cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Asteroidi: se li conosci, li eviti
Creators: Stefano Parisini
Publisher: name: Media Inaf
Year: 2016

Sentite già la mancanza del lander Philae, quello sulla cometa Rosetta? Coraggio: nei prossimi anni un paio di suoi cuginetti dovrebbero sbarcare su altrettanti asteroidi. Questi corpi celesti sono da conoscere meglio, anche per saperli deviare nel caso si dirigano verso la Terra. A proposito: l’asteroide del prossimo 5 marzo non è pericoloso, parola di Giovanni Valsecchi dell’INAF
Direct Numerical Simulations of Low-$Rm$ MHD turbulence based on the least dissipative modes
Creators: name: Pothérat, Alban
name: Dymkou, Vitali
Publisher: name: arXiv
Year: 2010
Subjects: subject: Fluid Dynamics (physics.flu-dyn)
subject: FOS: Physical sciences

description: We present a new spectral method for the Direct Numerical Simulation of Magnetohydrodynamic turbulence at low Magnetic Reynolds number. The originality of our approach is that instead of using traditional bases of functions, it relies on the basis of eigenmodes of the dissipation operator, which represents viscous and Joule dissipation. We apply this idea to the simple case of a periodic domain in the three directions of space, with an homogeneous magnetic field in the $\mathbf e_z$ direction. The basis is then still as subset of the Fourier space, but ordered by growing linear decay rate $|λ|$ (\emph{i.e} according to the \emph{least dissipative modes}). We show that because the lines of constant energy tend to follow those of constant $|λ|$ in the Fourier space, the scaling for the the smallest scales $|λ^{\rm max}|$ in a forced flow can be expressed using this single parameter, as a function of the Reynolds number as $\sqrt{|λ^{\rm max}|}/(2πk_f)\simeq 0.5\Rey^{1/2}$, where $k_f$ is the forcing wavelength, or as a function of the Grashof number $\Gr_f$, which gives a non-dimensional measure of the forcing, as $|λ^{\rm max}|^{1/2}/(2πk_f)\simeq 0.47\Gr_f^{0.20}$. This scaling is also found consistent with heuristic scalings, and which we are able to numerically quantify as $k_\perp^{\rm max}/k_f\simeq 0.5 \Rey^{1/2}$ and $k_z^{\rm max}/k_f\simeq 0.8k_f \Rey/Ha$. Finally, we show that the set of least dissipative modes gives a relevant prediction for the scale of the first three-dimensional structure to appear in a forced, initially two-dimensional turbulent flow. This completes our numerical demonstration that the least dissipative modes can be used to simulate both two- and three-dimensional low-Rm MHD flows.
description: 24 pages. Article accepted for publication in the Journal of Fluid Mechanics
Strong RF focusing for luminosity increase: short bunches at the IP
Creators: name: A. Gallo
name: P. Raimondi
name: M. Zobov
Publisher: name: INFN Open Access Repository
Year: 2004

description: One of the key-issues to increase the luminosity in the next generation
particle factories is to reduce the bunch length at the interaction point (IP)
as much as possible. This will allow reducing proportionally the transverse
beta functions at the IP and increasing the luminosity by the same factor. The
strong RF focusing consists in obtaining short bunches by substantially
increasing the lattice momentum compaction and the RF gradient. In this regime
the bunch length is modulated along the ring and could be minimized at the IP.
If the principal impedance generating elements of the ring are located where
the bunch is long (in the RF cavities region) it is possible to avoid microwave
instability and excessive bunch lengthening due to the potential well
distortion.
title: ÐÐ¸Ð°Ð³Ð½Ð¾ÑÑÐ¸ÐºÐ° Ð´Ð²Ð¸Ð³Ð°ÑÐµÐ»ÐµÐ¹. ÐÐ¾ÑÐ¾ÑÐ½Ð°Ñ Ð¸ ÑÐ¸ÑÑÐµÐ¼Ð½Ð°Ñ Ð´Ð¸Ð°Ð³Ð½Ð¾ÑÑÐ¸ÐºÐ° Ð°Ð²ÑÐ¾Ð¼Ð¾Ð±Ð¸Ð»ÑÐ½ÑÑ Ð´Ð²Ð¸Ð³Ð°ÑÐµÐ»ÐµÐ¹ Ð½Ð° ÑÑÐµÐ½Ð´Ðµ FSA 740
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ
titleType: Subtitle
Creators: name: ÐÐ²Ð°Ð½Ð¾Ð², ÐÐ»ÐµÐºÑÐ°Ð½Ð´Ñ
name: ÐÐ±ÑÐ·Ð¾Ð², ÐÐ»ÐµÐ³
name: ÐÐ°Ð»ÑÑÐµÐ², Ð®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: 2022
Subjects: ÐÐ²Ð¸Ð³Ð°ÑÐµÐ»Ð¸ Ð²Ð½ÑÑÑÐµÐ½Ð½ÐµÐ³Ð¾ ÑÐ³Ð¾ÑÐ°Ð½Ð¸Ñ
Ð¢ÐµÑ Ð½Ð¸ÑÐµÑÐºÐ°Ñ Ð´Ð¸Ð°Ð³Ð½Ð¾ÑÑÐ¸ÐºÐ°
ÐÑÐ¿ÑÑÐ°ÑÐµÐ»ÑÐ½ÑÐµ ÑÑÐµÐ½Ð´Ñ
ÑÐ¸ÑÑÐµÐ¼Ñ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð´Ð²Ð¸Ð³Ð°ÑÐµÐ»ÐµÐ¼
Ð½ÐµÐ¸ÑÐ¿ÑÐ°Ð²Ð½Ð¾ÑÑÐ¸
Ð½ÐµÐ¹ÑÑÐ°Ð»Ð¸Ð·Ð°ÑÐ¾ÑÑ
ÑÐ¾ÐºÑÐ¸ÑÐ½Ð¾ÑÑÑ Ð¾ÑÑÐ°Ð±Ð¾ÑÐ°Ð²ÑÐ¸Ñ Ð³Ð°Ð·Ð¾Ð²
ÑÑÐµÐ±Ð½Ð¸ÐºÐ¸ Ð¸ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ñ Ð´Ð»Ñ Ð²ÑÐ·Ð¾Ð²

description: Ð£ÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ Ð¿ÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¾ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾ÑÑÐ¸ 140501 Â«ÐÐ²Ð¸Ð³Ð°ÑÐµÐ»Ð¸ Ð²Ð½ÑÑÑÐµÐ½Ð½ÐµÐ³Ð¾ ÑÐ³Ð¾ÑÐ°Ð½Ð¸ÑÂ» Ð¿Ð¾ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ 13.03.03_04 Â«Ð­Ð½ÐµÑÐ³ÐµÑÐ¸ÑÐµÑÐºÐ¾Ðµ Ð¼Ð°ÑÐ¸Ð½Ð¾ÑÑÑÐ¾ÐµÐ½Ð¸ÐµÂ», Ð² ÑÑÐµÐ±Ð½ÑÐ¹ Ð¿Ð»Ð°Ð½ ÐºÐ¾ÑÐ¾ÑÑÑ Ð²ÑÐ¾Ð´Ð¸Ñ Ð¸Ð·ÑÑÐµÐ½Ð¸Ðµ ÐºÑÑÑÐ¾Ð² Â«ÐÐ¸Ð°Ð³Ð½Ð¾ÑÑÐ¸ÐºÐ° Ð¸ Ð½Ð°Ð´ÐµÐ¶Ð½Ð¾ÑÑÑ ÑÑÑÐ°Ð½Ð¾Ð²Ð¾Ðº Ñ Ð´Ð²Ð¸Ð³Ð°ÑÐµÐ»ÑÐ¼Ð¸ Ð²Ð½ÑÑÑÐµÐ½Ð½ÐµÐ³Ð¾ ÑÐ³Ð¾ÑÐ°Ð½Ð¸Ñ (ÐÐÐ¡)Â», Â«ÐÐ¸Ð°Ð³Ð½Ð¾ÑÑÐ¸ÐºÐ° ÐÐÐ¡Â». ÐÐ¾ÑÐ¾Ð±Ð¸Ðµ Ð²ÐºÐ»ÑÑÐ°ÐµÑ Ð² ÑÐµÐ±Ñ ÑÐ¸ÐºÐ» Ð»Ð°Ð±Ð¾ÑÐ°ÑÐ¾ÑÐ½ÑÑ ÑÐ°Ð±Ð¾Ñ Ð´Ð»Ñ Ð¿Ð¾Ð»ÑÑÐµÐ½Ð¸Ñ ÑÑÑÐ´ÐµÐ½ÑÐ°Ð¼Ð¸ Ð½ÐµÐ¾Ð±ÑÐ¾Ð´Ð¸Ð¼ÑÑ ÐºÐ¾Ð¼Ð¿ÐµÑÐµÐ½ÑÐ¸Ð¹ Ð¸ Ð½Ð°Ð²ÑÐºÐ¾Ð² ÑÐ°Ð±Ð¾ÑÑ Ð½Ð° ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½ÑÑ ÑÑÐµÐ½Ð´Ð°Ñ Ð¸ ÑÑÑÑÐ¾Ð¹ÑÑÐ²Ð°Ñ, Ð¿ÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð½ÑÑ Ð´Ð»Ñ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¸Ñ Ð´Ð¸Ð°Ð³Ð½Ð¾ÑÑÐ¸ÐºÐ¸ Ð°Ð²ÑÐ¾Ð¼Ð¾Ð±Ð¸Ð»ÑÐ½ÑÑ Ð´Ð²Ð¸Ð³Ð°ÑÐµÐ»ÐµÐ¹ Ð²Ð½ÑÑÑÐµÐ½Ð½ÐµÐ³Ð¾ ÑÐ³Ð¾ÑÐ°Ð½Ð¸Ñ. ÐÐ°Ð½Ð¾ Ð¾Ð¿Ð¸ÑÐ°Ð½Ð¸Ðµ Ð¸ Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½ ÑÐ¾ÑÑÐ°Ð² Ð¾Ð±Ð¾ÑÑÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð´Ð¸Ð°Ð³Ð½Ð¾ÑÑÐ¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑÐ° (ÑÑÐµÐ½Ð´Ð°) FSA 740 Ð´Ð»Ñ Ð¿ÑÐ¾Ð²ÐµÑÐºÐ¸ ÑÐ¸ÑÑÐµÐ¼ Ð°Ð²ÑÐ¾Ð¼Ð¾Ð±Ð¸Ð»ÑÐ½ÑÑ Ð´Ð²Ð¸Ð³Ð°ÑÐµÐ»ÐµÐ¹ Ð¸ Ð±Ð¾ÑÑÐ¾Ð²Ð¾Ð³Ð¾ ÑÐ»ÐµÐºÑÑÐ¾Ð¾Ð±Ð¾ÑÑÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ Ð°Ð²ÑÐ¾Ð¼Ð¾Ð±Ð¸Ð»ÐµÐ¹. ÐÐ·Ð»Ð¾Ð¶ÐµÐ½Ð° Ð¼ÐµÑÐ¾Ð´Ð¸ÐºÐ° Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¸Ñ Ð»Ð°Ð±Ð¾ÑÐ°ÑÐ¾ÑÐ½ÑÑ ÑÐ°Ð±Ð¾Ñ Ð¿Ð¾ Ð¼Ð¾ÑÐ¾ÑÐ½Ð¾Ð¹ Ð´Ð¸Ð°Ð³Ð½Ð¾ÑÑÐ¸ÐºÐµ Ð¸ Ð¿Ð¾ Ð´Ð¸Ð°Ð³Ð½Ð¾ÑÑÐ¸ÐºÐµ ÑÐ¸ÑÑÐµÐ¼ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð´Ð²Ð¸Ð³Ð°ÑÐµÐ»ÐµÐ¼ Ñ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸ÐµÐ¼ ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾ Ð¿Ð¾Ð´Ð¾Ð±ÑÐ°Ð½Ð½Ð¾Ð³Ð¾ Ð¸Ð»Ð»ÑÑÑÑÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð³Ð¾ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ð°.
Science,technology and society
Creators: name: G. Giacomelli
name: R. Giacomelli
Publisher: name: INFN Open Access Repository
Year: 2005

description: We shall discuss some aspects of science and technology, their increasing
role in the society, the fast advances in modern science, the apparent decrease
of interest of the young generation in basic sciences, the importance of proper
science popularization for better public education and awareness in scientific
fields.
The Opera Experiment
Creators: name: G. Giacomelli
name: M. Giorgini
Publisher: name: INFN Open Access Repository
Year: 2006

description: The physics motivations and the detector design of the long baseline OPERA
experiment are discussed; OPERA is a hybrid detector made of several types of
electronic subdetectors, 2 magnets and lead/nuclear emulsions ``brick'' walls.
It is located in the Gran Sasso underground lab, 732 km from CERN, on the CNGS
neutrino beam. A summary of the performances and of the physics plans are
presented.
Rising Total Hadron-Hadron Cross Sections
Creators: name: Giacomelli, Giorgio
Publisher: name: INFN Open Access Repository
Year: 2007

description: A historical summary is made on the measurements concerning the rising total
hadron-hadron cross sections at high energies. The first part of this paper
concerns the total cross section measurements performed at the Brookhaven,
Serpukhov and Fermilab fixed target accelerators; then the measurements at the
CERN Intersecting Storage Rings (ISR), and at the CERN and at the Tevatron
Fermilab proton-antiproton colliders; finally the cosmic ray measurements at
even higher energies. A short discussion on Conclusions and Perspectives
follows.
Testing fundamental physics with distant star clusters: theoretical models for pressure-supported stellar systems
Creators: name: Haghi, Hosein
name: Baumgardt, Holger
name: Kroupa, Pavel
name: Grebel, Eva K.
name: Hilker, Michael
name: Jordi, Katrin
Publisher: name: arXiv
Year: 2009
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We investigate the mean velocity dispersion and the velocity dispersion profile of stellar systems in MOND, using the N-body code N-MODY, which is a particle-mesh based code with a numerical MOND potential solver developed by Ciotti, Londrillo and Nipoti (2006). We have calculated mean velocity dispersions for stellar systems following Plummer density distributions with masses in the range of $10^4 M_\odot$ to $10^9 M_\odot$ and which are either isolated or immersed in an external field. Our integrations reproduce previous analytic estimates for stellar velocities in systems in the deep MOND regime ($a_i, a_e \ll a_0$), where the motion of stars is either dominated by internal accelerations ($a_i \gg a_e$) or constant external accelerations ($a_e \gg a_i$). In addition, we derive for the first time analytic formulae for the line-of-sight velocity dispersion in the intermediate regime ($a_i \sim a_e \sim a_0$). This allows for a much improved comparison of MOND with observed velocity dispersions of stellar systems. We finally derive the velocity dispersion of the globular cluster Pal 14 as one of the outer Milky Way halo globular clusters that have recently been proposed as a differentiator between Newtonian and MONDian dynamics.
description: 11 pages, 9 figures, Accepted in MNRAS
Hadron-nuclei collisions at high energies
Creators: name: G. Giacomelli
Publisher: name: Rom.Rep.Phys.60:193-204,2008
Year: 2008

description: A brief historical review is made of the hadron-hadron (hh) total cross
section and hadron-nucleus absorption cross section measurements, made mainly
at high energy proton synchrotrons. Then I shall discuss low p_tprocesses,
including diffraction processes and fragmentation of nuclei in nucleus-nucleus
collisions. Nucleus-nucleus collisions at higher energy colliders are then
considered, mainly in the context of the search for the gluon quark plasma.
Conclusions and a short discussion on perspectives follow.
Additional file 1: of Highly Stretchable All-Rubber-Based Thread-Shaped Wearable Electronics for Human Motion Energy-Harvesting and Self-Powered Biomechanical Tracking
Creators: name: Zhu, Jie
name: Wang, Xinghui
name: Xing, Yilan
name: Li, Jianyi
Publisher: name: figshare
Year: 2019
Subjects: subject: Biophysics
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Physiology
subject: Evolutionary Biology
subject: Information Systems not elsewhere classified
subject: Developmental Biology
subject: Hematology
subject: Infectious Diseases
subject: FOS: Health sciences
subject: Virology

description: Figure S1. The output voltages as a function of external load resistances from 1 MÎŠ to 1 GÎŠ. Figure S2. The output performances stability testing of the SPST is conducted for 10,000 cycles. (DOCX 15855 kb)
Il gigante addormentato
Creators: Elisa Nichelli
Publisher: name: Media Inaf
Year: 2016

La galassia NGC 4889 è apparentemente tranquilla, ma nel suo cuore si nasconde un vero e proprio gigante cosmico: un buco nero supermassiccio che contiene al suo interno la bellezza di 21 miliardi di volte la massa del Sole. La sua esistenza ci permette di capire meglio come e dove si sono formati i quasar
แนวทางการจัดสวัสดิการที่เหมาะสมสำหรับผู้สูงอายุแรงงานนอกระบบโดยการมีส่วนร่วมของชุมชน กรณีศึกษา : บ้านคำเมย ตำบลดูน อำเภอกันทรารมย์ จังหวัดศรีสะเกษ
Creators: name: อานนท์ ตั้งพิทักษ์ไกร
Publisher: name: Program in Political Science, Faculty of Humanities and Social Sciences, Surindra Rajabhat University
Year: 2022
Subjects: การจัดสวัสดิการที่เหมาะสม
ผู้สูงอายุแรงงานนอกระบบ
การมีส่วนร่วมของชุมชน

description: วารสารการบริหารการปกครองและนวัตกรรมท้องถิ่น, 6, 1, 69-82
Philae, ci sei?
Creators: Fulvia Croci
Publisher: name: Media Inaf
Year: 2016

La sonda dell'ESA Rosetta non perde le speranze di ritrovare il piccolo lander sulla cometa Chury. Dopo aver analizzato i dati ricevuti nel corso degli 8 contatti, i tecnici hanno formulato tre possibili scenari che spiegherebbero le difficoltà di stabilire un contatto con Philae
Theory of the phonon broadening of impurity spectral lines.
Creators: name: Nishikawa, Kyoji
Publisher: name: University of British Columbia
Year: 2011

description: The theory of the phonon broadening of impurity spectral lines in homopolar semi-conductors is discussed within the framework of a Kubo-type formulation of the adiabatic dielectric susceptibility and the subsequent calculation of this using the double-time Green's function method. The basic assumption is the smallness of the interaction of the electrons (or holes) bound to impurity sites with the lattice vibrations. This interaction is then treated as a small perturbation of the independent systems of electron and vibrating lattice; the use of the adiabatic approximation is thereby avoided. The so-called decoupling of the infinite hierarchy of equations for the relevant Green's functions is discussed in detail and is given its justification in the present problem. In the case of nondegenerate electronic levels, the line-shape function is obtained explicitly in terms of the matrix elements of the electron-phonon interaction. It is found that the absorption line consists of a sharp peak with a width arising from a finite life-time of the unperturbed states due to the electron-phonon interaction and of a continuous background arising from the multi-phonon processes which accompany the optical absorption. In the degenerate case, a general method of obtaining the line-shape function is discussed and is illustrated in an example. The results are compared with those obtained by previous workers in the field. The general theory is applied to shallow impurity levels in silicon with the use of a modified hydrogenic model and a deformation potential description of the electron-phonon interaction; numerical estimates are made for typical contributions to the widths of the lines in both acceptor and donor cases.
Workshop: Marie Sklodowska-Curie Actions
Creators: name: Cazzato, Elisa
Publisher: name: Zenodo
Year: 2023
Subjects: MSCA, European funding, Horizon 2020, European grants

description: Fund your research and foster your career with the Marie Curie fellowships sponsored by the European Commission

The aim of these postdoctoral fellowships is to foster career development and excellence in research, and both European and U.S. scholars are eligible to apply for them. They are designed for researchers with a PhD in all disciplines who wish to carry out their research activities abroad, acquire new skills, and develop their careers. MSC-PFs help researchers gain experience in other countries, different disciplines, and nonacademic sectors. Interested researchers submit an application to the EU together with a host organization, which can be a university or a research institution based in an EU Member State. The MSC-PFs support the recruited researcher in the form of a living stipend, a travel allowance, and, if applicable, funds to support family members, long-term leave, and special needs. In addition, funding is provided for research, training, and networking activities, as well as management and indirect costs.

This workshop is addressed to potential fellows interested in applying for a period of research and training in Europe, supervisors who wish to sponsor a scholar from abroad at NYU, and administrative staff who want to receive additional information on the MSCA awards. Speakers will share their personal experiences and provide additional information about the program and how to apply.
การรับรู้สภาพแวดล้อมการควบคุมและประสิทธิผลการปฏิบัติงานของบุคลากรด้านการเงินและบัญชีของสำนักงานการเงินในหน่วยทหาร กองทัพภาคที่ 3
Creators: name: นภนิวิฐ เภตรา
Publisher: name: Program in Political Science, Faculty of Humanities and Social Sciences, Surindra Rajabhat University
Year: 2022
Subjects: การรับรู้
สภาพแวดล้อมการควบคุม
ประสิทธิผลการปฏิบัติงาน

description: วารสารการบริหารการปกครองและนวัตกรรมท้องถิ่น, 6, 1, 83-92
Stochastic Schrödinger equations with coloured noise
Creators: name: Barchielli, A.
name: Pellegrini, C.
name: Petruccione, F.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: A natural non-Markovian extension of the theory of white noise quantum trajectories is presented. In order to introduce memory effects in the formalism an Ornstein-Uhlenbeck coloured noise is considered as the output driving process. Under certain conditions a random Hamiltonian evolution is recovered. Moreover, non-Markovian stochastic Schrödinger equations which unravel non-Markovian master equations are derived.
description: 4pages, revtex
title: ÐÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÐ¸ Ð¿Ð¾Ð¸ÑÐºÐ° ÑÐ°ÑÑÐ¸Ñ ÑÐµÐ¼Ð½Ð¾Ð¹ Ð¼Ð°ÑÐµÑÐ¸Ð¸ Ð² ÑÐºÑÐ¿ÐµÑÐ¸Ð¼ÐµÐ½ÑÐ°Ñ CMS Ð¸ ATLAS, ÐÐ LHC
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·ÑÐ½Ð¸Ð½, ÐÐ»Ð°Ð´Ð¸ÑÐ»Ð°Ð²
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2018
Subjects: ÑÐµÐ¼Ð½Ð°Ñ Ð¼Ð°ÑÐµÑÐ¸Ñ
ÐºÐ°Ð½Ð´Ð¸Ð´Ð°ÑÑ Ð½Ð° ÑÐ¾Ð»Ñ ÑÐµÐ¼Ð½Ð¾Ð¹ Ð¼Ð°ÑÐµÑÐ¸Ð¸
Ð½ÐµÐ¹ÑÑÐ¸Ð½Ð¾

description: Ð¦ÐµÐ»Ñ ÑÐ°Ð±Ð¾ÑÑ â Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¸Ðµ Ð½Ð°ÑÑÐ½Ð¾Ð³Ð¾ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐºÑÐ¿ÐµÑÐ¸Ð¼ÐµÐ½ÑÐ¾Ð² Ð¿Ð¾ Ð¿Ð¾Ð¸ÑÐºÑ ÑÐ°ÑÑÐ¸Ñ ÑÐµÐ¼Ð½Ð¾Ð¹ Ð¼Ð°ÑÐµÑÐ¸Ð¸. ÐÐ·Ð½Ð°ÐºÐ¾Ð¼Ð»ÐµÐ½Ð¸Ðµ Ñ ÑÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¸Ð¼Ð¸ Ð¿ÑÐµÐ´Ð¿Ð¾ÑÑÐ»ÐºÐ°Ð¼Ð¸ Ðº ÑÑÑÐµÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐµÐ¼Ð½Ð¾Ð¹ Ð¼Ð°ÑÐµÑÐ¸Ð¸. Ð Ð°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ð¸Ðµ Ð¼ÐµÑÐ¾Ð´Ð¾Ð² Ð¿Ð¾Ð¸ÑÐºÐ° ÑÐµÐ¼Ð½Ð¾Ð¹ Ð¼Ð°ÑÐµÑÐ¸Ð¸ Ð¸ Ð¸Ñ Ð¾ÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÐµÐ¹. Ð Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ Ð¾Ð¿Ð¸ÑÐ°Ð½Ñ ÑÑÑÐ°ÑÐµÐ³Ð¸Ð¸ Ð¿Ð¾Ð¸ÑÐºÐ° ÑÐ°ÑÑÐ¸Ñ ÑÐµÐ¼Ð½Ð¾Ð¹ Ð¼Ð°ÑÐµÑÐ¸Ð¸ Ð½Ð° ÐÐÐÐµ Ð¸ Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ñ Ð²ÐµÑÑÐ½Ð¸Ðµ Ð¿ÑÐµÐ´ÐµÐ»Ñ Ð´Ð»Ñ ÑÐµÑÐµÐ½Ð¸Ð¹ ÑÐ¾Ð¶Ð´ÐµÐ½Ð¸Ñ ÑÐ°ÑÑÐ¸Ñ ÑÐµÐ¼Ð½Ð¾Ð¹ Ð¼Ð°ÑÐµÑÐ¸Ð¸ Ð¿ÑÐ¸ ÑÑÐ¾Ð¼ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ñ ÑÐºÑÐ¿ÐµÑÐ¸Ð¼ÐµÐ½ÑÐ°Ð»ÑÐ½ÑÐµ Ð´Ð°Ð½Ð½ÑÐµ, Ð¿Ð¾Ð»ÑÑÐµÐ½Ð½ÑÐµ Ð² 2015-2016 Ð³Ð³. ÑÐºÑÐ¿ÐµÑÐ¸Ð¼ÐµÐ½ÑÐ°Ð¼Ð¸ CMS Ð¸ ATLAS. ÐÐ° Ð´Ð°Ð½Ð½ÑÐ¹ Ð¼Ð¾Ð¼ÐµÐ½Ñ Ð¿ÑÐ¾ÑÐ¾Ð´Ð¸Ñ Ð¾Ð±ÑÑÐ¶Ð´ÐµÐ½Ð¸Ñ Ð´Ð°Ð»ÑÐ½ÐµÐ¹ÑÐ¸Ñ Ð¿ÐµÑÑÐ¿ÐµÐºÑÐ¸Ð² Ð¿Ð¾Ð¸ÑÐºÐ° ÑÐµÐ¼Ð½Ð¾Ð¹ Ð¼Ð°ÑÐµÑÐ¸Ð¸.
title: ÐÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð¾ÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÐµÐ¹ ÑÐ¸Ð·Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÑÐ¾Ð²Ð½Ñ Ð¡Ð¨Ð ÑÐ¸ÑÑÐµÐ¼Ñ ÑÐ±Ð¾ÑÐ° Ð´Ð°Ð½Ð½Ñ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Ð°ÑÑÐ°ÐºÐ¾Ð²Ð°, 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: ÑÐ²ÐµÑÑ ÑÐ¸ÑÐ¾ÐºÐ¾Ð¿Ð¾Ð»Ð¾ÑÐ½ÑÐµ ÑÐ¸Ð³Ð½Ð°Ð»Ñ
Ð³Ð°ÑÑÑÐ¾Ð²Ñ Ð¸Ð¼Ð¿ÑÐ»ÑÑÑ
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Ð²ÐµÑÐ¾ÑÑÐ½Ð¾ÑÑÑ Ð¾ÑÐ¸Ð±ÐºÐ¸

description: Ð Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ Ð¾ÑÑÐ°Ð¶ÐµÐ½Ð° ÑÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ñ Ð¸Ð¼Ð¸ÑÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ Ð¼Ð¾Ð´ÐµÐ»Ð¸ Ð¡Ð¨Ð ÑÐ¸ÑÑÐµÐ¼Ñ Ñ Ð¿Ð¾Ð¼Ð¾ÑÑÑ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð½Ð¾Ð¹ ÑÑÐµÐ´Ñ MATLAB. ÐÑÐ» Ð¿Ð¾ÐºÐ°Ð·Ð°Ð½ Ð¿ÑÐ¾ÑÐµÑÑ ÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¸ Ð¿ÑÐ¸ÐµÐ¼Ð° Ð¡Ð¨Ð ÑÐ¸Ð³Ð½Ð°Ð»Ð°, ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½ ÑÐ¾ÑÐ¼Ð°Ñ Ð¿Ð°ÐºÐµÑÐ¾Ð² ÑÐ¸Ð·Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¸ ÐºÐ°Ð½Ð°Ð»ÑÐ½Ð¾Ð³Ð¾ ÑÑÐ¾Ð²Ð½ÐµÐ¹. Ð¡ Ð¿Ð¾Ð¼Ð¾ÑÑÑ Ð¸Ð¼Ð¸ÑÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ Ð¼Ð¾Ð´ÐµÐ»Ð¸ Ð±ÑÐ»Ð¸ ÑÐ½ÑÑÑ Ð·Ð°Ð²Ð¸ÑÐ¸Ð¼Ð¾ÑÑÐ¸ Ð²ÐµÑÐ¾ÑÑÐ½Ð¾ÑÑÐ¸ Ð¾ÑÐ¸Ð±ÐºÐ¸ Ð¸ Ð²ÐµÑÐ¾ÑÑÐ½Ð¾ÑÑÐ¸ Ð´Ð¾ÑÑÐ°Ð²ÐºÐ¸ Ð¾Ñ Ð¾ÑÐ½Ð¾ÑÐµÐ½Ð¸Ñ ÑÐ¸Ð³Ð½Ð°Ð»-ÑÑÐ¼, Ð¾Ñ Ð´Ð»Ð¸Ð½Ñ Ð¿ÑÐµÐ°Ð¼Ð±ÑÐ»Ñ, ÐºÐ¾Ð»Ð¸ÑÐµÑÑÐ²Ð° Ð¿ÐµÑÐµÐ´Ð°ÑÑÐ¸ÐºÐ¾Ð² Ð¸ ÐºÐ¾Ð»Ð¸ÑÐµÑÑÐ²Ð° Ð¿Ð¾Ð²ÑÐ¾ÑÐ¾Ð² Ð¿Ð°ÐºÐµÑÐ¾Ð².
Role of Coulomb interaction in the superconducting properties of CaC6 and H under pressure
Creators: name: Massidda, S.
name: Bernardini, F.
name: Bersier, C.
name: Continenza, A.
name: Cudazzo, P.
name: Floris, A.
name: Glawe, H.
name: Monni, M.
name: Pittalis, S.
name: Profeta, G.
name: Sanna, A.
name: Sharma, S.
name: Gross, E. K. U.
Publisher: name: arXiv
Year: 2008
Subjects: subject: Superconductivity (cond-mat.supr-con)
subject: FOS: Physical sciences

description: Superconductivity in intercalated graphite CaC6 and H under extreme pressure, in the framework of superconducting density functional theory, is discussed. A detailed analysis on how the electron-phonon and electron-electron interactions combine together to determine the superconducting gap and critical temperature of these systems is presented. In particular, we discuss the effect on the calculated Tc of the anisotropy of the electron-phonon interaction and of the different approximations for screening the Coulomb repulsion. These results contribute to the understanding of multigap and anisotropic superconductivity, which has received a lot of attention since the discovery of MgB2, and show how it is possible to describe the superconducting properties of real materials on a fully ab-initio basis.
description: 13 pages, 5 figures
Flavor asymmetry of the nucleon
Creators: name: R. Bijker
name: E. Santopinto
Publisher: name: INFN Open Access Repository
Year: 2008

description: The flavor asymmetry of the nucleon sea is discussed in an unquenched quark
model for baryons in which the effects of quark-antiquark pairs (u anti-u, d
anti-d and s anti-s) are taken into account in an explicit form. The inclusion
of q anti-q pairs leads automatically to an excess of anti-d over anti-u quarks
in the proton, in agreement with experimental data.
Un senso in più
Creators: Marco Malaspina
Publisher: name: Media Inaf
Year: 2016

Quello che le due “orecchie” laser di LIGO ci hanno regalato oggi non è solo la conferma dell’esistenza delle onde gravitazionali. È anche un senso nuovo di zecca. Per la prima volta nella storia dell’umanità, alla vista elettromagnetica s’è aggiunto l’udito gravitazionale. Ora possiamo iniziare a usarli insieme
title: ÐÐ½Ð°Ð»Ð¸Ð· Ð¸Ð½Ð´ÑÑÑÑÐ¸Ð¸ ÐºÑÐ°ÑÐ¾ÑÑ Ð² ÐÑÐ¿Ð°Ð½Ð¸Ð¸
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ¾ÑÐµÐ½Ñ, 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: 2017
Subjects: ÐºÑÐ°ÑÐ¾ÑÐ°
Ð¸Ð½Ð´ÑÑÑÑÐ¸Ñ
ÐºÐ¾ÑÐ¼ÐµÑÐ¸ÐºÐ°
ÑÐ°Ð»Ð¾Ð½ ÐºÑÐ°ÑÐ¾ÑÑ
ÐºÐ¾ÑÐ¿Ð¾ÑÐ°ÑÐ¸Ñ

description: ÐÐ°Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° ÑÐ¾Ð´ÐµÑÐ¶Ð¸Ñ Ð² ÑÐµÐ±Ðµ Ð°Ð½Ð°Ð»Ð¸ÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð´Ð°Ð½Ð½ÑÐµ Ð¾Ð± Ð¸Ð½Ð´ÑÑÑÑÐ¸Ð¸ ÐºÑÐ°ÑÐ¾ÑÑ Ð² ÐÑÐ¿Ð°Ð½Ð¸Ð¸. Ð¡ÑÐ°Ð²Ð¸Ñ Ð¿ÐµÑÐµÐ´ ÑÐ¾Ð±Ð¾Ð¹ ÑÐµÐ»Ñ Ð¾Ð¿Ð¸ÑÐ°ÑÑ Ð¾Ð±ÑÐµÐ¼ ÐºÐ¾ÑÐ¼ÐµÑÐ¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÑÐ½ÐºÐ° Ð¸ Ð¿ÑÐ¾Ð¼ÑÑÐ»ÐµÐ½Ð½Ð¾ÑÑÐ¸ Ð² ÑÑÑÐ°Ð½Ðµ, Ð²ÑÐ²ÐµÑÑÐ¸ Ð¿ÐµÑÑÐ¿ÐµÐºÑÐ¸Ð²Ñ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ.
Additional file 2: of Protocol for a process evaluation of a cluster randomized controlled trial of the Learning Club intervention for women's health, and infant's health and development in rural Vietnam
Creators: name: Fisher, Jane
name: Nguyen, Trang
name: Tran, Thach
name: Tran, Ha
name: Tran, Tuan
name: Luchters, Stanley
name: Hipgrave, David
name: Hanieh, Sarah
name: Biggs, Beverley-Ann
Publisher: name: figshare
Year: 2019
Subjects: subject: Medicine
subject: Cell Biology
subject: Sociology
subject: FOS: Sociology
subject: Developmental Biology
subject: Cancer
subject: Science Policy
subject: Infectious Diseases
subject: FOS: Health sciences
subject: Computational Biology

description: Indicators for assessing quality of maternal and newborn health services (DOCX 15 kb)
Study of positrons from cosmic rays interactions and cold dark matter
  annihilations in the galactic environment
Creators: name: Lineros, Roberto A.
Publisher: name: INFN Open Access Repository
Year: 2009

description: Positron and electron cosmic rays provide a complementary way to study the
galactic environment. The actual cosmic rays experiments, for instance PAMELA
and HEAT, have presented very exciting results in this field. The observed
positron fraction appears larger than the actual theoretical predictions for
energies larger than 10 GeV. The indirect evidences of Dark Matter in
connection with Beyond the Standard Model theories would suggest the existence
of an extra contribution present in the cosmic ray signal. We study and
calculate the positron signal produced by the annihilation of a generic Dark
Matter candidate. Especially, We analyze typical annihilation signatures and
the impact of CR propagation physics on the positron signal. In addition, we
study the positron signal related to spallation processes between nuclei
cosmic--rays and the interstellar gas. We analyze the effects of uncertainties
present in nuclear cross section, nuclei cosmic--ray and CR propagation
physics. The propagation of positrons is modeled according to the Two--Zone
Propagation Model which has been successfully tested in the study of nuclei
cosmic--ray and present an analytical approach to study the cosmic--ray
physics.
Openscapes: Supporting kinder science for future us
Creators: name: Lowndes, Julie
Publisher: name: Zenodo
Year: 2023
Subjects: Openscapes
Open Science
NOAA
NASA

description: A talk for Women in Data Science Conference, Stanford University (video, 15 mins) Abstract: At Openscapes, we believe open science can accelerate interoperable, data-driven solutions and increase diversity, equity, inclusion, and belonging in research and beyond. Our main activity is mentoring environmental and Earth science teams in open science, and connecting and elevating these researchers both through tech like R, Python, Quarto, and JupyterHubs and communities like RLadies, Black Women in Ecology Evolution, and Marine Science, Ladies of Landsat, and NASA. We will share stories and approaches about open science as a daily practice – better science for future us – and welcome you to join the movement.
Possible Interpretations of the High Energy Cosmic Ray Electron Spectrum measured with the Fermi Space Telescope
Creators: name: Grasso, Dario
name: For The Fermi-LAT Collaboration
Publisher: name: INFN Open Access Repository
Year: 2009

description: The Fermi Large Area Telescope has provided the measurement of the high
energy (20 GeV to 1 TeV) cosmic ray electrons and positrons spectrum with
unprecedented accuracy. This measurement represents a unique probe for studying
the origin and diffusive propagation of cosmic rays as well as for looking for
possible evidences of Dark Matter. In this contribution we focus mainly on
astrophysical sources of cosmic ray electrons and positrons which include the
standard primary and secondary diffuse galactic contribution, as well as nearby
point-sources which are expected to contribute more significantly to higher
energies. In this framework, we discuss possible interpretations of Fermi
results in relation with other recent experimental data on energetic electrons
and positrons (specifically the most recent ones reported by PAMELA, ATIC,
PPB-BETS and H.E.S.S.).
Dust in the York Canonical Basis of ADM Tetrad Gravity: the Problem of
  Vorticity
Creators: name: Alba, David
name: Lusanna, Luca
Publisher: name: INFN Open Access Repository
Year: 2011

description: Brown's formulation of dynamical perfect fluids in Minkowski space-time is
extended to ADM tetrad gravity in globally hyperbolic, asymptotically
Minkowskian space-times. For the dust we get the Hamiltonian description in
closed form in the York canonical basis, where we can separate the inertial
gauge variables of the gravitational field in the non-Euclidean 3-spaces of
global non-inertial frames from the physical tidal ones. After writing the
Hamilton equations of the dust, we identify the sector of irrotational motions
and the gauge fixings forcing the dust 3-spaces to coincide with the 3-spaces
of the non-inertial frame. The role of the inertial gauge variable York time
(the remnant of the clock synchronization gauge freedom) is emphasized. Finally
the Hamiltonian Post-Minkowskian linearization is studied. The future
application of this formalism will be the study of cosmological back-reaction
(as an alternative to dark energy) in the York canonical basis.
Another cluster of red supergiants close to RSGC1
Creators: name: Negueruela, Ignacio
name: Gonzalez-Fernandez, Carlos
name: Marco, Amparo
name: Clark, J. Simon
name: Martinez-Nunez, Silvia
Publisher: name: arXiv
Year: 2010
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Recent studies have revealed massive star clusters in a region of the Milky Way close to the tip of the Long Bar. These clusters are heavily obscured and are characterised by a population of red supergiants. We analyse a previously unreported concentration of bright red stars ~16' away from the cluster RSGC1. We utilised near IR photometry to identify candidate red supergiants and then K-band spectroscopy of a sample to characterise their properties. We find a compact clump of eight red supergiants and five other candidates at some distance, one of which is spectroscopically confirmed as a red supergiant. These objects must form an open cluster, which we name Alicante 8. Because of the high reddening and strong field contamination, the cluster sequence is not clearly seen in 2MASS or UKIDSS near-IR photometry. From the analysis of the red supergiants, we infer an extinction $A_{K_{\rm S}}=1.9$ and an age close to 20 Myr. Though this cluster is smaller than the three known previously, its properties still suggest a mass in excess of 10 000 $M_{\sun}$. Its discovery corroborates the hypothesis that star formation in this region has happened on a wide scale between ~10 and ~20 Myr ago.
description: Accepted for publication in Astronomy & Astrophysics. Figure 1 degraded and changed to B&W, Figure 2 degraded to meet size requirements
Event-related potentials of social comparisons in depression and social anxiety
Creators: name: Paz, Valentina
name: Nicolaisen, Eliana
name: Fernández-Theoduloz, Gabriela
name: Pérez, Alfonso
name: Cervantes-Constantino, Francisco
name: Martinez-Montes, Eduardo
name: Kessel, Dominique
name: Cabana, Alvaro
name: Gradin, Victoria Beatriz
Publisher: name: Forschungzentrum Jülich
Year: 2023

description: doi:10.21203/rs.3.rs-2762762/v1
description: Social comparison is central in human life and can be especially challenging in depression and social anxiety. We assessed event-related potentials and emotions when receiving feedback on both their own and a co-player’s performance, in participants with depression and/or social anxiety (n=63) and healthy controls (n=72). Participants reported more negative emotions for downward (being better than someone else) and upward (being worse) comparisons vs. even outcomes, with these effects being stronger in depression and social anxiety. At the Medial Frontal Negativity, both controls and depressed participants showed enhanced negativity for upward (participant wrong, co-player correct) comparison vs. both the participant and co-player performing wrong. Socially anxious subjects showed the opposite effect, possibly due to greater expectations about being worse than others. The P300 decreased for downward and upward comparisons compared to even outcomes, which may relate to the higher levels of conflict of social inequality. Depressed and socially anxious subjects showed a blunted P300 increase over time in response to the task outcomes, suggesting deficits in allocating resources for the attention of incoming social information. This may relate to difficulties in these disorders in learning how to deal with the cognitive/emotional demands of social comparison.
Nuove frontiere per l’astrofisica
Creators: Nichi D'Amico
Publisher: name: Media Inaf
Year: 2016

Un risultato da Nobel, quello annunciato oggi dalla collaborazione LIGO-Virgo, scrive il presidente dell'INAF Nichi D'Amico, congratulandosi con il team internazionale che ha rilevato per la prima volta in modo diretto le onde gravitazionali. Un risultato che inaugura un nuovo “canale” per osservare l’Universo
Cos’è che ha “sollevato l’onda”? Il ruolo dell’INAF
Creators: Ufficio stampa Inaf
Publisher: name: Media Inaf
Year: 2016

Con l’annuncio ufficiale della prima rivelazione di un’onda gravitazionale da parte dell’interferometro LIGO, si apre una nuova era per la ricerca astrofisica, in cui l’Italia con Istituto Nazionale di Astrofisica gioca un ruolo da protagonista a livello mondiale. Nicolò D'Amico, presidente INAF: «Una scoperta epocale che apre nuovi orizzonti per l’astrofisica e vede il nostro Istituto già proiettato nelle osservazioni delle possibili sorgenti di onde gravitazionali nell’universo»
Onde gravitazionali alla portata di tutti
Creators: Elisa Nichelli
Publisher: name: Media Inaf
Year: 2016

È la notizia del giorno, nonché la scoperta del secolo: l’esperimento LIGO (Laser Interferometer Gravitational-Wave Observatory) ha effettuato la prima osservazione diretta di onde gravitazionali. Ma cosa sono, come vengono emesse e da quali tipi di sorgenti? Un approfondimento per farvi un’idea più chiara su questi segnali cosmici sfuggenti
First ALICE results from heavy-ion collisions at the LHC
Creators: name: Dainese, Andrea
name: For The ALICE Collaboration
Publisher: name: INFN Open Access Repository
Year: 2011

description: The ALICE detector recorded Pb-Pb collisions at sqrtsNN = 2.76 TeV at the LHC
in November-December 2010. We present the results of the measurements that
provide a first characterization of the hot and dense state of
strongly-interacting matter produced in heavy-ion collisions at these energies.
In particular, we describe the measurements of the particle multiplicity,
collective flow, Bose-Einstein correlations, high-momentum suppression, and
their dependence on the collision centrality. These observables are related to
the energy density, the size, the viscosity, and the opacity of the system.
Finally, we give an outlook on the upcoming results, with emphasis on heavy
flavour production.
Onde gravitazionali: la parola all’esperto
Creators: Elisa Nichelli
Publisher: name: Media Inaf
Year: 2016

La notizia del secolo è arrivata: abbiamo la prima osservazione diretta delle onde gravitazionali. Per comprendere meglio la portata della scoperta abbiamo intervistato Andrea Possenti, astrofisico dell'INAF - Osservatorio Astronomico di Cagliari
title: ÐÑÐ½Ð¾Ð²Ñ ÑÐ¸Ð·Ð¸ÑÐµÑÐºÐ¾Ð¹ Ñ Ð¸Ð¼Ð¸Ð¸
title: ÑÑÐµÐ±Ð½Ð¾-Ð¼ÐµÑÐ¾Ð´Ð¸ÑÐµÑÐºÐ¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ
titleType: Subtitle
Creators: name: ÐÐ°Ð½ÐºÐ¸Ð½Ð°, ÐÐ»Ð¾Ð½Ð°
name: Ð¡Ð¼ÑÑÑÐºÐ°Ñ, 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: 2020
Subjects: Ð¤Ð¸Ð·Ð¸ÑÐµÑÐºÐ°Ñ Ñ Ð¸Ð¼Ð¸Ñ

description: ÐÐ·Ð´Ð°Ð½Ð¸Ðµ ÑÐ¾Ð´ÐµÑÐ¶Ð¸Ñ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ð¸Ðµ ÑÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ð°, ÑÐ¾Ð¾ÑÐ²ÐµÑÑÑÐ²ÑÑÑÐ¸Ðµ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐ¼ ÑÐ°Ð·Ð´ÐµÐ»Ð°Ð¼ ÐºÑÑÑÐ°, Ð¸ Ð»Ð°Ð±Ð¾ÑÐ°ÑÐ¾ÑÐ½ÑÐ¹ Ð¿ÑÐ°ÐºÑÐ¸ÐºÑÐ¼, Ð¿Ð¾Ð·Ð²Ð¾Ð»ÑÑÑÐ¸Ð¹ Ð±Ð¾Ð»ÐµÐµ Ð³Ð»ÑÐ±Ð¾ÐºÐ¾ Ð¾ÑÐ²Ð¾Ð¸ÑÑ Ð¸Ð·ÑÑÐ°ÐµÐ¼ÑÐ¹ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð» Ð¿Ð¾ ÐºÑÑÑÑ Â«ÐÑÐ½Ð¾Ð²Ñ ÑÐ¸Ð·Ð¸ÑÐµÑÐºÐ¾Ð¹ ÑÐ¸Ð¼Ð¸Ð¸Â». ÐÐ¾ÑÐ¾Ð±Ð¸Ðµ ÑÐ¿Ð¾ÑÐ¾Ð±ÑÑÐ²ÑÐµÑ Ð·Ð°ÐºÑÐµÐ¿Ð»ÐµÐ½Ð¸Ñ Ð¿ÑÐ¸ÐºÐ»Ð°Ð´Ð½ÑÑ Ð¸ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°ÑÐµÐ»ÑÑÐºÐ¸Ñ Ð½Ð°Ð²ÑÐºÐ¾Ð² Ñ Ð¾Ð±ÑÑÐ°ÑÑÐ¸ÑÑÑ, ÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð½ÐµÐ¾Ð±ÑÐ¾Ð´Ð¸Ð¼ÑÑ ÐºÐ¾Ð¼Ð¿ÐµÑÐµÐ½ÑÐ¸Ð¹. Ð ÐºÐ°Ð¶Ð´Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ ÑÐ°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÑÑÑÑ ÐºÐ¾Ð½ÑÑÐ¾Ð»ÑÐ½ÑÐµ Ð²Ð¾Ð¿ÑÐ¾ÑÑ, Ð¾ÑÐ²Ð°ÑÑÐ²Ð°ÑÑÐ¸Ðµ Ð²ÑÐµ ÑÐ¾ÑÑÐ°Ð²Ð»ÑÑÑÐ¸Ðµ ÑÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÐºÑÑÑÐ°.
ÐÐ¾ÑÐ¾Ð±Ð¸Ðµ Ð¿ÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¾ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² Ð²ÑÐ·Ð¾Ð², Ð¾Ð±ÑÑÐ°ÑÑÐ¸ÑÑÑ Ð¿Ð¾ ÑÐºÑÑÐ¿Ð½ÐµÐ½Ð½Ð¾Ð¹ Ð³ÑÑÐ¿Ð¿Ðµ ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾ÑÑÐµÐ¹ 19.00.00 Â«ÐÑÐ¾Ð¼ÑÑÐ»ÐµÐ½Ð½Ð°Ñ ÑÐºÐ¾Ð»Ð¾Ð³Ð¸Ñ Ð¸ Ð±Ð¸Ð¾ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¸Â».
LIGO: cosa c’è dietro la scoperta
Creators: Eleonora Ferroni
Publisher: name: Media Inaf
Year: 2016

Si chiama Laser Interferometer Gravitational-Wave Observatory e si trova negli Stati Uniti. Parliamo di due potenti interferometri che riescono a percepire i minimi  cambiamenti nella geometria del tessuto spazio-temporale. Come funziona? Scopritelo con noi
title: Ð­ÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ°Ñ ÑÐµÐ¾ÑÐ¸Ñ
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ
titleType: Subtitle
Creators: name: ÐÑÑÐ¼Ð°Ð½, Ð¡Ð²ÐµÑÐ»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: 2020
Subjects: ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ°Ñ ÑÐµÐ¾ÑÐ¸Ñ
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description: ÐÐ¾ÑÐ¾Ð±Ð¸Ðµ ÑÐ¾Ð¾ÑÐ²ÐµÑÑÑÐ²ÑÐµÑ ÑÐµÐ´ÐµÑÐ°Ð»ÑÐ½Ð¾Ð¼Ñ Ð³Ð¾ÑÑÐ´Ð°ÑÑÑÐ²ÐµÐ½Ð½Ð¾Ð¼Ñ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°ÑÐµÐ»ÑÐ½Ð¾Ð¼Ñ ÑÑÐ°Ð½Ð´Ð°ÑÑÑ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ¾Ð² Ð¿Ð¾ Ð¿ÑÐ¾ÑÐ¸Ð»Ñ 38.03.01 Â«Ð­ÐºÐ¾Ð½Ð¾Ð¼Ð¸ÐºÐ°Â». Ð ÑÑÐµÐ±Ð½Ð¾Ð¼ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ð¸ Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ñ Ð·Ð°Ð´Ð°Ð½Ð¸Ñ, ÐºÐ¾ÑÐ¾ÑÑÐµ Ð¾ÑÐ²Ð°ÑÑÐ²Ð°ÑÑ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ ÑÐµÐ¼Ñ ÑÑÐ°Ð½Ð´Ð°ÑÑÐ½Ð¾Ð³Ð¾ ÐºÑÑÑÐ° Â«ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ°Ñ ÑÐµÐ¾ÑÐ¸ÑÂ»: Ð²Ð¾Ð¿ÑÐ¾ÑÑ Ð¼Ð¸ÐºÑÐ¾ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð°Ð½Ð°Ð»Ð¸Ð·Ð°. Ð Ð°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ñ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð²ÑÐ±Ð¾ÑÐ°: ÑÐµÐ¾ÑÐ¸Ñ Ð¿Ð¾Ð²ÐµÐ´ÐµÐ½Ð¸Ñ Ð¿Ð¾ÑÑÐµÐ±Ð¸ÑÐµÐ»ÐµÐ¹ Ð¸ ÑÑÐ½Ð¾ÑÐ½ÑÐ¹ ÑÐ¿ÑÐ¾Ñ, ÑÐµÐ¾ÑÐ¸Ñ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²Ð° Ð¸ Ð¸Ð·Ð´ÐµÑÐ¶ÐµÐº, ÑÐµÐ¾ÑÐ¸Ñ ÑÐµÐ½Ð¾Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ñ Ð² ÑÐ°Ð·Ð½ÑÑ ÑÑÑÑÐºÑÑÑÐ°Ñ ÑÑÐ½ÐºÐ¾Ð² Ð³Ð¾ÑÐ¾Ð²Ð¾Ð¹ Ð¿ÑÐ¾Ð´ÑÐºÑÐ¸Ð¸ (ÑÐ¾Ð²ÐµÑÑÐµÐ½Ð½Ð°Ñ ÐºÐ¾Ð½ÐºÑÑÐµÐ½ÑÐ¸Ñ, Ð¼Ð¾Ð½Ð¾Ð¿Ð¾Ð»Ð¸Ñ, Ð¼Ð¾Ð½Ð¾Ð¿Ð¾Ð»Ð¸ÑÑÐ¸ÑÐµÑÐºÐ°Ñ ÐºÐ¾Ð½ÐºÑÑÐµÐ½ÑÐ¸Ñ, Ð¾Ð»Ð¸Ð³Ð¾Ð¿Ð¾Ð»Ð¸Ñ). ÐÐ¾ ÐºÐ°Ð¶Ð´Ð¾Ð¹ ÑÐµÐ¼Ðµ Ð² Ð¿Ð¾ÑÐ¾Ð±Ð¸Ð¸ Ð¿ÑÐ¸Ð²ÐµÐ´ÐµÐ½Ñ Ð·Ð°Ð´Ð°Ð½Ð¸ÑÐ¼Ð¸ Ð¼Ð½Ð¾Ð¶ÐµÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð²ÑÐ±Ð¾ÑÐ° (ÑÐµÑÑÑ) Ð¸ Ð·Ð°Ð´Ð°Ð½Ð¸Ñ Ð´Ð»Ñ ÑÐ°Ð¼Ð¾ÑÑÐ¾ÑÑÐµÐ»ÑÐ½Ð¾Ð³Ð¾ ÑÐµÑÐµÐ½Ð¸Ñ, ÑÐ°ÐºÐ¶Ðµ Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ñ Ð¼ÐµÑÐ¾Ð´Ð¸ÑÐµÑÐºÐ¸Ðµ ÑÐºÐ°Ð·Ð°Ð½Ð¸Ñ Ðº Ð½Ð°Ð¿Ð¸ÑÐ°Ð½Ð¸Ñ Ð ÐÐ , ÑÑÐ¾ ÑÐ¾Ð´ÐµÐ¹ÑÑÐ²ÑÐµÑ ÑÑÐ²Ð¾ÐµÐ½Ð¸Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÑ ÑÐµÐ¼ Ð´Ð¸ÑÑÐ¸Ð¿Ð»Ð¸Ð½Ñ Â«Ð­ÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ°Ñ ÑÐµÐ¾ÑÐ¸ÑÂ» Ð¸ Ð¸Ñ Ð¿ÑÐ¸ÐºÐ»Ð°Ð´Ð½Ð¾Ð¼Ñ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ñ. ÐÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ñ ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð°ÑÐ¸Ð¸ Ð¿Ð¾ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐµ ÐºÐ¾Ð½ÑÑÐ¾Ð»ÑÐ½Ð¾-Ð°ÑÑÐµÑÑÐ°ÑÐ¸Ð¾Ð½Ð½ÑÑ Ð¿ÐµÐ´Ð°Ð³Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ñ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ð¾Ð² Ð¿Ð¾ Ð´Ð¸ÑÑÐ¸Ð¿Ð»Ð¸Ð½Ðµ. ÐÐ¾ÑÐ¾Ð±Ð¸Ðµ Ð¿ÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¾ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² Ð´Ð½ÐµÐ²Ð½Ð¾Ð¹, Ð¾ÑÐ½Ð¾-Ð·Ð°Ð¾ÑÐ½Ð¾Ð¹ Ð¸ Ð·Ð°Ð¾ÑÐ½Ð¾Ð¹ ÑÐ¾ÑÐ¼ Ð¾Ð±ÑÑÐµÐ½Ð¸Ñ Ð¿ÑÐ¸ Ð¸Ð·ÑÑÐµÐ½Ð¸Ð¸ ÐºÑÑÑÐ° Â«Ð¡ÐµÐ¼Ð¸Ð½Ð°Ñ Ð¿Ð¾ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ð¹ ÑÐµÐ¾ÑÐ¸Ð¸Â».
Albert sul surf
Creators: Francesca Aloisio
Publisher: name: Media Inaf
Year: 2016

L’esattezza dell’intuizione che Einstein ebbe 100 anni fa è stata confermata dalla prima misurazione diretta delle onde gravitazionali. Ma come venne in mente al buon Albert di formulare tale teoria e, soprattutto, cosa direbbe alla luce dei risultati giunti oggi da LIGO? Non essendo semplice procedere a un’intervista con l’altro mondo, ci siamo rivolti a qualcuno che, in questo, su Einstein, il suo carattere e la sua vita ha scritto un libro divertente: Vincenzo Palermo, autore di “La versione di Albert”
title: Job. Join Our Business
title: a Text-Book for Students of Business
titleType: Subtitle
Creators: name: ÐÐ°Ð½ÐºÐµÐ²Ð¸Ñ, ÐÐµÐ¾Ð½Ð¸Ð´
name: ÐÐµÑÑÐ¾Ð²Ð°, ÐÐ»ÑÐ³Ð°
Publisher: name: [SPbSTU]
Year: 1996
Subjects: Ð°Ð½Ð³Ð»Ð¸Ð¹ÑÐºÐ¸Ð¹ ÑÐ·ÑÐº
ÑÑÐµÐ±Ð½Ð¸ÐºÐ¸ Ð¸ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ñ Ð´Ð»Ñ Ð²ÑÐ·Ð¾Ð²

description: Ð£ÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ JOB Ð¿ÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¾ Ð´Ð»Ñ Ð¾Ð±ÑÑÐ°ÑÑÐ¸ÑÑÑ Ð¿ÑÐ¾Ð´Ð²Ð¸Ð½ÑÑÐ¾Ð³Ð¾ ÑÐ·ÑÐºÐ¾Ð²Ð¾Ð³Ð¾ ÑÑÐ¾Ð²Ð½Ñ. ÐÐ½Ð¾ Ð¼Ð¾Ð¶ÐµÑ Ð±ÑÑÑ ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð¾Ð²Ð°Ð½Ð¾ Ð´Ð»Ñ Ð²ÑÐ·Ð¾Ð²ÑÐºÐ¸Ñ Ð³ÑÑÐ¿Ð¿ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¸Ñ ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾ÑÑÐµÐ¹ (ÑÑÐ¾Ð²ÐµÐ½Ñ Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ°) Ð¸ Ð¸Ð½Ð¶ÐµÐ½ÐµÑÐ½ÑÑ ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾ÑÑÐµÐ¹ (ÑÑÐ¾Ð²Ð½Ð¸ Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ° Ð¸ Ð¼Ð°Ð³Ð¸ÑÑÑÐ°), ÑÑÐ°ÑÐ¸ÑÑÑ ÑÐºÐ¾Ð» Ð¸ ÐºÐ¾Ð»Ð»ÐµÐ´Ð¶ÐµÐ¹ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ð¹ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð½Ð¾ÑÑÐ¸, ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² ÐºÑÑÑÐ¾Ð² Ð¸Ð½Ð¾ÑÑÑÐ°Ð½Ð½ÑÑ ÑÐ·ÑÐºÐ¾Ð², Ð° ÑÐ°ÐºÐ¶Ðµ Ð´Ð»Ñ ÑÐ°Ð¼Ð¾ÑÑÐ¾ÑÑÐµÐ»ÑÐ½Ð¾Ð³Ð¾ Ð¸Ð·ÑÑÐµÐ½Ð¸Ñ ÑÐ·ÑÐºÐ°. Ð¦ÐµÐ»ÑÑ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ñ ÑÐ²Ð»ÑÐµÑÑÑ ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑÐ½Ð¾Ðµ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ðµ Ð½Ð°Ð²ÑÐºÐ¾Ð² ÑÑÐµÐ½Ð¸Ñ Ð¸ ÑÑÑÐ½Ð¾Ð¹ ÑÐµÑÐ¸, Ð° ÑÐ°ÐºÐ¶Ðµ Ð·Ð½Ð°ÑÐ¸ÑÐµÐ»ÑÐ½Ð¾Ðµ ÑÐ°ÑÑÐ¸ÑÐµÐ½Ð¸Ðµ Ð°ÐºÑÐ¸Ð²Ð½Ð¾Ð³Ð¾ Ð²Ð¾ÐºÐ°Ð±ÑÐ»ÑÑÐ°, ÑÐ²ÑÐ·Ð°Ð½Ð½Ð¾Ð³Ð¾ Ñ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸ÐµÐ¹ ÑÑÑÐ´Ð° Ð¸ Ð±Ð¸Ð·Ð½ÐµÑÐ°, Ð¿ÑÐ¸ÑÐ¾Ð»Ð¾Ð³Ð¸ÐµÐ¹ Ð»Ð¸ÑÐ½Ð¾ÑÑÐ¸, ÑÐ°Ð±Ð¾ÑÐ¾Ð¹ Ñ ÐºÐ°Ð´ÑÐ°Ð¼Ð¸. ÐÐ¾ÑÐ¾Ð±Ð¸Ðµ ÑÐ¾Ð´ÐµÑÐ¶Ð¸Ñ 12 ÑÐ°ÑÑÐµÐ¹ (units), Ð¿Ð¾ÑÐ»ÐµÐ´Ð¾Ð²Ð°ÑÐµÐ»ÑÐ½Ð¾ Ð¾ÑÑÐ°Ð¶Ð°ÑÑÐ¸Ñ Ð¿ÑÐ¾ÑÐµÑÑ ÑÑÑÐ´Ð¾ÑÑÑÑÐ¾Ð¹ÑÑÐ²Ð° Ð¸ ÑÐ°Ð±Ð¾ÑÑ. ÐÐ¾Ð»ÑÑÐ°Ñ ÑÐ°ÑÑÑ Ð·Ð°Ð´Ð°Ð½Ð¸Ð¹ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ñ Ð¸Ð¼ÐµÐµÑ ÑÐ²Ð¾ÑÑÐµÑÐºÐ¸Ð¹ ÑÐ°ÑÐ°ÐºÑÐµÑ Ñ ÑÐµÐ»ÑÑ Ð¿Ð¾ÑÐ¾Ð¶Ð´ÐµÐ½Ð¸Ñ ÑÐ²Ð¾Ð±Ð¾Ð´Ð½ÑÑ Ð¼Ð¾Ð½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ñ Ð¸ Ð´Ð¸Ð°Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ñ ÐµÐ´Ð¸Ð½ÑÑÐ². Ð¤Ð¾ÑÐ¼Ð°Ð»ÑÐ½Ð°Ñ ÑÐ°ÑÑÑ Ð¸Ñ Ð·Ð°Ð´Ð°ÐµÑÑÑ ÑÐ·ÑÐºÐ¾Ð²ÑÐ¼Ð¸ Ð¿Ð¾Ð´ÑÐºÐ°Ð·ÐºÐ°Ð¼Ð¸. ÐÑ Ð¸ÑÑÐ¾Ð´Ð¸Ð¼ Ð¸Ð· ÑÐ¾Ð³Ð¾, ÑÑÐ¾ Ð¾ÑÐ½Ð¾Ð²Ð½Ð°Ñ Ð¼Ð°ÑÑÐ° ÑÑÐµÐ±Ð½ÑÑ Ð´ÐµÐ¹ÑÑÐ²Ð¸Ð¹ Ð¿Ð¾ ÐºÐ½Ð¸Ð³Ðµ Ð´Ð¾Ð»Ð¶Ð½Ð° Ð¸Ð¼ÐµÑÑ ÑÐ°ÑÐ°ÐºÑÐµÑ Ð¿Ð°ÑÐ½ÑÑ ÑÐ¿ÑÐ°Ð¶Ð½ÐµÐ½Ð¸Ð¹ ÑÐ¾ ÑÐ¼ÐµÐ½Ð¾Ð¹ ÑÐ¾Ð»ÐµÐ¹. ÐÑÐ¸ ÑÐ°Ð¼Ð¾ÑÑÐ¾ÑÑÐµÐ»ÑÐ½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ Ð½Ð°Ð´ Ð¿Ð¾ÑÐ¾Ð±Ð¸ÐµÐ¼ ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´ÑÐµÑÑÑ ÑÐ°ÑÐµ Ð¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°ÑÑÑÑ Ð¿ÑÐ¸ÐµÐ¼Ð¾Ð¼ Ð¾Ð±ÑÐ°ÑÐ½Ð¾Ð³Ð¾ Ð¿ÐµÑÐµÐ²Ð¾Ð´Ð° Ð¸ ÑÐ°Ð¼Ð¾ÐºÐ¾Ð½ÑÑÐ¾Ð»Ñ Ð¿Ð¾ Ð¿Ð¾Ð´ÑÐºÐ°Ð·ÐºÐ°Ð¼. ÐÐ¾ÑÐ¾Ð±Ð¸Ðµ ÑÐ¾Ð´ÐµÑÐ¶Ð¸Ñ Ð±Ð¾Ð»ÑÑÐ¾Ðµ ÐºÐ¾Ð»Ð¸ÑÐµÑÑÐ²Ð¾ Ð»ÐµÐºÑÐ¸ÐºÐ¾-Ð³ÑÐ°Ð¼Ð¼Ð°ÑÐ¸ÑÐµÑÐºÐ¸Ñ Ð¿Ð¾Ð´ÑÐºÐ°Ð·Ð¾Ðº Ð½ÐµÐ¿Ð¾ÑÑÐµÐ´ÑÑÐ²ÐµÐ½Ð½Ð¾ Ð¿Ð¾ÑÐ»Ðµ ÐºÐ°Ð¶Ð´Ð¾Ð³Ð¾ ÑÐµÐºÑÑÐ°, Ð° ÑÐ°ÐºÐ¶Ðµ ÐºÐ»ÑÑÐµÐ¹ Ðº ÑÐ¿ÑÐ°Ð¶Ð½ÐµÐ½Ð¸ÑÐ¼ Ð½Ð° Ð¿ÐµÑÐµÐ²Ð¾Ð´ Ð¸ ÑÐµÑÑÐ°Ð¼, Ð¿ÑÐ¸Ð²ÐµÐ´ÐµÐ½Ð½ÑÑ Ð² ÐºÐ¾Ð½ÑÐµ ÐºÐ½Ð¸Ð³Ð¸. ÐÐ½Ð¾Ð³Ð¸Ðµ ÑÐ»Ð¾Ð²Ð° Ð¼Ð¾Ð¶Ð½Ð¾ ÑÐ·Ð½Ð°ÑÑ Ð¸Ð· Unit 11, Ð³Ð´Ðµ Ð´Ð°Ð½Ñ ÑÐ°ÑÑÐ¸ÑÑÐ¾Ð²ÐºÐ¸ ÑÐ¾ÐºÑÐ°ÑÐµÐ½Ð¸Ð¹, Ð¿ÑÐ¸Ð½ÑÑÑÑ Ð² Ð³Ð°Ð·ÐµÑÐ½ÑÑ Ð¾Ð±ÑÑÐ²Ð»ÐµÐ½Ð¸ÑÑ.
description: ÐÐµÑÐ°ÑÐ°ÐµÑÑÑ Ð¿Ð¾ ÑÐµÑÐµÐ½Ð¸Ñ ÑÐµÐ´Ð°ÐºÑÐ¸Ð¾Ð½Ð½Ð¾-Ð¸Ð·Ð´Ð°ÑÐµÐ»ÑÑÐºÐ¾Ð³Ð¾ ÑÐ¾Ð²ÐµÑÐ° Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¾Ð³Ð¾ Ð³Ð¾ÑÑÐ´Ð°ÑÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑÐ°.
Evaluation of Intelligent Traffic Management Systems for Prioritizing Emergency Vehicles in Crisis Conditions
Creators: name: zare sefat, sajjad
name: Ebadi, Zeynab
Publisher: name: figshare
Year: 2025
Subjects: classificationCode: 350902
subject: Intelligent mobility
classificationCode: 400599
subject: Civil engineering not elsewhere classified

description: Traffic congestion in major cities such as Tehran significantly affects response times for emergency vehicles, which can result in severe consequences. This paper evaluates the application of Intelligent Traffic Management Systems (ITMS) to prioritize emergency vehicles during crises. The study explores various detection and prioritization techniques, such as signal phase changes and route optimization based on the type of emergency. The proposed framework aims to guide emergency vehicles through less congested routes using real-time data and traffic signal manipulation, ultimately improving service delivery and reducing fatalities in emergency scenarios.
ALICE naviga nel brodo primordiale
Creators: Elisa Nichelli
Publisher: name: Media Inaf
Year: 2016

Grazie alle enormi energie sviluppate all’interno del rivelatore ALICE del Large Hadron Collider, è stato possibile ricostruire le condizioni in cui si trovava l’Universo nei primi istanti della sua vita e di studiarne le caratteristiche fisiche. Con i commenti di Paolo Giubellino e di Federico Antinori
World-wide changes in the geomagnetic field
Creators: name: Nishida, Atsuhiro
Publisher: name: University of British Columbia
Year: 2011

description: The geomagnetic field is found to change quite frequently on a world-wide scale. In the three months' period near sunspot maximum, such changes are found on 90 "per cent of all days. Most of these changes are not registered either as sudden commencements or as sudden impulses, and are tentatively called in this thesis 'worldwide changes'. The frequent occurrence of world-wide changes seems to be consistent with the idea that world-wide features of the geomagnetic field are always influenced by a permanently flowing corpuscular stream from the sun. The physical state of the corpuscular stream may be as variable as that of the solar atmosphere, and sudden changes in it will give rise to sudden, world-wide changes in the geomagnetic field. The morphology of world-wide changes is studied, and the form of the change, the distribution of magnitude and the mode of spreading over the earth are clarified. It is found that world-wide changes can be classified into two groups according to the sign of the main part of the change which appears all over the world. Those with an increase in the total force are called positive changes and those with a decrease are called negative changes. Except for the sign of the change, negative changes are morphologically identicalto positive changes. Since the morphology of sudden commencements and sudden impulses is the same as that of world-wide changes, they must be produced by a common mechanism, and an explanation of negative changes is a new, fundamental requirement imposed upon any theory of these changes. The observed change in the geomagnetic field may originate at the magnetospheric boundary where the solar corpuscular stream interacts with the geomagnetic field. The change may be modulated by the screening effect of the ionosphere before it is observed at ground level. Although this effect has been shown to be negligible for changes with a time scale of the order of world-wide changes, incorrect assumptions have been made in existing theories. More accurate calculations show that this effect is actually significant for a certain mode of the incident field. [ ... ]
Observation of Half Quantum Vortices in an Exciton-Polariton Condensate
Creators: name: Lagoudakis, K. G.
name: Ostatnicky, T.
name: Kavokin, A. V.
name: Rubo, Y. G.
name: Andre, R.
name: Deveaud-Pledran, B.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Quantum Gases (cond-mat.quant-gas)
subject: FOS: Physical sciences

description: Singly quantized vortices have been already observed in many systems including the superfluid helium, Bose Einstein condensates of dilute atomic gases, and condensates of exciton polaritons in the solid state. Two dimensional superfluids carrying spin are expected to demonstrate a different type of elementary excitations referred to as half quantum vortices characterized by a pi rotation of the phase and a pi rotation of the polarization vector when circumventing the vortex core. We detect half quantum vortices in an exciton-polariton condensate by means of polarization resolved interferometry, real space spectroscopy and phase imaging. Half quantum vortices coexist with single quantum vortices in our sample.
Lorentz invariant quantization of the Yang-Mills theory free of Gribov ambiguity
Creators: name: Slavnov, A. A.
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: A new fomulation of the Yang-Mills theory which allows to avoid the problem of Gribov ambiguity of the gauge fixing is proposed.
description: 8 pages,no figures