cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
FHIR PIT: a geospatial and spatiotemporal data integration pipeline to support subject-level clinical research
Creators: name: Roupe, Griffin
name: Krishnamurthy, Ashok
name: Fecho, Karamarie
name: Yi, Hong
name: Garcia, Juan J.
Publisher: name: Springer Nature
Year: 2025

description:
Background Environmental exposures such as airborne pollutant exposures and socio-economic indicators are increasingly recognized as important to consider when conducting clinical research using electronic health record (EHR) data or other sources of clinical data such as survey data. While numerous public sources of geospatial and spatiotemporal data are available to support such research, the data are challenging to work with due to inconsistencies in file formats and spatiotemporal resolutions, computational challenges with large file sizes, and a lack of tools for patient- or subject-level data integration. Results We developed FHIR PIT (HL7® Fast Healthcare Interoperability Resources Patient data Integration Tool) as an open-source, modular, data-integration software pipeline that consumes EHR data in FHIR® format and integrates the data at the level of the patient or subject with environmental exposures data of varying spatiotemporal resolutions and file formats. We applied FHIR PIT to generate “integrated feature tables” containing patient- or subject-level EHR data integrated with environmental exposures data on two cohorts: one on patients with asthma and related common pulmonary disorders; and a second on patients with primary ciliary dyskinesia and related rare pulmonary disorders. The data were then exposed via the open Integrated Clinical and Environmental Exposures Service, which was then queried to explore relationships between exposures to two representative airborne pollutants (particulate matter and ozone) and annual emergency department or inpatient visits for respiratory issues. We found that hospitalizations for respiratory issues were more common among patients exposed to relatively high levels of particulate matter and ozone and were higher overall among patients with primary ciliary dyskinesia than among patients with asthma. Conclusions Our manuscript describes a major release of FHIR PIT v1.0 and includes a technical demonstration use case and a clinical application on the use of FHIR PIT to support research on environmental exposures and health outcomes related to asthma and primary ciliary dyskinesia. For application of the tool to common data models (CDMs) other than FHIR, we offer open-source conversion tools to map from the PCORnet, i2b2, and OMOP CDMs to FHIR.
Using Concept Maps for Nursing Education in Iran: A Systematic Review
Creators: name: Ghojazadeh, Morteza
name: Aghaei, Mir Hossein
name: Naghavi-Behzad, Mohammad
name: Piri, Reza
name: Hazrati, Hakimeh
name: Azami-Aghdash, Saber
Publisher: name: Tabriz University of Medical Sciences
Year: 2014
Subjects: subject: 610 Medical sciences; Medicine

description: Introduction: Considering the importance, complexity, and problems in nursing education, using efficient and new methods in nursing education seems to be necessary. One of the most important of these methods which has received attention in recent years is the use of concept maps. Therefore, the aim of this study was systematic review of studies conducted in this field. Methods: Required information for this systematic review study was collected using keywords of concept map, learning, retention, nursing education, critical thinking skill, and Iran and their English synonyms in data bases of Iranmedex, Magiran, Science Direct, PubMed, Google scholar, Medlib, and SID. No time limitation was considered for searching articles. Articles published in Farsi and English have been searched. Results: Results show that concept maps have a significant effect on improving critical thinking of learners. Compared to other educational methods such as lectures; using concept maps show higher efficiency in deep and meaningful learning. Besides, concept maps have a significant effect on learning (relationship of theory and practice, improvement of clinical experiences, organizing concepts, and self-regulation). Conclusion: According to the importance of nursing education and its available problems on one hand, and the use and applicability of concept maps on the other hand (as well as ignorance about this educational method), it seems necessary to plan for the development of using concept maps in educational nursing.
description: Research and Development in Medical Education; EISSN 2322-2719
The Bibliometric Properties of Article Readership Information
Creators: name: Kurtz, Michael J.
name: Eichhorn, Guenther
name: Accomazzi, Alberto
name: Grant, Carolyn S.
name: Demleitner, Markus
name: Murray, Stephen S.
name: Martimbeau, Nathalie
name: Elwell, Barbara
Publisher: name: arXiv
Year: 2009
Subjects: subject: Digital Libraries (cs.DL)
subject: Physics and Society (physics.soc-ph)
subject: FOS: Computer and information sciences
subject: FOS: Physical sciences

description: The NASA Astrophysics Data System (ADS), along with astronomy's journals and data centers (a collaboration dubbed URANIA), has developed a distributed on-line digital library which has become the dominant means by which astronomers search, access and read their technical literature. Digital libraries such as the NASA Astrophysics Data System permit the easy accumulation of a new type of bibliometric measure, the number of electronic accesses (``reads'') of individual articles. We explore various aspects of this new measure. We examine the obsolescence function as measured by actual reads, and show that it can be well fit by the sum of four exponentials with very different time constants. We compare the obsolescence function as measured by readership with the obsolescence function as measured by citations. We find that the citation function is proportional to the sum of two of the components of the readership function. This proves that the normative theory of citation is true in the mean. We further examine in detail the similarities and differences between the citation rate, the readership rate and the total citations for individual articles, and discuss some of the causes. Using the number of reads as a bibliometric measure for individuals, we introduce the read-cite diagram to provide a two-dimensional view of an individual's scientific productivity. We develop a simple model to account for an individual's reads and cites and use it to show that the position of a person in the read-cite diagram is a function of age, innate productivity, and work history. We show the age biases of both reads and cites, and develop two new bibliometric measures which have substantially less age bias than citations
description: ADS bibcode: 2005JASIS..56..111K This is the second paper (the first is Worldwide Use and Impact of the NASA Astrophysics Data System Digital Library) from the original article The NASA Astrophysics Data System: Sociology, Bibliometrics, and Impact, which went on-line in the summer of 2003
Bowline on a Bight : Doing Right by the Records of Lilian Bland
Creators: name: Malek, Claire
Publisher: name: The University of British Columbia
Year: 2022

description: Focusing on a case study that has at its axis myself and the records of Lilian Bland, I explore person-centred archival theory by engaging primarily with what Sara Ahmed conceptualizes as queer use. I draw on recent archival literature on love and grief, queer theory, feminist theory, anti-colonial methods, and new materialism to propose a radical somatics of critical archival love. I situate my knowledge and power within discourses of social justice, healing, liberatory memory work, and gender and sexuality to reflect on what it means to “do right”: to act ethically and with care toward ourselves and the myriad others we encounter in archival practice, and to be of use to one another.
title: ÐÐ°ÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½Ð¾âÐºÑÐ»ÑÑÑÑÐ½ÑÐµ Ð¾ÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÐ¸ Ð¿Ð¾ÑÐ»Ð¾Ð²Ð¸Ñ Ð¾ Ð¶ÐµÐ½ÑÐ¸Ð½Ð°Ñ Ð² Ð°Ð½Ð³Ð»Ð¸Ð¹ÑÐºÐ¾Ð¼, ÑÑÑÑÐºÐ¾Ð¼ Ð¸ ÑÐ°Ð´Ð¶Ð¸ÐºÑÐºÐ¾Ð¼ ÑÐ·ÑÐºÐ°Ñ (ÑÐ¾Ð¿Ð¾ÑÑÐ°Ð²Ð¸ÑÐµÐ»ÑÐ½ÑÐ¹ Ð°Ð½Ð°Ð»Ð¸Ð·)
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: Ð£ÑÐ¼Ð°Ð½Ð¾Ð²Ð°, ÐÐ¸Ð»Ð°ÑÑ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: 2016
Subjects: Ð¿Ð¾ÑÐ»Ð¾Ð²Ð¸ÑÑ
Ð»Ð¸Ð½Ð³Ð²Ð¾ÐºÑÐ»ÑÑÑÑÐ°
ÑÐ¾Ð»ÑÐºÐ»Ð¾Ñ
Ð½Ð°ÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½Ð¾-ÐºÑÐ»ÑÑÑÑÐ½ÑÐµ Ð¾ÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÐ¸
Ð³ÐµÐ½Ð´ÐµÑÐ½ÑÐµ ÑÑÐµÑÐµÐ¾ÑÐ¸Ð¿Ñ
proverbs
lingo-culture
national and cultural features
gender stereotypes

description: Ð Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ ÑÐ°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÐµÑÑÑ Ð½Ð°ÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½Ð¾ - ÐºÑÐ»ÑÑÑÑÐ½ÑÐµ Ð¾ÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÐ¸ Ð¿Ð¾ÑÐ»Ð¾Ð²Ð¸Ñ Ð¾ Ð¶ÐµÐ½ÑÐ¸Ð½Ð°Ñ Ð² Ð°Ð½Ð³Ð»Ð¸Ð¹ÑÐºÐ¾Ð¼, ÑÑÑÑÐºÐ¾Ð¼ Ð¸ ÑÐ°Ð´Ð¶Ð¸ÐºÑÐºÐ¾Ð¼ ÑÐ·ÑÐºÐ°Ñ. ÐÐºÑÑÐ°Ð»ÑÐ½Ð¾ÑÑÑ ÑÐµÐ¼Ñ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÑÐµÑÑÑ Ð½ÐµÐ¾Ð±ÑÐ¾Ð´Ð¸Ð¼Ð¾ÑÑÑÑ Ð²ÑÑÐ²Ð»ÐµÐ½Ð¸Ñ Ð¾Ð±ÑÐµÐ³Ð¾ Ð¸ ÑÐ¿ÐµÑÐ¸ÑÐ¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð² Ð¿Ð¾ÑÐ»Ð¾Ð²Ð¸ÑÐ°Ñ Ð½Ð° Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ðµ Ð°Ð½Ð³Ð»Ð¸Ð¹ÑÐºÐ¾Ð³Ð¾, ÑÑÑÑÐºÐ¾Ð³Ð¾ Ð¸ ÑÐ°Ð´Ð¶Ð¸ÐºÑÐºÐ¾Ð³Ð¾ ÑÐ·ÑÐºÐ¾Ð². ÐÐ°ÑÐµÑÐ¸Ð°Ð»Ð¾Ð¼ Ð´Ð»Ñ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¿Ð¾ÑÐ»ÑÐ¶Ð¸Ð»Ð¸ Ð»ÐµÐºÑÐ¸ÐºÐ¾Ð³ÑÐ°ÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð¸ÑÑÐ¾ÑÐ½Ð¸ÐºÐ¸ Ð¸ ÐÐ½ÑÐµÑÐ½ÐµÑ - ÑÐµÑÑÑÑÑ. Ð ÑÐ°Ð±Ð¾ÑÐµ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð»Ð¸ÑÑ Ð¿Ð¾ÑÐ»ÐµÐ´Ð½Ð¸Ðµ Ð´Ð¾ÑÑÐ¸Ð¶ÐµÐ½Ð¸Ñ Ð¾ÑÐµÑÐµÑÑÐ²ÐµÐ½Ð½Ð¾Ð¹ Ð¸ Ð·Ð°ÑÑÐ±ÐµÐ¶Ð½Ð¾Ð¹ Ð»Ð¸Ð½Ð³Ð²Ð¸ÑÑÐ¸ÐºÐ¸ Ð¸ Ð»Ð¸ÑÐµÑÐ°ÑÑÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¸Ñ. Ð¦ÐµÐ»ÑÑ Ð´Ð°Ð½Ð½Ð¾Ð³Ð¾ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ²Ð»ÑÐµÑÑÑ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ð¸Ðµ ÑÐ¾Ð»Ð¸ Ð¸ Ð²Ð¾ÑÐ¿ÑÐ¸ÑÑÐ¸Ðµ Ð¶ÐµÐ½ÑÐ¸Ð½Ñ Ñ Ð¿Ð¾Ð¼Ð¾ÑÑÑ Ð¿Ð¾ÑÐ»Ð¾Ð²Ð¸Ñ Ð² Ð°Ð½Ð³Ð»Ð¸Ð¹ÑÐºÐ¾Ð¹, ÑÑÑÑÐºÐ¾Ð¹ Ð¸ ÑÐ°Ð´Ð¶Ð¸ÐºÑÐºÐ¾Ð¹ ÐºÑÐ»ÑÑÑÑÐ°Ñ.
description: This diploma paper describes ethnic and cultural features of proverbs about women in English, Russian and Tajik languages. The rationale of the research is determined by the necessity to identify general and specific in proverbs of English, Russian and Tajik languages. Lexicographical sources and the Internet - resources were used for the research. We used the latest achievements of native and foreign linguistics and literary studies. The aim of the research is to examine the role and perception of women by using proverbs in English, Russian and Tajik cultures.
Polynomial tau-functions of the symplectic KP, orthogonal KP and BUC hierarchies
Creators: name: Li, Denghui
name: Yan, Zhaowen
Publisher: name: arXiv
Year: 2022
Subjects: subject: Exactly Solvable and Integrable Systems (nlin.SI)
subject: Mathematical Physics (math-ph)
subject: FOS: Physical sciences

description: This paper is concerned with the construction of the polynomial tau-functions of the symplectic KP (SKP), orthogonal KP (OKP) hierarchies and universal character hierarchy of B-type (BUC hierarchy), which are proved as zero modes of certain combinations of the generating functions. By applying the strategy of carrying out the action of the quantum fields on vacuum vector, the generating functions for symplectic Schur function, orthogonal Schur function and generalized Q-function have been presented. The remarkable feature is that polynomial tau-functions are the coefficients of certain family of generating functions. Furthermore, in terms of the Vandermonde-like identity and properties of Pfaffian, it is showed that the polynomial tau-functions of the SKP, OKP and BUC hierarchies canbe written as determinant and Pfaffian forms, respectively. In addition, the soliton solutions of the SKP and OKP hierarchies have been discussed.
Including All the Lines
Creators: name: Kurucz, Robert L.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: I present a progress report on including all the lines in the linelists, including all the lines in the opacities, including all the lines in the model atmosphere and spectrum synthesis calculations, producing high-resolution, high-signal-to-noise atlases that show (not quite) all the lines, so that finally we can determine the properties of stars from a few of the lines.
description: 9 pages, no figures. Presented at "Dimitrifest" conference in Boulder, Colorado, March 30 - April 3, 2009
title: ÐÑÐ½Ð¾Ð²Ð½ÑÐµ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ ÑÐ¾ÑÑÑÐ´Ð½Ð¸ÑÐµÑÑÐ²Ð° Ð¼ÐµÐ¶Ð´Ñ Ð Ð¾ÑÑÐ¸Ð¹ÑÐºÐ¾Ð¹ Ð¤ÐµÐ´ÐµÑÐ°ÑÐ¸ÐµÐ¹ Ð¸ ÑÑÑÐ°Ð½Ð°Ð¼Ð¸ ÐÐ°Ð¿Ð°Ð´Ð½Ð¾Ð¹ ÐÑÑÐ¸ÐºÐ¸ Ñ ÐºÐ¾Ð½ÑÐ° XX Ð²ÐµÐºÐ° - Ð½Ð°ÑÐ°Ð»Ð° XXI Ð²ÐµÐºÐ°
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name:  ÐÐ°Ð¿Ð¿Ð¾ ÐÐ¾Ð»Ð¸Ð½ ÐÐ°Ð°-ÐÐ´Ð¾Ð»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: 2017
Subjects: Ð´Ð²ÑÑÑÐ¾ÑÐ¾Ð½Ð½ÐµÐµ Ð¾ÑÐ½Ð¾ÑÐµÐ½Ð¸Ðµ
ÑÐµÐ³Ð¸Ð¾Ð½Ð°Ð»ÑÐ½ÑÐ¹
Ð¿Ð¾ÑÑÐºÐ¾Ð»Ð¾Ð½Ð¸Ð°Ð»ÑÐ½ÑÐ¹

description: Ð Ð´Ð¸Ð¿Ð»Ð¾Ð¼Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ Ð¿Ð¾Ð´ÑÐµÑÐºÐ¸Ð²Ð°ÐµÑÑÑ Ð¿Ð¾ÑÑÐµÐ¿ÐµÐ½Ð½Ð¾Ðµ ÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ ÑÐµÐ³Ð¸Ð¾Ð½Ð°Ð»ÑÐ½ÑÑ Ð¸ Ð´Ð²ÑÑÑÐ¾ÑÐ¾Ð½Ð½Ð¸Ñ Ð¾ÑÐ½Ð¾ÑÐµÐ½Ð¸Ð¹ Ð¼ÐµÐ¶Ð´Ñ Ð Ð¾ÑÑÐ¸ÐµÐ¹ (Ð¸ Ð±ÑÐ²ÑÐ¸Ð¼ Ð¡Ð¾Ð²ÐµÑÑÐºÐ¸Ð¼ Ð¡Ð¾ÑÐ·Ð¾Ð¼) Ð¸ Ð¿Ð¾ÑÑÐºÐ¾Ð»Ð¾Ð½Ð¸Ð°Ð»ÑÐ½ÑÐ¼Ð¸ Ð·Ð°Ð¿Ð°Ð´Ð½Ð¾Ð°ÑÑÐ¸ÐºÐ°Ð½ÑÐºÐ¸Ð¼Ð¸ Ð³Ð¾ÑÑÐ´Ð°ÑÑÑÐ²Ð°Ð¼Ð¸. Ð­ÑÐ¸ Ð´Ð²ÑÑÑÐ¾ÑÐ¾Ð½Ð½Ð¸Ðµ Ð¾ÑÐ½Ð¾ÑÐµÐ½Ð¸Ñ Ð¿Ð¾ÑÐ¾Ð´Ð¸Ð»Ð¸ ÑÐ°Ð·Ð»Ð¸ÑÐ½ÑÐµ ÑÑÐµÑÑ ÑÐ¾ÑÑÑÐ´Ð½Ð¸ÑÐµÑÑÐ²Ð° Ð² Ð¾Ð±Ð»Ð°ÑÑÐ¸ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÐºÐ¸, ÑÐ¾ÑÐ³Ð¾Ð²Ð»Ð¸, Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ñ, ÐºÑÐ»ÑÑÑÑÑ Ð¸ Ð´ÑÑÐ³Ð¸Ñ. Ð ÑÐ°Ð±Ð¾ÑÐµ ÑÐ°ÑÐºÑÑÐ²Ð°ÐµÑ ÑÐµÑÑÑÐµ ÐºÐ»ÑÑÐµÐ²ÑÑ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ ÑÐ¾ÑÑÑÐ´Ð½Ð¸ÑÐµÑÑÐ²Ð°, Ð° ÑÐ°ÐºÐ¶Ðµ Ð¿ÐµÑÑÐ¿ÐµÐºÑÐ¸Ð²Ð½ÑÐµ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¿Ð°ÑÑÐ½ÐµÑÑÑÐ²Ð° Ð² Ð±Ð»Ð¸Ð¶Ð°Ð¹ÑÐµÐ¼ Ð±ÑÐ´ÑÑÐµÐ¼.
Self-interacting fundamental strings and black holes
Creators: name: Chialva, Diego
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: We study the size distribution of very massive close string states and the typical string configuration as one slowly increase the string coupling, both in the case of zero and of non-zero Neveu-Schwarz charges. The computations are performed rigorously in string theory, starting from quantities that are well-defined in the theory and therefore clarify previous works on the subject which were based on various approximation techniques. We find that, starting from a value of the coupling in agreement with the one predicted by the black hole correspondence principle, the string ensemble is dominated in any dimensions by compact states whose size is within the correspondent black hole horizon radius, which is of the order of the string scale at the black hole/string transition point.
description: 31 pages plus references, final version accepted for publication
Dark Photons and Displaced Vertices at the MUonE Experiment
Creators: name: Galon, Iftah
name: Shih, David
name: Wang, Isaac R.
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: MUonE is a proposed experiment designed to measure the hadronic vacuum polarization contribution to muon $g-2$ through elastic $μ-e$ scattering. As such it employs an extremely high-resolution tracking apparatus. We point out that this makes MUonE also a very promising experiment to search for displaced vertices from light, weakly-interacting new particles. We demonstrate its potential by showing how it has excellent sensitivity to dark photons in the mass range $10~\mathrm{MeV} \le m_{A'} \le 100~\mathrm{MeV}$ and kinetic mixing parameter $10^{-5} \le εe \le 10^{-3}$, through the process $μ^{\pm}\, e^- \to μ^{\pm}\, e^-\, A'$ followed by $A'\to e^+e^-$.
description: PRD version, 10 pages, 5 figures
Simulating plasma instabilities in SU(3) gauge theory
Creators: name: Berges, J.
name: Gelfand, D.
name: Scheffler, S.
name: Sexty, D.
Publisher: name: arXiv
Year: 2008
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Lattice (hep-lat)
subject: High Energy Physics - Theory (hep-th)
subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: We compute nonequilibrium dynamics of plasma instabilities in classical-statistical lattice gauge theory in 3+1 dimensions. The simulations are done for the first time for the SU(3) gauge group relevant for quantum chromodynamics. We find a qualitatively similar behavior as compared to earlier investigations in SU(2) gauge theory. The characteristic growth rates are about 25 % lower for given energy density, such that the isotropization process is slower. Measured in units of the characteristic screening mass, the primary growth rate is independent of the number of colors.
description: 11 pages, 5 figures. Version accepted for publication in Physics Letters B, minor changes
Development assistance for UHC through health systems strengthening and health security
Creators: name: Kraus, Jessica
Publisher: name: Open Science Framework
Year: 2022
Subjects: subject: Public Health
subject: Medicine and Health Sciences
subject: Public Affairs, Public Policy and Public Administration
subject: Social and Behavioral Sciences
subject: Development assistance for health
subject: Health security
subject: Health systems strengthening
subject: Pandemic preparedness
subject: Universal health coverage

description: Measuring development assistance for health systems strengthening and health security: an analysis using the Creditor Reporting System database
title: ÐÐºÑÑÐ°Ð»ÑÐ½ÑÐµ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ñ Ð¿Ð¾ ÑÐ¾Ñ ÑÐ°Ð½ÐµÐ½Ð¸Ñ ÑÑÐ°Ð´Ð¸ÑÐ¸Ð¹ ÑÑÐ°ÑÐ¸Ð½Ð½Ð¾Ð¹ Ð¿ÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¾Ð¹ ÐºÑÑ Ð½Ð¸ Ð¸ Ð¿ÑÑÐ¸ Ð¸Ñ ÑÐµÑÐµÐ½Ð¸Ñ
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¸ÑÐ¸Ð½Ð°, ÐÑÐµÐ½Ð¸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¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³, Ð³Ð¾ÑÐ¾Ð´
ÐºÑÐ»Ð¸Ð½Ð°ÑÐ¸Ñ
ÐºÐ°ÑÑÐ¾ÑÐµÐºÐ° Ð±Ð»ÑÐ´
Ð¸Ð½Ð½Ð¾Ð²Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾Ðµ Ð¾Ð±Ð¾ÑÑÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ
ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ðµ ÑÐ²Ð¾Ð¹ÑÑÐ²Ð°

description: Ð ÑÐ°Ð±Ð¾ÑÐµ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð° Ð¸ÑÑÐ¾ÑÐ¸ÑÐµÑÐºÐ°Ñ Ð¿ÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ°Ñ ÐºÑÑÐ½Ñ Ð¸ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ñ, Ð²Ð¾Ð·Ð½Ð¸ÐºÐ°ÑÑÐ¸Ðµ Ð¿ÑÐ¸ ÐµÐµ ÑÐµÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð¸: Ð¿Ð¾Ð½ÑÑÐ¸Ñ Ð¿ÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¾Ð¹ ÐºÑÑÐ½Ð¸, ÑÑÑÑÐµÐ²Ð°Ñ Ð¸ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ°Ñ. ÐÐ° Ð¾ÑÐ½Ð¾Ð²Ðµ Ð°Ð½Ð°Ð»Ð¸Ð·Ð° Ð»Ð¸ÑÐµÑÐ°ÑÑÑÑ Ð±ÑÐ»Ð¸ Ð²ÑÑÐ²Ð»ÐµÐ½Ñ ÐµÐµ Ð¿Ð¾Ð¿ÑÐ»ÑÑÐ½ÑÐµ Ð±Ð»ÑÐ´Ð°, ÑÑÑÑÐµ, ÐºÐ¾ÑÐ¾ÑÐ¾Ðµ Ð´Ð»Ñ Ð½Ð¸Ñ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·ÑÐµÑÑÑ. ÐÐ° Ð¾ÑÐ½Ð¾Ð²Ðµ Ð´Ð°Ð½Ð½ÑÑ Ð¾ ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½Ð¾Ð¼ ÑÑÐ½ÐºÐµ, ÑÐ¿Ð¾ÑÐ¾Ð±Ð°Ñ Ð¿Ð¾Ð´Ð°ÑÐ¸ Ð¸ Ð¾Ð±Ð¾ÑÑÐ´Ð¾Ð²Ð°Ð½Ð¸Ð¸ Ð±ÑÐ»Ð¸ Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ñ Ð²Ð¾Ð·Ð¼Ð¾Ð¶Ð½ÑÐµ Ð¿ÑÑÐ¸ ÑÐµÑÐµÐ½Ð¸Ñ, Ð²Ð¾Ð·Ð½Ð¸ÐºÐ°ÑÑÐ¸Ñ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼.
Temporal variations of the CaXIX spectra in solar flares
Creators: name: Falewicz, R.
name: Rudawy, P.
name: Siarkowski, M.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Standard model of solar flares comprises a bulk expansion and rise of abruptly heated plasma (the chromospheric evaporation). Emission from plasma ascending along loops rooted on the visible solar disk should be often dominated, at least temporally, by a blue-shifted emission. However, there is only a very limited number of published observations of solar flares having spectra in which the blue-shifted component dominates the stationary one. In this work we compare observed X-ray spectra of three solar flares recorded during their impulsive phases and relevant synthetic spectra calculated using one-dimensional hydro-dynamic numerical model of these flares. The main aim of the work was to explain why numerous flares do not show blue-shifted spectra. The synthesized BCS spectra of the flares were compared with the relevant observed BCS spectra. We conclude that stationary component of the spectrum should be observed almost for all flares during their early phases of evolution. In opposite, the blue-shifted component of the spectrum could be not detected in flares having plasma rising along the flaring loop even with high velocity due to the geometrical dependences only. After the start of the up-flow motion, the blue-shifted component dominate temporally the synthetic spectra of the investigated flares at their early phases.
description: 9 pages, 6 figures, Astronomy and Astrophysics (accepted, September 2009)
SODA: Site Object Detection dAtaset for Deep Learning in Construction
Creators: name: Duan, Rui
name: Deng, Hui
name: Tian, Mao
name: Deng, Yichuan
name: Lin, Jiarui
Publisher: name: arXiv
Year: 2022
Subjects: subject: Computer Vision and Pattern Recognition (cs.CV)
subject: FOS: Computer and information sciences

description: Computer vision-based deep learning object detection algorithms have been developed sufficiently powerful to support the ability to recognize various objects. Although there are currently general datasets for object detection, there is still a lack of large-scale, open-source dataset for the construction industry, which limits the developments of object detection algorithms as they tend to be data-hungry. Therefore, this paper develops a new large-scale image dataset specifically collected and annotated for the construction site, called Site Object Detection dAtaset (SODA), which contains 15 kinds of object classes categorized by workers, materials, machines, and layout. Firstly, more than 20,000 images were collected from multiple construction sites in different site conditions, weather conditions, and construction phases, which covered different angles and perspectives. After careful screening and processing, 19,846 images including 286,201 objects were then obtained and annotated with labels in accordance with predefined categories. Statistical analysis shows that the developed dataset is advantageous in terms of diversity and volume. Further evaluation with two widely-adopted object detection algorithms based on deep learning (YOLO v3/ YOLO v4) also illustrates the feasibility of the dataset for typical construction scenarios, achieving a maximum mAP of 81.47%. In this manner, this research contributes a large-scale image dataset for the development of deep learning-based object detection methods in the construction industry and sets up a performance benchmark for further evaluation of corresponding algorithms in this area.
Additional file 1 of Novel CD19-specific γ/δ TCR-T cells in relapsed or refractory diffuse large B-cell lymphoma
Creators: name: Li, Chenggong
name: Zhou, Fen
name: Wang, Jing
name: Chang, Qi
name: Du, Mengyi
name: Luo, Wenjing
name: Zhang, Yinqiang
name: Xu, Jia
name: Tang, Lu
name: Jiang, Huiwen
name: Liu, Lin
name: Kou, Haiming
name: Lu, Cong
name: Liao, Danying
name: Wu, Jianghua
name: Wei, Qiuzhe
name: Ke, Sha
name: Deng, Jun
name: Liu, Cheng
name: Mei, Heng
name: Hu, Yu
Publisher: name: figshare
Year: 2023
Subjects: subject: Immunology
subject: FOS: Clinical medicine

description: Additional file 1: Supplementary methods, results, table, and figures.
title: Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð¾Ð¿ÐµÑÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÑÑÑÐ°ÑÐµÐ³Ð¸Ð¸ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ (Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ ÐÐÐ Â«ÐÐ¾Ð»Ð¿Ð¸Ð½ÑÐºÐ¸Ðµ Ð¸Ð½ÑÐµÑÐ½ÐµÑ-ÑÐµÑÐ¸Â»)
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: Ð¡Ð°Ð±Ð¸ÑÐ¾Ð², ÐÐ°ÐºÑÐ¸Ð¼
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¿ÐµÑÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÑÑÐ°ÑÐµÐ³Ð¸Ñ
Ð¸Ð½ÑÐµÑÐ½ÐµÑ-ÑÑÐ»ÑÐ³Ð¸
Ð°Ð½Ð°Ð»Ð¸Ð· Ð²Ð½ÐµÑÐ½ÐµÐ¹ ÑÑÐµÐ´Ñ
Ð¿ÑÐ¸Ð²Ð»ÐµÐºÐ°ÑÐµÐ»ÑÐ½Ð¾ÑÑÑ ÑÑÐ½ÐºÐ°
ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÑ

description: ÐÐ±ÑÐµÐºÑÐ¾Ð¼ ÑÐ°Ð±Ð¾ÑÑ ÑÐ²Ð»ÑÐµÑÑÑ ÐÐÐ Â«ÐÐ¾Ð»Ð¿Ð¸Ð½ÑÐºÐ¸Ðµ Ð¸Ð½ÑÐµÑÐ½ÐµÑ-ÑÐµÑÐ¸Â». Ð¦ÐµÐ»Ñ ÑÐ°Ð±Ð¾ÑÑ: ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ð¸Ð¹ Ð¿Ð¾ ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¾Ð¿ÐµÑÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÑÑÑÐ°ÑÐµÐ³Ð¸Ð¸ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ. ÐÐ°Ð´Ð°ÑÐ¸: - ÐÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ ÑÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¸Ñ Ð¾ÑÐ½Ð¾Ð² ÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¾Ð¿ÐµÑÐ°ÑÐ¸Ð¾Ð½-Ð½Ð¾Ð¹ ÑÑÑÐ°ÑÐµÐ³Ð¸Ð¸ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ; - ÐÐ½Ð°Ð»Ð¸Ð· ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ; - Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ð¸Ð¹ Ð¿Ð¾ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ Ð¾Ð¿ÐµÑÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ Ð´ÐµÑÑÐµÐ»Ñ-Ð½Ð¾ÑÑÐ¸ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ. Ð ÑÐ°Ð±Ð¾ÑÐµ Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð¿ÑÐµÐ´-Ð¿ÑÐ¸ÑÑÐ¸Ñ, Ð¾ÑÐµÐ½ÐµÐ½Ð° ÑÐµÐºÑÑÐ°Ñ Ð¾Ð¿ÐµÑÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÑÑÐ°ÑÐµÐ³Ð¸Ñ Ð¸ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ñ Ð¼Ðµ-ÑÐ¾Ð¿ÑÐ¸ÑÑÐ¸Ñ Ð¿Ð¾ ÐµÐµ ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ. ÐÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ñ ÑÐ°ÑÑÐµÑÑ Ð¿Ð¾ÐºÐ°Ð·Ð°Ð»Ð¸ ÑÐµÐ»ÐµÑÐ¾Ð¾Ð±ÑÐ°Ð·Ð½Ð¾ÑÑÑ ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð°ÑÐ¸Ð¹ Ðº Ð²Ð½ÐµÐ´ÑÐµÐ½Ð¸Ñ.
title: Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° ÑÐ¸ÑÐ¼ÐµÐ½Ð½Ð¾Ð³Ð¾ ÑÑÐ¸Ð»Ñ Ð³Ð°Ð»ÐµÑÐµÐ¸ ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¸ÑÐºÑÑÑÑÐ²Ð°.
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÑÑÐºÐ¾Ð²Ð°, 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: 2016
Subjects: ÑÐ¸ÑÐ¼ÐµÐ½Ð½ÑÐ¹ ÑÑÐ¸Ð»Ñ
ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½Ð¾Ðµ Ð¸ÑÐºÑÑÑÑÐ²Ð¾
ÑÑÐ¿ÑÐµÐ¼Ð°ÑÐ¸Ð·Ð¼

description: ÐÐ±ÑÐµÐºÑÐ¾Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ²Ð»ÑÐ»Ð¸ÑÑ Ð»Ð¾Ð³Ð¾ÑÐ¸Ð¿Ñ Ð¸Ð·Ð²ÐµÑÑÐ½ÑÑ Ð¼ÑÐ·ÐµÐµÐ² ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¸ÑÐºÑÑÑÑÐ²Ð°, ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½ÑÐµ ÑÐµÐ½Ð´ÐµÐ½ÑÐ¸Ð¸ Ð² Ð´Ð¸Ð·Ð°Ð¹Ð½Ðµ Ð»Ð¾Ð³Ð¾ÑÐ¸Ð¿Ð¾Ð², Ð¿Ð¾Ð½ÑÑÐ¸Ðµ Ð¸ Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¸Ðµ ÑÐ¸ÑÐ¼ÐµÐ½Ð½Ð¾Ð³Ð¾ ÑÑÐ¸Ð»Ñ, Ð¸Ð·Ð²ÐµÑÑÐ½ÑÐµ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¸ÑÐºÑÑÑÑÐ²Ð°. Ð¦ÐµÐ»Ñ ÑÐ°Ð±Ð¾ÑÑ - ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð»Ð¾Ð³Ð¾ÑÐ¸Ð¿Ð°, Ð½Ð°Ð·Ð²Ð°Ð½Ð¸Ñ Ð¸ ÑÐ¸ÑÐ¼ÐµÐ½Ð½Ð¾Ð³Ð¾ ÑÑÐ¸Ð»Ñ Ð´Ð»Ñ Ð³Ð°Ð»ÐµÑÐµÐ¸ ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¸ÑÐºÑÑÑÑÐ²Ð°. Ð Ð¿ÑÐ¾ÑÐµÑÑÐµ ÑÐ°Ð±Ð¾ÑÑ Ð¿ÑÐ¾Ð²Ð¾Ð´Ð¸Ð»ÑÑ Ð¾Ð±Ð·Ð¾Ñ Ð°Ð½Ð°Ð»Ð¾Ð³Ð¾Ð², Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ ÑÐ°ÐºÐ¸Ñ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ð¹ Ð² ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½Ð¾Ð¼ Ð¸ÑÐºÑÑÑÑÐ²Ðµ, ÐºÐ°Ðº ÐºÑÐ±Ð¸Ð·Ð¼, ÑÑÐ¿ÑÐµÐ¼Ð°ÑÐ¸Ð·Ð¼ ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð²Ð¸Ð·Ð¼. Ð ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐµ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ Ð±ÑÐ»Ð¸ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ñ ÑÑÐºÐ¸Ð·Ñ Ð»Ð¾Ð³Ð¾ÑÐ¸Ð¿Ð°, Ð²Ð°ÑÐ¸Ð°Ð½ÑÑ Ð½Ð°Ð·Ð²Ð°Ð½Ð¸Ñ Ð´Ð»Ñ Ð³Ð°Ð»ÐµÑÐµÐ¸. ÐÑÐ» Ð²ÑÐ±ÑÐ°Ð½ Ð»ÑÑÑÐ¸Ð¹ Ð²Ð°ÑÐ¸Ð°Ð½Ñ Ð»Ð¾Ð³Ð¾ÑÐ¸Ð¿Ð° Ð¸ Ðº Ð½ÐµÐ¼Ñ Ð±ÑÐ» ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½ ÑÐ¸ÑÐ¼ÐµÐ½Ð½ÑÐ¹ ÑÑÐ¸Ð»Ñ, Ð²ÐºÐ»ÑÑÐ°Ð²ÑÐ¸Ð¹ Ð² ÑÐµÐ±Ñ ÑÐ¸ÑÐ¼ÐµÐ½Ð½ÑÐ¹ Ð¿Ð°ÑÑÐµÑÐ½, Ð´ÐµÐ»Ð¾Ð²ÑÑ Ð´Ð¾ÐºÑÐ¼ÐµÐ½ÑÐ°ÑÐ¸Ñ, ÑÐµÐºÐ»Ð°Ð¼Ð½ÑÐµ Ð½Ð¾ÑÐ¸ÑÐµÐ»Ð¸ Ð¸ ÑÑÐ²ÐµÐ½Ð¸ÑÐ½ÑÑ Ð¿ÑÐ¾Ð´ÑÐºÑÐ¸Ñ.
Stochastic Causal Programming for Bounding Treatment Effects
Creators: name: Padh, Kirtan
name: Zeitler, Jakob
name: Watson, David
name: Kusner, Matt
name: Silva, Ricardo
name: Kilbertus, Niki
Publisher: name: arXiv
Year: 2022
Subjects: subject: Machine Learning (stat.ML)
subject: Machine Learning (cs.LG)
subject: FOS: Computer and information sciences

description: Causal effect estimation is important for many tasks in the natural and social sciences. We design algorithms for the continuous partial identification problem: bounding the effects of multivariate, continuous treatments when unmeasured confounding makes identification impossible. Specifically, we cast causal effects as objective functions within a constrained optimization problem, and minimize/maximize these functions to obtain bounds. We combine flexible learning algorithms with Monte Carlo methods to implement a family of solutions under the name of stochastic causal programming. In particular, we show how the generic framework can be efficiently formulated in settings where auxiliary variables are clustered into pre-treatment and post-treatment sets, where no fine-grained causal graph can be easily specified. In these settings, we can avoid the need for fully specifying the distribution family of hidden common causes. Monte Carlo computation is also much simplified, leading to algorithms which are more computationally stable against alternatives.
Fuzzy Supernova Templates II: Parameter Estimation
Creators: name: Rodney, Steven A.
name: Tonry, John L.
Publisher: name: arXiv
Year: 2010
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: Wide field surveys will soon be discovering Type Ia supernovae (SNe) at rates of several thousand per year. Spectroscopic follow-up can only scratch the surface for such enormous samples, so these extensive data sets will only be useful to the extent that they can be characterized by the survey photometry alone. In a companion paper (Rodney and Tonry, 2009) we introduced the SOFT method for analyzing SNe using direct comparison to template light curves, and demonstrated its application for photometric SN classification. In this work we extend the SOFT method to derive estimates of redshift and luminosity distance for Type Ia SNe, using light curves from the SDSS and SNLS surveys as a validation set. Redshifts determined by SOFT using light curves alone are consistent with spectroscopic redshifts, showing a root-mean-square scatter in the residuals of RMS_z=0.051. SOFT can also derive simultaneous redshift and distance estimates, yielding results that are consistent with the currently favored Lambda-CDM cosmological model. When SOFT is given spectroscopic information for SN classification and redshift priors, the RMS scatter in Hubble diagram residuals is 0.18 mags for the SDSS data and 0.28 mags for the SNLS objects. Without access to any spectroscopic information, and even without any redshift priors from host galaxy photometry, SOFT can still measure reliable redshifts and distances, with an increase in the Hubble residuals to 0.37 mags for the combined SDSS and SNLS data set. Using Monte Carlo simulations we predict that SOFT will be able to improve constraints on time-variable dark energy models by a factor of 2-3 with each new generation of large-scale SN surveys.
description: 20 pages, 7 figures, accepted to ApJ; paper 1 is arXiv:0910.3702
A decreasing upper bound of energy for time-fractional phase-field equations
Creators: name: Quan, Chaoyu
name: Tang, Tao
name: Wang, Boyi
name: Yang, Jiang
Publisher: name: arXiv
Year: 2022
Subjects: subject: Numerical Analysis (math.NA)
subject: FOS: Mathematics

description: In this article, we study the energy dissipation property of time-fractional Allen-Cahn equation. We propose a decreasing upper bound of energy that decreases with respect to time and coincides with the original energy at $t = 0$ and as $t$ tends to $\infty$. This upper bound can also be viewed as a nonlocal-in-time modified energy, the summation of the original energy and an accumulation term due to the memory effect of time fractional derivative. In particular, this indicates that the original energy indeed decays w.r.t. time in a small neighborhood at $t=0$. We illustrate the theory mainly with the time-fractional Allen-Cahn equation, but it could be applied to other time-fractional phase-field models such as the Cahn-Hilliard equation. On the discrete level, the first-order L1 and second-order L2 schemes for time-fractional Allen-Cahn equation have similar decreasing modified energies, so that the stability can be established. Some numerical results are provided to illustrate the behavior of this modified energy and to verify our theoretical results.
An elliptic hypergeometric integral with W(F_4) symmetry
Creators: name: van de Bult, Fokko J.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Classical Analysis and ODEs (math.CA)
subject: FOS: Mathematics
subject: 33D60

description: In this article we give a new transformation between elliptic hypergeometric beta integrals, which gives rise to a Weyl group symmetry of type F_4. The transformation is a generalization of a series transformation discovered by Langer, Schlosser, and Warnaar. Moreover we consider various limits of this transformation to basic hypergeometric functions obtained by letting p tend to 0.
Supplementary Information from Were all trilobites fully marine? Trilobite expansion into brackish water during the Early Palaeozoic
Creators: name: M. Gabriela Mángano
name: Buatois, Luis A.
name: Waisfeld, Beatriz G.
name: Muñoz, Diego F.
name: N. Emilio Vaccari
name: Astini, Ricardo A.
Publisher: name: The Royal Society
Year: 2021
Subjects: subject: 40308 Palaeontology (incl. Palynology)
subject: FOS: Earth and related environmental sciences

description: Text on body fossil preservation, stratigraphical sections, geological maps, photographic plates, and tables summarizing sedimentological and palaeobiological information
Spinal ependymoma diagnosed on MRI
Creators: name: Chu, Robert
Publisher: name: EURORAD
Year: 2014
Subjects: subject: Spine
subject: MR
subject: Diagnostic procedure
subject: Neoplasia

description: Clinical History Image Findings Discussion Find Diagnosis Differential Diagnosis
description: male, 50 years
description: Clinical History: 50-year-old male with lower back pain. MRI ordered to investigate suspected lumbar disc herniation. Final Diagnosis: Ependymoma (confirmed by pathology)
title: ÐÑÐ¾ÐµÐºÑ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ Ð¿Ð¸ÑÐ°Ð½Ð¸Ñ Ð² ÑÐµÐ½ÑÑÐµ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ ÑÐ¿Ð¾ÑÑÑÐ¼ÐµÐ½Ð¾Ð² Ð¿Ð¾ Ð²Ð¾Ð´Ð½ÑÐ¼ Ð²Ð¸Ð´Ð°Ð¼ ÑÐ¿Ð¾ÑÑÐ°
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Ð°ÑÐ°Ð²Ð²Ð°, 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: 2018
Subjects: ÐÐ¸ÑÐµÐ²ÑÐµ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ
ÑÐ¿Ð¾ÑÑÐ¸Ð²Ð½Ð¾Ðµ Ð¿Ð¸ÑÐ°Ð½Ð¸Ðµ
Ð¸Ð½Ð´Ð¸Ð²Ð¸Ð´ÑÐ°Ð»ÑÐ½ÑÐ¹ ÑÐ°ÑÐ¸Ð¾Ð½
Ð°ÑÑÐ¾ÑÑÐ¸Ð¼ÐµÐ½Ñ Ð¿ÑÐ¾Ð´ÑÐºÑÐ¸Ð¸

description: Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ñ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ðµ ÑÐµÑÐµÐ½Ð¸Ñ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ Ð¿Ð¸ÑÐ°Ð½Ð¸Ñ Ð´Ð»Ñ ÑÐµÐ½ÑÑÐ° Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ ÑÐ¿Ð¾ÑÑÑÐ¼ÐµÐ½Ð¾Ð² Ð¿Ð¾ Ð²Ð¾Ð´Ð½ÑÐ¼ Ð²Ð¸Ð´Ð°Ð¼ ÑÐ¿Ð¾ÑÑÐ°. Ð¡Ð¾ÑÑÐ°Ð²Ð»ÐµÐ½ Ð°ÑÑÐ¾ÑÑÐ¸Ð¼ÐµÐ½Ñ Ð¿ÑÐ¾Ð´ÑÐºÑÐ¸Ð¸ ÑÐ¾Ð¾ÑÐ²ÐµÑÑÑÐ²ÑÑÑÐ¸Ð¹ ÑÑÐµÐ±Ð¾Ð²Ð°Ð½Ð¸ÑÐ¼ ÑÐ¿Ð¾ÑÑÐ¸Ð²Ð½Ð¾Ð³Ð¾ Ð¿Ð¸ÑÐ°Ð½Ð¸Ñ. Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½ Ð°Ð»Ð³Ð¾ÑÐ¸ÑÐ¼ ÑÐ¾ÑÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¸Ð½Ð´Ð¸Ð²Ð¸Ð´ÑÐ°Ð»ÑÐ½ÑÑ ÑÐ°ÑÐ¸Ð¾Ð½Ð¾Ð², Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ñ Ð²Ð°ÑÐ¸Ð°Ð½ÑÑ Ð¸Ð½Ð´Ð¸Ð²Ð¸Ð´ÑÐ°Ð»ÑÐ½ÑÑ ÑÐ°ÑÐ¸Ð¾Ð½Ð¾Ð² Ð´Ð»Ñ ÑÐ°Ð·Ð»Ð¸ÑÐ½ÑÑ Ð¿ÐµÑÐ¸Ð¾Ð´Ð¾Ð² ÑÐ¿Ð¾ÑÑÐ¸Ð²Ð½Ð¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸. ÐÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½ ÑÐ°ÑÑÐµÑ Ð¾Ð±Ð¾ÑÑÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¸ Ð¿Ð¾Ð¼ÐµÑÐµÐ½Ð¸Ð¹, ÑÐ¸ÑÑÐµÐ¼: ÑÐ»ÐµÐºÑÑÐ¾ÑÐ½Ð°Ð±Ð¶ÐµÐ½Ð¸Ñ; Ð²Ð¾Ð´Ð¾ÑÐ½Ð°Ð±Ð¶ÐµÐ½Ð¸Ñ Ð¸ ÐºÐ°Ð½Ð°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸; Ð²ÐµÐ½ÑÐ¸Ð»ÑÑÐ¸Ð¸ Ð¸ ÐºÐ¾Ð½Ð´Ð¸ÑÐ¸Ð¾Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð²Ð¾Ð·Ð´ÑÑÐ°. Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ð¾ Ð¾Ð±ÑÐµÐ¼Ð½Ð¾ Ð¿Ð»Ð°Ð½Ð¸ÑÐ¾Ð²Ð¾ÑÐ½Ð¾Ðµ ÑÐµÑÐµÐ½Ð¸Ðµ Ð² ÑÐ¾Ð¾ÑÐ²ÐµÑÑÑÐ²Ð¸Ð¸ Ñ Ð½Ð¾ÑÐ¼Ð°ÑÐ¸Ð²Ð½ÑÐ¼Ð¸ Ð´Ð¾ÐºÑ-Ð¼ÐµÐ½ÑÐ°Ð¼Ð¸.
A simple design of an artificial electromagnetic black hole
Creators: name: Lu, Wanli
name: Jin, JunFeng
name: Chen, Huanyang
name: Lin, Zhifang
Publisher: name: arXiv
Year: 2010
Subjects: subject: Optics (physics.optics)
subject: FOS: Physical sciences

description: We study the properties of an artificial electromagnetic black hole for transverse magnetic modes rigorously. A multi-layered structure of such a black hole is then proposed as a reduced variety for easy experimental realizations. An actual design of composite materials based on the effective medium theory is given eventually with only five kinds of real isotropic materials. The finite element method confirms the functionality of such a simple design.
Strength of the Spin-Fluctuation-Mediated Pairing Interaction in a High-Temperature Superconductor
Creators: name: Dahm, T.
name: Hinkov, V.
name: Borisenko, S. V.
name: Kordyuk, A. A.
name: Zabolotnyy, V. B.
name: Fink, J.
name: Büchner, B.
name: Scalapino, D. J.
name: Hanke, W.
name: Keimer, B.
Publisher: name: arXiv
Year: 2008
Subjects: subject: Superconductivity (cond-mat.supr-con)
subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: Theories based on the coupling between spin fluctuations and fermionic quasiparticles are among the leading contenders to explain the origin of high-temperature superconductivity, but estimates of the strength of this interaction differ widely. Here we analyze the charge- and spin-excitation spectra determined by angle-resolved photoemission and inelastic neutron scattering, respectively, on the same crystals of the high-temperature superconductor YBa2Cu3O6.6. We show that a self-consistent description of both spectra can be obtained by adjusting a single parameter, the spin-fermion coupling constant. In particular, we find a quantitative link between two spectral features that have been established as universal for the cuprates, namely high-energy spin excitations and "kinks" in the fermionic band dispersions along the nodal direction. The superconducting transition temperature computed with this coupling constant exceeds 150 K, demonstrating that spin fluctuations have sufficient strength to mediate high-temperature superconductivity.
description: 25 pages, 7 figures, including supplementary information, accepted for publication in Nature Physics
ALP induced polarization effects on photons from galaxy clusters
Creators: name: Galanti, Giorgio
name: Roncadelli, Marco
name: Tavecchio, Fabrizio
name: Costa, Enrico
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Many extensions of the Standard Model of particle physics and in particular superstring and superbrane theories predict the existence of axion-like particles (ALPs). ALPs are very elusive, extremely light and interact primarily with photons. In the presence of an external magnetic field two effects show up: (i) photon-ALP oscillations and (ii) a change of the photon polarization state. The astrophysical context represents the best opportunity to get indirect evidence for the ALP existence thanks to various effects that the photon-ALP interaction produces in the sky. Great attention has been paid so far to photon-ALP oscillations, since they modify the transparency of the crossed media at very high energies and so the final spectra of faraway sources exhibit a flux excess and a characteristic oscillatory behavior. Two hints at the ALP existence have hitherto been discovered. But less interest has been attracted by the modification of the photon polarization. In this paper we address it in the X-ray and in the high energy (HE) bands. Specifically, we analyze the photon degree of linear polarization and the polarization angle induced by the photon-ALP interaction for photons generated in the central region of two galaxy clusters: Perseus and Coma. We find a substantial departure from conventional physics in both considered bands. We conclude that the ALP-induced polarization effects are more likely detectable with the proposed missions like COSI (approved to launch), e-ASTROGAM and AMEGO in the HE range. Still, possible ALP-induced effects on photon polarization could also be detected by IXPE (already operative) and by the proposed eXTP, XL-Calibur, NGXP and XPP in the X-ray band.
description: 14 pages, 12 figures, This version matches the published paper: Phys. Rev. D 107, 103007 (2023)
String Mass Shifts
Creators: name: Chialva, Diego
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: We study closed string one-loop amplitudes in string theory, in particular the average mass shift for states at given mass and Neveu-Schwarz charges. Our analysis is based only on well-defined string amplitudes and the exploitation of symmetries and unitarity properties of the torus amplitudes. We obtain the result Delta M^2 = - g_s^2 M^(2+(3-D)/2) in D spacetime dimensions for the average closed string mas-shift (Delta M^2 = - g_s^2 (M^2-Q^2)^(1+(3-D)/4) for states with non-zero Neveu-Schwarz charges Q). An interesting picture of one-loop corrections for the string in non-supersymmetric configurations comes out: the dominant interactions responsible for these corrections are of long-range type (namely gravitational) and it appears that perturbations theory is generally reliable on the spectrum of massive string states.
description: 38 pages plus references, typos corrected, notation and text improved
title: Ð¡Ð¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð¿ÑÐ°ÐºÑÐ¸ÐºÐ¸ ÐºÑÐµÐ´Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÑÐ¸Ð·Ð¸ÑÐµÑÐºÐ¸Ñ Ð»Ð¸Ñ ÐºÐ¾Ð¼Ð¼ÐµÑÑÐµÑÐºÐ¸Ð¼Ð¸ Ð±Ð°Ð½ÐºÐ°Ð¼Ð¸
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐµÐ»ÐµÐ·Ð½ÑÐºÐ¾Ð²Ð°, Ð®Ð»Ð¸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: 2017
Subjects: ÐºÑÐµÐ´Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ
ÑÐ¸Ð·Ð¸ÑÐµÑÐºÐ¸Ðµ Ð»Ð¸ÑÐ°
ÐºÐ¾Ð¼Ð¼ÐµÑÑÐµÑÐºÐ¸Ðµ Ð±Ð°Ð½ÐºÐ¸
ÐºÑÐµÐ´Ð¸ÑÐ½Ð°Ñ Ð¿Ð¾Ð»Ð¸ÑÐ¸ÐºÐ°

description: ÐÐ±ÑÐµÐºÑÐ¾Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ²Ð»ÑÐµÑÑÑ ÐÐÐ Â«Ð¥ÐÐ¤ÐÂ». 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°Ð½Ð°Ð»Ð¸Ð· ÐºÑÐµÐ´Ð¸ÑÐ½Ð¾Ð³Ð¾ Ð¿ÑÐ¾ÑÐµÑÑÐ° ÐÐÐ Â«Ð¥ÐÐ¤ÐÂ» Ð² Ð¾ÑÐ½Ð¾ÑÐµÐ½Ð¸Ð¸ ÑÐ¸Ð·Ð¸ÑÐµÑÐºÐ¸Ñ Ð»Ð¸Ñ Ð´Ð»Ñ Ð¿ÑÐ¸Ð½ÑÑÐ¸Ñ ÑÐµÑÐµÐ½Ð¸Ñ Ð¾ Ð¼ÐµÑÐ°Ñ Ð¿Ð¾ ÐµÐ³Ð¾ ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ. Ð Ð°ÑÑÐ¼Ð¾ÑÑÐµÐ½ ÐºÑÐµÐ´Ð¸ÑÐ½ÑÐ¹ Ð¿ÑÐ¾ÑÐµÑÑ Ð² ÐºÐ¾Ð¼Ð¼ÐµÑÑÐµÑÐºÐ¸Ñ Ð±Ð°Ð½ÐºÐ°Ñ Ð Ð¾ÑÑÐ¸Ð¹ÑÐºÐ¾Ð¹ Ð¤ÐµÐ´ÐµÑÐ°ÑÐ¸Ð¸ Ð¿Ð¾ ÑÑÐ°Ð²Ð½ÐµÐ½Ð¸Ñ Ñ ÐºÑÐµÐ´Ð¸ÑÐ½ÑÐ¼ Ð¿ÑÐ¾ÑÐµÑÑÐ¾Ð¼ ÐºÑÐµÐ´Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÑÐ¸Ð·Ð¸ÑÐµÑÐºÐ¸Ñ Ð»Ð¸Ñ Ð² Ð·Ð°ÑÑÐ±ÐµÐ¶Ð½ÑÑ Ð±Ð°Ð½ÐºÐ°Ñ. ÐÑÐ» Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½Ð¾Ð³Ð¾ ÑÐ¾ÑÑÐ¾ÑÐ½Ð¸Ñ Ð¿Ð¾ÑÑÐµÐ±Ð¸ÑÐµÐ»ÑÑÐºÐ¾Ð³Ð¾ ÐºÑÐµÐ´Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð Ð¤, Ð¿Ð¾Ð»Ð¾Ð¶ÐµÐ½Ð¸Ñ ÐÐÐ Â«Ð¥ÐÐ¤ÐÂ» Ð½Ð° ÑÑÐ½ÐºÐµ Ð¸ Ð²ÑÑÐ²Ð»ÐµÐ½Ð¾, ÑÑÐ¾ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐ¼Ð¸ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸ÑÐ¼Ð¸, ÑÑÐµÐ±ÑÑÑÐ¸Ð¼Ð¸ ÑÐ»ÑÑÑÐµÐ½Ð¸Ñ, ÑÐ²Ð»ÑÑÑÑÑ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð±Ð¾Ð»ÐµÐµ Ð³Ð¸Ð±ÐºÐ¸Ñ ÐºÑÐµÐ´Ð¸ÑÐ½ÑÑ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼, ÑÐ°Ð±Ð¾ÑÐ° Ñ Ð¿ÑÐ¾ÑÑÐ¾ÑÐµÐ½Ð½Ð¾Ð¹ Ð·Ð°Ð´Ð¾Ð»Ð¶ÐµÐ½Ð½Ð¾ÑÑÑÑ Ð¸ Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ðµ ÐºÐ°ÑÐµÑÑÐ²Ð° Ð¾Ð±ÑÐ»ÑÐ¶Ð¸Ð²Ð°Ð½Ð¸Ñ.
Linking jet emission and X-ray properties in the peculiar neutron star X-ray binary Circinus X-1
Creators: name: Soleri, Paolo
name: Tudose, Valeriu
name: Fender, Rob
name: van der Klis, Michiel
name: Jonker, Peter G.
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: We present the results of simultaneous X-ray and radio observations of the peculiar Z-type neutron star X-ray binary Cir X-1, observed with the Rossi X-ray timing explorer satellite and the Australia Telescope Compact Array in 2000 October and 2002 December. We identify typical Z source behaviour in the power density spectra as well as characteristic Z patterns drawn in an X-ray hardness-intensity diagram. Power spectra typical of bright atoll sources have also been identified at orbital phases after the periastron passage, while orbital phases before the periastron passage are characterized by power spectra that are typical neither of Z nor of atoll sources. We investigate the coupling between the X-ray and the radio properties, focusing on three orbital phases when an enhancement of the radio flux density has been detected, to test the link between the inflow (X-ray) and the outflow (radio jet) to/from the compact object. In two out of three cases we associate the presence of the radio jet to a spectral transition in the X-rays, although the transition does not precede the radio flare, as detected in other Z sources. An analogous behaviour has recently been found in the black hole candidate GX 339-4. In the third case, the radio light curve shows a similar shape to the X-ray light curve. We discuss our results in the context of jet models, considering also black hole candidates.
description: Accepted for publication in MNRAS
Interplay of bulk and interface effects in the electric-field driven transition in magnetite
Creators: name: Fursina, A. A.
name: Sofin, R. G. S.
name: Shvets, I. V.
name: Natelson, D.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: Contact effects in devices incorporating strongly-correlated electronic materials are comparatively unexplored. We have investigated the electrically-driven phase transition in magnetite (100) thin films by four-terminal methods. In the lateral configuration, the channel length is less than 2 $μ$m, and voltage-probe wires $\sim$100 nm in width are directly patterned within the channel. Multilead measurements quantitatively separate the contributions of each electrode interface and the magnetite channel. We demonstrate that on the onset of the transition contact resistances at both source and drain electrodes and the resistance of magnetite channel decrease abruptly. Temperature dependent electrical measurements below the Verwey temperature indicate thermally activated transport over the charge gap. The behavior of the magnetite system at a transition point is consistent with a theoretically predicted transition mechanism of charge gap closure by electric field.
description: 6 pages, 5 figures, to appear in PRB
Studia Historiae Scientiarum (kwestie aktualne | current issues)
Creators: name: Kokowski, Michal
Publisher: name: Zenodo
Year: 2020
Subjects: Studia Historiae Scientiarum
Komisja Historii Nauki PAU
Commission on the History of Science, Polish Academy of Arts and Sciences

description: Prezentacja omawia aktualne kwestie związane z rozwijaniem czasopisma Studia Historiae Scientiarum (e-ISSN: 2543-702X, p-ISSN: 2451-3202). | The presentation covers current issues related to the development of the journal Studia Historiae Scientiarum (e-ISSN: 2543-702X, p-ISSN: 2451-3202).
description: {"references": ["Kokowski, Micha\u0142 2020a: Evolutionary transformation of the journal. Part 7. Studia Historiae Scientiarum 19, ss. 13\u201321. DOI: 10.4467/2543702XSHS.20.001.12557.", "Kokowski, Micha\u0142 2020b: Ewolucyjna transformacja czasopisma. Cz\u0119\u015b\u0107 7. Studia Historiae Scientiarum 19, ss. 23\u201331. DOI: 10.4467/2543702XSHS.20.002.12558.", "Kokowski, Micha\u0142 2020c: Sprawa \"Wniosku o korekt\u0119 punktacji czasopisma Studia Historiae Scientiarum z 20 punkt\u00f3w na 70 punkt\u00f3w\". Studia Historiae Scientiarum 19, ss. 507\u2013541. DOI: 10.4467/2543702XSHS.20.016.12572."]}
title: Ð¯Ð·ÑÐºÐ¸ ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½Ð¾Ð¹ ÐÑÐ¿Ð°Ð½Ð¸Ð¸: Ð¸Ñ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ðµ Ð¸ Ð²Ð»Ð¸ÑÐ½Ð¸Ðµ Ð½Ð° Ð¿Ð¾Ð»Ð¸ÑÐ¸ÑÐµÑÐºÑÑ ÑÐ¸ÑÑÐ°ÑÐ¸Ñ
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Ð´Ð¸Ð½Ð°, ÐÐ½Ð°ÑÑÐ°ÑÐ¸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Ð¿Ð°Ð½ÑÐºÐ¸Ð¹ ÑÐ·ÑÐº
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