cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
title: ÐÑÐµÐ½ÐºÐ° Ð´Ð¾Ð· Ð¾Ð±Ð»ÑÑÐµÐ½Ð¸Ñ Ð½Ð°ÑÐµÐ»ÐµÐ½Ð¸Ñ Ð½Ð° ÑÐµÑÑÐ¸ÑÐ¾ÑÐ¸ÑÑ , Ð·Ð°Ð³ÑÑÐ·Ð½ÐµÐ½Ð½ÑÑ ÑÐ°Ð´Ð¸Ð¾Ð°ÐºÑÐ¸Ð²Ð½ÑÐ¼Ð¸ Ð¸Ð·Ð¾ÑÐ¾Ð¿Ð°Ð¼Ð¸
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ¾Ð»ÑÑÐ¸Ð½Ð°, ÐÐ¸ÐºÑÐ¾Ñ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: ÑÐ°Ð´Ð¸Ð°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ Ð±ÐµÐ·Ð¾Ð¿Ð°ÑÐ½Ð¾ÑÑÑ
ÑÐ°Ð´Ð¸Ð°ÑÐ¸Ð¾Ð½Ð½ÑÐ¹ ÑÐ¾Ð½
Ð½Ð°ÐºÐ¾Ð¿Ð»ÐµÐ½Ð½Ð°Ñ Ð´Ð¾Ð·Ð°
Ð¼Ð¾ÑÐ½Ð¾ÑÑÑ Ð´Ð¾Ð·Ñ

description: ÐÐ¾ Ð²ÑÐ¾ÑÐ¾Ð¹ Ð³Ð»Ð°Ð²Ðµ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð¸Ñ Ð¸ Ð¼ÐµÑÐ¾Ð´Ð¸ÐºÐ¸, Ð¾ÑÐµÐ½ÐºÐ¸ Ð´Ð¾Ð· Ð¾Ð±Ð»ÑÑÐµÐ½Ð¸Ñ Ð¿Ð¾ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐ°Ð¼ ÑÐµÐ°Ð»ÑÐ½ÑÑ Ð¸Ð·Ð¼ÐµÑÐµÐ½Ð¸Ð¹. Ð ÑÑÐµÑÑÐµÐ¹ Ð³Ð»Ð°Ð²Ðµ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¾ Ð¾Ð±Ð¾Ð±ÑÐµÐ½Ð¸Ðµ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐ¾Ð² Ð¸Ð·Ð¼ÐµÑÐµÐ½Ð¸Ð¹ Ð¸ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ñ ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð°ÑÐ¸Ð¹ Ð¿Ð¾ Ð·Ð°ÑÐ¸ÑÐµ Ð¾Ñ ÑÐ°Ð´Ð¸Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ Ð¾Ð¿Ð°ÑÐ½Ð¾ÑÑÐ¸ ÑÐ¾ÑÑÑÐ´Ð½Ð¸ÐºÐ¾Ð² ÐÐÐ Â«ÐÐÐÐ¥ÐÂ» Ð¸ Ð½Ð°ÑÐµÐ»ÐµÐ½Ð¸Ñ Ð³Ð¾ÑÐ¾Ð´Ð° ÐÑÐ°ÑÐ½Ð¾ÐºÐ°Ð¼ÐµÐ½ÑÐºÐ°. ÐÐ°ÐºÐ»ÑÑÐµÐ½Ð¸Ðµ ÑÐ¾Ð´ÐµÑÐ¶Ð¸Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ Ð²ÑÐ²Ð¾Ð´Ñ Ð¿Ð¾ ÑÐ°Ð±Ð¾ÑÐµ.
Nel labirinto della notte marziana
Creators: Marco Malaspina
Publisher: name: Media Inaf
Year: 2016

Il fondo d’antichi bacini di Marte potrebbe rappresentare un buon obiettivo per la ricerca di ambienti abitabili nel passato del pianeta. Un ambiente geologico simile – suggerisce Alexis Palmero Rodriguez su “Planetary and Space Science” – lo si può incontrare nei laghi del Tibet. Con un commento di Silvia Vernetto dell’INAF di Torino
Charge dynamics of the spin-density-wave state in BaFe$_2$As$_2$
Creators: name: Pfuner, F.
name: Analytis, J. G.
name: Chu, J. -H.
name: Fisher, I. R.
name: Degiorgi, L.
Publisher: name: arXiv
Year: 2008
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: We report on a thorough optical investigation of BaFe$_2$As$_2$ over a broad spectral range and as a function of temperature, focusing our attention on its spin-density-wave (SDW) phase transition at $T_{SDW}=135$ K. While BaFe$_2$As$_2$ remains metallic at all temperatures, we observe a depletion in the far infrared energy interval of the optical conductivity below $T_{SDW}$, ascribed to the formation of a pseudogap-like feature in the excitation spectrum. This is accompanied by the narrowing of the Drude term consistent with the $dc$ transport results and suggestive of suppression of scattering channels in the SDW state. About 20% of the spectral weight in the far infrared energy interval is affected by the SDW phase transition.
Pagine di Sole in biblioteca
Creators: Antonella Gasperini
Publisher: name: Media Inaf
Year: 2016

Sabato 13 febbraio, presso la Biblioteca delle Oblate, a Firenze, l’attrice Luisa Cattaneo leggerà fiabe e racconti dal libro per ragazze e ragazzi delle scuole elementari “Come catturare il Sole”. Seguirà un laboratorio scientifico con le autrici del libro
The 8 Micron Phase Variation of the Hot Saturn HD 149026b
Creators: name: Knutson, Heather A.
name: Charbonneau, David
name: Cowan, Nicolas B.
name: Fortney, Jonathan J.
name: Showman, Adam P.
name: Agol, Eric
name: Henry, Gregory W.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: We monitor the star HD 149026 and its Saturn-mass planet at 8.0 micron over slightly more than half an orbit using the Infrared Array Camera (IRAC) on the Spitzer Space Telescope. We find an increase of 0.0227% +/- 0.0066% (3.4 sigma significance) in the combined planet-star flux during this interval. The minimum flux from the planet is 45% +/- 19% of the maximum planet flux, corresponding to a difference in brightness temperature of 480 +/- 140 K between the two hemispheres. We derive a new secondary eclipse depth of 0.0411% +/- 0.0076% in this band, corresponding to a dayside brightness temperature of 1440 +/- 150 K. Our new secondary eclipse depth is half that of a previous measurement (3.0 sigma difference) in this same bandpass by Harrington et al. (2007). We re-fit the Harrington et al. (2007) data and obtain a comparably good fit with a smaller eclipse depth that is consistent with our new value. In contrast to earlier claims, our new eclipse depth suggests that this planet's dayside emission spectrum is relatively cool, with an 8 micron brightness temperature that is less than the maximum planet-wide equilibrium temperature. We measure the interval between the transit and secondary eclipse and find that that the secondary eclipse occurs 20.9 +7.2 / -6.5 minutes earlier (2.9 sigma) than predicted for a circular orbit, a marginally significant result. This corresponds to e*cos(omega) = -0.0079 +0.0027 / -0.0025 where e is the planet's orbital eccentricity and omega is the argument of pericenter.
description: 17 pages, 12 figure, accepted for publication in ApJ
ความพึงพอใจต่อคุณภาพการบริการของสำนักงานธนานุเคราะห์
Creators: name: ริญญาภัทร์ เขจรนันทน์
Publisher: name: Program in Political Science, Faculty of Humanities and Social Sciences, Surindra Rajabhat University
Year: 2022
Subjects: สำนักงานธนานุเคราะห์
โรงรับจำนำ
ความพึงพอใจ
การให้บริการ

description: วารสารการบริหารการปกครองและนวัตกรรมท้องถิ่น, 6, 1, 93-108
title: ÐÑÐ¾Ð±Ð»ÐµÐ¼Ñ Ð¼ÐµÐ¶ÐºÑÐ»ÑÑÑÑÐ½Ð¾Ð¹ ÐºÐ¾Ð¼Ð¼ÑÐ½Ð¸ÐºÐ°ÑÐ¸Ð¸: ÑÐ¿ÐµÑÐ¸ÑÐ¸ÐºÐ° ÑÐ¼Ð¾ÑÐ° Ð² Ð´ÐµÐ»Ð¾Ð²Ð¾Ð¼ Ð¾Ð±ÑÐµÐ½Ð¸Ð¸ ÑÐ°Ð·Ð½ÑÑ ÐºÑÐ»ÑÑÑÑ
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ¸Ð²Ð°ÐµÐ²Ð°, Ð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: ÑÐ¼Ð¾Ñ
Ð´ÐµÐ»Ð¾Ð²Ð¾Ðµ Ð¾Ð±ÑÐµÐ½Ð¸Ðµ
Ð¼ÐµÐ¶ÐºÑÐ»ÑÑÑÑÐ½Ð°Ñ ÐºÐ¾Ð¼Ð¼ÑÐ½Ð¸ÐºÐ°ÑÐ¸Ñ

description: ÐÐ±ÑÐµÐºÑ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ - Ð´ÐµÐ»Ð¾Ð²Ð¾Ðµ Ð¾Ð±ÑÐµÐ½Ð¸Ðµ ÑÐ°Ð·Ð»Ð¸ÑÐ½ÑÑ ÐºÑÐ»ÑÑÑÑ. ÐÑÐµÐ´Ð¼ÐµÑ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ - ÑÐ¼Ð¾Ñ Ð² Ð´ÐµÐ»Ð¾Ð²Ð¾Ð¼ Ð¾Ð±ÑÐµÐ½Ð¸Ð¸ ÑÐ°Ð·Ð»Ð¸ÑÐ½ÑÑ ÐºÑÐ»ÑÑÑÑ. Ð¦ÐµÐ»Ñ ÑÐ°Ð±Ð¾ÑÑ: Ð¸Ð·ÑÑÐµÐ½Ð¸Ðµ Ð¸ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÐ¾Ð»Ð¸ Ð¸ Ð¾ÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÐµÐ¹ ÑÐ¼Ð¾ÑÐ° Ð² ÑÐ°Ð¼ÐºÐ°Ñ Ð´ÐµÐ»Ð¾Ð²Ð¾Ð³Ð¾ Ð¾Ð±ÑÐµÐ½Ð¸Ñ Ð² ÑÑÑÑÐºÐ¾Ð¹, Ð°Ð½Ð³Ð»Ð¸Ð¹ÑÐºÐ¾Ð¹ Ð¸ Ð°Ð¼ÐµÑÐ¸ÐºÐ°Ð½ÑÐºÐ¾Ð¹ ÐºÑÐ»ÑÑÑÑÐ°Ñ. ÐÐ¾ Ð²Ð²ÐµÐ´ÐµÐ½Ð¸Ð¸ Ð¾Ð¿Ð¸ÑÑÐ²Ð°ÐµÑÑÑ Ð°ÐºÑÑÐ°Ð»ÑÐ½Ð¾ÑÑÑ ÑÐµÐ¼Ñ, Ð¿ÑÐµÐ´Ð¼ÐµÑ, Ð¾Ð±ÑÐµÐºÑ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ, ÑÐµÐ»Ñ, Ð·Ð°Ð´Ð°ÑÐ¸, Ð¼ÐµÑÐ¾Ð´Ñ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ. Ð¢ÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¿ÑÐ¾Ð²Ð¾Ð´Ð¸Ð»Ð¸ÑÑ Ð¼ÐµÑÐ¾Ð´Ð¾Ð¼ Ð°Ð½Ð°Ð»Ð¸Ð·Ð° Ð»Ð¸ÑÐµÑÐ°ÑÑÑÑ, Ð¸Ð·ÑÑÐµÐ½Ð¸Ñ Ð¸ Ð¾Ð±Ð¾Ð±ÑÐµÐ½Ð¸Ñ Ð¿Ð¾Ð»ÑÑÐµÐ½Ð½ÑÑ Ð´Ð°Ð½Ð½ÑÑ, ÐºÐ»Ð°ÑÑÐ¸ÑÐ¸ÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¿Ð¾Ð»ÑÑÐµÐ½Ð½Ð¾Ð¹ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¸. ÐÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¿ÑÐ¾Ð²Ð¾Ð´Ð¸Ð»Ð¸ÑÑ Ð¼ÐµÑÐ¾Ð´Ð¾Ð¼ ÑÑÐ°Ð²Ð½ÐµÐ½Ð¸Ñ.ÐÑÐ½Ð¾Ð²ÑÐ²Ð°ÑÑÑ Ð½Ð° ÑÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð¸ ÑÐ¼Ð¿Ð¸ÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð¼ÐµÑÐ¾Ð´Ñ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ, ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ Ð½Ð°ÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½ÑÐµ Ð¾ÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÐ¸ ÑÐ¼Ð¾ÑÐ° Ð¸ Ð¿ÑÐ¾Ð°Ð½Ð°Ð»Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ ÑÐ°ÐºÑÐ¾ÑÑ, Ð²Ð»Ð¸ÑÑÑÐ¸Ðµ Ð½Ð° ÑÐ°ÑÐ°ÐºÑÐµÑ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ¼Ð¾ÑÐ° Ð² Ð´ÐµÐ»Ð¾Ð²Ð¾Ð¼ Ð¾Ð±ÑÐµÐ½Ð¸Ð¸ Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð¸ÑÐµÐ»ÐµÐ¹ Ð°Ð½Ð³Ð»Ð¸Ð¹ÑÐºÐ¾Ð¹, Ð°Ð¼ÐµÑÐ¸ÐºÐ°Ð½ÑÐºÐ¾Ð¹ Ð¸ ÑÑÑÑÐºÐ¾Ð¹ ÐºÑÐ»ÑÑÑÑ. Ð ÐµÐ·ÑÐ»ÑÑÐ°ÑÑ Ð¼Ð¾Ð³ÑÑ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°ÑÑÑÑ ÐºÐ°Ðº ÑÑÐºÐ¾Ð²Ð¾Ð´ÑÑÐ²Ð¾ Ð¿Ð¾ ÑÑÐ¿ÐµÑÐ½Ð¾Ð¼Ñ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ¼Ð¾ÑÐ° Ð² Ð¿ÑÐ±Ð»Ð¸ÑÐ½ÑÑ Ð²ÑÑÑÑÐ¿Ð»ÐµÐ½Ð¸ÑÑ Ð¸ Ð² ÑÑÐµÐ±Ð½Ð¾Ð¼ Ð¿ÑÐ¾ÑÐµÑÑÐµ Ð´Ð»Ñ Ð¸Ð·ÑÑÐµÐ½Ð¸Ñ Ð½Ð°ÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½Ð¾ ÐºÐ¾Ð¼Ð¼ÑÐ½Ð¸ÐºÐ°ÑÐ¸Ð²Ð½ÑÑ Ð¾ÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÐµÐ¹ Ð¿Ð¾Ð²ÐµÐ´ÐµÐ½Ð¸Ñ Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð¸ÑÐµÐ»ÐµÐ¹ ÑÑÑÑÐºÐ¾Ð¹, Ð°Ð¼ÐµÑÐ¸ÐºÐ°Ð½ÑÐºÐ¾Ð¹ Ð¸ Ð°Ð½Ð³Ð»Ð¸Ð¹ÑÐºÐ¾Ð¹ ÐºÑÐ»ÑÑÑÑ Ð² Ð´ÐµÐ»Ð¾Ð²Ð¾Ð¼ Ð¾Ð±ÑÐµÐ½Ð¸Ð¸.
HD 97300, la stella sotto i riflettori
Creators: Redazione Media Inaf
Publisher: name: Media Inaf
Year: 2016

IC 2631 è illuminata dalla stella HD 97300, una delle più giovani - e anche delle più luminose e massicce - stelle della zona. La regione è piena di materiale per la costruzione di stelle. Le nebulose oscure sono così dense di gas e polvere che impediscono il passaggio della luce delle stelle di fondo
Continuous Matrix Product States for Quantum Fields
Creators: name: Verstraete, F.
name: Cirac, J. I.
Publisher: name: arXiv
Year: 2010
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: High Energy Physics - Lattice (hep-lat)
subject: High Energy Physics - Theory (hep-th)
subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We define matrix product states in the continuum limit, without any reference to an underlying lattice parameter. This allows to extend the density matrix renormalization group and variational matrix product state formalism to quantum field theories and continuum models in 1 spatial dimension. We illustrate our procedure with the Lieb-Liniger model.
Detecting relic gravitational waves in the CMB: Comparison of different methods
Creators: name: Zhao, W.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: In this paper, we discuss the constraint on the relic gravitational waves by both temperature and polarization anisotropies power spectra of cosmic microwave background radiation. Taking into account the instrumental noises of Planck satellite, we calculate the signal-to-noise ratio $S/N$ by the simulation and the analytic approximation methods. We find that, comparing with the $BB$ channel, the value of $S/N$ is much improved in the case where all the power spectra, $TT$, $TE$, $EE$ and $BB$, are considered. If the noise power spectra of Planck satellite increase for some reasons, the value of $S/N$ in $BB$ channel is much reduced. However, in the latter case where all the power spectra of cosmic microwave background radiation are considered, the value of $S/N$ is less influenced. We also find that the free parameters $A_s$, $n_s$ and $n_t$ have little influence on the value of $S/N$ in both cases.
description: 37 pages, 7 figures, published version
title: Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° ÑÑÑÐ°ÑÐµÐ³Ð¸Ð¸ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ Ð¸ ÐµÐµ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ðµ Ð¾Ð±Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð¸Ðµ (Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ ÐÐÐ Â«Ð Ð¾ÑÑÐµÐ»ÐµÐºÐ¾Ð¼Â»)
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°Ð½ÐºÐ¾Ð²Ð°, ÐÐ°Ð»ÐµÑ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Ð¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾-Ñ Ð¾Ð·ÑÐ¹ÑÑÐ²ÐµÐ½Ð½Ð°Ñ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÑ
ÑÐµÐ»ÐµÐºÐ¾Ð¼Ð¼ÑÐ½Ð¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½ÑÐ¹ ÑÑÐ½Ð¾Ðº
ÐºÐ¾Ð½ÐºÑÑÐµÐ½ÑÑ
Ð¸Ð½Ð²ÐµÑÑÐ¸ÑÐ¸Ð¾Ð½Ð½ÑÐµ Ð·Ð°ÑÑÐ°ÑÑ

description: Ð¦ÐµÐ»ÑÑ Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ ÑÐ²Ð»ÑÐµÑÑÑ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° ÑÑÑÐ°ÑÐµÐ³Ð¸Ð¸ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ ÐÐÐ Â«Ð Ð¾ÑÑÐµÐ»ÐµÐºÐ¾Ð¼Â» Ð¸ ÐµÐµ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ðµ Ð¾Ð±Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð¸Ðµ. ÐÑÐ» Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½ ÑÑÐ½Ð¾Ðº ÑÐµÐ»ÐµÐºÐ¾Ð¼Ð¼ÑÐ½Ð¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½ÑÑ ÑÑÐ»ÑÐ³, Ð¿ÑÐ¾Ð°Ð½Ð°Ð»Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ð° ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾-ÑÐ¾Ð·ÑÐ¹ÑÑÐ²ÐµÐ½Ð½Ð°Ñ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÑ ÐÐÐ Â«Ð Ð¾ÑÑÐµÐ»ÐµÐºÐ¾Ð¼Â», Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· ÐºÐ¾Ð½ÐºÑÑÐµÐ½ÑÐ¾Ð², Ð²ÑÑÐ²Ð»ÐµÐ½Ñ ÑÑÑÐµÑÑÐ²ÑÑÑÐ¸Ðµ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²ÑÐµ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ñ, ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½ Ð¿ÑÐ¾ÐµÐºÑ Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ñ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸, Ð¾ÑÐµÐ½ÐµÐ½Ð° ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÑ Ð¿ÑÐµÐ´Ð»Ð°Ð³Ð°ÐµÐ¼Ð¾Ð³Ð¾ Ð¿ÑÐ¾ÐµÐºÑÐ°.
title: Ð¡Ð»ÐµÐ´ÑÑÐ¸Ð¹ ÑÐ»ÐµÐºÑÑÐ¾Ð¿ÑÐ¸Ð²Ð¾Ð´ Ñ ÑÐ¸ÑÐ¾ÑÐ½Ð¾-Ð¸Ð¼Ð¿ÑÐ»ÑÑÐ½ÑÐ¼ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸ÐµÐ¼
title: Ð´Ð¸Ð¿Ð»Ð¾Ð¼Ð½ÑÐ¹ Ð¿ÑÐ¾ÐµÐºÑ
titleType: Subtitle
Creators: name: ÐÐ·ÐµÑÐ¾Ð², ÐÐ²Ð³ÐµÐ½Ð¸Ð¹
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2016
Subjects: ÑÐ»ÐµÐ´ÑÑÐ¸Ð¹ ÑÐ»ÐµÐºÑÑÐ¾Ð¿ÑÐ¸Ð²Ð¾Ð´
ÑÐ¸ÑÐ¾ÑÐ½Ð¾-Ð¸Ð¼Ð¿ÑÐ»ÑÑÐ½Ð¾Ðµ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ
ÑÐ¸Ð½ÑÐµÐ·
Ð¼Ð¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ

description: Ð Ð°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÐµÑÑÑ ÑÐ»ÐµÐ´ÑÑÐ¸Ð¹ ÑÐ»ÐµÐºÑÑÐ¾Ð¿ÑÐ¸Ð²Ð¾Ð´ Ñ ÑÐ¸ÑÐ¾ÑÐ½Ð¾-Ð¸Ð¼Ð¿ÑÐ»ÑÑÐ½ÑÐ¼ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸ÐµÐ¼. Ð Ð°Ð·ÑÐ°Ð±Ð°ÑÑÐ²Ð°ÐµÑÑÑ ÑÐ°ÑÑÐ¾ÑÐ½ÑÐ¹ Ð°Ð»Ð³Ð¾ÑÐ¸ÑÐ¼ ÑÐ¸Ð½ÑÐµÐ·Ð° Ð¸Ð¼Ð¿ÑÐ»ÑÑÐ½ÑÑ ÑÐ¸ÑÑÐµÐ¼ Ñ ÑÐ¸ÑÐ¾ÑÐ½Ð¾-Ð¸Ð¼Ð¿ÑÐ»ÑÑÐ½ÑÐ¼ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸ÐµÐ¼ Ð² Ð½ÐµÐ¿ÑÐµÑÑÐ²Ð½Ð¾Ð¼ Ð²ÑÐµÐ¼ÐµÐ½Ð¸ Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ðµ ÑÐ°ÑÑÐ¾ÑÐ½Ð¾Ð³Ð¾ Ð¿Ð¾Ð´ÑÐ¾Ð´Ð° Ðº ÑÐµÑÐµÐ½Ð¸Ñ Ð¾Ð±ÑÐ°ÑÐ½ÑÑ Ð·Ð°Ð´Ð°Ñ Ð´Ð¸Ð½Ð°Ð¼Ð¸ÐºÐ¸ Ð¿ÑÑÐµÐ¼ Ð¸ÑÐºÑÑÑÑÐ²ÐµÐ½Ð½Ð¾Ð¹ Ð¿ÐµÑÐ¸Ð¾Ð´Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð·Ð°Ð´Ð°Ð½Ð½ÑÑ Ð¿ÐµÑÐµÑÐ¾Ð´Ð½ÑÑ ÑÐ°ÑÐ°ÐºÑÐµÑÐ¸ÑÑÐ¸Ðº. ÐÑÐ¸Ð²Ð¾Ð´ÑÑÑÑ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÑ ÑÐ¸Ð½ÑÐµÐ·Ð° Ð¸ Ð¼Ð¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ.
Centinaia di galassie nascoste dietro la Via Lattea
Creators: Stefano Parisini
Publisher: name: Media Inaf
Year: 2016

Pubblicato il primo elenco completo della popolazione di galassie nascoste nell’ampia zona di cielo mascherata dalla polvere della nostra stessa galassia, una spessa coltre che le onde radio possono però attraversare. I risultati di questo campionamento aiuteranno a svelare il mistero sull'anomalia gravitazionale del Grande Attrattore. Con il commento di Steven Tingay (INAF)
Crematogaster captiosa Forel
Creators: name: Feldhaar, Heike
name: Maschwitz, Ulrich
name: Fiala, Brigitte
Publisher: name: Zenodo
Year: 2016
Subjects: Biodiversity
Taxonomy

description: Crematogaster captiosa Forel is a very widespread species occurring over the whole distributional range of the Crematogaster-Macaranga association (Peninsula Malaysia, Sumatra, and Borneo). The species has a wide host-range but is usually restricted to non-waxy hosts of the section Pachystemon (M. angulata, M. bancana, M. calcicola, M.
description: Published as part of Heike Feldhaar, Ulrich Maschwitz & Brigitte Fiala, 2016, Taxonomic Revision of the Obligate Plant-Ants of the Genus Crematogaster Lund (Hymenoptera: Formicidae: Myrmicinae), Associated with Macaranga Thouars (Euphorbiaceae) on Borneo and the Malay Peninsula, pp. 651-681 in Sociobiology 63 (1) on page 669, DOI: 10.13102/sociobiology.v63i1.949, http://zenodo.org/record/269814
Macaranga glandibracteolata
Creators: name: Feldhaar, Heike
name: Maschwitz, Ulrich
name: Fiala, Brigitte
Publisher: name: Zenodo
Year: 2016
Subjects: Biodiversity
Taxonomy

description: glandibracteolata, M. hullettii, M. indistincta, M. petanostyla, M. trachyphylla, M. umbrosa, the non-waxy form of M. aetheadenia, and the thinly wax-covered M. glandibracteolata as an exception of a glaucous host species). Queens colonize seedlings as well as the tips of mature hosts that have been abandoned due to the loss of the original colony. On Peninsula Malaysia secondarily polygynous colonies that contained several queens have been found locally in the Gombak area. In former publications by our group this species was referred to as Crematogaster msp. 4 (Fiala et al., 1999; Feldhaar et al., 2003a; Feldhaar et al., 2003b).
description: Published as part of Heike Feldhaar, Ulrich Maschwitz & Brigitte Fiala, 2016, Taxonomic Revision of the Obligate Plant-Ants of the Genus Crematogaster Lund (Hymenoptera: Formicidae: Myrmicinae), Associated with Macaranga Thouars (Euphorbiaceae) on Borneo and the Malay Peninsula, pp. 651-681 in Sociobiology 63 (1) on page 670, DOI: 10.13102/sociobiology.v63i1.949, http://zenodo.org/record/269814
description: {"references": ["Fiala, B., Jakob, A., Maschwitz, U. & Linsenmair, K. E. (1999). Diversity, evolutionary specialization and geographic distribution of a mutualistic ant-plant complex: Macaranga and Crematogaster in South East Asia. Biological Journal of the Linnean Society, 66: 305 - 331. doi: 10.1111 / j. 1095 - 8312.1999. tb 01893. x", "Feldhaar, H., Fiala, B., Gadau, J., Mohamed, M. & Maschwitz, U. (2003 a). Molecular phylogeny of Crematogaster subgenus Decacrema ants (Hymenoptera: Formicidae) and the colonization of Macaranga (Euphorbiaceae) trees. Molecular Phylogenetics and Evolution, 27: 441 - 452. doi: 10.1016 / S 1055 - 7903 (02) 00449 - 9", "Feldhaar, H., Fiala, B., Hashim, R. B. & Maschwitz, U. (2003 b). Patterns of the Crematogaster-Macaranga association: The ant partner makes the difference. Insectes Sociaux, 50: 9 - 19. doi: 10.1007 / s 000400300002"]}
APPROACHES TO INCREASING CANCER ALERTNESS AMONG PRIMARY CARE PHYSICIANS
Creators: name: Masharipov Polvonnazar  Doctor of Medical science, docent of the Department Nephrology, Hemodialysis Traumatology and Orthopedics  of the Urgench branch of Tashkent Medical Academy
Publisher: name: Zenodo
Year: 2023

description: Oncological diseases remain one of the pressing problems of modern medicine. According to WHO, more than 12 million cancer patients are registered annually in the world and 7 million people die from this disease. Despite the emergence of new methods for diagnosing malignant neoplasms (malignant neoplasms) (MRI, PETCT, etc.), the proportion of advanced cases of malignant neoplasms remains high. This is mainly due to the secrecy of the course in the early stages, the lack of oncological alertness among general practitioners, as well as the low level of oncological literacy among the population. Family clinics and consultative and diagnostic centers are the primary link in the process of establishing a diagnosis and timely detection of early symptoms of malignant neoplasms. The fate of the patient depends on the qualifications of the doctors of this unit. It should be noted that more than 90% of patients with various oncological diseases turn to these institutions.

Key words: diseases, fibrosis, nodular, etiological, vascular system
Status and Physics Reach of LHCb
Creators: name: Calvi, Marta
Publisher: name: INFN Open Access Repository
Year: 2009

description: LHCb is the experiment at the Large Hadron Collider devoted to studies of new
phenomena in CP violation and in rare decays. This review summarizes the status
of the experiment in the imminence of the data taking, the prospects for the
first measurements and highlights of its full physics program.
Beschäftigung und Verflechtungsbeziehungen in der Metropolregion Bremen-Oldenburg
Creators: name: Rippe, Julia
name: Thole, Jochen
Publisher: name: Arbeitnehmerkammer Bremen
Year: 2008
Subjects: subject: Automobilindustrie
subject: Zulieferer
subject: Bremen
subject: 330

description: Bremens Wirtschaftskraft basiert nach wie vor auf ihren industriellen Kernen. Die Automobilindustrie – im Klartext: das Bremer Daimler Werk – spielt dabei seit vielen Jahren eine zentrale Rolle. Eines hat sich allerdings geändert: Die Wertschöpfung in der Automobilindustrie verlagert sich zunehmend in die Zulieferindustrie, also in diejenigen Betriebe, deren Produkte mehr oder weniger ausschließlich für die Automobil-Endproduktion geliefert werden. Wenn man sich also mit den Entwicklungsmöglichkeiten der in Bremen angesiedelten Automobilindustrie beschäftigt – und damit natürlich auch mit der Sicherheit der Arbeitsplätze in dieser Branche – dann muss man sich zunehmend und intensiv mit der Zulieferindustrie beschäftigen. Das geschieht in der vorliegende Studie, nicht zuletzt dadurch, dass sie erstmals eine relativ umfassende Datenbasis für die in Bremen und umzu angesiedelte Branche vorlegt. Ihr eigentliches Thema aber ist die (mögliche) Cluster-Bildung in diesem sehr komplexen und manchmal auch sehr kleinteiligen Sektor. Denn Cluster bieten die Möglichkeit von Kooperation und Vernetzung, zum Beispiel bei Programmen zur Qualifizierung der Beschäftigten, und stärken damit die Ressourcen für Innovation.
Blind spots between quantum states
Creators: name: Zambrano, Eduardo
name: de Almeida, Alfredo M Ozorio
Publisher: name: arXiv
Year: 2009
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: The overlap of a large quantum state with its image, under tiny translations, oscillates swiftly. We here show that complete orthogonality occurs generically at isolated points. Decoherence, in the Markovian approximation, lifts the correlation minima from zero much more quickly than the Wigner function is smoothed into a positive phase space distribution. In the case of a superposition of coherent states, blind spots depend strongly on positions and amplitudes of the components, but they are only weakly affected by relative phases and the various degrees and directions of squeezing. The blind spots for coherent state triplets are special in that they lie close to an hexagonal lattice: Further superpositions of translated triplets, specified by nodes of one of the sublattices, are quasi-orthogonal to the original triplet and to any state, likewise constructed on the other sublattice.
description: 4 figures
Contribution from Duality Violations to the theoretical error on alpha_s
Creators: name: O. Cata
name: M. Golterman
name: S. Peris
Publisher: name: INFN Open Access Repository
Year: 2009

description: Duality Violations (DVs) is a nickname for the failure of the Operator
Product Expansion to describe QCD correlators on the physical axis. Using a
physically motivated ansatz, a fit to the spectral functions allows us to get a
quantitative estimate for the amount of DVs present in tau data. The quality of
the fit turns out to be better than expected. Since DVs have not been included
in the past in the determination of alpha_s, they amount to an additional
theoretical error which we estimate could be \delta alpha_s(m_{tau}) \sim
0.003-0.010 . Our ansatz satisfies, in particular, the 1st Weinberg sum rule,
which shows that this sum rule is not enough to force DVs to vanish.
Pianeti rocciosi: così simili eppure così lontani
Creators: Eleonora Ferroni
Publisher: name: Media Inaf
Year: 2016

Oltre il Sistema solare ci sono moltissimi pianeti simili al nostro: una crosta sottile all'esterno, uno spesso mantello e poi un nucleo fuso all'interno. Tutto questo potrebbe duplicarsi negli esopianeti rocciosi in altri sistemi planetari
The effects of taking up employment after pension age on self-rated health in Germany and the UK : evidence based on fixed effects models
Creators: name: Lux, Thomas
name: Scherger, Simone
Publisher: name: Oxford University Press (OUP)
Year: 2018
Subjects: subject: Pensions
subject: Employment
subject: Health
subject: Germany
subject: UK
subject: 300

description: This article analyses the effects on self-rated health of taking up paid work again after pension age. With the United Kingdom and Germany, two different institutional contexts are studied. Using fixed effects models and based on data from the German Socio-Economic Panel (GSOEP) and the British Household Panel Survey (BHPS), we estimate the individual effects of taking up work again on self-rated health, and differentiate between taking up work in a low occupational class and in a middle or high occupational class. In Germany, taking up work again after pension age tends to have positive effects on self-rated health in both class categories. In the United Kingdom, no effect at all can be seen in the case of taking up work in a low class, whereas working in a middle or higher class leads to small improvements in self-rated health. We discuss these results with regard to their limitations and their generalizability.
The BESS model revisited as a Higgsless Linear Moose @ the LHC
Creators: name: Curtis, Stefania De
Publisher: name: PoS (2008LHC) 008
Year: 2010

description: We study the phenomenological consequences of a four site Higgsless model
based on the SU(2)_L x SU(2)_1 x SU(2)_2 x U(1)_Y gauge symmetry, which
predicts two neutral and four charged extra gauge bosons, Z_{1,2} and W_{1,2}.
The model represents an extension of the minimal three site version (or BESS
model), largely investigated in the literature, which includes three heavy
vector bosons. We compute the properties of the new particles, and derive
indirect and direct limits on their masses and couplings from LEP and Tevatron
data and from the perturbative unitarity requirements. In contrast to other
Higgsless models characterized by fermiophobic extra gauge bosons, here
sizeable fermion-boson couplings are allowed by the electroweak precision data.
The prospects of detecting the new predicted particles in the favoured
Drell-Yan channel at the LHC are thus investigated. The outcome is that all six
extra gauge bosons could be discovered in the early stage of the LHC
low-luminosity run.
Cultural transmission, educational attainment and social mobility
Creators: name: Scherger, Simone
name: Savage, Mike
Publisher: name: Sage
Year: 2010
Subjects: subject: Educational attainment
subject: Cultural socialisation
subject: Intergeneration
subject: Social mobility
subject: Cultural activities
subject: 300

description: This paper examines the relationship between cultural socialisation, educational attainment and intergenerational social mobility. Picking up on debates about the transmission of cultural capital and social advantage, we use data from the Taking Part Survey of England to analyse how far socialisation into cultural activities and encouragement play a role in educational attainment, intergenerational mobility and in the reproduction of class. This survey has unprecedented data on whether respondents had been taken to museums/art galleries, theatre/dance/classical music performances, sites of historic interest, and libraries when they were growing up. This is buttressed by information on how much parents or other adults encouraged the respondents to read books or to be creatively active in different domains of the arts, literature and music. Using these rich measures of childhood socialisation, we can show that part of the effect of parental class on educational attainment is due to the transmission of this kind of cultural capital. Moreover, this transmission also has a direct effect on the level of educational attainment. In a similar fashion, respondents who have experienced a higher intensity of cultural socialisation are more likely to be upwardly mobile, and likewise, cultural transmission has a positive effect on the prevention of downward mobility among service class children. These results are discussed in the light of current issues in British mobility research and its treatment of cultural aspects of class and mobility.
Doppio salto rotazionale senza rompersi
Creators: Stefano Parisini
Publisher: name: Media Inaf
Year: 2016

Al PTB, l’istituto tedesco di metrologia, sono riusciti per la prima volta a stabilire lo stato quantistico rotazionale di uno ione molecolare - non fluorescente - lasciando intatta la molecola campione. Lo studio, pubblicato su Nature, ha implicazioni anche per astrochimica e astrofisica
Space-Time Structure of Loop Quantum Black Hole
Creators: name: Modesto, Leonardo
Publisher: name: arXiv
Year: 2008
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: In this paper we have improved the semiclassical analysis of loop quantum black hole (LQBH) in the conservative approach of constant polymeric parameter. In particular we have focused our attention on the space-time structure. We have introduced a very simple modification of the spherically symmetric Hamiltonian constraint in its holonomic version. The new quantum constraint reduces to the classical constraint when the polymeric parameter goes to zero.Using this modification we have obtained a large class of semiclassical solutions parametrized by a generic function of the polymeric parameter. We have found that only a particular choice of this function reproduces the black hole solution with the correct asymptotic flat limit. In r=0 the semiclassical metric is regular and the Kretschmann invariant has a maximum peaked in L-Planck. The radial position of the pick does not depend on the black hole mass and the polymeric parameter. The semiclassical solution is very similar to the Reissner-Nordstrom metric. We have constructed the Carter-Penrose diagrams explicitly, giving a causal description of the space-time and its maximal extension. The LQBH metric interpolates between two asymptotically flat regions, the r to infinity region and the r to 0 region. We have studied the thermodynamics of the semiclassical solution. The temperature, entropy and the evaporation process are regular and could be defined independently from the polymeric parameter. We have studied the particular metric when the polymeric parameter goes towards to zero. This metric is regular in r=0 and has only one event horizon in r = 2m. The Kretschmann invariant maximum depends only on L-Planck. The polymeric parameter does not play any role in the black hole singularity resolution. The thermodynamics is the same.
description: 17 pages, 19 figures
ALICE first physics results
Creators: name: A. Dainese
name: For The ALICE Collaboration
Publisher: name: INFN Open Access Repository
Year: 2010

description: ALICE is the dedicated heavy-ion experiment at the Large Hadron Collider. The
experiment has also a broad program of QCD measurements in proton-proton (pp)
collisions, which have two-fold interest: the study of particle production at
the highest energy frontier, and the definition of references for the
corresponding measurements in the upcoming Pb-Pb run. We present the first
results on the pseudorapidity and transverse-momentum dependence of charged
particle production in pp collisions at LHC energies, on the anti-p/p ratio and
on the Bose-Einstein particle correlations. As an outlook, we report on the
status of the ongoing analyses for strangeness and heavy-flavour production
measurements.
Neutrino flavor dynamics in post-bounce supernovae: the role of the
  electron component
Creators: name: Baldo, Marcello
name: Palmisano, Vincenzo
Publisher: name: INFN Open Access Repository
Year: 2012

description: In this paper we study the dynamics of flavor transformation for neutrinos
propagating in the very dense environment of astrophysical compact objects as
Type II supernova in post collapse phase and proto-neutron stars. The analysis
is based on the generalized Boltzmann equation, which incorporates the
neutrinoneutrino interaction. We focus the analysis on the possible collective
flavor dynamics, which can displays bipolar and synchronized flavor
oscillations, and the associated transition from single-angle to multi-angle
regime. To solve the kinetic equations we use an expansion in Legendre
polynomials and a two-flavor scheme. On the basis of the numerical simulations
we argue that neutrino flavor dynamics is suppressed by the presence of the
electron component up to a certain distance from the neutrino sphere, where a
transition to multi-angle regime occurs. This distance will move towards the
neutrino sphere as the neutrino emission epoch proceeds.
The ANTARES Detector: Electronics and Readout
Creators: name: M. Circella
name: For The ANTARES Collaboration
Publisher: name: INFN Open Access Repository
Year: 2007

description: In this paper, we illustrate the main features of the electronics and data
acquisition systems of the ANTARES apparatus, a large volume, deep-sea neutrino
telescope under construction in the Mediterranean Sea off the coast of Toulon,
France. The apparatus consists of an array of 900 large-area photomultipliers
arranged on 12 detection lines, 5 of which are in data acquisition since
January 2007. The schedule is to complete the apparatus construction in early
2008.
Warped 5-Dimensional Models: Phenomenological Status and Experimental Prospects
Creators: name: Davoudiasl, Hooman
name: Gopalakrishna, Shrihari
name: Ponton, Eduardo
name: Santiago, Jose
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: Warped 5-dimensional models, based on the original Randall-Sundrum geometry, have been extended beyond their initial purpose of resolving the gauge hierarchy problem. Over the past decade, various ingredients have been added to their basic structure in order to provide natural and predictive models of flavor and also to address existing constraints from precision data. In this review, we examine the theoretical and experimental status of realistic models that accommodate current data, while addressing the hierarchy and flavor puzzles of the Standard Model. We also discuss the prospects for future discovery of the TeV-scale Kaluza-Klein states that are predicted to emerge in these models, and outline some of the challenges that the detection of such particles pose for experiments at the Large Hadron Collider.
description: References added. To appear in the focus issue on Extra Space Dimensions of the New Journal of Physics
Cannibalismo stellare colto sul fatto
Creators: Elisa Nichelli
Publisher: name: Media Inaf
Year: 2016

Grazie alle osservazioni effettuate presso il telescopio Subaru per un gruppo di quattro stelle giovani con intensa attività luminosa, un team di scienziati ha potuto confermare il modello di frammentazione del disco, che è in grado di spiegare l’accrescimento di materiale da parte delle stelle nelle prime fasi di vita
Crematogaster angulosa Andre
Creators: name: Feldhaar, Heike
name: Maschwitz, Ulrich
name: Fiala, Brigitte
Publisher: name: Zenodo
Year: 2016
Subjects: Biodiversity
Taxonomy

description: Crematogaster angulosa André Crematogaster angulosa (André, 1896) Type material examined Crematogaster angulosa André. Holotype, 1 worker, Borneo (E. André) (MNHN). Worker measurements (n=1) HL 0.81, HW 0.78, EL 0.17, SL 0.57, WL 0.97, MTW 0.46, LHT 0.66, DPW 0.22, DPPW 0.21, CI 0.96, SI 0.73, REL 0.21, PI 1.01, RLEG 0.68 LPS 0.17 (TL 3.0) Description of worker Colour uniformly medium brown. Head and gaster shiny and with smooth surface, propodeum slightly striated. All body parts bear appressed pubescent hairs. Long flexuous setae present on head, gaster and abdomen. Head subquadratic but slightly elongated, being longer than wide and only slightly convex on sides. Anterior clypeal margin slightly convex and with a row of long erect hairs projecting anteriorly. Antennae relatively long in comparison to head width (SI 0.73) and covered in short pubescent hair. Terminal three funicular segments form a distinct club. Compound eyes elliptically shaped and not protruding over margin of head in full face view. Metanotal groove distinctly visible and more pronounced than in the Macaranga -associated Decacrema species.Propodeal spines long, acute and thin (see Fig. S2.1A and S2.1B). In dorsal view petiole and postpetiole round in shape, with petiole being slightly more elongate than postpetiole. Petiole slightly wider than the postpetiole. Femur distinctly thicker than other parts of legs. In dorsal view petiole and postpetiole round in shape. In lateral view the anterior face of the petiolar node flattened and sloping downwards anteriorly and petiole longer than postpetiole. Dorsal surface of the postpetiolar node in profile rounded, lateral nodes visible. Anteroventral tooth of petiole present.
description: Published as part of Heike Feldhaar, Ulrich Maschwitz & Brigitte Fiala, 2016, Taxonomic Revision of the Obligate Plant-Ants of the Genus Crematogaster Lund (Hymenoptera: Formicidae: Myrmicinae), Associated with Macaranga Thouars (Euphorbiaceae) on Borneo and the Malay Peninsula, pp. 651-681 in Sociobiology 63 (1) on page 681, DOI: 10.13102/sociobiology.v63i1.949, http://zenodo.org/record/269814
Il supervento di NGC 6240
Creators: Corrado Ruscica
Publisher: name: Media Inaf
Year: 2016

Una serie d'osservazioni realizzate con la Suprime-Cam installata presso il telescopio Subaru ha permesso di studiare, per la prima volta, la struttura complessa di uno dei principali venti galattici noti. I risultati, riportati su ApJ, suggeriscono che NGC 6240 abbia subito nel passato una violenta attività di formazione stellare per almeno tre volte, durante le quali ogni starburst ha dato luogo a un intenso supervento
Relativistic description of BCS-BEC crossover in nuclear matter
Creators: name: Sun, Bao Yuan
name: Toki, Hiroshi
name: Meng, Jie
Publisher: name: arXiv
Year: 2009
Subjects: subject: Nuclear Theory (nucl-th)
subject: Superconductivity (cond-mat.supr-con)
subject: Atomic Physics (physics.atom-ph)
subject: FOS: Physical sciences

description: We study theoretically the di-neutron spatial correlations and the crossover from superfluidity of neutron Cooper pairs in the $^1S_0$ pairing channel to Bose-Einstein condensation (BEC) of di-neutron pairs for both symmetric and neutron matter in the microscopic relativistic pairing theory. We take the bare nucleon-nucleon interaction Bonn-B in the particle-particle channel and the effective interaction PK1 of the relativistic mean-field approach in the particle-hole channel. It is found that the spatial structure of neutron Cooper pair wave function evolves continuously from BCS-type to BEC-type as density decreases. We see a strong concentration of the probability density revealed for the neutron pairs in the fairly small relative distance around $1.5 {\rm fm}$ and the neutron Fermi momentum $k_{Fn}\in[0.6,1.0] {\rm fm^{-1}}$. However, from the effective chemical potential and the quasiparticle excitation spectrum, there is no evidence for the appearance of a true BEC state of neutron pairs at any density. The most BEC-like state may appear at $k_{Fn}\thicksim0.2 {\rm fm^{-1}}$ by examining the density correlation function. From the coherence length and the probability distribution of neutron Cooper pairs as well as the ratio between the neutron pairing gap and the kinetic energy at the Fermi surface, some features of the BCS-BEC crossover are seen in the density regions, $0.05 {\rm fm^{-1}}
description: 7 pages, 6 figures, Accepted by Physics Letters B
DAFNE Operating Experience with Crab Waist Collisions
Creators: name: M. Zobov
name: For DAFNE Collaboration Team
Publisher: name: INFN Open Access Repository
Year: 2008

description: The Phi-factory DAFNE was upgraded in the second half of 2007 in order to
implement a recently proposed scheme of crab waist collisions aimed at
substantial luminosity increase. Commissioning of the modified collider started
in November 2007. In this paper we briefly describe the crab waist collision
concept and discuss in detail the DAFNE hardware upgrade and obtained
experimental results.
Quark Wigner Distributions
Creators: name: B. Pasquini
name: C. Lorcé
Publisher: name: INFN Open Access Repository
Year: 2011

description: We study the Wigner functions of the nucleon which provide multidimensional
images of the quark distributions in phase space and combine in a single
picture all the information contained in the generalized parton distributions
(GPDs) and the transverse-momentum dependent parton distributions (TMDs). In
particular, we present results for the distribution of unpolarized quark in a
longitudinally polarized nucleon. Treating this distribution as it was a
classical distribution, we also obtain the expectation value of the orbital
angular momentum operator and compare the corresponding results from different
quark models with the values obtained using alternative definitions of the
orbital angular momentum, as given in terms of the GPDs and the TMDs.
The partonic structure of the nucleon from generalized transverse
  momentum-dependent parton distributions
Creators: name: B. Pasquini
name: C. Lorce'
Publisher: name: INFN Open Access Repository
Year: 2013

description: We discuss the general formalism for the calculation in light-front quark
models of the fully unintegrated, off-diagonal quark-quark correlator of the
nucleon, parametrized in terms of generalized transverse momentum dependent
parton distributions (GTMDs). By taking specific limits or projections, these
GTMDs yield various transverse-momentum dependent and generalized parton
distributions, thus providing a unified framework to simultaneously model
different observables. The corresponding distributions in impact-parameter
space are the Wigner functions which provide multidimensional images of the
quark distributions in phase space. We present results within a light-front
constituent quark model, discussing some of the complementary aspects encoded
in the different distributions and the relation to the quark orbital angular
momentum of the proton.
title: Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð¸Ð½ÑÐµÑÐ½ÐµÑ-Ð¼Ð°Ð³Ð°Ð·Ð¸Ð½Ð° ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸ Ð½Ð° ÑÐ°Ð¹ÑÐµ Â«Ð¢Ð°Ð¾ ÐÐ°Ð¾Â»
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: Ð£ Ð§ÑÐ½Ñ
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
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Ð±Ð°Ð·Ñ Ð´Ð°Ð½Ð½ÑÑ

description: Ð¦ÐµÐ»Ñ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ¾ÑÑÐ¾Ð¸Ñ Ð² ÑÐ¾Ð·Ð´Ð°Ð½Ð¸Ð¸ Ð¸ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ¸ ÑÐ°Ð¹ÑÐ° Ð¸Ð½ÑÐµÑÐ½ÐµÑ-Ð¼Ð°Ð³Ð°Ð·Ð¸Ð½Ð° Â«Ð¢Ð°Ð¾-ÐÐ°Ð¾Â». Ð Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ Ð¾ÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÐ¸, Ð´Ð¾ÑÑÐ¾Ð¸Ð½ÑÑÐ²Ð° Ð¸ Ð½ÐµÐ´Ð¾ÑÑÐ°ÑÐºÐ¸ ÑÑÑÐµÑÑÐ²ÑÑÑÐ¸Ñ Ð¸Ð½ÑÐµÑÐ½ÐµÑ-Ð¼Ð°Ð³Ð°Ð·Ð¸Ð½Ð¾Ð². ÐÑÐ´ÐµÐ»ÐµÐ½Ñ ÑÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð¾ÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÐ¸ ÑÐ¾Ð·Ð´Ð°Ð½Ð¸Ñ Ð¸Ð½ÑÐµÑÐ½ÐµÑ-Ð¼Ð°Ð³Ð°Ð·Ð¸Ð½Ð°, Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ñ ÑÐ¿Ð¾ÑÐ¾Ð±Ñ Ð¾Ð¿Ð»Ð°ÑÑ ÑÐµÑÐµÐ· Ð¸Ð½ÑÐµÑÐ½ÐµÑ. Ð¢Ð°ÐºÐ¶Ðµ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð° ÑÐ°Ð±Ð¾ÑÐ° Ð¸Ð½ÑÐµÑÐ½ÐµÑ-Ð¼Ð°Ð³Ð°Ð·Ð¸Ð½Ð° Ð¢Ð°Ð¾ BÐ°Ð¾. Ð Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ¾Ð¹ ÑÐ°ÑÑÐ¸ Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ð° ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° ÑÐ°Ð¹ÑÐ° Ð¸Ð½ÑÐµÑÐ½ÐµÑ-Ð¼Ð°Ð³Ð°Ð·Ð¸Ð½Ð° Ð¢Ð°Ð¾-Bao. ÐÐ¿Ð¸ÑÐ°Ð½Ñ ÑÑÐ°Ð¿Ñ Ð²Ð½ÐµÐ´ÑÐµÐ½Ð¸Ñ Ð¸ ÑÐµÑÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÑÐ¸ÑÑÐµÐ¼Ñ.
Quantum Noncanonical Field Theory: Symmetries and Interaction
Creators: name: Carmona, J. M.
name: Cortes, J. L.
name: Indurain, J.
name: Mazon, D.
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: The symmetry properties of a proposal to go beyond relativistic quantum field theory based on a modification of the commutation relations of fields are identified. Poincaré invariance in an auxiliary spacetime is found in the Lagrangian version of the path integral formulation. This invariance is contrasted with the idea of Doubly (or Deformed) Special Relativity (DSR). This analysis is then used to go from the free theory of a complex field to an interacting field theory.
description: 11 pages, minor clarifying corrections added, final version to appear in PRD
Non-Gaussian Scatter in Cluster Scaling Relations
Creators: name: Shaw, Laurie D.
name: Holder, Gilbert P.
name: Dudley, Jonathan
Publisher: name: arXiv
Year: 2009
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We investigate the impact of non-Gaussian scatter in the cluster mass-observable scaling relation on the mass and redshift distribution of clusters detected by wide area surveys. We parameterize non-Gaussian scatter by incorporating the third and forth moments (skewness and kurtosis) into the distribution P(Mobs|M). We demonstrate that for low scatter mass proxies the higher order moments do not significantly affect the observed cluster mass and redshift distributions. However, for high scatter mass indicators it is necessary for the survey limiting mass threshold to be less than 10^14 h^-1 Msol to prevent the skewness from having a significant impact on the observed number counts, particularly at high redshift. We also show that an unknown level of non-Gaussianity in the scatter is equivalent to an additional uncertainty on the variance in P(Mobs|M) and thus may limit the constraints that can be placed on the dark energy equation of state parameter w. Furthermore, positive skewness flattens the mass function at the high mass end, and so one must also account for skewness in P(Mobs|M) when using the shape of the mass function to constrain cluster scaling-relations.
description: 6 Pages, 3 Figures, to be submitted to ApJ Letters
Cronaca di un’onda gravitazionale annunciata
Creators: Patrizia Caraveo
Publisher: name: Media Inaf
Year: 2016

Sappiamo che esistono, ma sono decenni che gli scienziati inseguono il sogno di rivelare direttamente queste increspature dello spazio-tempo. L’attesa è così spasmodica che ogni sussurro, amplificato a dismisura dalla rete, diventa un colpo di cannone
The Church Problem for Countable Ordinals
Creators: name: Rabinovich, Alexander
Publisher: name: arXiv
Year: 2008
Subjects: subject: Logic in Computer Science (cs.LO)
subject: FOS: Computer and information sciences
subject: F.4.1

description: A fundamental theorem of Buchi and Landweber shows that the Church synthesis problem is computable. Buchi and Landweber reduced the Church Problem to problems about ω-games and used the determinacy of such games as one of the main tools to show its computability. We consider a natural generalization of the Church problem to countable ordinals and investigate games of arbitrary countable length. We prove that determinacy and decidability parts of the Bu}chi and Landweber theorem hold for all countable ordinals and that its full extension holds for all ordinals < ω\^ω.
Community Law-Making and the Codification of Customary Laws - Social and Gender Issues in Samoa
Creators: name: Boodoosingh, Ramona
name: Schoeffel, Penelope
Publisher: name: Canberra, ACT: Dept. of Pacific Affairs, Research School of Pacific and Asian Studies, The Australian National University
Year: 2018

description: Samoa possesses two parallel systems through which social order and justice are maintained: the formal constitution-based judicial and legal system and the traditional justice mechanism provided by the village fono (councils) and matai (chiefs and orators). Local government in Samoa is administered by the Ministry of Women, Community and Social Development (MWCSD) through traditional village councils, and similar local government structures have been established in new settlements and suburban areas, albeit without historical traditional authority. This In Brief presents several social and gender issues which may emerge from the codification of customary laws as a result of the 2016 amendments to the Village Fono Act.
Holomorphic extension from the sphere to the ball
Creators: name: Baracco, L.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Complex Variables (math.CV)
subject: FOS: Mathematics
subject: 32

description: Real analytic functions on the boundary of the sphere which have separate holomorphic extension along the complex lines through a boundary point have holomorphic extension to the ball. This was proved in a previous preprint by an argument of CR geometry. We give here an elementary proof based on the expansion in holomorphic and antiholomorphic powers.
SRT a Tor Vergata
Creators: Livia Giacomini
Publisher: name: Media Inaf
Year: 2016

Al via il Master in Scienza e Tecnologia Spaziale dell'Università di Roma Tor Vergata con una lectio magistralis, martedì 9 febbraio, del Presidente INAF Nicolò D'Amico. Per l'occasione, D'Amico sarà intervistato dai liceali che partecipano allo stage in Comunicazione e Divulgazione della Scienza