑÑÐºÐ°ÑÐµÐ»ÑÐ½ÑÑ Ð¸ Ð³ÐµÐ¾Ð´ÐµÐ·Ð¸ÑÐµÑÐºÐ¸Ñ ÑÐ°Ð±Ð¾Ñ. ÐÐµÑÑÐ¸ÐºÐ°Ð»ÑÐ½Ð°Ñ Ð¿Ð»Ð°Ð½Ð¸ÑÐ¾Ð²ÐºÐ° ÑÐµÑÐµÐ½Ð° Ñ ÑÑÐµÑÐ¾Ð¼ ÑÑÑÐµÑÑÐ²ÑÑÑÐ¸Ñ Ð¾ÑÐ¼ÐµÑÐ¾Ðº Ð¿ÑÐ¸Ð»ÐµÐ³Ð°ÑÑÐ¸Ñ ÑÐµÑÑÐ¸ÑÐ¾ÑÐ¸Ð¹. ÐÑÐ²Ð¾Ð´ Ð¿Ð¾Ð²ÐµÑÑÐ½Ð¾ÑÑÐ½ÑÑ Ð²Ð¾Ð´ Ð¾ÑÑÑÐµÑÑÐ²Ð»ÐµÐ½ Ð² ÑÑÑÐµÑÑÐ²ÑÑÑÑÑ ÐºÐ°Ð½Ð°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¾Ð½Ð½ÑÑ ÑÐ¸ÑÑÐµÐ¼Ñ. Ð Ð´Ð¸Ð¿Ð»Ð¾Ð¼Ð½Ð¾Ð¼ Ð¿ÑÐ¾ÐµÐºÑÐµ Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ñ Ð°ÑÑÐ¸ÑÐµÐºÑÑÑÐ½ÑÐµ, Ð¾Ð±ÑÐµÐ¼Ð½Ð¾-Ð¿Ð»Ð°Ð½Ð¸ÑÐ¾Ð²Ð¾ÑÐ½ÑÐµ Ð¸ ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð²Ð½ÑÐµ ÑÐµÑÐµÐ½Ð¸Ñ Ð·Ð´Ð°Ð½Ð¸Ñ, ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ Ð²Ð¾Ð¿ÑÐ¾ÑÑ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¸ Ð¸ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸ ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÑÑÐ²Ð°. ÐÑÐ¾ÐµÐºÑ ÑÐ¾Ð´ÐµÑÐ¶Ð¸Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ ÑÐ²ÐµÐ´ÐµÐ½Ð¸Ñ Ð¾Ð± Ð¸Ð½Ð¶ÐµÐ½ÐµÑÐ½ÑÑ ÑÐ¸ÑÑÐµÐ¼Ð°Ñ Ð¸ Ð¾Ð±Ð¾ÑÑÐ´Ð¾Ð²Ð°Ð½Ð¸Ð¸, ÐºÐ¾ÑÐ¾ÑÑÐ¼ Ð±ÑÐ´ÐµÑ Ð¾ÑÐ½Ð°ÑÐµÐ½Ð¾ Ð·Ð´Ð°Ð½Ð¸Ðµ. Ð ÑÐ°Ð·Ð´ÐµÐ»Ðµ Â«Ð Ð°ÑÑÐµÑÐ½Ð¾-ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð²Ð½Ð°Ñ ÑÐ°ÑÑÑÂ» Ð¿ÑÐ¸Ð²ÐµÐ´ÐµÐ½Ñ ÑÐ°ÑÑÐµÑÑ Ð¶ÐµÐ»ÐµÐ·Ð¾Ð±ÐµÑÐ¾Ð½Ð½Ð¾Ð³Ð¾ ÑÑÐ¾Ð»Ð±ÑÐ°ÑÐ¾Ð³Ð¾ ÑÑÐ½Ð´Ð°Ð¼ÐµÐ½ÑÐ° ÑÑÐ°ÐºÐ°Ð½Ð½Ð¾Ð³Ð¾ ÑÐ¸Ð¿Ð°. Ð Ð°ÑÑÐµÑ Ð¿ÑÐ¾Ð¸Ð·Ð²ÐµÐ´ÐµÐ½ Ð²ÑÑÑÐ½ÑÑ. ÐÑÐ¿Ð¾Ð»Ð½ÐµÐ½ Ð¿ÑÐ¾ÐµÐºÑ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸ ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÑÑÐ²Ð°, ÐºÐ°Ð»ÐµÐ½Ð´Ð°ÑÐ½ÑÐ¹ Ð¿Ð»Ð°Ð½. Ð Ð°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ Ð²Ð¾Ð¿ÑÐ¾ÑÑ ÑÐµÑÐ½Ð¸ÐºÐ¸ Ð±ÐµÐ·Ð¾Ð¿Ð°ÑÐ½Ð¾ÑÑÐ¸, Ð¾ÑÑÐ°Ð½Ñ ÑÑÑÐ´Ð° Ð¸ Ð¾ÐºÑÑÐ¶Ð°ÑÑÐµÐ¹ ÑÑÐµÐ´Ñ.
Black hole mirages: electron lensing and Berry curvature effects in inhomogeneously tilted Weyl semimetals
Creators: name: Haller, Andreas
name: Hegde, Suraj
name: Xu, Chen
name: De Beule, Christophe
name: Schmidt, Thomas L.
name: Meng, Tobias
Publisher: name: arXiv
Year: 2022
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We study electronic transport in Weyl semimetals with spatially varying nodal tilt profiles. We find that the flow of electrons can be guided precisely by judiciously chosen tilt profiles. In a broad regime of parameters, we show that electron flow is described well by semiclassical equations of motion similar to the ones governing gravitational attraction. This analogy provides a physically transparent tool for designing tiltronic devices like electronic lenses. The analogy to gravity circumvents the notoriously difficult full-fledged description of inhomogeneous solids. A comparison to microscopic lattice simulations shows that it is only valid for trajectories sufficiently far from analogue black holes. We finally comment on the Berry curvature-driven transverse motion and relate the latter to spin precession physics.
description: Replaced with revised version for SciPost resubmission. 38 pages, 12 figures
title: Student perspectives on the relationship between assessment methods and retention of learning in higher education
Creators: name: Kanuga, Ingrid
Publisher: name: University of Reading
Year: 2019

description: Over the last two decades, higher education in the UK has gone through significant changes. With the implementation of the Teaching Excellence Framework and accreditation by the Higher Education Academy, there have been higher levels of accountability towards course development underpinned by researched pedagogy. Better understanding of the influences of the learning environment and the links between assessments and student’s approaches to learning has led to academics being more innovative in their methods of education and has seen them adopt a more student-centred approach. Although in higher education circles the importance of building soft skills, like critical thinking, are being underlined; employers are asking for graduates to also recall and demonstrate the professional knowledge and understanding they gained during their studies. With an interest to gain an insight into what learning approach might be lined to retention of knowledge, this thesis examines the student perception of different assessment methods and the factors that may influence surface and deeper learning from their point of view. Using an embedded mixed methods design, the study has considered student analytics of attainment and engagement data for three different assessments: an exam, an essay and a phased assessment for a cohort of 105 students over a two-year period. These were compared with the results of an assessment experience questionnaire and interviews with students and lecturers. The research took place at a modern University in London. The findings demonstrated that students want active classrooms with tutors who challenge their learning in a creative way using stories, case studies and assessment strategies which can be linked to their future learning skills and application to industry. Such learning, teaching and assessment strategies will help the student embed this learning into their longer-term memory. In response to the findings, the study offers a way to design and deliver curriculum and assessment methods to maximise student learning and retention of learning, in particular considering those students who have lesser engagement opportunities. The concept of “LAAAM” provides a framework to integrate these findings and act upon them, creating a platform which should stimulate a deep learning approach by students and help them retain the knowledge gained from their learning.
Light scalar mesons in QCD sum rules with inclusion of instantons
Creators: name: Zhang, J.
name: Jin, H. Y.
name: Zhang, Z. F.
name: Steele, T. G.
name: Lu, D. H.
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The light scalar meson nonet above 1 GeV ({\it i.e.\}the $a_{0}$, $K^{\ast}_{0}$ and $f_{0}$) are studied within the framework of QCD sum rules. In conventional QCD sum rules, the calculated masses of this nonet are degenerate, and the mass of $K^{\ast}_{0}$ is always larger than the $a_{0}$ in contradiction with the observed spectrum. After improving the correlation function by including instanton effects, the masses are well separated from each other. In particular, our results shows glueball content plays an important role in the underlying structure of $f_{0}(1500)$. The decay constants are also discussed.
description: 10 figs, 22 pages
Driving Sustainability Through Supply Chain Innovation: A Pathway to Success
Creators: name: Zurub, Hani Hossni
Publisher: name: Zenodo
Year: 2023
Subjects: Sustainability
Supply Chain
Reduce Costs
Productivity
Supply Chain Sustainability
Regulations
Laws
Government

description: Supply Chain Sustainability is very important these days to protect our environment from phenomena like Climate Change and its effects on our Earth planet, and it can also increase competitiveness and productivity in the business.
eta - eta' - glueball mixing
Creators: name: Kiesewetter, Simon
name: Vento, Vicente
Publisher: name: arXiv
Year: 2010
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We have revisited glueball mixing with the pseudoscalar mesons in the MIT bag model scheme. The calculation has been performed in the spherical cavity approximation to the bag using two different fermion propagators, the cavity and the free propagators. We obtain a very small probability of mixing for the eta at the level of $0.04-0.1% and a bigger for the eta' at the level of 4-12%. Our results differ from previous calculations in the same scheme but seem to agree with the experimental analysis. We discuss the origin of our difference which stems from the treatment of our time integrations.
description: 21 pages, 7 figures
Magnetotransport Properties and Fermi Surface Topology of Nodal line Semimetal InBi
Creators: name: Dan, Sambhab
name: Kargeti, Kuldeep
name: Sahoo, R. C.
name: Dan, Shovan
name: Pal, Debarati
name: Verma, Sunil
name: Chakravarty, Sujay
name: Panda, S. K.
name: Patil, S
Publisher: name: arXiv
Year: 2022
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: In the present study, we have discussed the up-turn behavior in the resistivity pattern of the topological nodal line semimetal InBi. We argued that such nature could be generalized with a mathematical model, that can be applied to any compounds exhibiting similar behavior. The extremely high magnetoresistance (XMR) has also been explained by the carrier compensation in the compound, estimated from the Hall conductivity. Moreover, from the study of Subhnikov-de Haas (SdH) oscillation and density functional theory (DFT), we obtained the complete three-dimensional (3D) Fermi surface topology of the compound InBi. A detailed understanding of carriers' behavior has been discussed using those studies. We have also unfurled the topology of each electron and hole pocket and its possible modulation with electron and hole doping.
title: Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° ÑÑÐ»Ð¾Ð²Ð¸Ð¹ Ð¿ÐµÑÐµÑÐ°Ð±Ð¾ÑÐºÐ¸ ÑÐ²Ð¸Ð½ÐµÑÑÐ¾Ð´ÐµÑÐ¶Ð°ÑÐ¸Ñ Ð¿ÑÐ»ÐµÐ¹ ÑÐµÑ Ð½Ð¾Ð³ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¿ÑÐ¾Ð¸ÑÑ Ð¾Ð¶Ð´ÐµÐ½Ð¸Ñ Ñ Ð¿Ð¾Ð»ÑÑÐµÐ½Ð¸ÐµÐ¼ ÑÐµÑÐ½Ð¾Ð²Ð¾Ð³Ð¾ ÑÐ²Ð¸Ð½ÑÐ°
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐµÑÑÐ¾ÑÑÐ½, ÐÑ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: 2016
Subjects: ÑÐ²Ð¸Ð½ÐµÑÑÐ¾Ð´ÐµÑÐ¶Ð°ÑÐ¸Ðµ Ð¿ÑÐ»Ð¸
ÑÐµÑÐ½Ð¾Ð²Ð¾Ð¹ ÑÐ²Ð¸Ð½ÐµÑ
Ð¿Ð¸ÑÐ¾Ð¼ÐµÑÐ°Ð»Ð»ÑÑÐ³Ð¸Ñ
Ð¾ÐºÑÐ¸Ð´ ÑÐ²Ð¸Ð½ÑÐ°

description: ÐÐ¸Ð¿Ð»Ð¾Ð¼Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð¿Ð¾ÑÐ²ÑÑÐµÐ½Ð° Ð²ÑÐ±Ð¾ÑÑ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¸ Ð¿ÐµÑÐµÑÐ°Ð±Ð¾ÑÐºÐ¸ ÑÐ²Ð¸Ð½ÐµÑÑÐ¾Ð´ÐµÑÐ¶Ð°ÑÐ¸Ñ Ð¿ÑÐ»ÐµÐ¹ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸ÑÑ, Ð¸ÑÐ¿Ð¾Ð»ÑÐ·ÑÑÑÐ¸Ñ Ð¿Ð¸ÑÐ¾Ð¼ÐµÑÐ°Ð»Ð»ÑÑÐ³Ð¸ÑÐµÑÐºÐ¸Ðµ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¸ Ð¿ÐµÑÐµÑÐ°Ð±Ð¾ÑÐºÐ¸ Ð¿Ð¾Ð»Ð¸Ð¼ÐµÑÐ°Ð»Ð»Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÑÐ»ÑÑÐ¸Ð´Ð½Ð¾Ð³Ð¾ ÑÑÑÑÑ. Ð¢Ð°Ðº Ð¶Ðµ Ð¼Ð½Ð¾Ñ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ Ð½ÐµÐºÐ¾ÑÐ¾ÑÑÐµ Ð´Ð¾ÑÑÑÐ¿Ð½ÑÐµ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¸ Ð¿ÐµÑÐµÑÐ°Ð±Ð¾ÑÐºÐ¸ ÑÐ²Ð¸Ð½ÐµÑÑÐ¾Ð´ÐµÑÐ¶Ð°ÑÐ¸Ñ Ð¿ÑÐ»ÐµÐ¹, Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð½ÑÐµ Ð½Ð° Ð³Ð¸Ð´ÑÐ¾- Ð¸ Ð¿Ð¸ÑÐ¾Ð¼ÐµÑÐ°Ð»Ð»ÑÑÐ³Ð¸Ð¸. ÐÑÐ¼ÐµÑÐµÐ½Ð¾, ÑÑÐ¾ Ð¿Ð¸ÑÐ¾Ð¼ÐµÑÐ°Ð»Ð»ÑÑÐ³Ð¸ÑÐµÑÐºÐ°Ñ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ñ Ð¿ÐµÑÐµÑÐ°Ð±Ð¾ÑÐºÐ¸ Ð¿ÑÐ»ÐµÐ¹, Ð½ÐµÑÐ¼Ð¾ÑÑÑ Ð½Ð° ÑÑÐ´ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ñ Ð½ÐµÐ´Ð¾ÑÑÐ°ÑÐºÐ¾Ð², ÑÐ²Ð»ÑÐµÑÑÑ Ð·Ð½Ð°ÑÐ¸ÑÐµÐ»ÑÐ½Ð¾ Ð±Ð¾Ð»ÐµÐµ Ð¿ÑÐ¾ÑÑÐ¾Ð¹ Ð¸ Ð¼ÐµÐ½ÐµÐµ Ð·Ð°ÑÑÐ°ÑÐ½Ð¾Ð¹ ÐºÐ°Ðº Ð¿Ð¾ ÐºÐ°Ð¿Ð¸ÑÐ°Ð»ÑÐ½ÑÐ¼, ÑÐ°Ðº Ð¸ Ð¿Ð¾ ÑÐºÑÐ¿Ð»ÑÐ°ÑÐ°ÑÐ¸Ð¾Ð½Ð½ÑÐ¼ ÑÐ°ÑÑÐ¾Ð´Ð°Ð¼, Ð¿Ð¾ ÑÑÐ°Ð²Ð½ÐµÐ½Ð¸Ñ Ñ Ð³Ð¸Ð´ÑÐ¾Ð¼ÐµÑÐ°Ð»Ð»ÑÑÐ³Ð¸ÑÐµÑÐºÐ¸Ð¼Ð¸ ÑÑÐµÐ¼Ð°Ð¼Ð¸.
title: ÐÑÐ¸Ð»Ð¾Ð¶ÐµÐ½Ð¸Ðµ Ð¿Ð¾Ð´ iOS Ñ Ð²Ð¾Ð·Ð¼Ð¾Ð¶Ð½Ð¾ÑÑÑÑ ÑÐ¸ÑÑÐ¾Ð²Ð°Ð½Ð¸Ñ/Ð´ÐµÑÐ¸ÑÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð´Ð°Ð½Ð½ÑÑ Ð¸ Ñ ÑÐ°Ð½ÐµÐ½Ð¸Ñ Ð·Ð°ÑÐ¸ÑÑÐ¾Ð²Ð°Ð½Ð½Ð¾Ð¹ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¸
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: Ð¡ÐµÐ»Ð¸Ð²ÐµÑÑÑÐ¾Ð², ÐÐ°Ð»ÐµÑ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: ios-Ð¿ÑÐ¸Ð»Ð¾Ð¶ÐµÐ½Ð¸Ñ
ÑÐ¸ÑÑÐ¾Ð²Ð°Ð½Ð¸Ðµ
ÐºÑÐ¸Ð¿ÑÐ¾Ð³ÑÐ°ÑÐ¸Ñ
Â«ÐºÑÐ·Ð½ÐµÑÐ¸ÐºÂ»
Ð¿ÑÐ¸Ð»Ð¾Ð¶ÐµÐ½Ð¸Ðµ Ð½Ð° iphone

description: Ð ÑÐ°Ð±Ð¾ÑÐµ Ð¾Ð¿Ð¸ÑÐ°Ð½Ð¾ ÑÐ¾Ð·Ð´Ð°Ð½Ð¸Ðµ Ð¿ÑÐ¸Ð»Ð¾Ð¶ÐµÐ½Ð¸Ñ Ð² ÑÑÐµÑÐµ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ Ð±ÐµÐ·Ð¾Ð¿Ð°ÑÐ½Ð¾ÑÑÐ¸. 1. ÐÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½ Ð¾Ð±Ð·Ð¾Ñ Ð¿ÑÐ¸Ð»Ð¾Ð¶ÐµÐ½Ð¸Ð¹ Ð´Ð»Ñ Ð¾Ð¿ÐµÑÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÑÐ¸ÑÑÐµÐ¼Ñ iOS Ñ ÑÑÐ½ÐºÑÐ¸ÑÐ¼Ð¸ Ð·Ð°ÑÐ¸ÑÑ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¸. 2. ÐÑÐ¸Ð²ÐµÐ´ÐµÐ½ Ð²ÑÐ±Ð¾Ñ Ð¸ÑÑÐ¾Ð´Ð½ÑÑ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ð¾Ð² Ð´Ð»Ñ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ¸ ÑÐ²Ð¾ÐµÐ³Ð¾ ÑÐµÑÐµÐ½Ð¸Ñ. 3. ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð° Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ°Ñ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð¿ÑÐ¸Ð»Ð¾Ð¶ÐµÐ½Ð¸Ñ Ñ Ð²Ð¾Ð·Ð¼Ð¾Ð¶Ð½Ð¾ÑÑÑÑ ÑÐ¸ÑÑÐ¾Ð²Ð°Ð½Ð¸Ñ/Ð´ÐµÑÐ¸ÑÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð´Ð°Ð½Ð½ÑÑ Ð¸ ÑÑÐ°Ð½ÐµÐ½Ð¸Ñ Ð·Ð°ÑÐ¸ÑÑÐ¾Ð²Ð°Ð½Ð½Ð¾Ð¹ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¸. 4. ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½Ñ ÑÐµÑÑÑ ÑÑÐ½ÐºÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½Ð¾ÑÑÐ¸ Ð¿ÑÐ¸Ð»Ð¾Ð¶ÐµÐ½Ð¸Ñ, Ð±ÐµÐ·Ð¾Ð¿Ð°ÑÐ½Ð¾ÑÑÐ¸ Ð´Ð°Ð½Ð½ÑÑ, ÑÐµÐ°ÐºÑÐ¸Ð¸ Ð½Ð° Ð¸ÑÐºÐ»ÑÑÐ¸ÑÐµÐ»ÑÐ½ÑÐµ ÑÐ¸ÑÑÐ°ÑÐ¸Ð¸ (ÑÐ°ÐºÐ¸Ðµ, ÐºÐ°Ðº Ð·Ð°Ð¿Ð¾Ð»Ð½ÐµÐ½Ð¸Ðµ Ð¿Ð°Ð¼ÑÑÐ¸ ÑÑÑÑÐ¾Ð¹ÑÑÐ²Ð° Ð¸Ð»Ð¸ ÑÐ±Ð¾Ð¹ Ð¿Ð¸ÑÐ°Ð½Ð¸Ñ).
The phase structure of cosmic ray driven outflows in stream fed disc galaxies
Creators: name: Peschken, Nicolas
name: Hanasz, Michał
name: Naab, Thorsten
name: Wóltański, Dominik
name: Gawryszczak, Artur
Publisher: name: arXiv
Year: 2022
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Feeding with gas in streams is predicted to be an important galaxy growth mechanism. Using an idealised setup, we study the impact of stream feeding (with 10$^7$ M$_{\odot}$ Myr$^{-1}$ rate) on the star formation and outflows of disc galaxies with $\sim$10$^{11}$ M$_{\odot}$ baryonic mass. The magneto-hydrodynamical simulations are carried out with the PIERNIK code and include star formation, feedback from supernova, and cosmic ray advection and diffusion. We find that stream accretion enhances galactic star formation. Lower angular momentum streams result in more compact discs, higher star formation rates and stronger outflows. In agreement with previous studies, models including cosmic rays launch stronger outflows travelling much further into the galactic halo. Cosmic ray supported outflows are also cooler than supernova only driven outflows. With cosmic rays, the star formation is suppressed and the thermal pressure is reduced. We find evidence for two distinct outflow phases. The warm outflows have high angular momentum and stay close to the galactic disc, while the hot outflow phase has low angular momentum and escapes from the centre deep into the halo. Cosmic rays can therefore have a strong impact on galaxy evolution by removing low angular momentum, possibly metal enriched gas from the disc and injecting it into the circumgalactic medium.
description: 18 pages, 19 figures. Submitted to MNRAS
Satellites of Milky Way- and M31-like galaxies with TNG50: quenched fractions, gas content, and star formation histories
Creators: name: Engler, Christoph
name: Pillepich, Annalisa
name: Joshi, Gandhali D.
name: Pasquali, Anna
name: Nelson, Dylan
name: Grebel, Eva K.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We analyse the quenched fractions, gas content, and star formation histories of ~1200 satellite galaxies with $M_* \geq 5 \times 10^6~{\rm M}_\odot$ around 198 Milky Way- (MW) and Andromeda-like (M31) hosts in TNG50, the highest-resolution simulation of IllustrisTNG. Satellite quenched fractions are larger for smaller masses, for smaller distances to their host galaxy, and in the more massive M31-like compared to MW-like hosts. As satellites cross their host's virial radius, their gas content drops: most satellites within 300 kpc lack detectable gas reservoirs at $z=0$, unless they are massive like the Magellanic Clouds and M32. Nevertheless, their stellar assembly exhibits a large degree of diversity. On average, the cumulative star formation histories are more extended for brighter, more massive satellites with a later infall, and for those in less massive hosts. Based on these relationships, we can even infer infall periods for observedMWand M31 dwarfs: e.g. 0-4 Gyr ago for the Magellanic Clouds and Leo I, 4-8 and 0-2 Gyr ago for M32 and IC 10, respectively. Ram pressure stripping (in combination with tidal stripping) deprives TNG50 satellites of their gas reservoirs and ultimately quenches their star formation, even though only a few per cent of the present-day satellites around the 198 TNG50 MW/M31-like hosts appear as jellyfish. The typical time since quenching for currently quenched TNG50 satellites is $6.9^{+2.5}_{-3.3}~{\rm Gyr}$ ago. The TNG50 results are consistent with the quenched fractions and stellar assembly of observed MW and M31 satellites, however, satellites of the SAGA survey with $M_* \sim 10^{8-9}~{\rm M}_\odot$ exhibit lower quenched fractions than TNG50 and other, observed analogues.
description: Accepted for publication in MNRAS
Correlators of supersymmetric Wilson loops at weak and strong coupling
Creators: name: Bassetto, Antonio
name: Griguolo, Luca
name: Pucci, Fabrizio
name: Seminara, Domenico
name: Thambyahpillai, Shiyamala
name: Young, Donovan
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We continue our study of the correlators of a recently discovered family of BPS Wilson loops in N=4 supersymmetric U(N) Yang-Mills theory. We perform explicit computations at weak coupling by means of analytical and numerical methods finding agreement with the exact formula derived from localization. In particular we check the localization prediction at order g^6 for different BPS "latitude" configurations, the N=4 perturbative expansion reproducing the expected results within a relative error of 10^(-4). On the strong coupling side we present a supergravity evaluation of the 1/8 BPS correlator in the limit of large separation, taking into account the exchange of all relevant modes between the string world-sheets. While reproducing the correct geometrical dependence, we find that the associated coefficient does not match the localization result.
description: 34 pages, 16 figures
title: ÐÐµÑÐµÐºÑÑ Ð¿Ð¾Ð»ÑÐ¿ÑÐ¾Ð²Ð¾Ð´Ð½Ð¸ÐºÐ¾Ð²
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ
titleType: Subtitle
Creators: name: Ð¡Ð°Ð¼Ð¾ÑÑÐºÐ¾Ð², ÐÐ¾ÑÐ¸Ñ
Publisher: name: ÐÐÐ Ð¸Ð¼ÐµÐ½Ð¸ Ð. Ð. ÐÐ°Ð»Ð¸Ð½Ð¸Ð½Ð°
Year: 1977
Subjects: ÐÐ¾Ð»ÑÐ¿ÑÐ¾Ð²Ð¾Ð´Ð½Ð¸ÐºÐ¸

description: Ð Ð¿Ð¾ÑÐ¾Ð±Ð¸Ð¸ Ð¸Ð·Ð»Ð°Ð³Ð°ÐµÑÑÑ ÑÐ°ÑÑÑ ÐºÑÑÑÐ° Â«Ð¤Ð¸Ð·Ð¸ÑÐµÑÐºÐ¸Ðµ Ð¸ ÑÐ¸Ð¼Ð¸ÑÐµÑÐºÐ¸Ðµ ÑÐ²Ð¾Ð¹ÑÑÐ²Ð° Ð¿Ð¾Ð»ÑÐ¿ÑÐ¾Ð²Ð¾Ð´Ð½Ð¸ÐºÐ¾Ð²Â», Ð¿Ð¾ÑÐ²ÑÑÐµÐ½Ð½Ð°Ñ Ð´ÐµÑÐµÐºÑÐ°Ð¼ Ð¿Ð¾Ð»Ñ Ð¿ÑÐ¾Ð²Ð¾Ð´Ð½Ð¸ÐºÐ¾Ð². Ð Ð°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ ÑÐµÐ¿Ð»Ð¾Ð²ÑÐµ, ÑÐ»ÐµÐºÑÑÐ¾Ð½Ð½ÑÐµ Ð¸ ÑÐ¾ÑÐµÑÐ½ÑÐµ Ð´ÐµÑÐµÐºÑÑ ÐºÑÐ¸ÑÑÐ°Ð»Ð»Ð¾Ð². ÐÑÐ¾Ð±Ð¾Ðµ Ð²Ð½Ð¸Ð¼Ð°Ð½Ð¸Ðµ ÑÐ´ÐµÐ»ÐµÐ½Ð¾ Ð¿ÑÐ¸Ð¼ÐµÑÑÐ¼ Ð¸ Ð¾ÑÐ½Ð¾Ð²Ð°Ð¼ Ð»ÐµÐ³Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¿Ð¾Ð»ÑÐ¿ÑÐ¾Ð²Ð¾Ð´Ð½Ð¸ÐºÐ¾Ð². Ð¡ ÑÐ¸Ð¼Ð¸ÑÐµÑÐºÐ¸Ñ Ð¿Ð¾Ð·Ð¸ÑÐ¸Ð¸ Ð¸Ð·Ð»Ð¾Ð¶ÐµÐ½Ñ Ð²Ð¾Ð¿ÑÐ¾ÑÑ ÑÐ°Ð²Ð½Ð¾Ð²ÐµÑÐ¸Ñ Ð¸ Ð²Ð·Ð°Ð¸Ð¼Ð¾Ð´ÐµÐ¹ÑÑÐ²Ð¸Ñ Ð´ÐµÑÐµÐºÑÐ¾Ð², Ð¿ÑÐ¸Ð²Ð¾Ð´ÑÑÑÑ Ð»Ð¸Ð½ÐµÐ¹Ð½ÑÐµ Ð¸ Ð¿Ð¾Ð²ÐµÑÑÐ½Ð¾ÑÑÐ½ÑÐµ Ð´ÐµÑÐµÐºÑÑ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ð¾Ð², Ð¾Ð±ÑÑÐ¶Ð´Ð°ÐµÑÑÑ Ð²Ð»Ð¸ÑÐ½Ð¸Ðµ Ð´ÐµÑÐµÐºÑÐ¾Ð² Ð½Ð° ÑÐ»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ¸Ðµ ÑÐ²Ð¾Ð¹ÑÑÐ²Ð° Ð¿Ð¾Ð»ÑÐ¿ÑÐ¾Ð²Ð¾Ð´Ð½Ð¸ÐºÐ¾Ð². Ð­ÑÐ¸ ÑÐ°Ð·Ð´ÐµÐ»Ñ Ð¸Ð¼ÐµÑÑ Ð¸ÑÐºÐ»ÑÑÐ¸ÑÐµÐ»ÑÐ½Ð¾ Ð±Ð¾Ð»ÑÑÐ¾Ðµ Ð·Ð½Ð°ÑÐµÐ½Ð¸Ðµ Ð´Ð»Ñ Ð¿Ð¾Ð½Ð¸Ð¼Ð°Ð½Ð¸Ñ ÑÐ²Ð¾Ð¹ÑÑÐ² Ð¿Ð¾Ð»ÑÐ¿ÑÐ¾Ð²Ð¾Ð´Ð½Ð¸ÐºÐ¾Ð²ÑÑ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ð¾Ð². ÐÐ¾ÑÐ¾Ð±Ð¸Ðµ Ð¿ÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¾ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² ÑÐ¿ÐµÑ. 0643, Ð° ÑÐ°ÐºÐ¶Ðµ Ð°ÑÐ¿Ð¸ÑÐ°Ð½ÑÐ¾Ð² Ð¸ Ð½Ð°ÑÑÐ½ÑÑ ÑÐ°Ð±Ð¾ÑÐ½Ð¸ÐºÐ¾Ð², ÑÐ¿ÐµÑÐ¸Ð°Ð»Ð¸Ð·Ð¸ÑÑÑÑÐ¸ÑÑÑ Ð² Ð¾Ð±Ð»Ð°ÑÑÐ¸ ÑÐ¸Ð·Ð¸ÐºÐ¸ Ð¸ ÑÐ¸Ð¼Ð¸Ð¸ Ð¿Ð¾Ð»ÑÐ¿ÑÐ¾Ð²Ð¾Ð´Ð½Ð¸ÐºÐ¾Ð².
title: ÐÐ¾Ð²ÑÑÐµÐ½Ð¸Ðµ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ ÑÐ¾ÑÑÐ¸ÑÐ¾Ð²ÐºÐ¸ Ð³ÐµÐ½ÐµÑÐ¸ÑÐµÑÐºÐ¸Ñ Ð¿Ð¾ÑÐ»ÐµÐ´Ð¾Ð²Ð°ÑÐµÐ»ÑÐ½Ð¾ÑÑÐµÐ¹ Ð² Ð¿ÑÐ¾ÐµÐºÑÐµ SAMtools Ð½Ð° Ð°ÑÑ Ð¸ÑÐµÐºÑÑÑÐ°Ñ MIMD
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ÑÑÐ°Ð²Ð»ÑÐ²Ð°, ÐÐ»ÐµÐºÑÐ°Ð½Ð´Ñ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: SAMTOOLS
INTEL AMPLIFIER
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ÑÐµÑÑ ÑÐ¾ÑÑÑÐ¸ÑÐ¾Ð²ÐºÐ¸
Ð°Ð²ÑÐ¾Ð²ÐµÐºÑÐ¾ÑÐ¸Ð·Ð°ÑÐ¸Ñ

description: Ð Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ ÑÐ°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÐµÑÑÑ ÑÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ðµ ÑÑÐ¸Ð»Ð¸ÑÑ ÑÐ¾ÑÑÐ¸ÑÐ¾Ð²ÐºÐ¸ Ð³ÐµÐ½ÐµÑÐ¸ÑÐµÑÐºÐ¾Ð¹ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¸ Ð² Ð¿ÑÐ¾ÐµÐºÑÐµ Ñ Ð¾ÑÐºÑÑÑÑÐ¼ Ð¸ÑÑÐ¾Ð´Ð½ÑÐ¼ ÐºÐ¾Ð´Ð¾Ð¼ SAMtools. ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¾ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð½Ð¾Ð²ÑÑ Ð°Ð»Ð³Ð¾ÑÐ¸ÑÐ¼Ð¾Ð², Ð¿Ð¾Ð´ÑÐ¾Ð´Ð¾Ð² Ð²ÐµÐºÑÐ¾ÑÐ¸Ð·Ð°ÑÐ¸Ð¸ Ð¸ Ð¿Ð°ÑÐ°Ð»Ð»ÐµÐ»Ð¸Ð·Ð°ÑÐ¸Ð¸ Ñ ÑÐµÐ»ÑÑ Ð²ÑÐ±Ð¾ÑÐ° Ð½Ð°Ð¸Ð»ÑÑÑÐµÐ¹ Ð¼Ð¾Ð´Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¸ Ð´Ð»Ñ Ð²Ð½ÐµÐ´ÑÐµÐ½Ð¸Ñ Ð² ÐºÐ¾Ð´ Ð¾ÑÐ¸ÑÐ¸Ð°Ð»ÑÐ½Ð¾Ð³Ð¾ ÑÐµÐ¿Ð¾Ð·Ð¸ÑÐ¾ÑÐ¸Ñ.
Ð ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐµ Ð±ÑÐ»Ð¸ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ñ Ð°Ð»Ð³Ð¾ÑÐ¸ÑÐ¼Ñ Ð¿Ð¾ÑÐ°Ð·ÑÑÐ´Ð½Ð¾Ð¹ ÑÐ¾ÑÑÐ¸ÑÐ¾Ð²ÐºÐ¸ Ð¸ ÑÐµÑÐ¸ ÑÐ¾ÑÑÐ¸ÑÐ¾Ð²ÐºÐ¸, Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´Ð¸ÑÐµÐ»ÑÐ½Ð¾ÑÑÑ ÐºÐ¾ÑÐ¾ÑÑÑ Ð»ÑÑÑÐµ Ð¸ÑÑÐ¾Ð´Ð½Ð¾Ð³Ð¾ Ð²Ð°ÑÐ¸Ð°Ð½ÑÐ° Ð¿Ð¾ ÑÐ°Ð·Ð½ÑÐ¼ Ð¾ÑÐµÐ½ÐºÐ°Ð¼ Ð¾Ñ 3 Ð´Ð¾ 9 ÑÐ°Ð·. ÐÐ±Ð¾Ð·Ð½Ð°ÑÐµÐ½Ñ Ð¿ÐµÑÑÐ¿ÐµÐºÑÐ¸Ð²Ñ Ð²ÐµÐºÑÐ¾ÑÐ¸Ð·Ð°ÑÐ¸Ð¸ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ð½ÑÑ Ð¼ÐµÑÐ¾Ð´Ð¾Ð². Ð ÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ñ Ð¿Ð¾ÑÐ°Ð·ÑÑÐ´Ð½Ð¾Ð¹ ÑÐ¾ÑÑÐ¸ÑÐ¾Ð²ÐºÐ¸ Ð±ÑÐ»Ð° Ð¿ÑÐ¸Ð½ÑÑÐ° Ð² Ð¸ÑÑÐ¾Ð´Ð½ÑÐ¹ ÐºÐ¾Ð´ Ð¾ÑÐ¸ÑÐ¸Ð°Ð»ÑÐ½Ð¾Ð³Ð¾ ÑÐµÐ¿Ð¾Ð·Ð¸ÑÐ¾ÑÐ¸Ñ SAMtools Ð¸ ÑÑÐ¿ÐµÑÐ½Ð¾ Ð¿ÑÐ¸Ð¼ÐµÐ½ÑÐµÑÑÑ Ð¿ÑÐ¸ ÑÐ°Ð±Ð¾ÑÐµ Ñ Ð³ÐµÐ½ÐµÑÐ¸ÑÐµÑÐºÐ¸Ð¼Ð¸ Ð´Ð°Ð½Ð½ÑÐ¼Ð¸ Ð² Ð¾Ð±Ð»Ð°ÑÑÐ¸ Ð¼ÐµÐ´Ð¸ÑÐ¸Ð½Ñ Ð¸ Ð±Ð¸Ð¾Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸ÐºÐ¸. â
PeV-scale leptogenesis, gravity waves and black holes from a SUSY-breaking phase transition
Creators: name: Cline, James M.
name: Laurent, Benoit
name: Raby, Stuart
name: Roux, Jean-Samuel
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: Supersymmetry is a highly motivated theoretical framework, whose scale of breaking may be at PeV energies, to explain null searches at the Large Hadron Collider. SUSY breaking through a first order phase transition may have occurred in the early universe, leading to potential gravitational wave signals. Constructing a realistic model for gauge-mediated supersymmetry breaking, we show that such a transition can also induce masses for heavy right-handed neutrinos and sneutrinos, whose CP-violating decays give leptogenesis at the PeV scale, and a novel mechanism of neutrino mass generation at one loop. For the same models we predict the possible gravity wave signals, and we study the possibility of production of primordial black holes during the phase transition.
description: 19 pages, 8 figures
title: Ð£ÑÐµÑ Ð¸ Ð°Ð½Ð°Ð»Ð¸Ð· Ð¸Ð·Ð´ÐµÑÐ¶ÐµÐº Ð¾Ð±ÑÐ°ÑÐµÐ½Ð¸Ñ (ÑÐ°ÑÑ Ð¾Ð´Ð¾Ð² Ð½Ð° Ð¿ÑÐ¾Ð´Ð°Ð¶Ñ) Ð² ÑÐ¸ÑÑÐµÐ¼Ðµ ÐºÐ¾Ð½ÑÑÐ¾Ð»Ñ Ð·Ð° ÑÐ°ÑÑ Ð¾Ð´Ð°Ð¼Ð¸ ÑÐ¾ÑÐ³Ð¾Ð²ÑÑ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¹
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ°ÑÐ°ÑÑÐ²Ð°, ÐÐ»Ñ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: 2016
Subjects: Ð¸Ð·Ð´ÐµÑÐ¶ÐºÐ¸ Ð¾Ð±ÑÐ°ÑÐµÐ½Ð¸Ñ
ÑÐµÐ·ÐµÑÐ²Ñ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸Ð¸
ÐºÐ¾Ð½ÑÑÐ¾Ð»Ñ Ð·Ð° ÑÐ°ÑÑ Ð¾Ð´Ð°Ð¼Ð¸

description: ÐÐ±ÑÐµÐºÑÐ¾Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ²Ð»ÑÐµÑÑÑ ÐÐ Â«Ð§ÐµÑÐµÐ¿Ð¾Ð²ÐµÑÐºÐ¸Ð¹ Ð¼ÑÑÐ¾ÐºÐ¾Ð¼Ð±Ð¸Ð½Ð°ÑÂ». ÐÑÐµÐ´Ð¼ÐµÑ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ - ÑÐ°ÑÑÐ¾Ð´Ñ Ð½Ð° Ð¿ÑÐ¾Ð´Ð°Ð¶Ñ ÐÐ Â«Ð§ÐÐÂ». Ð¦ÐµÐ»Ñ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ: Ð¸Ð·ÑÑÐµÐ½Ð¸Ðµ ÑÑÐµÑÐ° Ð¸ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¸Ðµ Ð°Ð½Ð°Ð»Ð¸Ð·Ð° Ð¸Ð·Ð´ÐµÑÐ¶ÐµÐº Ð¾Ð±ÑÐ°ÑÐµÐ½Ð¸Ñ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ, Ð° ÑÐ°ÐºÐ¶Ðµ ÑÐ¾Ð·Ð´Ð°Ð½Ð¸Ðµ Ð¸ ÑÐ¾ÑÐ¼ÑÐ»Ð¸ÑÐ¾Ð²ÐºÐ° ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð°ÑÐ¸Ð¹ Ð¿Ð¾ ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÑÐµÑÐ° Ð¸Ð·Ð´ÐµÑÐ¶ÐµÐº Ð¾Ð±ÑÐ°ÑÐµÐ½Ð¸Ñ, Ð¿Ð¾ Ð¸Ñ ÑÐ½Ð¸Ð¶ÐµÐ½Ð¸Ñ Ð´Ð»Ñ ÑÐ¿ÑÐ¾ÑÐ½ÐµÐ½Ð¸Ñ Ð¿Ð¾Ð·Ð¸ÑÐ¸Ð¹ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ Ð½Ð° ÑÑÐ½ÐºÐµ.
A fast, accurate, and easy to implement Kapur-Rokhlin quadrature scheme for singular integrals in axisymmetric geometries
Creators: name: Toler, E.
name: Cerfon, A. J.
name: Malhotra, D.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Plasma Physics (physics.plasm-ph)
subject: Mathematical Physics (math-ph)
subject: Computational Physics (physics.comp-ph)
subject: FOS: Physical sciences

description: Many applications in magnetic confinement fusion require the efficient calculation of surface integrals with singular integrands. The singularity subtraction approaches typically used to handle such singularities are complicated to implement and low order accurate. In contrast, we demonstrate that the Kapur-Rokhlin quadrature scheme is well-suited for the logarithmically singular integrals encountered for a toroidally axisymmetric confinement system, is easy to implement, and is high order accurate. As an illustration, we show how to apply this quadrature scheme for the efficient and accurate calculation of the normal component of the magnetic field due to the plasma current on the plasma boundary, via the virtual casing principle.
description: 21 pages, 4 figures
title: Leaf-specific weed control for vegetable crops in the UK
Creators: name: Koukiasas, Nikolaos
Publisher: name: University of Reading
Year: 2019

description: Weed control in field vegetables in the UK is becoming increasingly challenging due to the loss of herbicide actives and demands by policy makers and consumers for lower pesticide use. Research at University of Reading in conjunction with Concurrent Solutions LLC in the USA, is developing a robotic weeder for field vegetables using image analysis to locate weed leaves and a novel Drop-on-Demand (DoD) applicator to apply droplets of herbicides to these leaves. No chemical is applied to the crop and none directly to the soil. Leaf-specific application of herbicide droplets is an alternative to selective chemistry or biotechnology while potentially reducing herbicide use. Although targeted micro-rates of herbicides have been studied, little is known about the exact rates needed to control weeds when microdoses are applied as one droplet to a single leaf or plant. In glasshouse trials, individual weed seedlings were controlled by applying a single droplet of herbicide and dose-response relationships were quantified. As a general recommendation, weeds that are up to the 4-leaf stage can be controlled with a dose of 32 μg of glyphosate and 28 μg of glufosinate-ammonium when they are applied as a single droplet per seedling. In order to answer the question if the efficacy is reproducible in the field, manually applied droplets of glyphosate and glufosinateammonium were made to the naturally occurring weed population in transplanted cabbage and leek crop. Droplet applications made on three and ten occasions after transplanting the cabbages and leeks, respectively reduced residual weed biomass at harvest by over 90% compared to the weedy control. Also, droplet treatments gave a crop yield, which did not differ significantly from the weed-free control. At the same time, the total amount of herbicide active ingredient applied was up to 82% and 94% lower than currents spraying methods for the leeks and cabbages, respectively. Because of the high value of the crop and the higher yields associated with ultraprecise droplet application, it would appear to be economical to apply these droplets using a robotic weeder. The applicator which was developed by Concurrent Solutions LLC in the USA for Drop-on-Demand droplet applications was tested under indoor conditions. The effect of pressure, distance from the target, wind direction and motion of the applicator was tested on the targeting accuracy of the applicator. Recommendations for future field applications suggested that the applicator should operate at 138 kPa pressure and set at 15 cm height from weeds.
title: ÐÐ´Ð°Ð½Ð¸Ðµ ÑÐºÐ»Ð°Ð´Ð° Ñ Ð°Ð´Ð¼Ð¸Ð½Ð¸ÑÑÑÐ°ÑÐ¸Ð²Ð½Ð¾-Ð±ÑÑÐ¾Ð²ÑÐ¼ ÐºÐ¾ÑÐ¿ÑÑÐ¾Ð¼. ÐÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ñ ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÑÑÐ²Ð°
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ°Ð²Ð»Ð¾Ð²ÑÐºÐ¸Ð¹, ÐÐ¸ÑÐ°Ð»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: 2016
Subjects: ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÑÑÐ²Ð¾
Ð³ÐµÐ½Ð¿Ð»Ð°Ð½
Ð¿ÑÐ¾Ð¼ÑÑÐ»ÐµÐ½Ð½Ð¾Ðµ Ð·Ð´Ð°Ð½Ð¸Ðµ

description: ÐÑÐ¾ÐµÐºÑ Ð¿Ð¾ÑÐ²ÑÑÐµÐ½ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸ ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÑÑÐ²Ð° Ð·Ð´Ð°Ð½Ð¸Ñ ÑÐºÐ»Ð°Ð´Ð° Ñ Ð°Ð´Ð¼Ð¸Ð½Ð¸ÑÑÑÐ°ÑÐ¸Ð²Ð½Ð¾-Ð±ÑÑÐ¾Ð²ÑÐ¼ ÐºÐ¾ÑÐ¿ÑÑÐ¾Ð¼. ÐÐ»Ð¾ÑÐ°Ð´ÐºÐ°, Ð¾ÑÐ²ÐµÐ´ÐµÐ½Ð½Ð°Ñ Ð¿Ð¾Ð´ ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÑÑÐ²Ð¾ ÑÐ°Ð·Ð¼ÐµÑÐµÐ½Ð° Ð² Ð¿Ð¾ÑÐµÐ»ÐºÐµ ÐÑÐ°ÑÐ½Ð°Ñ ÐÐ°ÑÑ, ÐÑÐµÐ²Ð¾Ð»Ð¾Ð¶ÑÐºÐ¾Ð³Ð¾ ÑÐ°Ð¹Ð¾Ð½Ð° ÐÐµÐ½Ð¸Ð½Ð³ÑÐ°Ð´ÑÐºÐ¾Ð¹ Ð¾Ð±Ð»Ð°ÑÑÐ¸. Ð Ð¿ÑÐ¾ÐµÐºÑÐµ Ð¿ÑÐ¸Ð²Ð¾Ð´ÑÑÑÑ ÑÐ²ÐµÐ´ÐµÐ½Ð¸Ñ Ð¾ Ð¿ÑÐ¸ÑÐ¾Ð´Ð½ÑÑ Ð¸ Ð¸Ð½Ð¶ÐµÐ½ÐµÑÐ½Ð¾-Ð³ÐµÐ¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ñ ÑÑÐ»Ð¾Ð²Ð¸ÑÑ Ð¿Ð»Ð¾ÑÐ°Ð´ÐºÐ¸. Ð Ð°ÑÑÐ¸ÑÐµÐºÑÑÑÐ½Ð¾-ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÐ½Ð¾Ð¼ ÑÐ°Ð·Ð´ÐµÐ»Ðµ ÑÐ°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÑÑÑÑ Ð°ÑÑÐ¸ÑÐµÐºÑÑÑÐ½ÑÐµ, Ð¾Ð±ÑÐµÐ¼Ð½Ð¾-Ð¿Ð»Ð°Ð½Ð¸ÑÐ¾Ð²Ð¾ÑÐ½ÑÐµ Ð¸ ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð²Ð½ÑÐµ ÑÐµÑÐµÐ½Ð¸Ñ. ÐÐµÑÑÑÐ¸Ðµ ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð¸ Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ñ Ð² ÑÐ¾ÑÐ¼Ðµ ÑÐµÑÑÑÐµÑÐ¿ÑÐ¾Ð»ÐµÑÐ½ÑÑ ÑÐ°Ð¼ Ð¿ÑÐ¾Ð»ÐµÑÐ¾Ð¼ 12,0 Ð¼ Ð¸ ÑÐ°Ð³Ð¾Ð¼ 12,0Ð¼ Ð¸Ð· Ð¼ÐµÑÐ°Ð»Ð»Ð¸ÑÐµÑÐºÐ¸Ñ ÐºÐ¾Ð»Ð¾Ð½Ð½ Ð¸ ÑÑÑÐ¾Ð¿Ð¸Ð»ÑÐ½ÑÑ ÑÐµÑÐ¼. Ð¤ÑÐ½Ð´Ð°Ð¼ÐµÐ½ÑÑ ÑÐ²Ð°Ð¹Ð½ÑÐµ Ñ Ð¶ÐµÐ»ÐµÐ·Ð¾Ð±ÐµÑÐ¾Ð½Ð½ÑÐ¼ ÑÐ¾ÑÑÐ²ÐµÑÐºÐ¾Ð¼. Ð Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÑÐ°ÑÑÐ¸ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½ ÐºÐ°Ð»ÐµÐ½Ð´Ð°ÑÐ½ÑÐ¹ Ð¿Ð»Ð°Ð½ Ð¸ ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÐ½ÑÐ¹ Ð³ÐµÐ½ÐµÑÐ°Ð»ÑÐ½ÑÐ¹ Ð¿Ð»Ð°Ð½. Ð¢Ð°ÐºÐ¶Ðµ Ð² ÑÐ°Ð±Ð¾ÑÐµ Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½ ÑÐ°Ð·Ð´ÐµÐ» Ð¾ÑÑÐ°Ð½Ñ Ð¾ÐºÑÑÐ¶Ð°ÑÑÐµÐ¹ ÑÑÐµÐ´Ñ.
Plausible constraints on the range of bulk terrestrial exoplanet compositions in the Solar neighbourhood
Creators: name: Spaargaren, Rob J.
name: Wang, Haiyang S.
name: Mojzsis, Stephen J
name: Ballmer, Maxim D
name: Tackley, Paul J
Publisher: name: arXiv
Year: 2022
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Rocky planet compositions regulate planetary evolution by affecting core sizes, mantle properties, and melting behaviours. Yet, quantitative treatments of this aspect of exoplanet studies remain generally under-explored. We attempt to constrain the range of potential bulk terrestrial exoplanet compositions in the solar neighbourhood (<200 pc). We circumscribe probable rocky exoplanet compositions based on a population analysis of stellar chemical abundances from the Hypatia and GALAH catalogues. We apply a devolatilization model to simulate compositions of hypothetical, terrestrial-type exoplanets in the habitable zones around Sun-like stars, considering elements O, S, Na, Si, Mg, Fe, Ni, Ca, and Al. We further apply core-mantle differentiation by assuming constant oxygen fugacity, and model the consequent mantle mineralogy with a Gibbs energy minimisation algorithm. We report statistics on several compositional parameters and propose a reference set of (21) representative planet compositions for using as end-member compositions in imminent modelling and experimental studies. We find a strong correlation between stellar Fe/Mg and metallic core sizes, which can vary from 18 to 35 wt%. Furthermore, stellar Mg/Si gives a first-order indication of mantle mineralogy, with high-Mg/Si stars leading to weaker, ferropericlase-rich mantles, and low-Mg/Si stars leading to mechanically stronger mantles. The element Na, which modulates crustal buoyancy and mantle clinopyroxene fraction, is affected by devolatilization the most. While we find that planetary mantles mostly consist of Fe/Mg-silicates, core sizes and relative abundances of common minerals can nevertheless vary significantly among exoplanets. These differences likely lead to different evolutionary pathways among rocky exoplanets in the solar neighbourhood.
description: Accepted by the Astrophysical Journal
The Lagrangian and Hamiltonian formalisms for the classical relativistic electrodynamics models revisited
Creators: name: Bogolubov, N. N.
name: Prykarpatsky, A. K.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Mathematical Physics (math-ph)
subject: FOS: Physical sciences
subject: pacs 11.10.Ef

description: The work is devoted to studying some new classical electrodynamics models of interacting charged point particles and the aspects of the quantization via the Dirac procedure related to them. Based on the vacuum field theory no-geometry approach developed in [6,7,9], the Lagrangian and Hamiltonian reformulations of some alternative classical electrodynamics models are devised. The Dirac-type quantization procedure for the considered alternative electrodynamics models, based on the obtained canonical Hamiltonian formulations, is developed.
description: 9 pages
Swelling-induced pattern transformations of periodic hydrogels -- from the wrinkling of internal surfaces to the buckling of thin films
Creators: name: Polukhov, Elten
name: Pytel, Laura
name: Keip, Marc-Andre
Publisher: name: arXiv
Year: 2022
Subjects: subject: Numerical Analysis (math.NA)
subject: FOS: Mathematics

description: We investigate pattern transformations of periodic hydrogel systems that are triggered by swelling-induced structural instabilities. The types of microstructures considered in the present work include single-phase and two-phase voided hydrogel structures as well as reinforced hydrogel thin films. While the observed transformations of the single-phase structures show good agreement with experimental findings, the two-phase materials provide novel patterns associated with wrinkling of internal surfaces. Furthermore, an extensive parametric study on the reinforced hydrogel thin films reveals new opportunities for the design of complex out-of-plane surface modes caused by swelling-induced instabilities. Next to the mentioned buckling-type instabilities, we encountered the development of micro-creases at the internal surfaces of periodic media before the loss of strong ellipticity of effective moduli.
Additional file 2 of Single-cell RNA sequencing reveals enhanced antitumor immunity after combined application of PD-1 inhibitor and Shenmai injection in non-small cell lung cancer
Creators: name: Yu, Dingyi
name: Yang, Penghui
name: Lu, Xiaoyan
name: Huang, Shaoze
name: Liu, Li
name: Fan, Xiaohui
Publisher: name: figshare
Year: 2023
Subjects: subject: Immunology
subject: FOS: Clinical medicine

description: Additional file 2: Table S1 The representative marker genes of eight cell types. Table S2 Biological pathways analysis using Metascape analysis. Table S3 Top ten TFs in the tumor subclusters. Table S4 The representative marker genes of T and NK cell subclusters.
title: ÐÐ°ÐºÐ¾Ð½Ñ ÑÐµÑÐ¼Ð¾Ð´Ð¸Ð½Ð°Ð¼Ð¸ÐºÐ¸ Ð¸ ÑÐ¸ÐºÐ»Ñ ÑÐµÐ¿Ð»Ð¾ÑÐ½ÐµÑÐ³ÐµÑÐ¸ÑÐµÑÐºÐ¸Ñ ÑÑÑÐ°Ð½Ð¾Ð²Ð¾Ðº Ð¸ Ð´Ð²Ð¸Ð³Ð°ÑÐµÐ»ÐµÐ¹
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ
titleType: Subtitle
Creators: name: ÐÑÑÐµÐ½ÐºÐ¾, ÐÐµÑÐ¼Ð°Ð½
Publisher: name: ÐÐÐÐ°Ñ
Year: 2006
Subjects: Ð¢ÐµÐ¿Ð»Ð¾ÑÐ½ÐµÑÐ³ÐµÑÐ¸ÑÐµÑÐºÐ¸Ðµ ÑÑÑÐ°Ð½Ð¾Ð²ÐºÐ¸

description: ÐÐ·Ð»Ð¾Ð¶ÐµÐ½Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ ÑÐ¸Ð·Ð¸ÑÐµÑÐºÐ¸Ðµ Ð¿Ð¾Ð½ÑÑÐ¸Ñ, Ð¿ÑÐ¸Ð²ÐµÐ´ÐµÐ½Ñ Ð¿ÐµÑÐ²ÑÐ¹ Ð¸ Ð²ÑÐ¾ÑÐ¾Ð¹ Ð·Ð°ÐºÐ¾Ð½Ñ ÑÐµÑÐ¼Ð¾Ð´Ð¸Ð½Ð°Ð¼Ð¸ÐºÐ¸, ÑÐ°Ð·Ð¾Ð²ÑÐµ Ð¿ÐµÑÐµÑÐ¾Ð´Ñ. Ð Ð°ÑÑÐ¼Ð¾ÑÑÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ ÑÐ¸ÐºÐ»Ð¾Ð² ÑÐµÐ¿Ð»Ð¾ÑÐ½ÐµÑÐ³Ð¾ÑÑÑÐ°Ð½Ð¾Ð²Ð¾Ðº. Ð Ð°ÑÐºÑÑÑÐ° ÑÐµÑÐ¼Ð¾Ð´Ð¸Ð½Ð°Ð¼Ð¸ÑÐµÑÐºÐ°Ñ ÑÑÑÐ½Ð¾ÑÑÑ Ð¿ÑÐ¾ÑÐµÑÑÐ° Ð¿Ð°ÑÐ¾Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¿ÑÐ¸ Ð¿Ð¾ÑÑÐ¾ÑÐ½Ð½Ð¾Ð¼ Ð´Ð°Ð²Ð»ÐµÐ½Ð¸Ð¸. Ð£Ð´ÐµÐ»ÐµÐ½Ð¾ Ð²Ð½Ð¸Ð¼Ð°Ð½Ð¸Ðµ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÑÐ¸Ñ Ð·Ð°ÐºÐ¾Ð½Ð¾Ð² Ð´Ð»Ñ Ð°Ð½Ð°Ð»Ð¸Ð·Ð° Ð¸ ÑÐ°ÑÑÐµÑÐ° ÑÐ¸ÐºÐ»Ð¾Ð² Ð¿Ð¾ÑÑÐ½ÐµÐ²ÑÑ ÑÐµÐ¿Ð»Ð¾Ð²ÑÑ Ð´Ð²Ð¸Ð³Ð°ÑÐµÐ»ÐµÐ¹ Ð¸ ÐºÐ¾Ð¼Ð¿ÑÐµÑÑÐ¾ÑÐ¾Ð², Ð³Ð°Ð·Ð¾ÑÑÑÐ±Ð¸Ð½Ð½ÑÑ ÑÑÑÐ°Ð½Ð¾Ð²Ð¾Ðº, Ð° ÑÐ°ÐºÐ¶Ðµ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ ÑÐ¸ÐºÐ»Ñ Ð¿Ð°ÑÐ¾ÑÑÑÐ±Ð¸Ð½Ð½ÑÑ ÑÑÑÐ°Ð½Ð¾Ð²Ð¾Ðº. ÐÐ°ÑÐµÑÐ¸Ð°Ð» Ð¸Ð·Ð»Ð¾Ð¶ÐµÐ½ Ñ Ð°ÐºÑÐµÐ½ÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸ÐµÐ¼ Ð½Ð° Ð¿ÐµÑÑÐ¿ÐµÐºÑÐ¸Ð²Ñ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ ÑÑÐ°ÑÐ¸Ð¾Ð½Ð°ÑÐ½Ð¾Ð³Ð¾ ÑÐµÐ¿Ð»Ð¾ÑÐ½ÐµÑÐ³ÐµÑÐ¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¾Ð±Ð¾ÑÑÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ, Ð¿ÑÐ¸Ð²ÐµÐ´ÐµÐ½Ñ Ð´Ð¾ÑÑÐ¸Ð³Ð½ÑÑÑÐµ Ð½Ð°ÑÐ°Ð»ÑÐ½ÑÐµ Ð¿Ð°ÑÐ°Ð¼ÐµÑÑÑ ÑÐ°Ð±Ð¾ÑÐµÐ³Ð¾ ÑÐµÐ»Ð° Ð² ÑÐ°Ð·Ð»Ð¸ÑÐ½ÑÑ ÑÐµÐ¿Ð»Ð¾Ð²ÑÑ Ð´Ð²Ð¸Ð³Ð°ÑÐµÐ»ÑÑ, Ð¿Ð¾Ð»ÑÑÐµÐ½Ð½ÑÐµ ÐÐÐ Ð¸ Ð¿ÐµÑÑÐ¿ÐµÐºÑÐ¸Ð²Ñ Ð¸Ñ ÑÐ²ÐµÐ»Ð¸ÑÐµÐ½Ð¸Ñ. ÐÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¾ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² Ð¸ Ð°ÑÐ¿Ð¸ÑÐ°Ð½ÑÐ¾Ð² Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¾Ð³Ð¾ Ð¸Ð½ÑÑÐ¸ÑÑÑÐ° Ð¼Ð°ÑÐ¸Ð½Ð¾ÑÑÑÐ¾ÐµÐ½Ð¸Ñ (ÐÐÐ-ÐÐ¢Ð£Ð).
The Giant Accreting Protoplanet Survey (GAPlanetS) -- Results from a Six Year Campaign to Image Accreting Protoplanets
Creators: name: Follette, Katherine B.
name: Close, Laird M.
name: Males, Jared R.
name: Ward-Duong, Kimberly
name: Balmer, William O.
name: Redai, Jea Adams
name: Morales, Julio
name: Sarosi, Catherine
name: Dacus, Beck
name: De Rosa, Robert J.
name: Toro, Fernando Garcia
name: Leonard, Clare
name: Macintosh, Bruce
name: Morzinski, Katie M.
name: Mullen, Wyatt
name: Palmo, Joseph
name: Saitoti, Raymond Nzaba
name: Spiro, Elijah
name: Treiber, Helena
name: Wang, Jason
name: Wang, David
name: Watson, Alex
name: Weinberger, Alycia J.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: FOS: Physical sciences

description: Accreting protoplanets represent a window into planet formation processes. We report Hα differential imaging results from the deepest and most comprehensive accreting protoplanet survey to date, acquired with the Magellan Adaptive Optics (MagAO) system's VisAO camera. The fourteen transitional disks targeted are ideal candidates for protoplanet discovery due to their wide, heavily depleted central cavities, wealth of non-axisymmetric circumstellar disk features evocative of ongoing planet formation, and ongoing stellar accretion. To address the twin challenges of morphological complexity in the target systems and PSF instability, we develop novel approaches for frame selection and optimization of the Karhounen-Loeve Image Processing algorithm pyKLIP. We detect one new candidate protoplanet, CS Cha "c", at a separation of 75mas and a Delta mag of 5.1 and robustly recover the HD142527 B and HD100453 B low mass stellar companions across multiple epochs. Though we cannot rule out a substantial scattered light contribution to its emission, we also recover LkCa 15 b. Its presence inside of the cleared disk cavity and consistency with a forward-modeled point source suggest that it remains a viable protoplanet candidate. The protoplanet PDS 70 c was marginally recovered under our conservative general methodology. However, through targeted optimization in H-alpha} imagery, we tentatively recover PDS 70 c in three epochs and PDS 70 b in one epoch. Of the many other previously-reported companions and companion candidates around objects in the sample, we do not recover any additional robust candidates. However, lack of recovery at moderate H-alpha contrast does not rule out the presence of protoplanets at these locations, and we report limiting H-alpha contrasts in such cases.
description: Final version, in press at AJ
Divergent stiffness of one-dimensional growing interfaces
Creators: name: Minoguchi, Mutsumi
name: Sasa, Shin-ichi
Publisher: name: arXiv
Year: 2022
Subjects: subject: Statistical Mechanics (cond-mat.stat-mech)
subject: Classical Physics (physics.class-ph)
subject: FOS: Physical sciences

description: When a spatially localized stress is applied to a growing one-dimensional interface, the interface deforms. This deformation is described by the effective surface tension representing the stiffness of the interface. We present that the stiffness exhibits divergent behavior in the large system size limit for a growing interface with thermal noise, which has never been observed for equilibrium interfaces. Furthermore, by connecting the effective surface tension with a space-time correlation function, we elucidate the mechanism that anomalous dynamical fluctuations lead to divergent stiffness.
description: 6 pages, 4 figures (Supplemental Material: 11 pages, 8 figures)
The Bardeen-Petterson Effect as an Observable Support for the Blanford-Payne Process Black Hole Jet Production
Creators: name: Jang, Uicheol
name: Kim, Hongsu
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: Relativistic jets are observed around accreting black holes, from stellar mass to super massive black holes. But Its origin has not been fully understood. Although Blanford-Payne process has been considered as most reliable theory of jet production It has no observational proof or supports. In this problem, We suggested the way to display that Bardeen-Petterson effect can become a supporter as providing observational idea of Blanford-Payne process. And we studied black hole jet production by Blanford-Payne process and Bardeen-Peterson effect. As a result, we could calculate observable timescale of black hole jet preccetion
Exact-Diagonalization Studies of Inelastic Light Scattering in Self-Assembled Quantum Dots
Creators: name: Delgado, Alain
name: Dominguez, Adriel
name: Perez, Ricardo
name: Lockwood, D. J.
name: Gonzalez, Augusto
Publisher: name: arXiv
Year: 2008
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: We report exact diagonalization studies of inelastic light scattering in few-electron quantum dots under the strong confinement regime characteristic of self-assembled dots. We apply the orthodox (second-order) theory for scattering due to electronic excitations, leaving for the future the consideration of higher-order effects in the formalism (phonons, for example), which seem relevant in the theoretical description of available experiments. Our numerical results stress the dominance of monopole peaks in Raman spectra and the breakdown of selection rules in open-shell dots. The dependence of these spectra on the number of electrons in the dot and the incident photon energy is explicitly shown. Qualitative comparisons are made with recent experimental results.
description: 11 pages, 11 figures