cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
title: Ð Ð°ÑÑÐµÑÑ Ð¿Ð¾Ð»ÐµÐ¹ Ð¸ ÑÐ¾ÐºÐ¾Ð² Ð² Ð¿Ð¾Ð»ÑÐ¿ÑÐ¾Ð²Ð¾Ð´Ð½Ð¸ÐºÐ¾Ð²ÑÑ ÑÑÑÑÐºÑÑÑÐ°Ñ
title: ÑÐ±Ð¾ÑÐ½Ð¸Ðº Ð·Ð°Ð´Ð°Ñ Ð¸ ÑÐ¿ÑÐ°Ð¶Ð½ÐµÐ½Ð¸Ð¹
titleType: Subtitle
Creators: name: ÐÐ°ÐºÑÐµÐ²Ð°, ÐÑÐ´Ð¼Ð¸Ð»Ð°
name: ÐÐ»ÑÐ¸Ð½, ÐÐ»Ð°Ð´Ð¸Ð¼Ð¸Ñ
name: ÐÑÑÐ¸ÑÐ¸Ð½, Ð¡ÐµÑÐ³ÐµÐ¹
Publisher: name: ÐÐ·Ð´-Ð²Ð¾ Ð¡ÐÐ±ÐÐÐ£
Year: 1997
Subjects: ÐÐ¾Ð»ÑÐ¿ÑÐ¾Ð²Ð¾Ð´Ð½Ð¸ÐºÐ¾Ð²ÑÐµ Ð¿ÑÐ¸Ð±Ð¾ÑÑ

description: Ð¡Ð±Ð¾ÑÐ½Ð¸Ðº Ð·Ð°Ð´Ð°Ñ Ð¸ ÑÐ¿ÑÐ°Ð¶Ð½ÐµÐ½Ð¸Ð¹ ÑÐ¾Ð¾ÑÐ²ÐµÑÑÑÐ²ÑÐµÑ Ð°Ð²ÑÐ¾ÑÑÐºÐ¸Ð¼ ÐºÑÑÑÐ°Ð¼ Ð´Ð¸ÑÑÐ¸Ð¿Ð»Ð¸Ð½ "Ð¢ÐµÐ¾ÑÐ¸Ð¸ Ð¾Ð¿ÑÐ¸ÐºÐ¸ ÑÐ»ÐµÐºÑÑÐ¾Ð½Ð½ÑÑ Ð¿ÑÐ¸Ð±Ð¾ÑÐ¾Ð²â Ð¸ "ÐÐ¾Ð»ÑÐ¿ÑÐ¾Ð²Ð¾Ð´Ð½Ð¸ÐºÐ¾Ð²Ð°Ñ ÑÐ»ÐµÐºÑÑÐ¾Ð½Ð¸ÐºÐ°" Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ¾Ð¹ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ 553100 "Ð¢ÐµÑÐ½Ð¸ÑÐµÑÐºÐ°Ñ ÑÐ¸Ð½Ð¸ÐºÐ°" Ð¸ 550700 "Ð­Ð»ÐµÐºÑÑÐ¾Ð½Ð¸ÐºÐ° Ð¸ Ð¼Ð¸ÐºÑÐ¾ÑÐ»ÐµÐºÑÑÐ¾Ð½Ð¸ÐºÐ°".
ÐÑÐ¸Ð²ÐµÐ´ÐµÐ½Ñ ÑÐµÑÐµÐ½Ð¸Ñ Ð·Ð°Ð´Ð°Ñ Ð¸ Ð¾ÑÐ²ÐµÑÑ Ð½Ð° Ð²Ð¾Ð¿ÑÐ¾ÑÑ, Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ð½ÑÐµ ÑÑÑÐ´ÐµÐ½ÑÐ°Ð¼ Ð² ÑÑÐµÐ±Ð½Ð¾Ð¼ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ð¸: ÐÐ»ÑÐ½Ð¸Ð½ Ð. Ð., ÐÑÑÐ¸ÑÐ¸Ð½ Ð. Ð¤. ÐÑÐ½Ð¾Ð²Ñ ÑÐµÐ¾ÑÐ¸Ð¸ Ð½Ð¾
Ð¿Ð¾Ð»ÑÐ¿ÑÐ¾Ð²Ð¾Ð´Ð½Ð¸ÐºÐ¾Ð²ÑÑ Ñ Ð¿ ÑÑÑÑÐºÑÑÑ- Ð¸ ÐºÐ¾Ð½ÑÐ°ÐºÑÐ¾Ð² Ð¼ÐµÑÐ°Ð»Ð» Ð¿Ð¾Ð»ÑÐ¿ÑÐ¾Ð²Ð¾Ð´Ð½Ð¸Ðº./Ð¡ÐÐ±ÐÐ¢Ð£. Ð¡ÐÐ± 1994 Ð³. 92 Ñ. ÐÐ°Ð½Ñ Ð½Ð¾Ð²ÑÐµ Ð·Ð°Ð´Ð°ÑÐ¸ Ð¸ Ð¸Ñ ÑÐµÑÐµÐ½Ð¸Ð¸, ÑÐºÐ°Ð·Ð°Ð½Ñ
Ð¸ÑÑÐ¾ÑÐ½Ð¸ÐºÐ¸ Ð´Ð¾Ð¿Ð¾Ð»Ð½Ð¸ÑÐµÐ»ÑÐ½ÑÑ Ð·Ð°Ð´Ð°Ð½Ð¸Ð¹ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð². ÐÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¾ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² ÑÐµÑÐ²ÐµÑÑÐ¾Ð³Ð¾ ÐºÑÑÑÐ° ÑÐ°Ð´Ð¸Ð¾ÑÐ¸Ð·Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÐ°ÐºÑÐ»ÑÑÐµÑÐ° Ð¸ Ð¿ÑÑÐ¾Ð³Ð¾ ÐºÑÑÑÐ° Ð²ÐµÑÐµÑÐ½ÐµÐ³Ð¾ ÑÐ»ÐµÐºÑÑÐ¾ÑÐ°Ð´Ð¸Ð¾ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÐ°ÐºÑÐ»ÑÑÐµÑÐ°, Ð¸Ð·ÑÑÐ°ÑÑÐ¸Ñ Ð´Ð¸ÑÑÐ¸Ð¿Ð»Ð¸Ð½Ñ "Ð¢ÐµÐ¾ÑÐ¸Ñ Ð¾Ð¿ÑÐ¸ÐºÐ° ÑÐ»ÐµÐºÑÑÐ¾Ð½Ð½ÑÑ Ð¿ÑÐ¸Ð±Ð¾ÑÐ¾Ð²" Ð¸ "ÐÐ¾Ð»ÑÐ¿ÑÐ¾Ð²Ð¾Ð´Ð½Ð¸ÐºÐ¾Ð²Ð°Ñ ÑÐ»ÐµÐºÑÑÐ¾Ð½Ð¸ÐºÐ°" Ð² ÑÐ°Ð¼ÐºÐ°Ñ Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ¾Ð¹ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸, Ð¿ÑÐµÐ¿Ð¾Ð´Ð°Ð²Ð°ÑÐµÐ»ÑÐ¼, ÑÐ¸ÑÐ°ÑÑÐ¸Ð¼ ÐºÑÑÑ ÑÐµÐ¾ÑÐ¸Ð¸ Ð¿Ð¾Ð»ÑÐ¿ÑÐ¾Ð²Ð¾Ð´Ð½Ð¸ÐºÐ¾Ð²ÑÑ Ð¿ÑÐ¸Ð±Ð¾ÑÐ°Ñ Ð¸ ÑÑÐºÐ¾Ð²Ð¾Ð´ÑÑÐ¸Ð¼ ÑÐ°Ð¼Ð¾ÑÑÐ¾ÑÑÐµÐ»ÑÐ½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐ¾Ð¹ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² Ð¿Ð¾ ÐºÑÑÑÑ, Ð°ÑÐ¿Ð¸ÑÐ°Ð½ÑÐ°Ð¼ Ð¸ ÑÐ¾Ð¸ÑÐºÐ°ÑÐµÐ»ÑÐ¼, ÑÐ°Ð¼Ð¾ÑÑÐ¾ÑÑÐµÐ»ÑÐ½Ð¾ Ð¸Ð·ÑÑÐ°ÑÑÐ¸Ñ ÑÐ¸Ð·Ð¸ÐºÑ Ð¿Ð¾Ð»ÑÐ¿ÑÐ¾Ð²Ð¾Ð´Ð½Ð¸ÐºÐ¾Ð²ÑÑ Ð¿ÑÐ¸Ð±Ð¾ÑÐ¾Ð².
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 Ð³Ð¾Â­ÑÑÐ´Ð°ÑÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑÐ°.
Reducing the Heterotic Supergravity on nearly-Kahler coset spaces
Creators: name: Chatzistavrakidis, A.
name: Manousselis, P.
name: Zoupanos, G.
Publisher: name: arXiv
Year: 2008
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We study the dimensional reduction of the ${\cal N}=1$, ten-dimensional Heterotic Supergravity to four dimensions, at leading order in $α'$, when the internal space is a nearly-Kähler manifold. Nearly-Kähler manifolds in six dimensions are all the non-symmetric coset spaces and a group manifold. Here we reduce the theory using as internal manifolds the three six-dimensional non-symmetric coset spaces, omitting the case of the group manifold in the prospect of obtaining chiral fermions when the gauge fields will be included. We determine the effective actions for these cases, which turn out to describe ${\cal N}=1$ four-dimensional supergravities of the no-scale type and we study the various possibilities concerning their vacuum.
description: 18 pages, references added, comments added, a shorter version will appear in the proceedings of the 4th workshop of the RTN project 'Constituents, Fundamental Forces and Symmetries of the Universe', Varna
Space holidays: sognando il turismo spaziale
Creators: Davide Coero Borga
Publisher: name: Media Inaf
Year: 2016

Locandine e pubblicità di una sedicente e seducente agenzia di viaggi spaziali promettono mete da sogno. Vi porteremo ai confini del Sistema solare. Ma dietro grafiche accattivanti e slogan orecchiabili si nasconde nientemeno che l'agenzia spaziale statunitense: un esperimento coraggioso di comunicazione scientifica
Chiral-Odd Generalized Parton Distributions and Transversity in
  Light-Front Constituent Quark Models
Creators: name: M. Pincetti
name: B. Pasquini
name: S. Boffi
Publisher: name: Czech.J.Phys.56:F229-F236,2006
Year: 2006

description: We present the general framework to calculate chiral-odd generalized parton
distributions in the overlap representation using the Fock-state decomposition
in the transverse spin basis. In the forward limit we derive the transversity
distribution, the tensor charge and the angular momentum sum rule for quarks
with transverse polarization in an unpolarized nucleon. Numerical results are
obtained by applying the formalism to the case of light-cone wavefunctions of
constituent quark models.
La supernova a rilascio lento
Creators: Elisa Nichelli
Publisher: name: Media Inaf
Year: 2016

Una serie d’osservazioni effettuate con il telescopio spaziale Hubble ha rivelato l’affievolirsi molto prolungato nel tempo di SN 2012cg, una supernova di tipo Ia. Questo risultato può aiutare i ricercatori a comprendere meglio come funziona questo prezioso strumento cosmologico
Thermal conductance of graphene and dimerite
Creators: name: Jiang, Jin-Wu
name: Wang, Jian-Sheng
name: Li, Baowen
Publisher: name: arXiv
Year: 2009
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: We investigate the phonon thermal conductance of graphene regarding the graphene sheet as the large-width limit of graphene strips in the ballistic limit. We find that the thermal conductance depends weakly on the direction angle $θ$ of the thermal flux periodically with period $π/3$. It is further shown that the nature of this directional dependence is the directional dependence of group velocities of the phonon modes in the graphene, originating from the $D_{6h}$ symmetry in the honeycomb structure. By breaking the $D_{6h}$ symmetry in graphene, we see more obvious anisotropic effect in the thermal conductance as demonstrated by dimerite.
description: enlarged version, in PRB
title: Ð£Ð¹Ð³ÑÑÑÐºÐ¸Ð¹ ÑÐµÐ¿Ð°ÑÐ°ÑÐ¸Ð·Ð¼ ÐºÐ°Ðº Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ð° Ð½Ð°ÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½Ð¾Ð¹ Ð±ÐµÐ·Ð¾Ð¿Ð°ÑÐ½Ð¾ÑÑÐ¸ ÐÐÐ (2012-2017 Ð³Ð³.)
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Ð°ÑÐµÐ½ÐºÐ¾, 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: Ð½Ð°ÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½Ð°Ñ Ð±ÐµÐ·Ð¾Ð¿Ð°ÑÐ½Ð¾ÑÑÑ
ÑÐµÐ¿Ð°ÑÐ°ÑÐ¸Ð·Ð¼
ÐÐÐ
ÑÐ¹Ð³ÑÑÑ

description: Ð Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ Ð¸Ð·Ð»Ð¾Ð¶ÐµÐ½Ð° ÑÑÑÐ½Ð¾ÑÑÑ ÑÐ³ÑÐ¾Ð·Ñ ÑÐµÐ¿Ð°ÑÐ°ÑÐ¸ÑÑÑÐºÐ¸Ñ Ð´Ð²Ð¸Ð¶ÐµÐ½Ð¸Ð¹ Ð¡Ð¸Ð½ÑÑÐ·ÑÐ½-Ð£Ð¹Ð³ÑÑÑÐºÐ¾Ð³Ð¾ Ð°Ð²ÑÐ¾Ð½Ð¾Ð¼Ð½Ð¾Ð³Ð¾ ÑÐ°Ð¹Ð¾Ð½Ð° Ð¿Ð¾ Ð¾ÑÐ½Ð¾ÑÐµÐ½Ð¸Ñ Ðº ÐÐ¸ÑÐ°Ð¹ÑÐºÐ¾Ð¹ ÐÐ°ÑÐ¾Ð´Ð½Ð¾Ð¹ Ð ÐµÑÐ¿ÑÐ±Ð»Ð¸ÐºÐµ. Ð Ð°ÑÐºÑÑÐ²Ð°ÐµÑÑÑ ÑÑÑÑÐºÑÑÑÐ° Ð¿Ð¾Ð½ÑÑÐ¸Ð¹ Ð½Ð°ÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½Ð¾Ð¹ Ð±ÐµÐ·Ð¾Ð¿Ð°ÑÐ½Ð¾ÑÑÐ¸ Ð¸ ÑÐµÐ¿Ð°ÑÐ°ÑÐ¸Ð·Ð¼Ð°. Ð Ð°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ Ð¿ÑÐ¸ÑÐ¸Ð½Ñ Ð¸ Ð¸ÑÑÐ¾ÑÐ½Ð¸ÐºÐ¸ Ð²Ð¾Ð·Ð½Ð¸ÐºÐ½Ð¾Ð²ÐµÐ½Ð¸Ñ ÑÑÐ½Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÐµÐ¿Ð°ÑÐ°ÑÐ¸Ð·Ð¼Ð° Ð² Ð¡Ð¸Ð½ÑÑÐ·ÑÐ½Ðµ. ÐÐ·ÑÑÐµÐ½Ñ Ð¼ÐµÑÐ¾Ð´Ñ ÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÐºÐ¸ÑÐ°Ð¹ÑÐºÐ¸Ð¼Ð¸ Ð²Ð»Ð°ÑÑÑÐ¼Ð¸ ÑÑÐ°Ð±Ð¸Ð»ÑÐ½Ð¾Ð¹ Ð¾Ð±ÑÑÐ°Ð½Ð¾Ð²ÐºÐ¸ Ð² ÑÑÑÐ°Ð½Ðµ, Ð° ÑÐ°ÐºÐ¶Ðµ ÑÑÑÐ°ÑÐµÐ³Ð¸Ð¸ ÐÐÐ  Ð² Ð±Ð¾ÑÑÐ±Ðµ Ñ ÑÐ³ÑÐ¾Ð·Ð°Ð¼Ð¸ ÑÐµÐ¿Ð°ÑÐ°ÑÐ¸Ð·Ð¼Ð°.
Proton spin-lattice relaxation in acetone-water mixtures
Creators: name: Sharma, Surendra Nath
Publisher: name: University of British Columbia
Year: 2011

description: The work reported here is concerned with the measurement of the spin-lattice relaxation of protons in water, acetone, a D₂O - acetone mixture and various aqueous solutions of acetone. The theory to account for the decay rates has been outlined for a general case and has been applied in particular to acetone-water mixtures. The NMR technique has been described briefly. Temperature dependences of T₁ for all solutions have been investigated. It has been found that the relaxation in mixtures are slower than predicted by the theory.
Schwinger-Dyson Equation, Area Law and Chiral Symmetry in QCD
Creators: name: G. M. Prosperi
Publisher: name: INFN Open Access Repository
Year: 1997

description: A Schwinger-Dyson equation for the quark propagator is derived in the context
of a Bethe-Salpeter second order formalism developped in preceding papers and
of the Minimal Area Law model for the evaluation of the Wilson loop. We discuss
how the equal time straight line approximation has to be modified to include
correctly trajectories going backwards in time. We also show, by an appropriate
selection of the solution of the SD equation, that in the limit of zero quark
mass chiral symmetry breaking and a zero mass pseudoscalar meson actually
occur. The inclusion of backward quark trajectories proves to be essential to
make the model consistent with Goldstone's theorem.
Come boe nell’oceano della gravità
Creators: Marco Malaspina
Publisher: name: Media Inaf
Year: 2016

Ottime notizie dallo spazio. Da lunedì scorso i due cubetti alloggiati nel cuore della sonda LISA Pathfinder dell’ESA sono in balìa delle sole increspature della trama dello spazio-tempo. Una pietra miliare che dimostra la validità delle tecnologie per l’osservazione dallo spazio delle onde gravitazionali
Controlling diffusive transport in confined geometries
Creators: name: Burada, P. S.
name: Schmid, G.
name: Li, Y.
name: Hanggi, P.
Publisher: name: arXiv
Year: 2010
Subjects: subject: Statistical Mechanics (cond-mat.stat-mech)
subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: We analyze the diffusive transport of Brownian particles in narrow channels with periodically varying cross-section. The geometrical confinements lead to entropic barriers, the particle has to overcome in order to proceed in transport direction. The transport characteristics exhibit peculiar behaviors which are in contrast to what is observed for the transport in potentials with purely energetic barriers. By adjusting the geometric parameters of the channel one can effectively tune the transport and diffusion properties. A prominent example is the maximized enhancement of diffusion for particular channel parameters. The understanding of the role of channel-shape provides the possibility for a design of stylized channels wherein the quality of the transport can be efficiently optimized.
description: accepted for publication in Acta Physica Polonica B
Due buchi neri nati nella stessa stella
Creators: Stefano Parisini
Publisher: name: Media Inaf
Year: 2016

Per dare origine, oltre che all’onda gravitazionale rivelata da LIGO, anche al lampo di luce gamma visto dal satellite Fermi, i due famosi buchi neri dovrebbero aver avuto una vita brevissima: nati dalla medesima stella morente e fusi l’uno nell’altro pochi minuti dopo. Prospettiva entusiasmante, ma prima bisognerebbe porsi la domanda su “cosa ha veramente visto Fermi”, commenta Pietro Ubertini dell’INAF di Roma
title: ÐÐ¸Ð¾Ð½Ð¸ÑÐµÑÐºÐ¸Ð¹ Ð´Ð¸Ð·Ð°Ð¹Ð½
Creators: name: ÐÐ¾ÑÐ¾Ð²ÐºÐ¾Ð², ÐÐ»ÐµÐºÑÐµÐ¹
name: ÐÐ°ÑÑÑÐµÐ²Ð°, Ð.
name: Ð ÑÐ±Ð¾Ð², Ð®.
name: Ð©ÐµÑÐ±Ð¸Ð½Ð°, Ð.
Publisher: name: ÐÐ·Ð´-Ð²Ð¾ ÐÐ¾Ð»Ð¸ÑÐµÑÐ½. ÑÐ½-ÑÐ°
Year: 2015
Subjects: ÐÐ¸Ð¾Ð½Ð¸ÐºÐ°
Ð¥ÑÐ´Ð¾Ð¶ÐµÑÑÐ²ÐµÐ½Ð½Ð¾Ðµ ÐºÐ¾Ð½ÑÑÑÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ
Ð´Ð¸Ð·Ð°Ð¹Ð½

description: ÐÐ¾Ð½Ð¾Ð³ÑÐ°ÑÐ¸Ñ ÑÐ¾Ð´ÐµÑÐ¶Ð¸Ñ Ð°Ð½Ð°Ð»Ð¸ÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ñ Ð¿Ð¾ Ð°ÐºÑÑÐ°Ð»ÑÐ½Ð¾Ð¼Ñ ÑÑÐµÐ½Ð´Ñ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ Ð½Ð° ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½Ð¾Ð¼ ÑÑÐ°Ð¿Ðµ - Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ñ Ð±Ð¸Ð¾Ð½Ð¸ÑÐµÑÐºÐ¸Ñ Ð¿ÑÐ¸Ð½ÑÐ¸Ð¿Ð¾Ð² Ð² Ð¿ÑÐ¾ÑÐµÑÑÐµ Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¿ÑÐ¾Ð´ÑÐºÑÐ¾Ð² Ð½Ð¾Ð²Ð¾Ð³Ð¾ Ð¿Ð¾ÐºÐ¾Ð»ÐµÐ½Ð¸Ñ. Ð Ð°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ Ð¿Ð¾Ð½ÑÑÐ¸Ñ Â«Ð±Ð¸Ð¾Ð½Ð¸ÐºÐ°Â», Â«Ð±Ð¸Ð¾Ð¼Ð¸Ð¼ÐµÑÐ¸ÐºÐ°Â» Ð¸ Â«Ð±Ð¸Ð¾Ð¼Ð¸Ð¼Ð¸ÐºÑÐ¸ÑÂ». ÐÐ¿ÐµÑÐ²ÑÐµ Ð² Ð»Ð¸ÑÐµÑÐ°ÑÑÑÐµ Ð´Ð°ÐµÑÑÑ Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð¸Ðµ Ð±Ð¸Ð¾Ð½Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð´Ð¸Ð·Ð°Ð¹Ð½Ð° (Simulation & Optimization)-Driven Bionic Design ÐºÐ°Ðº Ð¿ÑÐ¸Ð½ÑÐ¸Ð¿Ð¸Ð°Ð»ÑÐ½Ð¾ Ð½Ð¾Ð²Ð¾Ð³Ð¾ Ð¿Ð¾Ð´ÑÐ¾Ð´Ð° Ðº Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¸ ÑÐ¾Ð·Ð´Ð°Ð½Ð¸Ñ Â«best-in-classÂ» Ð¾Ð¿ÑÐ¸Ð¼Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ð½ÑÑ ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð¹ Ð² ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐµ ÐºÐ¾Ð½Ð²ÐµÑÐ³ÐµÐ½ÑÐ¸Ð¸ Ð¸ ÑÐ¸Ð½ÐµÑÐ³Ð¸Ð¸ Ð´Ð²ÑÑ Ð³Ð»Ð¾Ð±Ð°Ð»ÑÐ½ÑÑ ÑÑÐµÐ½Ð´Ð¾Ð² - ÑÑÑÐµÐ¼Ð¸ÑÐµÐ»ÑÐ½Ð¾Ð³Ð¾ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ ÐºÐ¾Ð¼Ð¿ÑÑÑÐµÑÐ½Ð¾Ð³Ð¾ Ð¸Ð½Ð¶Ð¸Ð½Ð¸ÑÐ¸Ð½Ð³Ð°, Ð²ÐºÐ»ÑÑÐ°Ñ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¸ Ð¾Ð¿ÑÐ¸Ð¼Ð¸Ð·Ð°ÑÐ¸Ð¸, Ð¸ Ð°Ð´Ð´Ð¸ÑÐ¸Ð²Ð½ÑÑ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¹. ÐÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ð° Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ñ Ð¾ Ð¿ÑÐ¸Ð¼ÐµÑÐ°Ñ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ñ Ð±Ð¸Ð¾Ð½Ð¸ÑÐµÑÐºÐ¸Ñ Ð¿ÑÐ¸Ð½ÑÐ¸Ð¿Ð¾Ð² Ð² Ð°ÑÑÐ¸ÑÐµÐºÑÑÑÐµ, Ð¿ÑÐ¾Ð¼ÑÑÐ»ÐµÐ½Ð½Ð¾Ð¼ Ð´Ð¸Ð·Ð°Ð¹Ð½Ðµ Ð¸ ÑÐ°Ð·Ð»Ð¸ÑÐ½ÑÑ Ð¾ÑÑÐ°ÑÐ»ÑÑ Ð¿ÑÐ¾Ð¼ÑÑÐ»ÐµÐ½Ð½Ð¾ÑÑÐ¸ - Ð°Ð²ÑÐ¾Ð¼Ð¾Ð±Ð¸Ð»ÐµÑÑÑÐ¾ÐµÐ½Ð¸Ð¸, Ð°Ð²Ð¸Ð°ÐºÐ¾ÑÐ¼Ð¸ÑÐµÑÐºÐ¾Ð¹ Ð¾ÑÑÐ°ÑÐ»Ð¸, ÑÐ¾Ð±Ð¾ÑÐ¾ÑÐµÑÐ½Ð¸ÐºÐµ Ð¸ Ð¾Ð±Ð¾ÑÐ¾Ð½Ð½Ð¾Ð¿ÑÐ¾Ð¼ÑÑÐ»ÐµÐ½Ð½Ð¾Ð¼ ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑÐµ.
Benvenuti al sud della cometa 67P
Creators: Elisa Nichelli
Publisher: name: Media Inaf
Year: 2016

La sonda Rosetta è riuscita ad avvicinarsi di nuovo al nucleo di 67P/ Churyumov-Gerasimenko, e ora si trova alla distanza di 35 km dalla sua superficie. La camera ad angolo stretto di OSIRIS ha raccolto immagini alla risoluzione di 80 cm per pixel, scoprendo tre nuove regioni nel suo emisfero australe
Critical phenomena: 150 years since Cagniard de la Tour
Creators: name: Berche, Bertrand
name: Henkel, Malte
name: Kenna, Ralph
Publisher: name: arXiv
Year: 2009
Subjects: subject: History and Philosophy of Physics (physics.hist-ph)
subject: Statistical Mechanics (cond-mat.stat-mech)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: Critical phenomena were discovered by Cagniard de la Tour in 1822, who died 150 years ago. In order to mark this anniversary, the context and the early history of his discovery is reviewed. We then follow with a brief sketch of the history of critical phenomena, indicating the main lines of development until the present date. Os fenómenos cr\'ıticos foram descobertos pelo Cagniard de la Tour em Paris em 1822. Para comemorar os 150 anos da sua morte, o contexto e a história initial da sua descoberta é contada. Conseguimos com uma descrição breve da história dos fenémenos cr\'ıticos, indicando as linhas principais do desenvolvimento até o presente.
description: Latex2e, 8 pp, 3 eps figures included
Monopole-like Excitations as a Source of Confinement in the
  SU(2)-Gluodynamics
Creators: name: Antonov, Dmitri
name: Ebert, Dietmar
Publisher: name: INFN Open Access Repository
Year: 1999

description: By making use of the Abelian projection method, a dual version of the
SU(2)-gluodynamics with manifest monopole-like excitations, arising from the
integration over singular gauge transformations, is formulated in the continuum
limit. The resulting effective theory emerges due to the summation over the
grand canonical ensemble of these excitations in the dilute gas approximation.
As a result, the dual Abelian gauge boson acquires a nonvanishing (magnetic)
mass due to the Debye screening effects in such a gas. The obtained theory is
then used for the construction of the corresponding effective potential of
monopole loop currents and the string representation. Finally, by virtue of
this representation, confining properties of the SU(2)-gluodynamics are
emphasized.
Ecco il “luogo di nascita” di un lampo radio
Creators: Marco Galliani
Publisher: name: Media Inaf
Year: 2016

Individuato per la prima volta da un gruppo internazionale di astronomi, tra cui Marta Burgay, Delphine Perrodin e Andrea Possenti dell’INAF di Cagliari, il luogo d’origine di un lampo radio: una categoria di enigmatici segnali radio, della durata di appena qualche millisecondo, che appaiono senza preavviso nel cielo. Il risultato su Nature
title: ÐÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ñ Ð½Ð°Ð·ÐµÐ¼Ð½ÑÑ ÑÑÐ°Ð½ÑÐ¿Ð¾ÑÑÐ½ÑÑ Ð¼Ð°ÑÐ¸Ð½. ÐÐ·ÑÑÐµÐ½Ð¸Ðµ Ð»Ð¸Ð½Ð¸Ð¸ Ð¿ÑÐ¾Ð²ÐµÑÐºÐ¸ ÑÐ¾ÑÑÐ¾ÑÐ½Ð¸Ñ Ñ Ð¾Ð´Ð¾Ð²Ð¾Ð¹ ÑÐ¸ÑÑÐµÐ¼Ñ Ð°Ð²ÑÐ¾Ð¼Ð¾Ð±Ð¸Ð»Ñ
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ
titleType: Subtitle
Creators: name: ÐÐµÐ¼Ð¸Ð´Ð¾Ð², ÐÐ¸ÐºÐ¾Ð»Ð°Ð¹
name: ÐÑÐ°ÑÐ¸Ð»ÑÐ½Ð¸ÐºÐ¾Ð², ÐÐ½Ð´ÑÐµÐ¹
Publisher: name: ÐÐ·Ð´-Ð²Ð¾ ÐÐ¾Ð»Ð¸ÑÐµÑÐ½. ÑÐ½-ÑÐ°
Year: 2018
Subjects: ÐÐ²ÑÐ¾Ð¼Ð¾Ð±Ð¸Ð»Ð¸
ÐÐ²ÑÐ¾Ð¼Ð¾Ð±Ð¸Ð»ÑÐ½ÑÐµ Ð¿Ð¾Ð´Ð²ÐµÑÐºÐ¸

description: ÐÑÐ¾Ð°Ð½Ð°Ð»Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ñ ÑÐµÐ½Ð´ÐµÐ½ÑÐ¸Ð¸ Ð²Ð¸Ð´Ð¾Ð¸Ð·Ð¼ÐµÐ½ÐµÐ½Ð¸Ñ Ð¿ÐµÑÐ°ÑÐ½ÑÑ ÑÑÐµÐ´ÑÑÐ² Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¸, ÑÐºÐ°Ð·Ð°Ð½Ñ Ð¿ÑÐ¸ÑÐ¸Ð½Ñ Ð·Ð°ÑÐ¾Ð¶Ð´ÐµÐ½Ð¸Ñ Ð¸ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ Ð¾Ð¿ÐµÑÐ°ÑÐ¸Ð²Ð½Ð¾Ð¹ Ð¿Ð¾Ð»Ð¸Ð³ÑÐ°ÑÐ¸Ð¸, Ð¾Ð¿Ð¸ÑÐ°Ð½Ñ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ðµ ÑÑÐµÐ¼Ñ Ð¸ Ð¾Ð±Ð¾ÑÑÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð´Ð»Ñ ÐµÐµ ÑÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸. Ð Ð°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ ÑÐ¸Ð·Ð¸ÑÐµÑÐºÐ¸Ðµ Ð·Ð°ÐºÐ¾Ð½Ð¾Ð¼ÐµÑÐ½Ð¾ÑÑÐ¸, Ð»ÐµÐ¶Ð°ÑÐ¸Ðµ Ð² Ð¾ÑÐ½Ð¾Ð²Ðµ Ð¿ÑÐ¾ÑÐµÑÑÐ¾Ð² Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²Ð° Ð¿ÐµÑÐ°ÑÐ½Ð¾Ð¹ Ð¿ÑÐ¾Ð´ÑÐºÑÐ¸Ð¸ Ð¼ÐµÑÐ¾Ð´Ð°Ð¼Ð¸ Ð¾Ð¿ÐµÑÐ°ÑÐ¸Ð²Ð½Ð¾Ð¹ Ð¿Ð¾Ð»Ð¸Ð³ÑÐ°ÑÐ¸Ð¸. ÐÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¾ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² Ð¸ Ð°ÑÐ¿Ð¸ÑÐ°Ð½ÑÐ¾Ð², Ð¸Ð·ÑÑÐ°ÑÑÐ¸Ñ Ð¿Ð¾Ð»Ð¸Ð³ÑÐ°ÑÐ¸ÑÐµÑÐºÐ¸Ðµ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¸ Ð¸ Ð¾Ð±Ð¾ÑÑÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ, ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÐºÑ Ð¸ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸ÑÐ¼Ð¸ Ð¿Ð¾Ð»Ð¸Ð³ÑÐ°ÑÐ¸ÑÐµÑÐºÐ¾Ð¹ Ð¿ÑÐ¾Ð¼ÑÑÐ»ÐµÐ½Ð½Ð¾ÑÑÐ¸.
description: ÐÐµÑÐ°ÑÐ°ÐµÑÑÑ Ð¿Ð¾ ÑÐµÑÐµÐ½Ð¸Ñ Ð¡Ð¾Ð²ÐµÑÐ° Ð¿Ð¾ Ð¸Ð·Ð´Ð°ÑÐµÐ»ÑÑÐºÐ¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð£ÑÐµÐ½Ð¾Ð³Ð¾ ÑÐ¾Ð²ÐµÑÐ° Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¾Ð³Ð¾ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑÐ° ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾.
Effective Field Theory, Past and Future
Creators: name: Weinberg, Steven
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: History and Philosophy of Physics (physics.hist-ph)
subject: FOS: Physical sciences

description: This is a written version of the opening talk at the 6th International Workshop on Chiral Dynamics, at the University of Bern, Switzerland, July 6, 2009, to be published in the proceedings of the Workshop. In it, I reminisce about the early development of effective field theories of the strong interactions, comment briefly on some other applications of effective field theories, and then take up the idea that the Standard Model and General Relativity are the leading terms in an effective field theory. Finally, I cite recent calculations that suggest that the effective field theory of gravitation and matter is asymptotically safe.
description: Correction to footnote 29 and associated text. 21 pages
L’unione fa la forza… galattica
Creators: Francesca Aloisio
Publisher: name: Media Inaf
Year: 2016

Cos'ha reionizzato l’Universo? Prova a rispondere uno studio pubblicato su ApJ Letters da un team di scienziati guidato da Marco Castellano, dell’Osservatorio astronomico dell’INAF di Roma. Studio che individua il contributo al processo di ionizzazione da parte d’una struttura di galassie lontane
ATLASGAL, survey a grande area della Via Lattea
Creators: Redazione Media Inaf
Publisher: name: Media Inaf
Year: 2016

Leonardo Testi (ESO e INAF): «ATLASGAL ci ha permesso di lanciare uno sguardo nuovo al mezzo interstellare denso della nostra galassia, la Via Lattea, e di conseguenza di trasformare la nostra visione della formazione stellare»
title: ÐÐ¾Ð´ÐµÑÐ½Ð¸Ð·Ð°ÑÐ¸Ñ Ð¸ Ð²Ð½ÐµÐ´ÑÐµÐ½Ð¸Ðµ ÑÐ¸ÑÑÐµÐ¼Ñ Ð¾Ð¿ÐµÑÐ°ÑÐ¸Ð²Ð½Ð¾Ð³Ð¾ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²Ð¾Ð¼ Ð² ÐÐÐ Â«Geneticlab NutritionÂ»
title: Ð¼Ð°Ð³Ð¸ÑÑÐµÑÑÐºÐ°Ñ Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ñ
titleType: Subtitle
Creators: name: ÐÑÑÐ»ÐµÐ², ÐÐ°Ð½Ð¸Ð¸Ð»
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2017
Subjects: ÐÐ½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¾Ð½Ð½ÑÐµ ÑÐ¸ÑÑÐµÐ¼Ñ
ÐÐ²ÑÐ¾Ð¼Ð°ÑÐ¸Ð·Ð°ÑÐ¸Ñ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²Ð°
Ð±Ð¸Ð·Ð½ÐµÑ-Ð¿ÑÐ¾ÑÐµÑÑÑ
ÑÐµÐ¸Ð½Ð¶Ð¸Ð½Ð¸ÑÐ¸Ð½Ð³

description: Ð¦ÐµÐ»ÑÑ Ð¼Ð°Ð³Ð¸ÑÑÐµÑÑÐºÐ¾Ð¹ Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ð¸ ÑÐ²Ð»ÑÐµÑÑÑ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð°ÑÐ¸Ð¹ Ð¿Ð¾ ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ¸ÑÑÐµÐ¼ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²ÐµÐ½Ð½ÑÐ¼Ð¸ Ð¿ÑÐ¾ÑÐµÑÑÐ°Ð¼Ð¸ Ð¸ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð´Ð°Ð½Ð½ÑÐ¼Ð¸ Ð¾Ð± Ð¸Ð·Ð´ÐµÐ»Ð¸Ð¸ Ð½Ð° Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ð¸ ÐÐÐ Â«Geneticlab NutritionÂ». ÐÐ±ÑÐµÐºÑÐ¾Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ ÑÐ²Ð»ÑÐµÑÑÑ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ðµ ÐÐÐ Â«Geneticlab NutritionÂ», Ð¾ÑÐ½Ð¾Ð²Ð½Ð¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÑÑ ÐºÐ¾ÑÐ¾ÑÐ¾Ð³Ð¾ ÑÐ²Ð»ÑÐµÑÑÑ Ð²ÑÐ¿ÑÑÐº Ð¸ Ð¿ÑÐ¾Ð´Ð°Ð¶Ð° ÑÐ¿Ð¾ÑÑÐ¸Ð²Ð½Ð¾Ð³Ð¾ Ð¿Ð¸ÑÐ°Ð½Ð¸Ñ. Ð ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐµ Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¸Ñ Ð¼Ð°Ð³Ð¸ÑÑÐµÑÑÐºÐ¾Ð¹ Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ð¸, Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð¸Ð¸ ÑÑÑÐ°ÑÐµÐ³Ð¸ÑÐµÑÐºÐ¸Ñ ÑÐµÐ»ÐµÐ¹ ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸, Ð° ÑÐ°ÐºÐ¶Ðµ ÑÑÐµÐ±Ð¾Ð²Ð°Ð½Ð¸Ð¹ ÐºÐ»ÑÑÐµÐ²ÑÑ Ð±Ð¸Ð·Ð½ÐµÑ - Ð¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°ÑÐµÐ»ÐµÐ¹, ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ñ Ð¸ ÑÐµÐ°Ð»Ð¸Ð·Ð¾Ð²Ð°Ð½Ñ ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð°ÑÐ¸Ð¸ Ð¿Ð¾ ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ¸ÑÑÐµÐ¼ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²ÐµÐ½Ð½ÑÐ¼Ð¸ Ð¿ÑÐ¾ÑÐµÑÑÐ°Ð¼Ð¸ Ð¸ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð´Ð°Ð½Ð½ÑÐ¼Ð¸ Ð¾Ð± Ð¸Ð·Ð´ÐµÐ»Ð¸Ð¸, ÑÐ¾ÑÑÐ°Ð²Ð»ÐµÐ½ ÑÐµÐ³Ð»Ð°Ð¼ÐµÐ½Ñ ÑÐ°Ð±Ð¾ÑÑ Ð¸ Ð½Ð°Ð¿Ð¸ÑÐ°Ð½Ñ Ð´Ð¾Ð»Ð¶Ð½Ð¾ÑÑÐ½ÑÐµ Ð¸Ð½ÑÑÑÑÐºÑÐ¸Ð¸ Ð¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°ÑÐµÐ»ÐµÐ¹.
Additional file 1 of Uncovering heterogeneous cognitive trajectories in mild cognitive impairment: a data-driven approach
Creators: name: Wang, Xiwu
name: Ye, Teng
name: Zhou, Wenjun
name: Zhang, Jie
Publisher: name: figshare
Year: 2023
Subjects: subject: Biochemistry
subject: Medicine
subject: Neuroscience
subject: Biotechnology
subject: Chemical Sciences not elsewhere classified
subject: Sociology
subject: FOS: Sociology
subject: Biological Sciences not elsewhere classified
subject: Mental Health

description: Additional file 1.
Electronic and Magnetic Properties of Partially-Open Carbon Nanotubes
Creators: name: Huang, Bing
name: Son, Young-Woo
name: Kim, Gunn
name: Duan, Wenhui
name: Ihm, Jisoon
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: On the basis of the spin-polarized density functional theory calculations, we demonstrate that partially-open carbon nanotubes (CNTs) observed in recent experiments have rich electronic and magnetic properties which depend on the degree of the opening. A partially-open armchair CNT is converted from a metal to a semiconductor, and then to a spin-polarized semiconductor by increasing the length of the opening on the wall. Spin-polarized states become increasingly more stable than nonmagnetic states as the length of the opening is further increased. In addition, external electric fields or chemical modifications are usable to control the electronic and magnetic properties of the system. We show that half-metallicity may be achieved and the spin current may be controlled by external electric fields or by asymmetric functionalization of the edges of the opening. Our findings suggest that partially-open CNTs may offer unique opportunities for the future development of nanoscale electronics and spintronics.
description: 6 figures, to appear in J. Am. Chem. Soc
title: ÐÑÐ´Ð¸Ñ. Ð§. 2
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ
titleType: Subtitle
Creators: name: ÐÑÐºÐ¸ÑÐµÐ²Ð°, ÐÐ»ÐµÐºÑÐ°Ð½Ð´ÑÐ°
name: Ð¢Ð¾Ð¼ÑÐ¸Ð½ÑÐºÐ°Ñ, ÐÑÐ¸Ð½Ð°
name: ÐÐ°Ð½Ð¾Ð², ÐÐ»ÐµÐºÑÐµÐ¹
Publisher: name: Ð¡ÐÐ±ÐÐ¢Ð­Ð£
Year: 2013
Subjects: Ð°ÑÐ´Ð¸Ñ
ÑÑÐµÐ±Ð½Ð¸ÐºÐ¸ Ð¸ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ñ Ð´Ð»Ñ Ð²ÑÐ·Ð¾Ð²

description: ÐÐ¾ÑÐ¾Ð±Ð¸Ðµ Â«ÐÑÐ´Ð¸ÑÂ» (II ÑÐ°ÑÑÑ) Ð¿Ð¾ÑÐ²ÑÑÐµÐ½Ð¾ Ð²ÐµÑÐ¾ÑÑÐ½Ð¾ÑÑÐ½Ð¾Ð¼Ñ Ð¿Ð¾Ð´ÑÐ¾Ð´Ñ Ð² Ð°ÑÐ´Ð¸ÑÐµ. Ð­ÑÐ¾Ñ Ð¿Ð¾Ð´ÑÐ¾Ð´ ÑÐ²Ð»ÑÐµÑÑÑ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐ¼ Ð¿ÑÐ¸ ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½Ð¾Ð¼ Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¸Ð¸ Ð²Ð½ÐµÑÐ½ÐµÐ³Ð¾ Ð°ÑÐ´Ð¸ÑÐ°. Ð Ð¿Ð¾ÑÐ¾Ð±Ð¸Ð¸ Ð´ÐµÑÐ°Ð»ÑÐ½Ð¾ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ð° Ð¾ÑÐµÐ½ÐºÐ° ÑÐ¸ÑÐºÐ° Ð² Ð°ÑÐ´Ð¸ÑÐµ Ð½Ð° ÑÐ°Ð·Ð»Ð¸ÑÐ½ÑÑ ÐµÐ³Ð¾ ÑÑÐ°Ð´Ð¸ÑÑ. ÐÑÐ¾Ð±Ð¾Ðµ Ð²Ð½Ð¸Ð¼Ð°Ð½Ð¸Ðµ ÑÐ´ÐµÐ»ÐµÐ½Ð¾ ÐºÐ¾Ð½ÑÐµÐ¿ÑÐ¸Ð¸ Â«ÑÑÑÐµÑÑÐ²ÐµÐ½Ð½Ð¾ÑÑÑÂ». Ð Ð¿Ð¾ÑÐ¾Ð±Ð¸Ð¸ ÑÐ°ÐºÐ¶Ðµ Ð¿Ð¾ÐºÐ°Ð·Ð°Ð½Ð¾, ÐºÐ°ÐºÐ¸Ðµ ÑÑÐµÐ±Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¿ÑÐµÐ´ÑÑÐ²Ð»ÑÑÑÑÑ Ðº Ð°ÑÐ´Ð¸ÑÐ¾ÑÑ Ð¿ÑÐ¸ ÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ð¸ Ð²ÐµÑÐ¾ÑÑÐ½Ð¾ÑÑÐ½Ð¾Ð¼Ñ Ð¿Ð¾Ð´ÑÐ¾Ð´Ñ Ð² ÑÐ¾Ð¾ÑÐ²ÐµÑÑÑÐ²Ð¸Ð¸ Ñ MCA 315 Â«ÐÑÑÐ²Ð»ÐµÐ½Ð¸Ðµ Ð¸ Ð¾ÑÐµÐ½ÐºÐ° ÑÐ¸ÑÐºÐ¾Ð² ÑÑÑÐµÑÑÐ²ÐµÐ½Ð½ÑÑ Ð¸ÑÐºÐ°Ð¶ÐµÐ½Ð¸Ð¹ Ð² ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐµ Ð´Ð¾ÑÑÐ¸Ð¶ÐµÐ½Ð¸Ñ Ð¿Ð¾Ð½Ð¸Ð¼Ð°Ð½Ð¸Ñ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ Ð¸ ÐµÐ³Ð¾ ÑÑÐµÐ´ÑÂ». ÐÐ¾ÐºÐ°Ð·Ð°Ð½Ñ Ð¿ÑÐµÐ¸Ð¼ÑÑÐµÑÑÐ²Ð° Ð¸ Ð½ÐµÐ´Ð¾ÑÑÐ°ÑÐºÐ¸ Ð¿ÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸Ñ ÑÐ¾ÑÐ¼Ð°Ð»Ð¸Ð·Ð¾Ð²Ð°Ð½Ð½ÑÑ Ð¿Ð¾Ð´ÑÐ¾Ð´Ð¾Ð² Ð² Ð°ÑÐ´Ð¸Ñ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¸ Â«ÐÑÑÐ³Ð°Ð»ÑÐµÑÑÐºÐ¸Ð¹ ÑÑÐµÑ, Ð°Ð½Ð°Ð»Ð¸Ð· Ð¸ Ð°ÑÐ´Ð¸ÑÂ», ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ¸Ð°ÑÐ° Ð¿Ð¾ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Â«Ð­ÐºÐ¾Ð½Ð¾Ð¼Ð¸ÐºÐ°Â» Ð¸ Ð¼Ð°Ð³Ð¸ÑÑÑÐ°ÑÑÑÑ, Ð¸Ð·ÑÑÐ°ÑÑÐ¸Ñ Ð´Ð¸ÑÑÐ¸Ð¿Ð»Ð¸Ð½Ñ Â«ÐÑÐ´Ð¸ÑÂ». ÐÐ½Ð¾ ÑÐ°ÐºÐ¶Ðµ Ð¼Ð¾Ð¶ÐµÑ Ð±ÑÑÑ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¾ Ð¿ÑÐµÐ¿Ð¾Ð´Ð°Ð²Ð°ÑÐµÐ»ÑÐ¼Ð¸, Ð°ÑÐ¿Ð¸ÑÐ°Ð½ÑÐ°Ð¼Ð¸ Ð¸ Ð»Ð¸ÑÐ°Ð¼Ð¸, Ð¿ÑÐ¾ÑÐ²Ð»ÑÑÑÐ¸Ð¼Ð¸ Ð¸Ð½ÑÐµÑÐµÑ Ðº ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ Ð°ÑÐ´Ð¸ÑÐ°.
Towards an octonionic world
Creators: name: S. De Leo
name: K. Abdel-Khalek
Publisher: name: Int.J.Theor.Phys. 37 (1998) 1945
Year: 1999

description: In order to obtain a consistent formulation of octonionic quantum mechanics
(OQM), we introduce left-right barred operators. Such operators enable us to
find the translation rules between octonionic numbers and $8\times 8$ real
matrices (a translation is also given for $4\times 4$ complex matrices). The
use of a complex geometry allows us to overcome the hermiticity problem and
define an appropriate momentum operator within OQM. As an application of our
results, we develop an octonionic relativistic free wave equation, linear in
the derivatives. Even if the wave functions are only one-component we show that
four independent solutions, corresponding to those of the Dirac equation,
exist.
Laser frequency stabilization to highly excited state transitions using electromagnetically induced transparency in a cascade system
Creators: name: Abel, R. P.
name: Mohapatra, A. K.
name: Bason, M. G.
name: Pritchard, J. D.
name: Weatherill, K. J.
name: Raitzsch, U.
name: Adams, C. S.
Publisher: name: arXiv
Year: 2008
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We demonstrate laser frequency stabilization to excited state transitions using cascade electromagnetically induced transparency (EIT). Using a room temperature Rb vapor cell as a reference, we stabilize a first diode laser to the D2 transition and a second laser to a transition from the intermediate state to a Rydberg state with principal quantum number n=19 - 70. A combined laser linewidth of 280 kHz over a 0.1 ms time period is achieved. This method may be applied generally to any cascade system and allows laser stabilization to an atomic reference in the absence of strong optical transitions.
description: 3 pages, 4 figures, with corrections
Salvatore Capozziello: «È un trionfo per la Fisica»
Creators: Corrado Ruscica
Publisher: name: Media Inaf
Year: 2016

Perché le onde gravitazionali sono così deboli? Anche noi ne solleviamo, per esempio quando acceleriamo con l’auto o freniamo al semaforo? Tutto quello che avreste voluto sapere sulle onde gravitazionali (ma non avete mai osato chiedere), Media INAF lo ha chiesto per voi al Presidente della Società Italiana di Relatività Generale e Fisica della Gravitazione
Renormalization-group flow in the 3D Georgi-Glashow model
Creators: name: Antonov, Dmitri
Publisher: name: INFN Open Access Repository
Year: 2001

description: The renormalization-group (RG) flow in the finite-temperature
(2+1)-dimensional Georgi-Glashow model is explored. This is done in the limit
when the squared electric coupling constant is much larger than the mass of the
Higgs field. The novel equation describing the evolution of the Higgs mass is
derived and integrated along the separatrices of the RG flow in the limit when
the original theory reduces to the 2D XY model. In particular, it is checked
that in the vicinity of the phase-transition point, there exists a range of
parameters allowing to the Higgs mass evolved along some of the separatrices to
remain much smaller than the squared electric coupling constant.
Un lander sulla luna ghiacciata Europa
Creators: Stefano Parisini
Publisher: name: Media Inaf
Year: 2016

Uno studio statunitense propone di utilizzare la potente emissione radio naturale di Giove come trasmettitore, e una sonda sulla superficie di Europa - una delle sue lune - come ricevitore passivo dell’eco radar riflessa dall’oceano nascosto sotto la sua crosta ghiacciata. Il commento di Roberto Orosei (INAF Bologna) e Lorenzo Bruzzone (Università di Trento)
Three-Dimensional Solutions of Supersymmetrical Intertwining Relations and Pairs of Isospectral Hamiltonians
Creators: name: Cannata, F.
name: Ioffe, M. V.
name: Nishnianidze, D. N.
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: Mathematical Physics (math-ph)
subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: The general solution of SUSY intertwining relations for three-dimensional Schrödinger operators is built using the class of second order supercharges with nondegenerate constant metric. This solution includes several models with arbitrary parameters. We are interested only in quantum systems which are not amenable to separation of variables, i.e. can not be reduced to lower dimensional problems. All constructed Hamiltonians are partially integrable - each of them commutes with a symmetry operator of fourth order in momenta. The same models can be considered also for complex values of parameters leading to a class of non-Hermitian isospectral Hamiltonians.
description: 14 pages
Generalized Eulerian Coordinates for Relativistic Fluids: Hamiltonian
  Rest-Frame Instant Form, Relative Variables, Rotational Kinematics
Creators: name: Alba, David
name: Lusanna, Luca
Publisher: name: INFN Open Access Repository
Year: 2003

description: We study the rest-frame instant form of a new formulation of relativistic
perfect fluids in terms of new generalized Eulerian configuration coordinates.
After the separation of the relativistic center of mass from the relative
variables on the Wigner hyper-planes, we define orientational and shape
variables for the fluid, viewed as a relativistic extended deformable body, by
introducing dynamical body frames. Finally we define Dixon's multipoles for the
fluid.
Additional file 3 of The co-development of a linguistic and culturally tailored tele-retinopathy screening intervention for immigrants living with diabetes from China and African-Caribbean countries in Ottawa, Canada
Creators: name: Umaefulam, Valerie
name: Wilson, Mackenzie
name: Boucher, Marie Carole
name: Brent, Michael H.
name: Dogba, Maman Joyce
name: Drescher, Olivia
name: Grimshaw, Jeremy M.
name: Ivers, Noah M.
name: Lawrenson, John G.
name: Lorencatto, Fabiana
name: Maberley, David
name: McCleary, Nicola
name: McHugh, Sheena
name: Sutakovic, Olivera
name: Thavorn, Kednapa
name: Witteman, Holly O.
name: Yu, Catherine
name: Cheng, Hao
name: Han, Wei
name: Hong, Yu
name: Idrissa, Balkissa
name: Leech, Tina
name: Malette, Joffré
name: Mongeon, Isabelle
name: Mugisho, Zawadi
name: Nguebou, Marlyse Mbakop
name: Pabla, Sara
name: Rahman, Siffan
name: Samandoulougou, Azaratou
name: Visram, Hasina
name: You, Richard
name: Zhao, Junqiang
name: Presseau, Justin
Publisher: name: figshare
Year: 2023
Subjects: subject: Medicine
subject: Biotechnology
subject: Sociology
subject: FOS: Sociology
subject: Biological Sciences not elsewhere classified
subject: Marine Biology
subject: Science Policy

description: Additional file 3.
3D Georgi-Glashow model and confining strings at zero and finite
  temperatures
Creators: name: D. Antonov
name: M. C. Diamantini
Publisher: name: INFN Open Access Repository
Year: 2004

description: In this review, we discuss the confining and finite-temperature properties of
the 3D SU(N) Georgi-Glashow model, and of 4D compact QED. At zero temperature,
we derive string representations of both theories, thus constructing the
SU(N)-version of Polyakov's theory of confining strings. We discuss the
geometric properties of confining strings, as well as the appearance of the
string theta-term from the field-theoretical one in 4D, and k-string tensions
at N larger than 2. In particular, we point out the relevance of negative
stiffness for stabilizing confining strings, an effect recently re-discovered
in material science. At finite temperature, we present a derivation of the
confining-string free energy and show that, at the one-loop level and for a
certain class of string models in the large-D limit, it matches that of QCD at
large N. This crucial matching is again a consequence of the negative
stiffness. In the discussion of the finite-temperature properties of the 3D
Georgi-Glashow model, in order to be closer to QCD, we mostly concentrate at
the effects produced by some extensions of the model by external matter fields,
such as dynamical fundamental quarks or photinos, in the supersymmetric
generalization of the model.
New Directions in Non-Relativistic and Relativistic Rotational and
  Multipole Kinematics for N-Body and Continuous Systems
Creators: name: D. Alba
name: L. Lusanna
name: M. Pauri
Publisher: name: INFN Open Access Repository
Year: 2005

description: In non-relativistic mechanics the center of mass of an isolated system is
easily separated out from the relative variables. For a N-body system these
latter are usually described by a set of Jacobi normal coordinates, based on
the clustering of the centers of mass of sub-clusters. The Jacobi variables are
then the starting point for separating {\it orientational} variables, connected
with the angular momentum constants of motion, from {\it shape} (or {\it
vibrational}) variables. Jacobi variables, however, cannot be extended to
special relativity. We show by group-theoretical methods that two new sets of
relative variables can be defined in terms of a {\it clustering of the angular
momenta of sub-clusters} and directly related to the so-called {\it dynamical
body frames} and {\it canonical spin bases}. The underlying group-theoretical
structure allows a direct extension of such notions from a non-relativistic to
a special- relativistic context if one exploits the {\it rest-frame instant
form of dynamics}. The various known definitions of relativistic center of mass
are recovered. The separation of suitable relative variables from the so-called
{\it canonical internal} center of mass leads to the correct kinematical
framework for the relativistic theory of the orbits for a N-body system with
action -at-a-distance interactions. The rest-frame instant form is also shown
to be the correct kinematical framework for introducing the Dixon multi-poles
for closed and open N-body systems, as well as for continuous systems,
exemplified here by the configurations of the Klein-Gordon field that are
compatible with the previous notions of center of mass.
Constraining the MSSM Higgs sector using precise Higgs mass predictions
Creators: name: Bahl, Henning
Publisher: name: Deutsches Elektronen-Synchrotron, DESY, Hamburg
Year: 2019

description: Rencontres de Moriond QCD & High Energy Interactions, La Thuile, Italy, 23 Mar 2019 - 30 Mar 2019
Additional file 3: of Functional characterization of Gh_A08G1120 (GH3.5) gene reveal their significant role in enhancing drought and salt stress tolerance in cotton
Creators: name: Kirungu, Joy
name: Magwanga, Richard
name: Lu, Pu
name: Cai, Xiaoyan
name: Zhou, Zhongli
name: Wang, Xingxing
name: Peng, Renhai
name: Wang, Kunbo
name: Liu, Fang
Publisher: name: figshare
Year: 2019
Subjects: subject: Space Science
subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Plant Biology

description: Table S3. Go analysis of the upland cotton, G. hirsutum GH3 genes. (DOCX 21 kb)
La galassia con la scia
Creators: Elisa Nichelli
Publisher: name: Media Inaf
Year: 2016

Il Canada France Hawaii Telescope ha puntato i suoi strumenti per la prima volta su una galassia dell’ammasso della Vergine: NGC 4569. Quello che ha scoperto è un’enorme scia, lunga più di 300 mila anni luce, composta da idrogeno gassoso, che corrisponde al gas mancante nella galassia. Il commento di Alessandro Boselli del Laboratoire d'Astrophysique de Marseille
A caccia di galassie ultra-compatte con il VST
Creators: Marco Galliani
Publisher: name: Media Inaf
Year: 2016

Uno studio guidato dal team di astronomi dell’INAF coinvolti nella campagna osservativa KiDS dell'ESO conferma l’esistenza di galassie che hanno massa superiore alla nostra Via Lattea ma una dimensione fino a un quinto più piccola, ossia densità di materia più di cento volte superiori a quelle della nostra Galassia
title: Ð¡Ð¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð¼ÐµÑ Ð°Ð½Ð¸Ð·Ð¼Ð¾Ð² ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÑÑ Ð¸ Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ñ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ð¹ ÑÑÑÐ¾Ð¹ÑÐ¸Ð²Ð¾ÑÑÐ¸ ÐºÐ¾ÑÐ¿Ð¾ÑÐ°ÑÐ¸Ð²Ð½ÑÑ Ð¿ÑÐ¾Ð¼ÑÑÐ»ÐµÐ½Ð½ÑÑ ÑÑÑÑÐºÑÑÑ
Creators: name: Ð¡Ð¾ÐºÐ¾Ð»Ð¸ÑÑÐ½, ÐÐ»ÐµÐºÑÐ°Ð½Ð´Ñ
name: ÐÐ²Ð°Ð½Ð¾Ð², ÐÐ°ÐºÑÐ¸Ð¼
name: Ð¡Ð¾ÐºÐ¾Ð»Ð¸ÑÑÐ½Ð°, ÐÐ°ÑÐ°Ð»ÑÑ
Publisher: name: ÐÐ·Ð´-Ð²Ð¾ ÐÐ¾Ð»Ð¸ÑÐµÑÐ½. ÑÐ½-ÑÐ°
Year: 2016
Subjects: ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð°Ñ ÑÑÑÐ¾Ð¹ÑÐ¸Ð²Ð¾ÑÑÑ
ÐºÐ¾ÑÐ¿Ð¾ÑÐ°ÑÐ¸Ð²Ð½Ð¾Ðµ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ
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description: Ð Ð¼Ð¾Ð½Ð¾Ð³ÑÐ°ÑÐ¸Ð¸ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ñ Ð²Ð°Ð¶Ð½ÐµÐ¹ÑÐ¸Ðµ Ð·Ð°Ð´Ð°ÑÐ¸ ÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ, ÑÑÐ½ÐºÑÐ¸Ð¾Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¸ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ ÐºÐ¾ÑÐ¿Ð¾ÑÐ°ÑÐ¸Ð²Ð½ÑÑ Ð¿ÑÐ¾Ð¼ÑÑÐ»ÐµÐ½Ð½ÑÑ ÑÐ¸ÑÐ¼. Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ñ Ð±Ð°Ð»Ð°Ð½Ñ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾-ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²ÑÑ Ð¿Ð¾ÑÐ¾ÐºÐ¾Ð² Ð¿ÑÐ¾Ð¼ÑÑÐ»ÐµÐ½Ð½ÑÑ ÑÐ¸ÑÐ¼ Ð¸ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÐºÐ¾-Ð¼Ð°ÑÐµÐ¼Ð°ÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð¼Ð¾Ð´ÐµÐ»Ð¸ ÑÐ¾Ð³Ð»Ð°ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¸Ñ Ð¸Ð½ÑÐµÑÐµÑÐ¾Ð² Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ð¹ Ð³Ð¾ÑÐ¸Ð·Ð¾Ð½ÑÐ°Ð»ÑÐ½Ð¾-Ð¸Ð½ÑÐµÐ³ÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð½ÑÑ, Ð´Ð¸Ð²ÐµÑÑÐ¸ÑÐ¸ÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð½ÑÑ Ð¸ Ð²ÐµÑÑÐ¸ÐºÐ°Ð»ÑÐ½Ð¾-Ð¸Ð½ÑÐµÐ³ÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð½ÑÑ ÑÐ¸ÑÐ¼. ÐÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ñ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÑ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐµÐ»ÐµÐ¹ Ð´Ð¸Ð²ÐµÑÑÐ¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¸ ÐºÐ°Ðº Ð²Ð°Ð¶Ð½ÐµÐ¹ÑÐµÐ³Ð¾ Ð¼ÐµÑÐ°Ð½Ð¸Ð·Ð¼Ð° Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ñ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ Ð¿ÑÐ¾Ð¼ÑÑÐ»ÐµÐ½Ð½ÑÑ ÑÐ¸ÑÐ¼ Ð¸ Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð¸Ñ ÐºÑÐ¸ÑÐ¸ÑÐµÑÐºÐ¸Ñ Ð·Ð½Ð°ÑÐµÐ½Ð¸Ð¹ Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»ÐµÐ¹ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ð¹ ÑÑÑÐ¾Ð¹ÑÐ¸Ð²Ð¾ÑÑÐ¸ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ð¹ ÐºÐ¾ÑÐ¿Ð¾ÑÐ°ÑÐ¸Ð²Ð½ÑÑ ÑÐ¸ÑÐ¼. Ð¡ÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ñ Ð¼Ð¾Ð´ÐµÐ»Ð¸ Ð¸ Ð°Ð»Ð³Ð¾ÑÐ¸ÑÐ¼Ñ Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð¸Ñ ÐºÑÐ°ÑÐºÐ¾ÑÑÐ¾ÑÐ½Ð¾Ð³Ð¾ ÐºÑÐµÐ´Ð¸ÑÐ° Ð¿Ð¾Ð´ Ð¾Ð±Ð¾ÑÐ¾ÑÐ½ÑÐµ, ÐºÑÐ°ÑÐºÐ¾ÑÑÐ¾ÑÐ½Ð¾Ð³Ð¾ Ð¸ Ð´Ð¾Ð»Ð³Ð¾ÑÑÐ¾ÑÐ½Ð¾Ð³Ð¾ ÐºÑÐµÐ´Ð¸ÑÐ¾Ð² Ð¿Ð¾Ð´ Ð²Ð½ÐµÐ¾Ð±Ð¾ÑÐ¾ÑÐ½ÑÐµ Ð¸ Ð¾Ð±Ð¾ÑÐ¾ÑÐ½ÑÐµ Ð°ÐºÑÐ¸Ð²Ñ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ Ð¸ Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ñ ÐµÐ³Ð¾ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ð¹ ÑÑÑÐ¾Ð¹ÑÐ¸Ð²Ð¾ÑÑÐ¸. ÐÑÐ¾Ð°Ð½Ð°Ð»Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ñ Ð¾ÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÐ¸ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ ÐÐ§Ð Ð² ÑÐ¾ÑÑÐ¸Ð¹ÑÐºÐ¸Ñ ÑÑÐ»Ð¾Ð²Ð¸ÑÑ. ÐÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ñ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÑ Ð°Ð¿ÑÐ¾Ð±Ð°ÑÐ¸Ð¸ Ð¼ÐµÑÐ°Ð½Ð¸Ð·Ð¼Ð¾Ð² ÑÐ¾Ð³Ð»Ð°ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¸Ñ Ð¸Ð½ÑÐµÑÐµÑÐ¾Ð² Ð¿ÑÐ±Ð»Ð¸ÑÐ½Ð¾Ð³Ð¾ Ð¸ ÑÐ°ÑÑÐ½ÑÑ Ð¿Ð°ÑÑÐ½ÐµÑÐ¾Ð² â ÐºÐ¾ÑÐ¿Ð¾ÑÐ°ÑÐ¸Ð²Ð½ÑÑ Ð¿ÑÐ¾Ð¼ÑÑÐ»ÐµÐ½Ð½ÑÑ ÑÐ¸ÑÐ¼. Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ð° Ð¼Ð¾Ð´ÐµÐ»Ñ Ð¾Ð¿ÑÐ¸Ð¼Ð°Ð»ÑÐ½Ð¾Ð³Ð¾ ÑÐ°ÑÐ¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð¸Ñ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²ÑÑ ÑÐµÑÑÑÑÐ¾Ð² Ð¼ÐµÐ¶Ð´Ñ ÑÑÐ°ÑÑÐ½Ð¸ÐºÐ°Ð¼Ð¸ ÐÐ§Ð-Ð¿ÑÐ¾ÐµÐºÑÐ¾Ð². ÐÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð° Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð², Ð°ÑÐ¿Ð¸ÑÐ°Ð½ÑÐ¾Ð², Ð¿ÑÐµÐ¿Ð¾Ð´Ð°Ð²Ð°ÑÐµÐ»ÐµÐ¹ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¸Ñ ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾ÑÑÐµÐ¹ Ð²ÑÐ·Ð¾Ð², ÑÑÐºÐ¾Ð²Ð¾Ð´ÑÑÐ¸Ñ ÑÐ°Ð±Ð¾ÑÐ½Ð¸ÐºÐ¾Ð² ÑÐ¸ÑÐ¼, ÑÐ¸ÑÐ¾ÐºÐ¾Ð³Ð¾ ÐºÑÑÐ³Ð° ÑÐ¸ÑÐ°ÑÐµÐ»ÐµÐ¹, Ð¸Ð½ÑÐµÑÐµÑÑÑÑÐ¸ÑÑÑ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ð°Ð¼Ð¸ Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ñ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ Ð´Ð¸Ð²ÐµÑÑÐ¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¸ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð¿ÑÐ¾Ð¼ÑÑÐ»ÐµÐ½Ð½ÑÑ ÑÐ¸ÑÐ¼.
Hierarchical star formation in the Milky Way disk
Creators: name: Marcos, R. de la Fuente
name: Marcos, C. de la Fuente
Publisher: name: arXiv
Year: 2009
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Hierarchical star formation leads to a progressive decrease in the clustering of star clusters both in terms of spatial scale and age. Consistently, the statistical analysis of positions and ages of clusters in the Milky Way disk strongly suggests that a correlation between the duration of star formation in a region and its size does exist. The average age difference between pairs of open clusters increases with their separation as the ~0.16 power. In contrast and for the Large Magellanic Cloud, Efremov & Elmegreen (1998) found that the age difference scales with the ~0.35 power of the region size. This discrepancy may be tentatively interpreted as an argument in support of intrinsically shorter (faster) star formation time-scales in smaller galaxies. However, if both the effects of cluster dissolution and incompleteness are taken into consideration, the average age difference between cluster pairs in the Galaxy increases with their separation as the ~0.4 power. This result implies that the characteristic time-scale for coherent, clustered-mode star formation is nearly 1 Myr. Therefore, the overall consequence of ignoring the effect of cluster dissolution is to overestimate the star formation time-scale. On the other hand, in the Galactic disk and for young clusters separated by less than three times the characteristic cluster tidal radius (10 pc), the average age difference is 16 Myr, which suggests common origin. (Abridged)
description: 26 pages, 7 figures, 1 table. Accepted for publication in ApJ
title: ÐÐ¸Ð¾Ñ Ð¸Ð¼Ð¸ÑÐµÑÐºÐ¸Ð¹ Ð°Ð½Ð°Ð»Ð¸Ð· ÐºÑÐ¾Ð²Ð¸ ÑÑÐ´Ð° Ð¿Ð¾ÑÐ¾Ð´ ÑÐ²Ð¸Ð½ÐµÐ¹ Ð¸ Ð¸Ñ Ð³Ð¸Ð±ÑÐ¸Ð´Ð¾Ð²
title: Ð¼Ð¾Ð½Ð¾Ð³ÑÐ°ÑÐ¸Ñ
titleType: Subtitle
Creators: name: ÐÐ°Ð¹ÑÐµÐ², Ð¡ÐµÑÐ³ÐµÐ¹
name: ÐÐ¾Ð³Ð¾Ð»ÑÐ±Ð¾Ð²Ð°, ÐÐ°Ð´ÐµÐ¶Ð´Ð°
name: ÐÐ¾Ð»ÑÐ½Ð¾Ð²Ð°, ÐÐ°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: 2022
Subjects: Ð²ÐµÑÐµÑÐ¸Ð½Ð°ÑÐ¸Ñ
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The Nuclear response in the isoscalar channel
Creators: name: R. Cenni
name: F. Conte
name: P. Saracco
Publisher: name: INFN Open Access Repository
Year: 1996

description: The nuclear response is evaluated in the frame of the bosonic loop expansion
in a purely nucleonic dynamical scheme, which seems to be reliable in handling
those channels where a direct excitation of a $\Delta$-resonance is not
allowed. It is shown that the response strongly depends upon the effective
interaction in the spin-transverse isovector channel. New experiments at CEBAF
on parity-violating electron scattering could further constrain the form of the
effective interaction.
Compton reflection in AGN with Simbol-X
Creators: name: Beckmann, V.
name: Courvoisier, T. J. -L.
name: Gehrels, N.
name: Lubinski, P.
name: Malzac, J.
name: Petrucci, P. O.
name: Shrader, C. R.
name: Soldi, S.
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: AGN exhibit complex hard X-ray spectra. Our current understanding is that the emission is dominated by inverse Compton processes which take place in the corona above the accretion disk, and that absorption and reflection in a distant absorber play a major role. These processes can be directly observed through the shape of the continuum, the Compton reflection hump around 30 keV, and the iron fluorescence line at 6.4 keV. We demonstrate the capabilities of Simbol-X to constrain complex models for cases like MCG-05-23-016, NGC 4151, NGC 2110, and NGC 4051 in short (10 ksec) observations. We compare the simulations with recent observations on these sources by INTEGRAL, Swift and Suzaku. Constraining reflection models for AGN with Simbol-X will help us to get a clear view of the processes and geometry near to the central engine in AGN, and will give insight to which sources are responsible for the Cosmic X-ray background at energies above 20 keV.
description: 4 pages, 1 figure, to appear in the proceedings of the second Simbol-X Symposium "Simbol-X - Focusing on the Hard X-ray Universe", AIP Conf. Proc. Series, P. Ferrando and J. Rodriguez eds
SKA: 5 milioni di euro dall’Unione Europea
Creators: Eleonora Ferroni
Publisher: name: Media Inaf
Year: 2016

Questi fondi verranno re-investiti nel programma INfrastructure SKA (IN-SKA), che coinvolge il quartiere generale di SKA nel Regno Unito, le infrastrutture australiane e quelle sudafricane. Si va verso la fase di progettazione di dettaglio