cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
title: Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° ÑÑÑÐ°ÑÐµÐ³Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¿Ð»Ð°Ð½Ð° ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ (Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ ÐÐÐ Â«ÐÐ°Ð½ÑÐ°ÑÐ°Â»)
title: Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ»Ð°Ð´Ð¶ÑÐ½, Ð ÐµÐ±ÐµÐºÐ°
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ÑÑÐ°ÑÐµÐ³Ð¸Ñ
ÑÑÑÐ°ÑÐµÐ³Ð¸ÑÐµÑÐºÐ¸Ð¹ Ð¿Ð»Ð°Ð½
ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ðµ ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸
Ð²Ð½ÐµÑÐ½ÑÑ ÑÑÐµÐ´Ð°
ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÑ

description: ÐÐ±ÑÐµÐºÑ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ â ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ñ Â«ÐÐ°Ð½ÑÐ°ÑÐ°Â».
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Nucleon Form Factors from 5D Skyrmions
Creators: name: Panico, Giuliano
name: Wulzer, Andrea
Publisher: name: arXiv
Year: 2008
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Theory (hep-th)
subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: Several aspects of hadron physics are well described by a simple 5D effective field theory. Baryons arise in this scenario as "large" (and therefore calculable) 5D skyrmions. We extend and refine the existing analysis of this 5D soliton, which is fairly non-trivial due to the need of numerical methods. We perform the complete quantization of those collective coordinates which are relevant for computing the static observables like the nucleon form factors. We compare the result with simple expectations about large-N_c QCD and with the experimental data. An agreement within 30% is found.
description: 30 pages, 6 figures; v2: References added and typos corrected; v3: Version published in Nucl. Phys. A
Mars Express accarezza Phobos
Creators: Elisa Nichelli
Publisher: name: Media Inaf
Year: 2016

Il 14 gennaio la Sonda Mars Express dell’ESA ha sorvolato, a una distanza di appena 53 km dalla superficie, la più grande fra le lune di Marte. I dati raccolti durante questa delicata operazione forniranno informazioni con dettagli senza precedenti, utili anche per le future missioni. Il commento di Giancarlo Bellucci dell’INAF-IAPS di Roma
Direct capture reactions O16 (p,[gamma])F17 and D (p,[gamma])He3
Creators: name: Lal, Mohan
Publisher: name: University of British Columbia
Year: 2011

description: This thesis is concerned with two nuclear reactions which have astrophysical significance. First, for the reaction O¹⁶(p, γ)F¹⁷ a theoretical analysis of the currently available data has been made. Second, for the reaction D(p, γ)He³, experimental results have been obtained at lower energies than previously reported and a crude theoretical analysis of the data is presented. The analysis of the reaction O¹⁶(p, γ)F¹⁷ is based on a relatively simple nuclear model. The system, O¹⁶+p, is described in terms of a single particle wave function for the odd proton, moving in a potential provided by the O¹⁶ core. The proton is assumed to be captured directly from the continuum to one of the final bound states of F¹⁷ with the emission of gamma rays. A square well plus, coulomb potential is assumed to represent the interaction between the O¹⁶ core and the odd proton. A check on the bound state wave functions produced by the model was made by calculating the lifetime for the quadrupole transition between the 2s[subscript ½] first excited state and 1d[subscript 5/2] ground state. A similar check on the validity of the continuum wave functions given by the present model was made by comparing the O¹⁶(p,p)O¹⁶ scattering cross section predicted by the model with the experimental data of Eppling. For direct capture, the radial integrals for electric dipole transitions from continuum P-states to final 2s[subscript ½] and 1d[subscript 5/2] states were evaluated numerically for radii of 4.8 and 3.65 fermis. For 4.8 fermi radius, the absolute cross section, energy dependence and ratio of the transitions to the first excited and to the ground states are in good agreement with the experimental data. The cross sections for the 3.65 fermi radius are a factor of two low. For energies lower than 0.5 Mev, there is a considerable increase in the astrophysical S factor contributed by S[subscript s], corresponding to the first excited state transition, while S[subscript d], corresponding to the ground state transition remains practically constant over the whole energy range. [ ... ]
Quella pentola galattica sta per traboccare
Creators: Stefano Parisini
Publisher: name: Media Inaf
Year: 2016

La galassia più luminosa che si conosca ha problemi in cucina: lo spesso strato di polvere che circonda la fornace centrale provoca il surriscaldamento del gas interstellare. Se va avanti così, dicono gli scienziati che l’hanno analizzata con il radiotelescopio ALMA, le mancheranno gli ingredienti per sfornare nuove stelle
Local Multicoloring Algorithms: Computing a Nearly-Optimal TDMA Schedule in Constant Time
Creators: name: Kuhn, Fabian
Publisher: name: arXiv
Year: 2009
Subjects: subject: Discrete Mathematics (cs.DM)
subject: Data Structures and Algorithms (cs.DS)
subject: FOS: Computer and information sciences

description: The described multicoloring problem has direct applications in the context of wireless ad hoc and sensor networks. In order to coordinate the access to the shared wireless medium, the nodes of such a network need to employ some medium access control (MAC) protocol. Typical MAC protocols control the access to the shared channel by time (TDMA), frequency (FDMA), or code division multiple access (CDMA) schemes. Many channel access schemes assign a fixed set of time slots, frequencies, or (orthogonal) codes to the nodes of a network such that nodes that interfere with each other receive disjoint sets of time slots, frequencies, or code sets. Finding a valid assignment of time slots, frequencies, or codes hence directly corresponds to computing a multicoloring of a graph $G$. The scarcity of bandwidth, energy, and computing resources in ad hoc and sensor networks, as well as the often highly dynamic nature of these networks require that the multicoloring can be computed based on as little and as local information as possible.
Plutone: possibile criovulcanismo
Creators: Davide Coero Borga
Publisher: name: Media Inaf
Year: 2016

Il più grande di quelli che sono con tutta probabilità due criovulcani, individuato fin dalle prime rilevazioni di New Horizons, ora è ricostruito grazie a un'immagine composita ottenuta con i dati degli strumenti LORRI e Ralph: 150 chilometri di diametro, 4 di altezza e un solo grande cratere di recente formazione
title: ÐÐ¸Ð½Ð¸Ð¼Ð¸Ð·Ð°ÑÐ¸Ñ ÑÐ°ÑÑ Ð¾Ð´ÑÐµÐ¼Ð¾Ð³Ð¾ Ð¼ÐµÑÑÐ° Ð² Ñ ÑÐ°Ð½Ð¸Ð»Ð¸ÑÐµ Ð´Ð°Ð½Ð½ÑÑ Ð¿ÑÐ¸ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ð¸ ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸Ð¸ Ð±Ð»Ð¾ÐºÑÐµÐ¹Ð½
title: Minimization of waste space in the data storage when using blockchain technology
Creators: name: ÐÐµÑÐºÑÐ»Ð¾Ð², ÐÐ½Ð´ÑÐµÐ¹
name: ÐÑÑÐµÐ¼Ð¾Ð², ÐÑÑÐµÐ¼
name: "Ð¡Ð¸ÑÑÐµÐ¼Ð½ÑÐ¹ Ð°Ð½Ð°Ð»Ð¸Ð· Ð² Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ð¸ Ð¸ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ð¸", Ð¼ÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½Ð°Ñ Ð½Ð°ÑÑÐ½Ð¾-Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ°Ñ ÐºÐ¾Ð½ÑÐµÑÐµÐ½ÑÐ¸Ñ (26; 2022; Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³)
Publisher: name: ÐÐÐÐÐ¢ÐÐ¥-ÐÐ ÐÐ¡Ð¡
Year: 2023
Subjects: ÐÐ°Ð·Ñ Ð´Ð°Ð½Ð½ÑÑ
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ÑÐ¼ÐµÐ½ÑÑÐµÐ½Ð¸Ðµ Ð´Ð¸ÑÐºÐ¾Ð²Ð¾Ð³Ð¾ Ð¿ÑÐ¾ÑÑÑÐ°Ð½ÑÑÐ²Ð°
minimization
blockchain
disk space reduction

description: Ð¢ÐµÐ¼Ð° ÑÑÐ¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ: Â«ÐÐ¸Ð½Ð¸Ð¼Ð¸Ð·Ð°ÑÐ¸Ñ ÑÐ°ÑÑÐ¾Ð´ÑÐµÐ¼Ð¾Ð³Ð¾ Ð¼ÐµÑÑÐ° Ð² ÑÑÐ°Ð½Ð¸Ð»Ð¸ÑÐµ Ð´Ð°Ð½Ð½ÑÑ Ð¿ÑÐ¸ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ð¸ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¸ Ð±Ð»Ð¾ÐºÑÐµÐ¹Ð½Â». ÐÐ°Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð¿Ð¾ÑÐ²ÑÑÐµÐ½Ð° Ð¸Ð·ÑÑÐµÐ½Ð¸Ñ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¸ Ð±Ð»Ð¾ÐºÑÐµÐ¹Ð½ Ð¸ Ð¼Ð¸Ð½Ð¸Ð¼Ð¸Ð·Ð°ÑÐ¸Ð¸ ÑÐ°ÑÑÐ¾Ð´ÑÐµÐ¼Ð¾Ð³Ð¾ Ð¼ÐµÑÑÐ° Ð² ÑÑÐ°Ð½Ð¸Ð»Ð¸ÑÐµ Ð´Ð°Ð½Ð½ÑÑ Ð¿ÑÐ¸ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ð¸ Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¸. Ð ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐµ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ Ð±ÑÐ´ÐµÑ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½ Proof of Concept Ð±Ð»Ð¾ÐºÑÐµÐ¹Ð½, ÐºÐ¾ÑÐ¾ÑÑÐ¹ Ð±ÑÐ´ÐµÑ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°ÑÑ Ð¼ÐµÐ½ÑÑÐµ Ð´Ð¸ÑÐºÐ¾Ð²Ð¾Ð³Ð¾ Ð¿ÑÐ¾ÑÑÑÐ°Ð½ÑÑÐ²Ð° Ð´Ð»Ñ ÑÑÐ°Ð½ÐµÐ½Ð¸Ñ Ð±Ð»Ð¾ÐºÐ¾Ð², ÑÐµÐ¼ Ð¸Ð¼ÐµÑÑÐ¸ÐµÑÑ Ð³Ð¾ÑÐ¾Ð²ÑÐµ ÑÐµÑÐµÐ½Ð¸Ñ.
description: The topic of this work: âMinimization the space consumed in the data warehouse whenusing blockchain technology.â This work is devoted to the study of blockchain technology and minimization of the consumed space in the data warehouse when using this technology. As a result of the study, a Proof of Concept blockchain will be developed that will use less disk space to store blocks than existing ready-made solutions.
Finding new sub-stellar co-moving companion candidates - the case of CT Cha
Creators: name: Schmidt, T. O. B.
name: Neuhäuser, R.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We have searched for close and faint companions around T Tauri stars in the Chamaeleon star forming region. Two epochs of direct imaging data were taken with the VLT Adaptive Optics instrument NaCo in February 2006 and March 2007 in Ks band for the classical T Tauri star CT Cha together with a Hipparcos binary for astrometric calibration. Moreover a J band image was taken in March 2007 to get color information. We found CT Cha to have a very faint companion (Ks{0} = 14.6 mag) of ~ 2.67" separation corresponding to ~ 440 AU. We show that CT Cha A and the faint object form a common proper motion pair and that the companion is not a non-moving background object (with 4 sigma significance).
description: 5 pages, 2 figures, Proceedings of the IAU Symposium 249: Exoplanets: Detection, Formation and Dynamics, Suzhou - China, 22-26 October 2007
La supernova ancora più super
Creators: Marco Galliani
Publisher: name: Media Inaf
Year: 2016

La più brillante supernova al suo massimo ha raggiunto la luminosità di ben 570 miliardi di volte quella del nostro Sole. E' stata scoperta da un gruppo di astronomi guidato da Subo Dong, del Kavli Institute for Astrophysics di Pechino in Cina a cui ha partecipato Filomena Bufano, dell’INAF-Osservatorio Astrofisico di Catania
Tutti gli astrofisici di Tornatore
Creators: Marco Malaspina
Publisher: name: Media Inaf
Year: 2016

Intervista a Pietro Ubertini, direttore dell’INAF IAPS di Roma, al quale Giuseppe Tornatore si è rivolto per verificare la correttezza dei contenuti scientifici della sua ultima opera, in uscita oggi nelle sale italiane. Protagonista della storia, un professore d’astrofisica  interpretato da Jeremy Irons
Ciak al telescopio per “La corrispondenza”
Creators: Lina Tomasella
Publisher: name: Media Inaf
Year: 2016

L'ultimo film di Giuseppe Tornatore esce oggi, 14 gennaio, nelle sale italiane. Racconta la storia di un professore di astrofisica, Jeremy Irons, e di una sua allieva, Olga Kurylenko. E alcune scene sono state girate presso un telescopio dell'INAF di Padova. Il reportage di Lina Tomasella, astronoma e responsabile della Stazione osservativa
title: Ð£ÑÐµÑÐ½Ð°Ñ Ð¿Ð¾Ð»Ð¸ÑÐ¸ÐºÐ° Ð¸ Ð¿Ð¾ÑÑÐ´Ð¾Ðº ÐµÐµ ÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð² ÑÐµÐ»ÑÑ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸ÐµÐ¹
title: Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ°Ð·ÐµÐ¿Ð¾Ð²Ð°, Ð Ð°Ð¸ÑÐ°
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2018
Subjects: ÑÑÐµÑÐ½Ð°Ñ Ð¿Ð¾Ð»Ð¸ÑÐ¸ÐºÐ°
Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÑÑÑÐºÑÑÑÐ°
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ÐºÐ¾ÑÑÑÐ¸ÑÐ¸ÐµÐ½ÑÐ½ÑÐ¹ Ð°Ð½Ð°Ð»Ð¸Ð·

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Ð¾Ð²ÑÐµ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¸Â».
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Line formation in AGB atmospheres including velocity effects. Molecular line profile variations of long period variables
Creators: name: Nowotny, W.
name: Hoefner, S.
name: Aringer, B.
Publisher: name: arXiv
Year: 2010
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: The atmospheres of evolved red giants are considerably influenced by pulsations of the stellar interiors and developing stellar winds. The resulting complex velocity fields severely affect molecular line profiles observable in NIR spectra. With the help of model calculations the complex line formation process in AGB atmospheres was explored with the focus on velocity effects. Furthermore, we aimed for atmospheric models which are able to quantitatively reproduce line profile variations found in observed spectra of pulsating late-type giants. Models describing pulsation-enhanced dust-driven winds were used to compute synthetic spectra under the assumptions of chemical equilibrium and LTE and by solving the radiative transfer in spherical geometry including velocity effects. Radial velocities derived from Doppler-shifted synthetic line profiles provide information on the gas velocities in the line-forming region of the spectral features. On the basis of dynamic models we investigated in detail the finding that various molecular features in AGB spectra originate at different geometrical depths of the very extended atmospheres. We show that the models are able to quantitatively reproduce the characteristic line profile variations of lines sampling the deep photosphere. The global velocity fields of typical LPVs are also realistically reproduced. Possible reasons for discrepancies concerning other modelling results are outlined. In addition, we present a model showing variations of CO dv=3 line profiles comparable to observed spectra of SRVs and discuss that the non-occurence of line doubling in these objects may be due to a density effect. The results of our line profile modelling are another indication that the dynamic models studied here are approaching a realistic representation of the outer layers of AGB stars.
description: 26 pages, 27 (colour) figures, accepted for publication in A&A
A theoretical study of space charge and hyrdomagnetic waves in solids
Creators: name: Cook, John George
Publisher: name: University of British Columbia
Year: 2011

description: This thesis is a theoretical study of some aspects of space charge waves and hydromagnetic waves in solids. Dispersion equations obtained in the hydrodynamic approximation are studied to gain Information concerning transverse waves propagating along an applied magnetic field, and the conditions for which space charge waves may grow. For the hydromagnetic waves various assumptions are made as to the ratio of the electron and hole masses and electron and hole number densities. Particular attention is paid to the extrinsic and intrinsic cases. It is shown that often waves which are apparently different from waves previously studied, may be considered as simple extensions or special cases of the type of wave motion that are well established. In studying growing space charge waves it is assumed that the solid is intrinsic, the hole mass equals the electron mass, and the plasma found in the solid is cold. Recombination and damping of the carriers is taken into account at all times. For this model exact conditions are given for which growth of space charge waves propagating along an applied electric field may occur.
Casimir forces between spheres
Creators: name: Babington, James
Publisher: name: arXiv
Year: 2009
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We discuss the calculation of Casimir forces between a collection of $N$-dielectric spheres. This is done by evaluating directly the force on a sphere constructed from a stress tensor, rather than an interaction energy. Two and three body forces between the spheres are evaluated for setups of two and three sphere systems respectively. An approximate large-$N$ limit is also obtained for the functional dependence on the number of spheres.
description: 5 pages, 3 figures, talk presented at CEWQO09, Turku, Finland
La sonda Juno batte ogni record
Creators: Redazione Media Inaf
Publisher: name: Media Inaf
Year: 2016

Juno è stata lanciata il 5 agosto 2011 a bordo di un razzo Atlas V da Cape Canaveral e arriverà nell'orbita di Giove il 4 luglio di quest'anno. Nei prossimi 16 mesi Juno raggiungerà la distanza massima 832 milioni di chilometri dal Sole
title: ÐÐ½Ð°Ð»Ð¸Ð· ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ð³Ð¾ ÑÐ¾ÑÑÐ¾ÑÐ½Ð¸Ñ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð¸ Ð¾ÑÐµÐ½ÐºÐ° Ð¿ÐµÑÑÐ¿ÐµÐºÑÐ¸Ð² ÐµÐ³Ð¾ ÑÐ°Ð·Ð²Ð¸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ÐºÐµÑÐ¾Ð²Ð°, ÐÑÐ½Ð°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°Ð½Ð°Ð»Ð¸Ð· ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ð³Ð¾ ÑÐ¾ÑÑÐ¾ÑÐ½Ð¸Ñ
Ð¸Ð¼ÑÑÐµÑÑÐ²ÐµÐ½Ð½Ð¾Ðµ Ð¿Ð¾Ð»Ð¾Ð¶ÐµÐ½Ð¸Ðµ
ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð°Ñ ÑÑÑÐ¾Ð¹ÑÐ¸Ð²Ð¾ÑÑÑ
Ð»Ð¸ÐºÐ²Ð¸Ð´Ð½Ð¾ÑÑÑ
ÑÐµÐ½ÑÐ°Ð±ÐµÐ»ÑÐ½Ð¾ÑÑÑ

description: ÐÐ±ÑÐµÐºÑÐ¾Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ²Ð»ÑÐµÑÑÑ ÐÐ Â«ÐÐÐ¢-Ð¤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¿ÑÐ¾Ð²Ðµ-Ð´ÐµÐ½Ð¸Ðµ Ð°Ð½Ð°Ð»Ð¸Ð·Ð° ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ð³Ð¾ ÑÐ¾ÑÑÐ¾ÑÐ½Ð¸Ñ ÐÐ Â«ÐÐÐ¢-Ð¤ÐÐÐÐÂ», Ð¾ÑÐµÐ½ÐºÐ° Ð¿ÐµÑÑÐ¿ÐµÐºÑÐ¸Ð² ÐµÐ³Ð¾ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ Ð¸ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð°ÑÐ¸Ð¹ Ð¿Ð¾ ÐµÐ³Ð¾ ÑÐ»ÑÑÑÐµ-Ð½Ð¸Ñ.
ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð° Ð¾ÑÐµÐ½ÐºÐ° Ð¸Ð¼ÑÑÐµÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¿Ð¾Ð»Ð¾Ð¶ÐµÐ½Ð¸Ñ Ð¸ Ð²ÐµÑÐ¾ÑÑÐ½Ð¾ÑÑÐ¸ Ð½ÐµÑÐ¾ÑÑÐ¾ÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ (Ð±Ð°Ð½ÐºÑÐ¾ÑÑÑÐ²Ð°) ÐÐ Â«ÐÐÐ¢-Ð¤ÐÐÐÐÂ». ÐÐ° Ð¾ÑÐ½Ð¾Ð²Ðµ Ð°Ð½Ð°-Ð»Ð¸Ð·Ð° ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ð¹ ÑÑÑÐ¾Ð¹ÑÐ¸Ð²Ð¾ÑÑÐ¸, Ð»Ð¸ÐºÐ²Ð¸Ð´Ð½Ð¾ÑÑÐ¸ Ð¸ Ð¿Ð»Ð°ÑÐµÐ¶ÐµÑÐ¿Ð¾ÑÐ¾Ð±Ð½Ð¾ÑÑÐ¸, Ð´ÐµÐ»Ð¾Ð²Ð¾Ð¹ Ð°ÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ Ð¸ ÑÐµÐ½ÑÐ°Ð±ÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð±ÑÐ»Ð¾ Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð¾ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ðµ ÑÐ¾ÑÑÐ¾ÑÐ½Ð¸Ðµ ÐÐ Â«ÐÐÐ¢-Ð¤ÐÐÐÐÂ».
ÐÑÐ»Ð¸ Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ñ Ð¼ÐµÑÑ Ð¿Ð¾ ÑÐ»ÑÑÑÐµÐ½Ð¸Ñ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ð³Ð¾ ÑÐ¾ÑÑÐ¾Ñ-Ð½Ð¸Ñ Ð¸ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð° Ð¾ÑÐµÐ½ÐºÐ° Ð¸Ñ Ð²Ð»Ð¸ÑÐ½Ð¸Ñ Ð½Ð° Ð²ÐµÐ»Ð¸ÑÐ¸Ð½Ñ Ð¿ÑÐ¸Ð±ÑÐ»Ð¸ ÐÐ Â«ÐÐÐ¢-Ð¤ÐÐÐÐÂ».
Ð ÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ñ ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð°ÑÐ¸Ð¹ Ð¿ÑÐ¸Ð²ÐµÐ´ÐµÑ Ðº ÐµÑÐµ Ð±Ð¾Ð»ÑÑÐµÐ¹ ÑÑÑÐµÐºÑÐ¸Ð²-Ð½Ð¾ÑÑÐ¸ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ ÐÐ Â«ÐÐÐ¢-Ð¤ÐÐÐÐÂ».
title: Ð¢ÑÑÐ´Ð¾Ð²ÑÐµ ÑÐµÑÑÑÑÑ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ ÑÐ¾ÑÐ³Ð¾Ð²Ð»Ð¸, ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÑ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¸ Ð¿ÑÑÐ¸ ÐµÐµ Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ñ
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: Ð¥Ð¼ÐµÐ»Ð¸Ð½ÑÐºÐ¸Ð¹, ÐÐ³Ð¾Ñ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: Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´Ð¸ÑÐµÐ»ÑÐ½Ð¾ÑÑÑ ÑÑÑÐ´Ð°
Ð·Ð°ÑÐ°Ð±Ð¾ÑÐ½Ð°Ñ Ð¿Ð»Ð°ÑÐ°
ÑÑÑÐ´Ð¾Ð²ÑÐµ ÑÐµÑÑÑÑÑ
Ð¾ÑÐµÐ½ÐºÐ° ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸
Ð°Ð½Ð°Ð»Ð¸Ð· ÑÐ°ÑÑ Ð¾Ð´Ð¾Ð²
Ð¿Ð»Ð°Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»ÐµÐ¹

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 ÑÑÐ°Ð»ÐºÐ°Â». Ð¦ÐµÐ»Ñ Ð²ÑÐ¿ÑÑÐºÐ½Ð¾Ð¹ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ - Ð°Ð½Ð°Ð»Ð¸Ð· ÑÑÑÐ´Ð¾Ð²ÑÑ ÑÐµÑÑÑÑÐ¾Ð² Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ, ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ð¸Ðµ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¸ Ð²ÑÑÐ²Ð»ÐµÐ½Ð¸Ðµ Ð¿ÑÑÐµÐ¹ ÐµÐµ Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ñ. ÐÐ° Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð¸Ð¸ Ð°Ð½Ð°Ð»Ð¸Ð·Ð° ÑÑÑÐ´Ð¾Ð²ÑÑ ÑÐµÑÑÑÑÐ¾Ð² ÑÐ´ÐµÐ»Ð°Ð½ Ð²ÑÐ²Ð¾Ð´ Ð¾ Ð¿ÐµÑÑÐ¿ÐµÐºÑÐ¸Ð²Ð°Ñ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ. ÐÑÐ¿Ð¾Ð»Ð½ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÐ°ÑÑÐ¾Ð´Ð¾Ð² Ð½Ð° Ð¾Ð¿Ð»Ð°ÑÑ ÑÑÑÐ´Ð° Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ ÐÐÐ Â«Ð ÑÑÐ°Ð»ÐºÐ°Â», ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ð° Ð¾ÑÐµÐ½ÐºÐ° ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ ÑÐ¾Ð·ÑÐ¹ÑÑÐ²ÐµÐ½Ð½Ð¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸. ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¾ Ð¿Ð»Ð°Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»ÐµÐ¹ Ð¿Ð¾ ÑÑÑÐ´Ñ Ð¸ Ð·Ð°ÑÐ°Ð±Ð¾ÑÐ½Ð¾Ð¹ Ð¿Ð»Ð°ÑÐµ.
A mixed methods investigation into sleep inertia management for emergency service personnel
Creators: name: Kovac, Katya
Publisher: name: CQUniversity
Year: 2023
Subjects: Industrial and organisational psychology (incl. human factors)

description: Sleep inertia is the temporary period of impairment to performance and alertness found upon waking. Due to the impairments associated with this phenomenon, sleep inertia is a safety risk for those who must perform tasks soon after waking. Emergency service personnel are one such cohort who can be impacted by sleep inertia due to the prevalent use of on-call and shift-work arrangements. These work arrangements place personnel in situations where they may be woken to respond to an emergency event. Due to the necessity to respond quickly to emergency events, a period of sleep inertia may occur while personnel are undertaking safety critical activities such as driving or performing skilled tasks as part of their role, potentially endangering themselves, colleagues, and the individuals they are attending to. Given the safety risk that sleep inertia poses for emergency service personnel, the broad objective of this thesis was to examine the causes, consequences, and potential safety measures for sleep inertia for emergency service personnel. This information could then be used to develop evidence-based sleep inertia management strategies for emergency service personnel. To accomplish this objective, this thesis used a mixed methods approach resulting in four separate studies to better understand the impact and management of sleep inertia on emergency service personnel.
title: ÐÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ðµ ÐºÐ»ÐµÑÐ¾ÑÐ½ÑÑ ÐºÑÐ»ÑÑÑÑ ÑÐµÐ»Ð¾Ð²ÐµÐºÐ° Ð¸ Ð¶Ð¸Ð²Ð¾ÑÐ½ÑÑ Ð¿ÑÐ¸ Ð¼Ð¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ð¸ ÐºÐ»ÐµÑÐ¾ÑÐ½Ð¾Ð³Ð¾ Ð¾ÑÐ²ÐµÑÐ°
title: Using human and animal cell cultures in the modeling of cell response
Creators: name: ÐÐ²Ð°Ð½Ð¾Ð²Ð°, Ð.
name: "ÐÐ¾Ð»Ð»ÐµÐºÑÐ¸Ð¸ ÐºÑÐ»ÑÑÑÑ ÐºÐ»ÐµÑÐ¾Ðº ÑÐµÐ»Ð¾Ð²ÐµÐºÐ° Ð¸ Ð¶Ð¸Ð²Ð¾ÑÐ½ÑÑ : ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½ÑÐµ Ð²ÑÐ·Ð¾Ð²Ñ Ð¸ ÑÐµÑÐµÐ²ÑÐµ ÑÐµÑÐµÐ½Ð¸Ñ", Ð²ÑÐµÑÐ¾ÑÑÐ¸Ð¹ÑÐºÐ°Ñ ÑÐºÐ¾Ð»Ð°-ÐºÐ¾Ð½ÑÐµÑÐµÐ½ÑÐ¸Ñ (2022; Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³)
Publisher: name: ÐÐÐÐÐ¢ÐÐ¥-ÐÐ ÐÐ¡Ð¡
Year: 2022
Subjects: ÐÐ»ÐµÑÐºÐ° (Ð±Ð¸Ð¾Ð».)

description: Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° ÑÐ¿Ð¾ÑÐ¾Ð±Ð¾Ð² Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð½Ð¾Ð¹ ÑÐµÐ³ÑÐ»ÑÑÐ¸Ð¸ ÑÑÐ½ÐºÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½Ð¾Ð¹ Ð°ÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ ÐºÐ»ÐµÑÐ¾Ðº ÑÐ°Ð·Ð»Ð¸ÑÐ½Ð¾Ð³Ð¾ Ð¿ÑÐ¾Ð¸ÑÑÐ¾Ð¶Ð´ÐµÐ½Ð¸Ñ Ð¾ÑÐ½Ð¾ÑÐ¸ÑÑÑ Ðº Ð²Ð°Ð¶Ð½ÐµÐ¹ÑÐ¸Ð¼ Ð·Ð°Ð´Ð°ÑÐ°Ð¼ Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ¾Ð¹ Ð¼ÐµÐ´Ð¸ÑÐ¸Ð½Ñ. Ð ÑÑÐ¾Ð¹ ÑÐ²ÑÐ·Ð¸ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ðµ ÐºÐ»ÐµÑÐ¾ÑÐ½ÑÑ ÐºÑÐ»ÑÑÑÑ Ñ Ð·Ð°Ð´Ð°Ð½Ð½ÑÐ¼ Ð½Ð°Ð±Ð¾ÑÐ¾Ð¼ ÑÐ¸Ð·Ð¸Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ñ ÑÐ°ÑÐ°ÐºÑÐµÑÐ¸ÑÑÐ¸Ðº Ð² ÐºÐ°ÑÐµÑÑÐ²Ðµ ÑÐºÑÐ¿ÐµÑÐ¸Ð¼ÐµÐ½ÑÐ°Ð»ÑÐ½Ð¾Ð¹ Ð¼Ð¾Ð´ÐµÐ»Ð¸ Ð´Ð»Ñ Ð¸Ð·ÑÑÐµÐ½Ð¸Ñ Ð°ÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð½ÑÑ ÐºÐ»ÐµÑÐ¾ÑÐ½ÑÑ Ð¼Ð¸ÑÐµÐ½ÐµÐ¹ Ð¿Ð¾Ð´ Ð²Ð¾Ð·Ð´ÐµÐ¹ÑÑÐ²Ð¸ÐµÐ¼ ÑÐ°Ð·Ð»Ð¸ÑÐ½ÑÑ Ð²Ð½ÐµÑÐ½Ð¸Ñ ÑÐ°ÐºÑÐ¾ÑÐ¾Ð² (Ð¿ÑÐ¸ÑÐ¾Ð´Ð½ÑÐµ Ð¸Ð»Ð¸ ÑÐ¸Ð½ÑÐµÑÐ¸ÑÐµÑÐºÐ¸Ðµ ÑÐµÐ³ÑÐ»ÑÑÐ¾ÑÐ½ÑÐµ ÑÐ¾ÐµÐ´Ð¸Ð½ÐµÐ½Ð¸Ñ, Ð³ÐµÐ½Ð½ÑÐµ Ð¿ÑÐ¾Ð´ÑÐºÑÑ Ð¸ Ñ.Ð´.) ÑÐ²Ð»ÑÐµÑÑÑ Ð°Ð±ÑÐ¾Ð»ÑÑÐ½Ð¾ Ð¾Ð¿ÑÐ°Ð²Ð´Ð°Ð½Ð½ÑÐ¼.
Wave functions of the nucleon and its parity partner from lattice QCD
Creators: name: Warkentin, Nikolaus
name: Braun, Vladimir M.
name: Göckeler, Meinulf
name: Kaltenbrunner, Thomas
name: Schäfer, Andreas
name: Schierholz, Gerrit
name: Nakamura, Yoshifumi
name: Pleiter, Dirk
name: Horsley, Roger
name: Zanotti, James M.
name: Rakow, Paul E. L.
name: Stüben, Hinnerk
Publisher: name: arXiv
Year: 2008
Subjects: subject: High Energy Physics - Lattice (hep-lat)
subject: FOS: Physical sciences

description: We compute moments of distribution amplitudes using gauge configurations with two flavors of clover fermions from QCDSF/DIK and operators which are optimized with respect to their behavior under the lattice symmetries. The knowledge of these quantities helps in understanding the internal structure of hadrons and in the analysis of (semi-)exclusive processes. We present results for the nucleon distribution amplitude which suggest that the asymmetries (the deviations from the asymptotic form) are smaller than indicated by sum rule calculations. Using the same approach we were also able to calculate the same quantities for the $N^\star(1535)$, the parity partner of the nucleon. These results show a stronger deviation from the asymptotic form.
description: Presented at 26th International Symposium on Lattice Field Theory, Williamsburg, Virginia, USA. 8 pages, 2 tables, 2 figures
title: ÐÐ²ÑÐ¾Ð¼Ð¾Ð±Ð¸Ð»ÑÐ½ÑÐ¹ Ð´Ð¸Ð·ÐµÐ»ÑÐ½ÑÐ¹ Ð´Ð²Ð¸Ð³Ð°ÑÐµÐ»Ñ Ð¼Ð¾ÑÐ½Ð¾ÑÑÑÑ 126 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ÑÐ°ÐµÐ², ÐÐ½Ð°Ñ
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2018
Subjects: Ð´Ð²Ð¸Ð³Ð°ÑÐµÐ»Ñ Ð²Ð½ÑÑÑÐµÐ½Ð½ÐµÐ³Ð¾ ÑÐ³Ð¾ÑÐ°Ð½Ð¸Ñ
Ð°Ð²ÑÐ¾Ð¼Ð¾Ð±Ð¸Ð»ÑÐ½ÑÐ¹ Ð´Ð¸Ð·ÐµÐ»ÑÐ½ÑÐ¹ Ð´Ð²Ð¸Ð³Ð°ÑÐµÐ»Ñ
ÑÐ°ÑÑÐµÑ Ð¿ÑÐ¾ÑÐ½Ð¾ÑÑÐ¸
ÑÐ¸Ð»Ñ Ð¸ Ð¼Ð¾Ð¼ÐµÐ½ÑÑ
Ð´Ð¸Ð°Ð³ÑÐ°Ð¼Ð¼Ð° Ð¢Ð¾Ð»Ð»Ðµ Ð¸ ÐÑÐ¸ÐºÑÐ°

description: Ð Ð°Ð±Ð¾ÑÐ° Ð¿Ð¾ÑÐ²ÑÑÐµÐ½Ð° ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐµ Ð°Ð²ÑÐ¾Ð¼Ð¾Ð±Ð¸Ð»ÑÐ½Ð¾Ð³Ð¾ Ð´Ð¸Ð·ÐµÐ»ÑÐ½Ð¾Ð³Ð¾ Ð´Ð²Ð¸Ð³Ð°ÑÐµÐ»Ñ Ð²Ð½ÑÑÑÐµÐ½Ð½ÐµÐ³Ð¾ ÑÐ³Ð¾ÑÐ°Ð½Ð¸Ñ Ð¼Ð¾ÑÐ½Ð¾ÑÑÑÑ 126 Ð».Ñ. (92 ÐºÐÑ). Ð ÑÐ¾Ð´Ðµ Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¸Ñ ÑÐ°Ð±Ð¾ÑÑ ÑÐ°ÑÑÑÐ¸ÑÐ°Ð½Ñ: ÑÐ°Ð±Ð¾ÑÐ¸Ð¹ Ð¿ÑÐ¾ÑÐµÑÑ Ð´Ð²Ð¸Ð³Ð°ÑÐµÐ»Ñ, Ð¿Ð¾ÑÑÑÐ¾ÐµÐ½Ð° Ð¸Ð½Ð´Ð¸ÐºÐ°ÑÐ¾ÑÐ½Ð°Ñ Ð´Ð¸Ð°Ð³ÑÐ°Ð¼Ð¼Ð°, Ð´Ð¸Ð°Ð³ÑÐ°Ð¼Ð¼Ð° Ð¢Ð¾Ð»Ð»Ðµ Ð¸ ÐÑÐ¸ÐºÑÐ°, Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½ Ð´Ð¸Ð½Ð°Ð¼Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ°ÑÑÐµÑ, Ð¿ÑÐ¾Ð°Ð½Ð°Ð»Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ð° ÑÑÐ°Ð²Ð½Ð¾Ð²ÐµÑÐµÐ½Ð½Ð¾ÑÑÑ Ð´Ð²Ð¸Ð³Ð°ÑÐµÐ»Ñ, Ð¿ÑÐ¾Ð¸Ð·Ð²ÐµÐ´ÐµÐ½Ñ ÑÐ°ÑÑÐµÑÑ Ð¿ÑÐ¾ÑÐ½Ð¾ÑÑÐ¸, Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½ ÑÐ°ÑÑÐµÑ Ð°Ð³ÑÐµÐ³Ð°ÑÐ¾Ð² ÑÐ¸ÑÑÐµÐ¼ ÑÐ¼Ð°Ð·ÑÐ²Ð°Ð½Ð¸Ñ Ð¸ Ð¾ÑÐ»Ð°Ð¶Ð´ÐµÐ½Ð¸Ñ, Ð¿ÑÐ¸Ð²ÐµÐ´ÐµÐ½Ð¾ Ð¾Ð¿Ð¸ÑÐ°Ð½Ð¸Ðµ ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð¸ Ð´Ð²Ð¸Ð³Ð°ÑÐµÐ»Ñ Ð¸ ÑÐ¸ÑÑÐµÐ¼. ÐÐ° Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð¸Ð¸ ÑÐ°ÑÑÐµÑÐ¾Ð² ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ñ Ð¿ÑÐ¾Ð´Ð¾Ð»ÑÐ½ÑÐ¹ Ð¸ Ð¿Ð¾Ð¿ÐµÑÐµÑÐ½ÑÐ¹ ÑÐ°Ð·ÑÐµÐ·Ñ Ð´Ð²Ð¸Ð³Ð°ÑÐµÐ»Ñ, Ð° ÑÐ°ÐºÐ¶Ðµ ÑÑÐµÐ¼Ñ ÑÐ¼Ð°Ð·ÐºÐ¸, Ð¾ÑÐ»Ð°Ð¶Ð´ÐµÐ½Ð¸Ñ Ð¸ ÑÐ¾Ð¿Ð»Ð¸Ð²Ð¾Ð¿Ð¾Ð´Ð°ÑÐ¸.
Onde gravitazionali, fra rumors e “big dogs”
Creators: Marco Malaspina
Publisher: name: Media Inaf
Year: 2016

In attesa che le indiscrezioni sulla possibilità che l’interferometro LIGO possa aver captato un segnale di onda gravitazionale ricevano una conferma o una smentita ufficiale, abbiamo chiesto a Marica Branchesi e a Enzo Brocato d’illustrarci il funzionamento di una potenziale “terza possibilità”
Aerogel Waveplates
Creators: name: Bhupathi, P.
name: Hwang, J.
name: Martin, R. M.
name: Blankstein, J.
name: Jaworski, L.
name: Mulders, N.
name: Tanner, D. B.
name: Lee, Y.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Other Condensed Matter (cond-mat.other)
subject: FOS: Physical sciences

description: Optical transmission measurements were made on 98% porosity silica aerogel samples under various degrees of uniaxial strain. Uniaxially compressed aerogels exhibit large birefringence, proportional to the amount of compression, up to the 15% strain studied. The birefringence is mostly reversible and reproducible through multiple compression-decompression cycles. Our study demonstrates that uniaxially strained high porosity aerogels can be used as tunable waveplates in a broad spectral range.
description: 7 pages, 4 figures, submitted to Optics Express
Z boson transverse momentum spectrum from the lepton angular distributions
Creators: name: Boonekamp, Maarten
name: Schott, Matthias
Publisher: name: arXiv
Year: 2010
Subjects: subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: In view of recent discussions concerning the possibly limiting energy resolution systematics on the measurement of the Z boson transverse momentum distribution at hadron colliders, we propose a novel measurement method based on the angular distributions of the decay leptons. We also introduce a phenomenological parametrization of the transverse momentum distribution that adapts well to all currently available predictions, a useful tool to quantify their differences.
description: 12 pages, 6 figures
title: ÐÐ½Ð°Ð»Ð¸Ð· ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ð³Ð¾ ÑÐ¾ÑÑÐ¾ÑÐ½Ð¸Ñ Ð¸ Ð¿Ð»Ð°Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ (Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ ÐÐÐ Â«ÐÐ¡Ð Â»)
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ°ÑÐµÑ, Ð¡ÐµÑÐ³ÐµÐ¹
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: ÑÐ»ÐµÐºÑÑÐ¾ÑÐµÑ Ð½Ð¸ÑÐµÑÐºÐ°Ñ Ð¿ÑÐ¾Ð´ÑÐºÑÐ¸Ñ
ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð°Ñ Ð´Ð¸Ð°Ð³Ð½Ð¾ÑÑÐ¸ÐºÐ°
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description: ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÑÐ½ÐºÐ° Ð½Ð¸Ð·ÐºÐ¾Ð²Ð¾Ð»ÑÑÐ½Ð¾Ð¹ ÑÐ»ÐµÐºÑÑÐ¾ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¾Ð¹ Ð¿ÑÐ¾Ð´ÑÐºÑÐ¸Ð¸. ÐÐ°Ð½Ð° Ð¾Ð±ÑÐ°Ñ ÑÐ°ÑÐ°ÐºÑÐµÑÐ¸ÑÑÐ¸ÐºÐ° ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸ Ð¸ Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· ÐºÐ¾Ð½ÐºÑÑÐµÐ½ÑÐ¾Ð² Ð² Ð¾ÑÑÐ°ÑÐ»Ð¸. ÐÐ¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ñ ÐºÐ»ÑÑÐµÐ²ÑÐµ Ð¸ÑÑÐ¾ÑÐ½Ð¸ÐºÐ¸ ÑÐ¾ÑÑÐ°. ÐÑÐ¾Ð¸Ð·Ð²ÐµÐ´ÐµÐ½Ð° ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð°Ñ Ð´Ð¸Ð°Ð³Ð½Ð¾ÑÑÐ¸ÐºÐ° Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ. Ð¡Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ñ Ð²Ð°ÑÐ¸Ð°Ð½ÑÑ Ð¾ÑÐºÑÑÑÐ¸Ñ Ð½Ð¾Ð²Ð¾Ð³Ð¾ ÑÐ¾ÑÐ³Ð¾Ð²Ð¾Ð³Ð¾ Ð¿Ð¾Ð´ÑÐ°Ð·Ð´ÐµÐ»ÐµÐ½Ð¸Ñ. ÐÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ñ ÑÐ°ÑÑÐµÑÑ ÑÐµÐºÑÑÐ¸Ñ Ð¸ Ð¸Ð½Ð²ÐµÑÑÐ¸ÑÐ¸Ð¾Ð½Ð½ÑÑ Ð·Ð°ÑÑÐ°Ñ Ð¿Ð¾ Ð½Ð¸Ð¼. ÐÑÐ¾Ð¸Ð·Ð²ÐµÐ´ÐµÐ½Ñ ÑÐ°ÑÑÐµÑÑ Ð¿ÑÐ¾ÑÑÑÑ Ð¸ Ð´Ð¸ÑÐºÐ¾Ð½ÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð½ÑÑ Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»ÐµÐ¹ ÐºÐ¾Ð¼Ð¼ÐµÑÑÐµÑÐºÐ¾Ð¹ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ Ð¿ÑÐ¾ÐµÐºÑÐ¾Ð². Ð¡Ð´ÐµÐ»Ð°Ð½ Ð°Ð½Ð°Ð»Ð¸Ð· Ð±ÐµÐ·ÑÐ±ÑÑÐ¾ÑÐ½Ð¾ÑÑÐ¸ Ð¿ÑÐ¾ÐµÐºÑÐ¾Ð².
Blazars: the next gamma-ray view of GLAST
Creators: name: Ciprini, Stefano
Publisher: name: Mem.Soc.Ast.It. 3 (2003) 238
Year: 2003

description: Blazars, the extreme family of AGN, can be strong gamma-ray emitters and
constitute the largest fraction of identified point sources of EGRET. The next
Gamma-ray Large Area Space Telescope (GLAST) is a high energy (30MeV-300GeV)
gamma-ray astronomy mission, planned for launch at the end of 2006. GLAST
performances will allow to detect few thousands of gamma-ray blazars, with a
broad band coverage and temporal resolution, also in quiescent emission phases,
providing probably many answers about these sources.
Time evolution of thermodynamic entropy for conservative and dissipative
  chaotic maps
Creators: name: M. Baranger
name: V. Latora
name: A. Rapisarda
Publisher: name: Chaos Solitons and Fractals 13 (2001) 471
Year: 2000

description: We consider several low--dimensional chaotic maps started in
far-from-equilibrium initial conditions and we study the process of relaxation
to equilibrium. In the case of conservative maps the Boltzmann-Gibbs entropy
S(t) increases linearly in time with a slope equal to the Kolmogorov-Sinai
entropy rate. The same result is obtained also for a simple case of dissipative
system, the logistic map, when considered in the chaotic regime. A very
interesting results is found at the chaos threshold. In this case, the usual
Boltzmann-Gibbs is not appropriate and in order to have a linear increase, as
for the chaotic case, we need to use the generalized q-dependent Tsallis
entropy $S_q(t)$ with a particular value of a q different from 1 (when q=1 the
generalized entropy reduces to the Boltzmann-Gibbs). The entropic index q
appears to be characteristic of the dynamical system.
Status Report of the MACRO Experiment for the year 2001
Creators: name: G. Giacomelli
name: A. Margiotta
name: For The MACRO Collaboration
Publisher: name: INFN Open Access Repository
Year: 2002

description: In this 2001 status report of the MACRO experiment, results are presented on
atmospheric neutrinos and neutrino oscillations, high energy neutrino
astronomy, searches for WIMPs, search for low energy stellar gravitational
collapse neutrinos, stringent upper limits on GUT magnetic monopoles,
nuclearites and lightly ionizing particles, high energy downgoing muons,
primary cosmic ray composition and shadowing of primary cosmic rays by the Moon
and the Sun.
Solving the large discrepancy between inclusive and exclusive measurements of the ${}^8{\rm Li}+{}^4{\rm He}\to{}^{11}{\rm B}+n$ reaction cross section at astrophysical energies
Creators: name: La Cognata, M.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: A solution of the large discrepancy existing between inclusive and exclusive measurements of the ${}^8{\rm Li}+{}^4{\rm He}\to{}^{11}{\rm B}+n$ reaction cross section at $E_{cm} <3$ MeV is evaluated. This problem has profound astrophysical relevance for this reaction is of great interest in Big-Bang and r-process nucleosynthesis. By means of a novel technique, a comprehensive study of all existing ${}^8{\rm Li}+{}^4{\rm He}\to{}^{11}{\rm B}+n$ cross section data is carried out, setting up a consistent picture in which all the inclusive measurements provide the reliable value of the cross section. New unambiguous signatures of the strong branch pattern non-uniformities, near the threshold of higher ${}^{11}{\rm B}$ excited levels, are presented and their possible origin, in terms of the cluster structure of the involved excited states of ${}^{11}{\rm B}$ and ${}^{12}{\rm B}$ nuclei, is discussed.
description: 5 pages, 4 figures, 1 table
Magnetic monopole searches in the cosmic radiation
Creators: name: Mitri, Ivan De
Publisher: name: INFN Open Access Repository
Year: 2002

description: There has been a big effort in the past twenty years with at least a couple
of generations of experiments which searched for supermassive GUT magnetic
monopoles in the cosmic radiation.
  Here a short review of these searches is given, together with a brief
description of the theoretical framework and of the detection techniques.
MACRO results on atmospheric neutrinos
Creators: name: G. Giacomelli
name: A. Margiotta
Publisher: name: INFN Open Access Repository
Year: 2005

description: We discuss the final results of the MACRO experiment on atmospheric neutrino
oscillations. The data concern event topologies with average neutrino energies
of ~3 and ~50 GeV. Multiple Coulomb Scattering of the high energy muons was
used to estimate the neutrino energy event by event. The angular distributions,
the L/E_nu distribution, the particle ratios and the absolute fluxes all favor
nu_mu --> nu_tau oscillations with maximal mixing and Delta m^2 ~0.0023 eV^2.
Emphasis is given to measured ratios which are not affected by Monte Carlo (MC)
absolute normalization; a discussion is made on MC uncertainties. A preliminary
search for possible Lorentz invariance violation contributions to atmospheric
neutrino oscillations is presented and discussed.
Il ‘venticello’ che spegne le stelle
Creators: Marco Galliani
Publisher: name: Media Inaf
Year: 2016

Un team di astronomi a cui hanno partecipato due ricercatori INAF  ha individuato per la prima volta un vento ad alta velocità che fuoriesce dal buco nero ospitato nella regione centrale di una galassia a spirale, molto simile per conformazione alla nostra. Questo vento può interagire con l’ambiente galattico e riuscire a spazzare via il gas in essa presente, andando così a ostacolare il processo di formazione di nuove stelle
Clan Structure in Rapidity Intervals
Creators: name: R. Ugoccioni
name: A. Giovannini
name: S. Lupia
Publisher: name: INFN Open Access Repository
Year: 1995

description: We present a cascading model for a single jet, inspired to QCD and to the
phenomenological analysis of multiplicity distributions. The model, describing
as it does a two dimensional evolution in virtuality and rapidity, allows
analytical predictions for clan analysis parameters to be made.
Improved Determination of the b-Quark Mass at the Z Peak
Creators: name: Rodrigo, German
name: Arcadi Santamaria
name: Bilenky, Mikhail
Publisher: name: INFN Open Access Repository
Year: 1999

description: Next-to-leading order calculations of heavy quark three-jet production in e^+
e^- annihilation are reviewed. Their application for the measurement of the
b-quark mass at LEP/SLC and to the test of the flavour independence of the
strong coupling constant are discussed. Prospects for future improvements are
studied.
title: ÐÑÐ¾Ð´Ð²Ð¸Ð¶ÐµÐ½Ð¸Ðµ Ð¼ÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½ÑÑ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼ Ð¼Ð°Ð³Ð¸ÑÑÑÐ°ÑÑÑÑ Ð½Ð° Ð·Ð°ÑÑÐ±ÐµÐ¶Ð½ÑÑ ÑÑÐ½ÐºÐ°Ñ (Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ Ð¡ÐÐ±Ð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ÑÑÐ¾ÑÐµÐ½ÐºÐ¾, ÐÐ°Ð½Ð½Ð°
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: Ð¼Ð°ÑÐºÐµÑÐ¸Ð½Ð³
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Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ñ Ð¼Ð°Ð³Ð¸ÑÑÑÐ°ÑÑÑÑ

description: Ð ÑÐ°Ð±Ð¾ÑÐµ Ð¸Ð·ÑÑÐµÐ½Ñ ÑÐµÐ½Ð´ÐµÐ½ÑÐ¸Ð¸ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ Ð²ÑÑÑÐµÐ³Ð¾ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ñ, Ð¸Ð·ÑÑÐµÐ½Ñ Ð¾ÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÐ¸ Ð¼Ð°ÑÐºÐµÑÐ¸Ð½Ð³Ð° Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°ÑÐµÐ»ÑÐ½ÑÑ ÑÑÐ»ÑÐ³, Ð´Ð°Ð½Ð° ÐºÐ»Ð°ÑÑÐ¸ÑÐ¸ÐºÐ°ÑÐ¸Ñ Ð¸Ð½ÑÑÑÑÐ¼ÐµÐ½ÑÐ¾Ð² Ð¼Ð°ÑÐºÐµÑÐ¸Ð½Ð³Ð° Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°ÑÐµÐ»ÑÐ½ÑÑ ÑÑÐ»ÑÐ³. ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½ Ð¾Ð±Ð·Ð¾Ñ ÐµÐ²ÑÐ¾Ð¿ÐµÐ¹ÑÐºÐ¾Ð³Ð¾ Ð¸ ÑÐ¾ÑÑÐ¸Ð¹ÑÐºÐ¾Ð³Ð¾ ÑÑÐ½ÐºÐ¾Ð² Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼ Ð¼Ð°Ð³Ð¸ÑÑÑÐ°ÑÑÑÑ. Ð¡ÑÐ¾ÑÐ¼ÑÐ»Ð¸ÑÐ¾Ð²Ð°Ð½ ÑÑÐ´ ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð°ÑÐ¸Ð¹ Ð¿Ð¾ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð¸ Ð¿ÑÐ¾Ð´Ð²Ð¸Ð¶ÐµÐ½Ð¸Ñ Ñ ÑÐµÐ»ÑÑ ÑÐ²ÐµÐ»Ð¸ÑÐµÐ½Ð¸Ñ Ð½Ð°Ð±Ð¾ÑÐ° Ð¸Ð½Ð¾ÑÑÑÐ°Ð½Ð½ÑÑ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð².
Nel ghiaccio indizi sull’evoluzione della cometa
Creators: Marco Galliani
Publisher: name: Media Inaf
Year: 2016

Ghiaccio sulla cometa 67P Churyumov-Gerasimenko. A confermarlo sono stati i dati dello strumento VIRTIS a bordo della sonda Rosetta dell'ESA. Il ghiaccio è stato rilevato in due diversi punti della regione denominata Imhotep, fornendoci importanti informazioni sui processi di creazione degli strati di ghiaccio all’interno della cometa. Il presidente dell'INAF Nicolò D'Amico: «Grande soddisfazione per l'INAF che ha investito notevoli risorse e intellettualità su questo ambizioso progetto internazionale»
Computer simulation studies of finite-size broadening of solid-liquid interfaces: From hard spheres to nickel
Creators: name: Zykova-Timan, T.
name: Rozas, R. E.
name: Horbach, J.
name: Binder, K.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: Using Molecular Dynamics (MD) and Monte Carlo (MC) simulations interfacial properties of crystal-fluid interfaces are investigated for the hard sphere system and the one-component metallic system Ni (the latter modeled by a potential of the embedded atom type). Different local order parameters are considered to obtain order parameter profiles for systems where the crystal phase is in coexistence with the fluid phase, separated by interfaces with (100) orientation of the crystal. From these profiles, the mean-squared interfacial width w^2 is extracted as a function of system size. We rationalize the prediction of capillary wave theory that w^2 diverges logarithmically with the lateral size of the system. We show that one can estimate the interfacial stiffness from the interfacial broadening, obtaining 0.5 k_B T/sigma^2 for hard spheres and 0.18 J/m^2 for Ni.
description: 15 pages, 7 figures
L’Universo primordiale svelato
Creators: Elisa Nichelli
Publisher: name: Media Inaf
Year: 2016

Da tempo gli astronomi ritengono che la reionizzazione, quella fase durante la quale l’Universo primordiale si è riscaldato ionizzando nuovamente l’idrogeno, sia stata causata da radiazione emessa dalle galassie. Un team internazionale di ricercatori pubblica oggi uno studio su Nature grazie al quale questa ipotesi trova la sua prima prova sperimentale
Fare i conti con il viaggio nel tempo
Creators: Stefano Parisini
Publisher: name: Media Inaf
Year: 2016

Metti il turbo al computer quantistico con un viaggio nel tempo, ma senza farti accorgere. Secondo un recente studio su Nature, sfruttando il fenomeno di “entanglement”, le particelle quantistiche inviate su una curva spaziotemporale aperta possono fornire super potenza di calcolo, a patto che non interagiscono con niente nel passato. Il commento di Mariateresa Crosta (INAF)
Note on the pseudo-Nambu-Goldstone Boson of Meta-stable SUSY Violation
Creators: name: Banks, Tom
name: Haber, Howard E.
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: Many models of meta-stable supersymmetry (SUSY) breaking lead to a very light scalar pseudo-Nambu Goldstone boson (PNGB), P, associated with spontaneous breakdown of a baryon number like symmetry in the hidden sector. Current particle physics data provide no useful constraints on the existence of P. For example, the predicted decay rates for both K --> pi + P, b--> s + P and Upsilon --> photon + P are many orders of magnitude below the present experimental bounds. We also consider astrophysical implications of the PNGB and find a significant constraint from its effect on the evolution of red giants. This constraint either rules out models with a hidden sector gauge group larger than SU(4), or requires a new intermediate scale, of order at most 10^{10} GeV, at which the hidden sector baryon number is explicitly broken.
description: 17 pages, 3 figures. Version 2: minor typographical errors fixed. Version 3: a more reliable estimate for the decay rate of K-->pi+PNGB is provided, and the predicted rate for b-->s+PNGB is now included
GRAVITY, la sonda per i buchi neri
Creators: Redazione Media Inaf
Publisher: name: Media Inaf
Year: 2016

GRAVITY può misurare la posizione degli oggetti astronomici su scale minutissime e può anche realizzare immagini e spettri per mezzo dell'interferometria. Esplorerà cosa accade nel campo gravitazionale estremo vicino all'orizzonte degli eventi del buco nero supermassiccio al centro della Via Lattea
Future geodesic completeness of some spatially homogeneous solutions of the vacuum Einstein equations in higher dimensions
Creators: name: Goedeke, Arne
name: Rendall, Alan D.
Publisher: name: arXiv
Year: 2010
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: It is known that all spatially homogeneous solutions of the vacuum Einstein equations in four dimensions which exist for an infinite proper time towards the future are future geodesically complete. This paper investigates whether the analogous statement holds in higher dimensions. A positive answer to this question is obtained for a large class of models which can be studied with the help of Kaluza-Klein reduction to solutions of the Einstein-scalar field equations in four dimensions. The proof of this result makes use of a criterion for geodesic completeness which is applicable to more general spatially homogeneous models.
description: 18 pages
title: ÐÐµÑÐµÐ´Ð¾Ð²ÑÐµ ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸Ð¸ Ð² ÑÑÐµÑÐµÐ¾ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ¾Ð¹ Ð±Ð¸Ð¾Ð¿ÑÐ¸Ð¸ Ð¼Ð¾Ð»Ð¾ÑÐ½Ð¾Ð¹ Ð¶ÐµÐ»ÐµÐ·Ñ
title: Advanced technologies in stereotactic breast biopsy
Creators: name: ÐÐ°ÑÐ°Ð»Ð¾Ð², ÐÐ»ÐµÐºÑÐ°Ð½Ð´Ñ
Publisher: name: ÐÐÐÐÐ¢ÐÐ¥-ÐÐ ÐÐ¡Ð¡
Year: 2022
Subjects: ÑÐ¾Ð¼Ð¾ÑÐ¸Ð½ÑÐµÐ· Ð¼Ð¾Ð»Ð¾ÑÐ½Ð¾Ð¹ Ð¶ÐµÐ»ÐµÐ·Ñ
ÐºÐ¾Ð½ÑÑÐ°ÑÑÐ½Ð°Ñ ÑÐ¿ÐµÐºÑÑÐ°Ð»ÑÐ½Ð°Ñ Ð¼Ð°Ð¼Ð¼Ð¾Ð³ÑÐ°ÑÐ¸Ñ
ÑÑÑÐµÑÐ¾ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ°Ñ Ð±Ð¸Ð¾Ð¿ÑÐ¸Ñ
digital breast tomosynthesis
contrast enhance mammography
stereotaxic biopsy

description: Ð ÑÑÐ°ÑÑÐµ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ Ð½Ð¾Ð²ÑÐµ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¸ Ð»ÑÑÐµÐ²Ð¾Ð³Ð¾ Ð½Ð°Ð²ÐµÐ´ÐµÐ½Ð¸Ñ Ð¿ÑÐ¸ ÑÑÐµÑÐµÐ¾ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ¾Ð¹ Ð±Ð¸Ð¾Ð¿ÑÐ¸Ð¸ Ð¼Ð¾Ð»Ð¾ÑÐ½Ð¾Ð¹ Ð¶ÐµÐ»ÐµÐ·Ñ. ÐÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ñ Ð¿ÑÐµÐ¸Ð¼ÑÑÐµÑÑÐ²Ð° Ð¸ Ð¾ÑÐ»Ð¸ÑÐ¸ÑÐµÐ»ÑÐ½ÑÐµ Ð¾ÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÐ¸ Ð²ÑÐ±Ð¾ÑÐ° Ð´Ð°Ð½Ð½ÑÑ Ð¼ÐµÑÐ¾Ð´Ð¸Ðº.
description: The article considers new beam guidance technologies for stereotactic breast biopsy. The advantages and distinctive features of the choice of these methods are presented.