cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Third-harmonic generation in silica wedge resonators
Creators: name: Soares, Jorge H.
name: Santos, Laís Fujii Dos
name: Santos, Felipe G. S.
name: Inga, Marvyn
name: Espinel, Yovanny A. V.
name: Wiederhecker, Gustavo S.
name: Alegre, Thiago P. Mayer
Publisher: name: arXiv
Year: 2022
Subjects: subject: Optics (physics.optics)
subject: FOS: Physical sciences

description: Whispering-gallery-mode microcavities are known to have high optical quality factor, making them suitable for nonlinear optical interactions. Here, third-harmonic generation is observed using a relatively small radius wedge silicon oxide optical microcavity. The small radii wedge microdisks can be dispersion-tailored to obtain either normal or anomalous group velocity dispersion. In our case, we operate in the normal dispersion regime preventing frequency comb generation by suppressing infrared cascading four-wave mixing. This allows for a clean third harmonic generation at phase-matched visible optical modes. Tunability of the third-harmonic emission is obtained due to a combination of the thermo-optical and Kerr effects. An additional thermal control of the phase matching condition allows for optimizing third-harmonic generation, and agreement between this process and couple-mode theory is demonstrated.
description: 6 pages, 6 figures
Asymptotic behavior of dynamical variables and naked singularity formation in spherically symmetric gravitational collapse
Creators: name: Kawakami, Hayato
name: Mitsuda, Eiji
name: Nambu, Yasusada
name: Tomimatsu, Akira
Publisher: name: arXiv
Year: 2009
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: Considering gravitational collapse of matter, it is important problem to clarify what kind of conditions leads to the formation of naked singularity. For this purpose, we apply the 1+3 orthonormal frame formalism introduced by Uggla \textit{et al.} to spherically symmetric gravitational collapse of perfect fluid. This formalism allows us to construct an autonomous system of evolution and constraint equations for scale-invariant dynamical variables normalized by the volume expansion rate of the timelike orthonormal frame vector. We investigate the asymptotic evolution of such dynamical variables towards the formation of a central singularity and present a conjecture that the steep spatial gradient for the normalized density function is a characteristic of the naked singularity formation.
description: Version published in PRD
Brilliant Pebbles: A Method for Detection of Very Large Interstellar Grains
Creators: name: Socrates, Aristotle
name: Draine, Bruce T.
Publisher: name: arXiv
Year: 2008
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: A photon of wavelength lambda ~1 micron interacting with a dust grain of radius a_p ~ 1 mm (a "pebble") undergoes scattering in the forward direction, largely within a small characteristic diffraction angle theta_s ~ lambda/a_p ~ 100". Though mm-size dust grains contribute negligibly to the interstellar medium's visual extinction, the signal they produce in scattered light may be detectable, especially for variable sources. Observations of light scattered at small angles allows for the direct measurement of the large grain population; variable sources can also yield tomographic information of the interstellar medium's mass distribution. The ability to detect brilliant pebble halos require a careful understanding of the instrument PSF.
description: 5 pages, ApJL accepted
title: Ð­Ð»ÐµÐºÑÑÐ¾Ð½Ð¸ÐºÐ° Ð¸ Ð¼Ð¸ÐºÑÐ¾ÑÐ»ÐµÐºÑÑÐ¾Ð½Ð¸ÐºÐ°. Ð¤Ð¸Ð·Ð¸ÐºÐ¾-ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ðµ Ð¾ÑÐ½Ð¾Ð²Ñ
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ
titleType: Subtitle
Creators: name: ÐÐ°ÑÐ°ÑÐ¾Ð²Ð°, ÐÑÐ¸Ð½Ð°
name: ÐÑÐ±ÐºÐ¾Ð²Ð°, Ð¢Ð°Ð¼Ð°ÑÐ°
Publisher: name: [ÐÐ·Ð´-Ð²Ð¾ Ð¡ÐÐ±ÐÐ¢Ð£]
Year: 1996
Subjects: Ð­Ð»ÐµÐºÑÑÐ¾Ð½Ð¸ÐºÐ° ÑÐ¸Ð·Ð¸ÑÐµÑÐºÐ°Ñ
ÐÐ¸ÐºÑÐ¾ÑÐ»ÐµÐºÑÑÐ¾Ð½Ð¸ÐºÐ°

description: Ð¡Ð¾Ð´ÐµÑÐ¶Ð¸Ñ ÐºÑÐ°ÑÐºÐ¸Ð¹ Ð¾Ð±Ð·Ð¾Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÑ ÑÐ¾Ð¾ÑÐ½Ð¾ÑÐµÐ½Ð¸Ð¹ ÑÐ¸Ð·Ð¸ÐºÐ¾-ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ñ Ð¾ÑÐ½Ð¾Ð² Ð¼Ð¸ÐºÑÐ¾ÑÐ»ÐµÐºÑÑÐ¾Ð½Ð¸ÐºÐ¸, ÑÐ¾ÑÐ¼ÑÐ»Ñ Ð´Ð»Ñ ÑÐµÑÐµÐ½Ð¸Ñ ÑÐ¸Ð¿Ð¸ÑÐ½ÑÑ Ð·Ð°Ð´Ð°Ñ Ð¸ ÐºÐ¾Ð¼Ð¼ÐµÐ½ÑÐ°ÑÐ¸Ð¸, ÐºÐ°ÑÐ°ÑÑÐ¸ÐµÑÑ ÑÑÑÐ½Ð¾ÑÑÐ¸ ÑÐ¸Ð·Ð¸ÑÐµÑÐºÐ¸Ñ ÑÐ²Ð»ÐµÐ½Ð¸Ð¹, a ÑÐ°ÐºÐ¶Ðµ ÑÐ¿Ð¸ÑÐ¾Ðº Ð»Ð¸ÑÐµÑÐ°ÑÑÑÑ Ð¸ Ð´Ð°Ð½Ð½ÑÐµ Ð½ÐµÐºÐ¾ÑÐ¾ÑÑÑ Ð¿Ð°ÑÐ°Ð¼ÐµÑÑÐ¾Ð² Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ð¾Ð², Ð¿ÑÐ¸Ð±Ð¾ÑÐ¾Ð² Ð¸ ÑÐ¸Ð·Ð¸ÑÐµÑÐºÐ¸Ñ Ð²ÐµÐ»Ð¸ÑÐ¸Ð½. ÐÑÐ¸Ð²ÐµÐ´ÐµÐ½Ñ ÑÐµÐºÑÑÑ Ð·Ð°Ð´Ð°Ð½Ð¸Ð¹, ÑÐºÐ°Ð·Ð°Ð½Ð¸Ñ Ð¿Ð¾ Ð¼ÐµÑÐ¾Ð´Ð¸ÐºÐµ Ð¸Ñ Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¸Ñ, Ð¾ÑÐ¾ÑÐ¼Ð»ÐµÐ½Ð¸Ñ Ð¸ Ð·Ð°ÑÐ¸ÑÑ. ÐÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¾ ÑÑÑÐ´ÐµÐ½ÑÐ°Ð¼ Ð´Ð½ÐµÐ²Ð½Ð¾Ð¹ Ð¸ Ð²ÐµÑÐµÑÐ½ÐµÐ¹ ÑÐ¾ÑÐ¼ Ð¾Ð±ÑÑÐµÐ½Ð¸Ñ, Ð¸Ð·ÑÑÐ°ÑÑÐ¸Ð¼ Ð´Ð¸ÑÑÐ¸Ð¿Ð»Ð¸Ð½Ñ "ÐÐ¸ÐºÑÐ¾ÑÐ»ÐµÐºÑÑÐ¾Ð½Ð¸ÐºÐ°" Ð² ÑÐ°Ð¼ÐºÐ°Ñ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ Ð¿Ð¾ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸ÑÐ¼ 553100" Ð¢ÐµÑÐ½Ð¸ÑÐµÑÐºÐ°Ñ ÑÐ¸Ð·Ð¸ÐºÐ°" Ð¸ 550700 "Ð­Ð»ÐµÐºÑÑÐ¾Ð½Ð¸ÐºÐ° Ð¸ Ð¼Ð¸ÐºÑÐ¾ÑÐ»ÐµÐºÑÑÐ¾Ð½Ð¸ÐºÐ°", Ñ Ð¿Ð¾ÑÐ»ÐµÐ´ÑÑÑÐ¸Ð¼ Ð¿ÑÐ¾Ð´Ð¾Ð»Ð¶ÐµÐ½Ð¸ÐµÐ¼ Ð¸Ð½Ð¶ÐµÐ½ÐµÑÐ½Ð¾Ð³Ð¾ Ð¸Ð»Ð¸ Ð¼Ð°Ð³Ð¸ÑÑÐµÑÑÐºÐ¾Ð³Ð¾ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¿Ð¾ Ð¿ÑÐ¾ÑÐ¸Ð»ÑÐ¼ ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾ÑÑÐ¸ 200100 "ÐÐ°ÑÐµÑÐ¸Ð°Ð»Ñ Ð¸ ÐºÐ¾Ð¼Ð¿Ð¾Ð½ÐµÐ½ÑÑ ÑÐ²ÐµÑÐ´Ð¾ÑÐµÐ»ÑÐ½Ð¾Ð¹ ÑÐ»ÐµÐºÑÑÐ¾Ð½Ð¸ÐºÐ¸" (Ð½Ð° ÑÐ°Ð´Ð¸Ð¾ÑÐ¸Ð·Ð¸ÑÐµÑÐºÐ¾Ð¼ Ð¸ Ð²ÐµÑÐµÑÐ½ÐµÐ¼ ÑÐ»ÐµÐºÑÑÐ¾ÑÐ°Ð´Ð¸Ð¾ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¾Ð¼ ÑÐ°ÐºÑÐ»ÑÑÐµÑÐ°Ñ) Ð¸ 190700 "ÐÐ¿ÑÐ¸ÐºÐ¾-ÑÐ»ÐµÐºÑÑÐ¾Ð½Ð½ÑÐµ Ð¿ÑÐ¸Ð±Ð¾ÑÑ Ð¸ ÑÐ¸ÑÑÐµÐ¼Ñ".
description: ÐÐµÑÐ°ÑÐ°ÐµÑÑÑ Ð¿Ð¾ ÑÐµÑÐµÐ½Ð¸Ñ ÑÐµÐ´Ð°ÐºÑÐ¸Ð¾Ð½Ð½Ð¾-Ð¸Ð·Ð´Ð°ÑÐµÐ»ÑÑÐºÐ¾Ð³Ð¾ ÑÐ¾Ð²ÐµÑÐ° Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¾Ð³Ð¾ Ð³Ð¾ÑÑÐ´Ð°ÑÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑÐ°.
title: Ð¡ÑÑÐ°ÑÐµÐ³Ð¸Ñ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð¼ÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½Ð¾Ð¹ ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸ Ð½Ð° ÑÐ¾ÑÑÐ¸Ð¹ÑÐºÐ¾Ð¼ ÑÑÐ½ÐºÐµ B2G
title: Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð¼Ð°Ð³Ð¸ÑÑÑÐ°
titleType: Subtitle
Creators: name: ÐÐ°ÑÑÑÐ½Ð¾Ð²Ð°, ÐÐ°Ñ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: 2018
Subjects: ÑÑÐ½Ð¾Ðº B2G
ÑÐ¸ÑÑÐµÐ¼Ð° Ð·Ð°ÐºÑÐ¿Ð¾Ðº
Ð¼ÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½Ð°Ñ ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ñ
ÑÑÑÐ°ÑÐµÐ³Ð¸Ñ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸
ÑÑÑÐ°ÑÐµÐ³Ð¸ÑÐµÑÐºÐ¾Ðµ Ð¿Ð»Ð°Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ
Ð¼Ð°ÑÐºÐµÑÐ¸Ð½Ð³Ð¾Ð²Ð¾Ðµ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ

description: ÐÐ±ÑÐµÐºÑÐ¾Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ²Ð»ÑÐµÑÑÑ ÑÐ¾ÑÑÐ¸Ð¹ÑÐºÐ¸Ð¹ ÑÑÐ½Ð¾Ðº B2G. Ð¦ÐµÐ»Ñ Ð²ÑÐ¿ÑÑÐºÐ½Ð¾Ð¹ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ â 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ÑÑÐ°ÑÐµÐ³Ð¸Ð¸ Ð¼ÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½Ð¾Ð¹ ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸ Ð² Ð½ÐµÑÑÐ°Ð±Ð¸Ð»ÑÐ½ÑÑ ÑÑÐ»Ð¾Ð²Ð¸ÑÑ ÑÐ¾ÑÑÐ¸Ð¹ÑÐºÐ¾Ð³Ð¾ ÑÑÐ½ÐºÐ° B2G. ÐÐ° Ð¾ÑÐ½Ð¾Ð²Ðµ Ð°Ð½Ð°Ð»Ð¸Ð·Ð° ÑÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¸Ñ Ð¸ÑÑÐ¾ÑÐ½Ð¸ÐºÐ¾Ð² Ð¸ Ð¾Ð±Ð¾Ð±ÑÐµÐ½Ð¸Ñ ÑÐ¾Ð±ÑÐ°Ð½Ð½Ð¾Ð¹ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¸ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ð° Ð¼ÐµÑÐ¾Ð´Ð¸ÐºÐ° Ð°Ð½Ð°Ð»Ð¸Ð·Ð° Ð²Ð½ÐµÑÐ½Ð¸Ñ ÑÐ°ÐºÑÐ¾ÑÐ¾Ð², Ð²Ð»Ð¸ÑÑÑÐ¸Ñ Ð½Ð° Ð¼ÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½ÑÑ ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ñ, ÐºÐ¾ÑÐ¾ÑÐ°Ñ Ð¾ÑÑÑÐµÑÑÐ²Ð»ÑÐµÑ ÑÐ²Ð¾Ñ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÑ Ð½Ð° ÑÐ¾ÑÑÐ¸Ð¹ÑÐºÐ¾Ð¼ ÑÑÐ½ÐºÐµ B2G. ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¾ ÐºÐ¾Ð»Ð¸ÑÐµÑÑÐ²ÐµÐ½Ð½Ð¾Ðµ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð²Ð½ÐµÑÐ½Ð¸Ñ ÑÐ°ÐºÑÐ¾ÑÐ¾Ð² Ñ Ð¿Ð¾Ð¼Ð¾ÑÑÑ Ð¾ÑÐµÐ½Ð¾Ðº ÑÐºÑÐ¿ÐµÑÑÐ¾Ð². ÐÐ¾ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐ°Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¿ÑÐ¾Ð¸Ð·Ð²ÐµÐ´ÐµÐ½Ð° Ð¿ÑÐ¾ÑÐµÐ´ÑÑÐ° ÑÐ°Ð½Ð¶Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð²Ð½ÐµÑÐ½Ð¸Ñ ÑÐ°ÐºÑÐ¾ÑÐ¾Ð² Ð¿Ð¾ Ð¾ÑÐµÐ½ÐºÐµ Ð¾Ñ Ð½Ð°Ð¸Ð±Ð¾Ð»ÑÑÐµÐ³Ð¾ Ðº Ð½Ð°Ð¸Ð¼ÐµÐ½ÑÑÐµÐ¼Ñ ÑÐ°ÐºÑÐ¾ÑÑ. Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ñ ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð°ÑÐ¸Ð¸ Ð¿Ð¾ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð²Ð½ÐµÑÐ½Ð¸Ð¼Ð¸ ÑÐ°ÐºÑÐ¾ÑÐ°Ð¼Ð¸, Ð²Ð»Ð¸ÑÑÑÐ¸Ð¼Ð¸ Ð½Ð° Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ñ. ÐÐ° Ð¸Ñ Ð¾ÑÐ½Ð¾Ð²Ðµ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ñ Ð²Ð°ÑÐ¸Ð°Ð½ÑÑ ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÑÑÐ°ÑÐµÐ³Ð¸Ð¸ ÑÐ¸ÑÐ¼Ñ Ð² Ð½ÐµÑÑÐ°Ð±Ð¸Ð»ÑÐ½ÑÑ ÑÑÐ»Ð¾Ð²Ð¸ÑÑ.
Thermal spikes from the urban heat island increase mortality and alter physiology of lizard embryos
Creators: name: Hall, Joshua M.
name: Warner, Daniel A.
Publisher: name: The Company of Biologists
Year: 2018
Subjects: anolis
Anolis
body condition
constant
egg survival
Embryonic development
evolution
Global change
Heart rate
patterns
phenotypes
Plasticity
responses
temperatures
Thermal adaptation
tolerance
Urbanization

description: Effects of global change (i.e. urbanization, climate change) on adult organisms are readily used to predict the persistence of populations. However, effects on embryo survival and patterns of development are less studied, even though embryos are particularly sensitive to abiotic conditions that are altered by global change (e.g. temperature). In reptiles, relatively warm incubation temperatures increase developmental rate and often enhance fitness-relevant phenotypes, but extremely high temperatures cause death. Due to the urban heat island effect, human-altered habitats (i.e. cities) potentially create unusually warm nest conditions that differ from adjacent natural areas in both mean and extreme temperatures. Such vanation may exert selection pressures on embryos. To address this, we measured soil temperatures in places where the Puerto Rican crested anole lizard (Anolis cristatellus) nests in both city and forest habitats. We bred anoles in the laboratory and subjected their eggs to five incubation treatments that mimicked temperature regimes from the field, three of which included brief exposure to extremely high temperatures (i.e. thermal spikes) measured in the city. We monitored growth and survival of hatchlings in the laboratory for 3 months and found that warmer, city temperatures increase developmental rate, but brief, thermal spikes reduce survival. Hatchling growth and survival were unaffected by incubation treatment. The urban landscape can potentially create selection pressures that influence organisms at early (e.g. embryo) and late life stages. Thus, research aimed at quantifying the impacts of urbanization on wildlife populations must include multiple life stages to gain a comprehensive understanding of this important aspect of global change.
A Fast and Efficient Algorithm for Slater Determinant Updates in Quantum Monte Carlo Simulations
Creators: name: Nukala, Phani K. V. V.
name: Kent, P. R. C.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: We present an efficient low-rank updating algorithm for updating the trial wavefunctions used in Quantum Monte Carlo (QMC) simulations. The algorithm is based on low-rank updating of the Slater determinants. In particular, the computational complexity of the algorithm is O(kN) during the k-th step compared with traditional algorithms that require O(N^2) computations, where N is the system size. For single determinant trial wavefunctions the new algorithm is faster than the traditional O(N^2) Sherman-Morrison algorithm for up to O(N) updates. For multideterminant configuration-interaction type trial wavefunctions of M+1 determinants, the new algorithm is significantly more efficient, saving both O(MN^2) work and O(MN^2) storage. The algorithm enables more accurate and significantly more efficient QMC calculations using configuration interaction type wavefunctions.
Error suppression by a virtual two-qubit gate
Creators: name: Yamamoto, Takahiro
name: Ohira, Ryutaro
Publisher: name: arXiv
Year: 2022
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: Sparse connectivity of a superconducting quantum computer results in the large experimental overheads of SWAP gates. In this study, we consider employing a virtual two-qubit gate (VTQG) as an error suppression technique. The VTQG enables a non-local operation between a pair of distant qubits using only single qubit gates and projective measurements. Here, we apply the VTQG to the digital quantum simulation of the transverse-field Ising model on an IBM quantum computer to suppress the errors due to the noisy two-qubit operations. We present an effective use of VTQG, where the reduction of multiple SWAP gates results in increasing the fidelity of the output states. The obtained results indicate that the VTQG can be useful for suppressing the errors due to the additional SWAP gates. Additionally, by combining a pulse-efficient transpilation method with the VTQG, further suppression of the errors is observed. In our experiments, we have observed one order of magnitude improvement in accuracy for the quantum simulation of the transverse-field Ising model with 8 qubits.
description: 5 pages, 6 figures
title: ÐÐ½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ¸ÑÑÐµÐ¼Ð° Ð°Ð²ÑÐ¾Ð¼Ð°ÑÐ¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ð½Ð¾Ð³Ð¾ ÑÐµÑÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÑÐ¸ÑÑÐµÐ¼ Ñ ÑÐ°Ð½ÐµÐ½Ð¸Ñ Ð´Ð°Ð½Ð½ÑÑ Unity
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§ÐµÑÐ½Ð¸ÐºÐ¾Ð², ÐÐµÑÑ
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2018
Subjects: Ð°Ð²ÑÐ¾Ð¼Ð°ÑÐ¸Ð·Ð°ÑÐ¸Ñ ÑÐµÑÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ
ÑÐ¸ÑÑÐµÐ¼Ð° Ñ ÑÐ°Ð½ÐµÐ½Ð¸Ñ Ð´Ð°Ð½Ð½ÑÑ
Ð²Ð¸ÑÑÑÐ°Ð»ÑÐ½Ð°Ñ ÑÑÐµÐ´Ð°
VMware vSphere

description: Ð¦ÐµÐ»ÑÑ Ð²ÑÐ¿ÑÑÐºÐ½Ð¾Ð¹ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ ÑÐ²Ð»ÑÐµÑÑÑ ÑÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ðµ ÑÑÐ½ÐºÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½Ð¾ÑÑÐ¸ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÑÐ¸ÑÑÐµÐ¼Ñ Ð°Ð²ÑÐ¾Ð¼Ð°ÑÐ¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ð½Ð¾Ð³Ð¾ ÑÐµÑÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¿ÑÑÐµÐ¼ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ¸ ÑÐ¸ÑÑÐµÐ¼Ñ Ð°ÑÐ¸Ð½ÑÑÐ¾Ð½Ð½Ð¾Ð³Ð¾ Ð²Ð·Ð°Ð¸Ð¼Ð¾Ð´ÐµÐ¹ÑÑÐ²Ð¸Ñ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÑÐ¸ÑÑÐµÐ¼Ñ Ð°Ð²ÑÐ¾Ð¼Ð°ÑÐ¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ð½Ð¾Ð³Ð¾ ÑÐµÑÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ñ Ð²Ð¸ÑÑÑÐ°Ð»ÑÐ½Ð¾Ð¹ ÑÑÐµÐ´Ð¾Ð¹ VMware vSphere. Ð Ð°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ ÑÑÑÐµÑÑÐ²ÑÑÑÐ¸Ðµ Ð¼ÐµÑÐ¾Ð´Ñ Ð²Ð·Ð°Ð¸Ð¼Ð¾Ð´ÐµÐ¹ÑÑÐ²Ð¸Ñ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÑÐ¸ÑÑÐµÐ¼Ñ Ð°Ð²ÑÐ¾Ð¼Ð°ÑÐ¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ð½Ð¾Ð³Ð¾ ÑÐµÑÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ñ Ð²Ð¸ÑÑÑÐ°Ð»ÑÐ½Ð¾Ð¹ ÑÑÐµÐ´Ð¾Ð¹. ÐÑÐ¾Ð°Ð½Ð°Ð»Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ñ Ð¿Ð¾Ð´ÑÐ¾Ð´Ñ Ðº ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐµ Ð½Ð¾Ð²Ð¾Ð¹ ÑÑÐ½ÐºÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½Ð¾ÑÑÐ¸. Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ð° ÑÐ¸ÑÑÐµÐ¼Ð° Ð°ÑÐ¸Ð½ÑÑÐ¾Ð½Ð½Ð¾Ð³Ð¾ Ð²Ð·Ð°Ð¸Ð¼Ð¾Ð´ÐµÐ¹ÑÑÐ²Ð¸Ñ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÑÐ¸ÑÑÐµÐ¼Ñ Ñ Ð²Ð¸ÑÑÑÐ°Ð»ÑÐ½Ð¾Ð¹ ÑÑÐµÐ´Ð¾Ð¹. ÐÑÐ¾Ð¸Ð·Ð²ÐµÐ´ÐµÐ½Ð° Ð°Ð¿ÑÐ¾Ð±Ð°ÑÐ¸Ñ Ð¸ Ð²Ð½ÐµÐ´ÑÐµÐ½Ð¸Ðµ Ð½Ð¾Ð²Ð¾Ð¹ ÑÑÐ½ÐºÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½Ð¾ÑÑÐ¸.
Reliable extrapolation of deep neural operators informed by physics or sparse observations
Creators: name: Zhu, Min
name: Zhang, Handi
name: Jiao, Anran
name: Karniadakis, George Em
name: Lu, Lu
Publisher: name: arXiv
Year: 2022
Subjects: subject: Machine Learning (cs.LG)
subject: Computational Physics (physics.comp-ph)
subject: FOS: Computer and information sciences
subject: FOS: Physical sciences

description: Deep neural operators can learn nonlinear mappings between infinite-dimensional function spaces via deep neural networks. As promising surrogate solvers of partial differential equations (PDEs) for real-time prediction, deep neural operators such as deep operator networks (DeepONets) provide a new simulation paradigm in science and engineering. Pure data-driven neural operators and deep learning models, in general, are usually limited to interpolation scenarios, where new predictions utilize inputs within the support of the training set. However, in the inference stage of real-world applications, the input may lie outside the support, i.e., extrapolation is required, which may result to large errors and unavoidable failure of deep learning models. Here, we address this challenge of extrapolation for deep neural operators. First, we systematically investigate the extrapolation behavior of DeepONets by quantifying the extrapolation complexity via the 2-Wasserstein distance between two function spaces and propose a new behavior of bias-variance trade-off for extrapolation with respect to model capacity. Subsequently, we develop a complete workflow, including extrapolation determination, and we propose five reliable learning methods that guarantee a safe prediction under extrapolation by requiring additional information -- the governing PDEs of the system or sparse new observations. The proposed methods are based on either fine-tuning a pre-trained DeepONet or multifidelity learning. We demonstrate the effectiveness of the proposed framework for various types of parametric PDEs. Our systematic comparisons provide practical guidelines for selecting a proper extrapolation method depending on the available information, desired accuracy, and required inference speed.
Effect of Radiative Feedbacks for Resonant Transitions during Cosmological Recombination
Creators: name: Kholupenko, E. E
name: Ivanchik, A. V.
name: Varshalovich, D. A
Publisher: name: arXiv
Year: 2009
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: The inhibition of the total HI $n\leftrightarrow 1$ transition rate by delayed resonant reabsorption of HI $(n+1)\to 1$ photons by HI $n\to 1$ line which is possible due to cosmological redshift is considered semi-analytically. The method taking into account this effect in the frame of simple three-level approximation model of recombination is suggested. It is confirmed that the resonant feedbacks affect ionization fraction at the level about 0.2% for the epoch of last scattering. Similar consideration of HeI $2^1P\leftrightarrow 1^1S$ $\Rightarrow$ HeI $2^3P\leftrightarrow 1^1S$ feedback for helium is provided. It is confirmed that allowance of this feedback leads to increase of predicted free electron fraction by 0.12% at $z\simeq 2300$. It is shown that taking into account absorption and thermalization of HeI $2^1P\leftrightarrow 1^1S$ resonant superequilibrium photons (during their redshifting to the HeI $2^3P\leftrightarrow 1^1S$ frequency) by small amount of neutral hydrogen ($10^{\rm -7} - 10^{\rm -4}$ of total number of hydrogen atoms and ions) existing in helium recombination epoch is important for correct consideration of this helium feedback.
description: 22 pages, 11 figures, 1 table
title: Ð£Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ Ð¼ÐµÑÐ¾Ð¿ÑÐ¸ÑÑÐ¸ÑÐ¼Ð¸ Ð¿Ð¾ Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ñ ÑÐ½ÐµÑÐ³Ð¾ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ Ð³ÑÐ°Ð¶Ð´Ð°Ð½ÑÐºÐ¸Ñ Ð·Ð´Ð°Ð½Ð¸Ð¹
title: Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð¼Ð°Ð³Ð¸ÑÑÑÐ°
titleType: Subtitle
Creators: name: ÐÐ¸Ð²Ð¸ÑÐ°ÑÑÑ, Ð Ð¾Ð½
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2018
Subjects: ÐÑÐ°Ð¶Ð´Ð°Ð½ÑÐºÐ¾Ðµ ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÑÑÐ²Ð¾
ÑÐ½ÐµÑÐ³Ð¾ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÑ
Ð´Ð¸Ð½Ð°Ð¼Ð¸ÑÐµÑÐºÐ¾Ðµ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ
Ð¸Ð½Ð²ÐµÑÑÐ¸ÑÐ¸Ð¸

description: ÐÐ¸ÑÑÐµÑÑÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ðµ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð¿Ð¾ÑÐ²ÑÑÐµÐ½Ð¾ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐµ Ð¼ÐµÑÐ¾Ð´Ð° ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¸Ð½Ð²ÐµÑÑÐ¸ÑÐ¸ÑÐ¼Ð¸ Ð¿ÑÐ¸ ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÑÑÐ²Ðµ ÑÐ½ÐµÑÐ³Ð¾ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾Ð³Ð¾ Ð³ÑÐ°Ð¶Ð´Ð°Ð½ÑÐºÐ¾Ð³Ð¾ Ð·Ð´Ð°Ð½Ð¸Ñ. ÐÑÐ¾Ð°Ð½Ð°Ð»Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ñ Ð²Ð¾Ð·Ð¼Ð¾Ð¶Ð½ÑÐµ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¸Ðµ Ð¿ÑÐµÐ¸Ð¼ÑÑÐµÑÑÐ²Ð° Ð¾Ñ ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑÐ½Ð¾Ð³Ð¾ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¼ÐµÑ Ð¿Ð¾ Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ñ ÑÐ½ÐµÑÐ³Ð¾ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸. Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ð° Ð¼Ð°ÑÐµÐ¼Ð°ÑÐ¸ÑÐµÑÐºÐ°Ñ Ð¼Ð¾Ð´ÐµÐ»Ñ ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÑÑÐ²Ð° ÑÐ½ÐµÑÐ³Ð¾ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾Ð³Ð¾ Ð¾Ð±ÑÐµÐºÑÐ° Ð¶Ð¸Ð»Ð¾Ð³Ð¾ ÑÐ¾Ð½Ð´Ð°, Ð° ÑÐ°ÐºÐ¶Ðµ ÑÑÑÐ°ÑÐµÐ³Ð¸Ñ ÑÐ°ÑÐ¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð¸Ñ Ð¸Ð½Ð²ÐµÑÑÐ¸ÑÐ¸Ð¹ Ð² ÑÐ¾Ð´Ðµ ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÑÑÐ²Ð°.
Additional file 2 of Transcriptome analysis reveals FABP5 as a key player in the development of chicken abdominal fat, regulated by miR-122-5p targeting
Creators: name: Zhai, Bin
name: Li, Hongtai
name: Li, Shuaihao
name: Gu, Jinxing
name: Zhang, Hongyuan
name: Zhang, Yanhua
name: Li, Hong
name: Tian, Yadong
name: Li, Guoxi
name: Wang, Yongcai
Publisher: name: figshare
Year: 2023
Subjects: subject: Biophysics
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Chemical Sciences not elsewhere classified
subject: Immunology
subject: FOS: Clinical medicine
subject: Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Computational Biology

description: Supplementary Material 2
Antenna Array Module
Creators: name: Martín Bartrina, Álvaro
name: Vázquez-Roy, José Luis
name: Inclán Sánchez, Luis
name: Rajo-Iglesias, Eva
Publisher: name: Zenodo
Year: 2023

description: European Patent EP 4122046 B1

Application number: 21712819.8

Proprietor: Maritime IoT Solutions BV

 
description: The present invention relates to an antenna array module for a communication system on a cargo ship, comprising at least a first , a second and a third antenna element, each mounted on a ground plane and containing an antenna feed. The first antenna element is tilted with respect to the second antenna element. The first and the second antenna element are arranged to radiate mainly towards a first path along the cargo ship and the third antenna element is arranged to radiate mainly towards a second path opposite to the first path.
title: Language processing in bilingual children and adults: evidence from filler-gap dependencies and garden path sentences
Creators: name: Pontikas, George
Publisher: name: University of Reading
Year: 2021

description: The present thesis examines morphosyntactic processing in bilingual children and adults. It bridges gaps in the existing literature in three ways. Firstly, previous work on bilingual children has focused on inflectional morphology but has not examined the timecourse of processing in terms of misinterpretation and real time reanalysis or use of information of different sources to aid disambiguation. Second, it extends the use of the visual world eye-tracking paradigm to research in morphosyntactic processing in bilingual children. Third, for the adults, it compares early/native bilinguals to monolinguals and late bilinguals / L2 learners. Two linguistic phenomena were investigated with adults and children; which-questions and garden-path sentences in English. Overall, both bilingual children and adults showed qualitatively similar patterns of processing to their monolingual counterparts. All groups experienced greater difficulty with structures where there was ambiguity and a need for syntactic reanalysis, i.e. object which-questions and garden-path sentences, suggesting incremental processing. The main difference between monolinguals and bilinguals is that of speed; bilinguals appeared to process sentences slower than monolinguals even when their comprehension accuracy was equally as high. This difference was found for both children and adults, as evidenced by the reaction times or changes in the gaze data, and was generally not more pronounced in sentences where reanalysis is required. With regards to the bilingual adults, the early/native bilinguals clustered with the L2 learners in terms of processing speed but more so with the monolingual adults in terms of accuracy. The bilingual groups showed a reduced utilisation of information from various sources to aid processing. Bilingual adults and children made use of number mismatch between the two noun phrases in the study on which-questions to facilitate disambiguation; however, they showed this effect just for off-line comprehension accuracy and not for real time processing, i.e. in the gaze data. The bilinguals also did not show consistent use of referential context to disambiguate in the study on garden path sentences, although this was also the case for the monolingual adults and children. In sum, the results from the studies in this thesis suggest the both bilingual adults and children were equally as able as their monolingual counterparts at an end stage but differed to the monolinguals on more fine-grained measures of real time processing. These measures point to qualitatively similar but more protracted over time processing for bilinguals and with more limited use of facilitatory information to disambiguate.
title: Ð­Ð½ÐµÑÐ³Ð¾ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÑ ÑÐ°ÑÑÐ¾ÑÐ½Ð¾ ÑÐµÐ³ÑÐ»Ð¸ÑÑÐµÐ¼Ð¾Ð³Ð¾ Ð²ÑÑÐ¾ÐºÐ¾ÑÐºÐ¾ÑÐ¾ÑÑÐ½Ð¾Ð³Ð¾ Ð´Ð²Ð¸Ð³Ð°ÑÐµÐ»Ñ Ð¼Ð¾ÑÐ½Ð¾ÑÑÑÑ Ð =119 ÐºÐÑ Ñ Ð¼Ð½Ð¾Ð³Ð¾ÑÑÐ¾Ð²Ð½ÐµÐ²ÑÐ¼ Ð¿ÑÐµÐ¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°ÑÐµÐ»ÐµÐ¼ Ñ ÑÑÐµÐ¹ÐºÐ¾-Ð³Ð½ÐµÐ·Ð´Ð¾Ð²Ð¾Ð¹ ÑÑÑÑÐºÑÑÑÐ¾Ð¹
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: Ð¯ÐºÐ¾Ð²Ð»ÐµÐ², ÐÐ»Ð°Ð´Ð¸ÑÐ»Ð°Ð²
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2016
Subjects: ÑÐ»ÐµÐºÑÑÐ¾Ð¿ÑÐ¸Ð²Ð¾Ð´Ñ
Ð¿ÑÐµÐ¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°ÑÐµÐ»Ð¸
ÑÐ½ÐµÑÐ³Ð¾ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÑ
drive
converter
efficiency

description: ÐÐ°Ð½Ð½Ð°Ñ Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ° Ð¿Ð¾ÑÐ²ÑÑÐµÐ½Ð° ÑÑÐ°Ð²Ð½ÐµÐ½Ð¸Ñ ÑÐ½ÐµÑÐ³Ð¾ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ Ð´Ð²ÑÑ ÑÐ°Ð·Ð»Ð¸ÑÐ½ÑÑ ÑÐ¸Ð¿Ð¾Ð² Ð¿ÑÐµÐ¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°ÑÐµÐ»ÐµÐ¹ ÑÐ°ÑÑÐ¾ÑÑ, ÐºÐ¾ÑÐ¾ÑÑÐµ Ð¿ÑÐ¸Ð¼ÐµÐ½ÑÑÑÑÑ Ð² ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½ÑÑ Ð²ÑÑÐ¾ÐºÐ¾ÑÐºÐ¾ÑÐ¾ÑÑÐ½ÑÑ ÑÐ»ÐµÐºÑÑÐ¾Ð¿ÑÐ¸Ð²Ð¾Ð´Ð°Ñ. Ð ÑÐ°Ð±Ð¾ÑÐµ ÑÐ°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÑÑÑÑ Ð¿ÑÐ¸Ð½ÑÐ¸Ð¿Ñ ÑÐ°Ð±Ð¾ÑÑ Ð¿ÑÐµÐ¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°ÑÐµÐ»ÐµÐ¹ ÑÐ°ÑÑÐ¾ÑÑ, Ð° ÑÐ°ÐºÐ¶Ðµ Ð¾Ð¿Ð¸ÑÐ°Ð½Ñ ÑÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¸Ðµ ÑÐ²ÐµÐ´ÐµÐ½Ð¸Ñ, Ð² Ð¾ÑÐ½Ð¾Ð²Ðµ ÐºÐ¾ÑÐ¾ÑÑÑ Ð»ÐµÐ¶Ð¸Ñ Ð¿ÑÐ¸Ð½ÑÐ¸Ð¿ ÑÐ°ÑÑÐ¾ÑÐ½Ð¾Ð³Ð¾ ÑÐµÐ³ÑÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÑÐ»ÐµÐºÑÑÐ¾Ð¿ÑÐ¸Ð²Ð¾Ð´Ð°. Ð ÑÐ¾Ð´Ðµ ÑÑÐ°Ð²Ð½ÐµÐ½Ð¸Ñ Ð±ÑÐ»Ð¸ Ð²ÑÑÐ²Ð»ÐµÐ½Ñ Ð¿ÑÐµÐ¸Ð¼ÑÑÐµÑÑÐ²Ð° Ð¸ Ð½ÐµÐ´Ð¾ÑÑÐ°ÑÐºÐ¸ Ð¿ÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸Ñ Ð¿ÑÐµÐ¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°ÑÐµÐ»Ñ Ñ ÑÑÐµÐ¹ÐºÐ¾-Ð³Ð½ÐµÐ·Ð´Ð¾Ð²Ð¾Ð¹ ÑÑÑÑÐºÑÑÑÐ¾Ð¹.
description: This bachelor's graduation work is devoted to a comparison of energy efficiency of two different types of frequency converters, which are applied in modern high-speed electric drives. This work deals with the principles of frequency converters, as well as the information described in theory, based on the principle of frequency control drive. During the comparison, advantages and disadvantages of the use of the converter with low voltage cells structure were shown.
Analysis of test beam data taken with a prototype of TPC with resistive Micromegas for the T2K Near Detector upgrade
Creators: name: Attié, D.
name: Ballester, O.
name: Batkiewicz-Kwasniak, M.
name: Billoir, P.
name: Blanchet, A.
name: Blondel, A.
name: Bolognesi, S.
name: Boullon, R.
name: Calvet, D.
name: Casado, M. P.
name: Catanesi, M. G.
name: Cicerchia, M.
name: Cogo, G.
name: Colas, P.
name: Collazuol, G.
name: Dalmazzone, C.
name: Daret, T.
name: Delbart, A.
name: De Lorenzis, A.
name: Dolan, S.
name: Dygnarowicz, K.
name: Dumarchez, J.
name: Emery-Schrenk, S.
name: Ershova, A.
name: Eurin, G.
name: Feltre, M.
name: Forza, C.
name: Giannessi, L.
name: Giganti, C.
name: Gramegna, F.
name: Grassi, M.
name: Guigue, M.
name: Hamacher-Baumann, P.
name: Hassani, S.
name: Henaff, D.
name: Iacob, F.
name: Jesús-Valls, C.
name: Joshi, S.
name: Kurjata, R.
name: Lamoureux, M.
name: Langella, A.
name: Laporte, J. F.
name: Lavitola, L.
name: Lehuraux, M.
name: Longhin, A.
name: Lux, T.
name: Magaletti, L.
name: Marchi, T.
name: Mellet, L.
name: Mezzetto, M.
name: Munteanu, L.
name: Nguyen, Q. V.
name: Orain, Y.
name: Pari, M.
name: Parraud, J. -M.
name: Pastore, C.
name: Pepato, A.
name: Pierre, E.
name: Garcia, C. Pio
name: Popov, B.
name: Porthault, J.
name: Przybiliski, H.
name: Pupilli, F.
name: Radermacher, T.
name: Radicioni, E.
name: Rossi, F.
name: Roth, S.
name: Russo, S.
name: Rychter, A.
name: Scomparin, L.
name: Smyczek, D.
name: Steinmann, J.
name: Suvorov, S.
name: Swierblewski, J.
name: Terront, D.
name: Thamm, N.
name: Toussenel, F.
name: Valentino, V.
name: Varghese, M.
name: Vasseur, G.
name: Virginet, U.
name: Yevarouskaya, U.
name: Ziembicki, M.
name: Zito, M.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Instrumentation and Detectors (physics.ins-det)
subject: FOS: Physical sciences

description: In this paper we describe the performance of a prototype of the High Angle Time Projection Chambers (HA-TPCs) that are being produced for the Near Detector (ND280) upgrade of the T2K experiment. The two HA-TPCs of ND280 will be instrumented with eight Encapsulated Resistive Anode Micromegas (ERAM) on each endplate, thus constituting in total 32 ERAMs. This innovative technique allows the detection of the charge emitted by ionization electrons over several pads, improving the determination of the track position. The TPC prototype has been equipped with the first ERAM module produced for T2K and with the HA-TPC readout electronics chain and it has been exposed to the DESY Test Beam in order to measure spatial and dE/dx resolution. In this paper we characterize the performances of the ERAM and, for the first time, we compare them with a newly developed simulation of the detector response. Spatial resolution better than 800 ${μ\rm m}$ and dE/dx resolution better than 10% are observed for all the incident angles and for all the drift distances of interest. All the main features of the data are correctly reproduced by the simulation and these performances fully fulfill the requirements for the HA-TPCs of T2K.
Indian Reserves Allotted for Fishing Purposes in British Columbia, 1849-1925 : [supplement to “Landing Native Fisheries: Indian Reserves and Fishing Rights in British Columbia, 1849-1925”]
Creators: name: Harris, Douglas C.
Publisher: name: UBC Press
Year: 2008

description: This table accompanies Douglas C. Harris' book 'Landing Native Fisheries: Indian Reserves and Fishing Rights in British Columbia, 1849-1925' (Vancouver: UBC Press, 2008). It provides additional and supporting detail for the Indian reserves that were specifically allotted for fishing purposes. For more information about the book, see http://www.ubcpress.ca/search/title_book.asp?BookID=5266
Manipulating the motion of large neutral molecules
Creators: name: Küpper, Jochen
name: Filsinger, Frank
name: Meijer, Gerard
Publisher: name: arXiv
Year: 2009
Subjects: subject: Atomic Physics (physics.atom-ph)
subject: Atomic and Molecular Clusters (physics.atm-clus)
subject: Chemical Physics (physics.chem-ph)
subject: FOS: Physical sciences

description: Large molecules have complex potential-energy surfaces with many local minima. They exhibit multiple stereo-isomers, even at very low temperatures. In this paper we discuss the different approaches for the manipulation of the motion of large and complex molecules, like amino acids or peptides, and the prospects of state- and conformer-selected, focused, and slow beams of such molecules for studying their molecular properties and for fundamental physics studies. Accepted for publication in Faraday Disc. 142 (2009), DOI: 10.1039/b820045a
description: 12 pages
Leftward, Rightward and Complete Exit Time Distributions of Jump Processes
Creators: name: Klinger, Jérémie
name: Voituriez, Raphaël
name: Bénichou, Olivier
Publisher: name: arXiv
Year: 2022
Subjects: subject: Statistical Mechanics (cond-mat.stat-mech)
subject: Probability (math.PR)
subject: FOS: Physical sciences
subject: FOS: Mathematics

description: First-passage properties of continuous stochastic processes confined in a 1--dimensional interval are well described. However, for jump processes (discrete random walks), the characterization of the corresponding observables remains elusive, despite their relevance in various contexts. Here we derive exact asymptotic expressions for the leftward, rightward and complete exit time distributions from the interval $[0,x]$ for symmetric jump processes starting from $x_0=0$, in the large $x$ and large time limit. We show that both the leftward probability $F_{\underline{0},x}(n)$ to exit through $0$ at step $n$ and rightward probability $F_{0,\underline{x}}(n)$ to exit through $x$ at step $n$ exhibit a universal behavior dictated by the large distance decay of the jump distribution parameterized by the Levy exponent $μ$. In particular, we exhaustively describe the $n\ll x^μ$ and $n\gg x^μ$ limits and obtain explicit results in both regimes. Our results finally provide exact asymptotics for exit time distributions of jump processes in regimes where continuous limits do not apply.
description: 5 pages, 4 figures, Supplementary Material(5 pages)
MRI  of permanent righ-to-left shunt in patent foramen ovale
Creators: name: Olivetti, Lucio
Publisher: name: EURORAD
Year: 2014
Subjects: subject: Cardiac
subject: Neuroradiology brain
subject: Echocardiography
subject: Echocardiography (transoesophageal)
subject: MR
subject: Diagnostic procedure
subject: Haemodynamics / Flow dynamics
subject: Ischaemia / Infarction

description: Clinical History Image Findings Discussion Find Diagnosis Differential Diagnosis
description: female, 51 years
description: Clinical History: A 51 years old  woman presented at Emergency Department with stroke. The medical history excluded hypertension, diabetes mellitus, heart disease and smoking; the patient did not use oral contraceptives. An accurate but negative clinical history was taken ... Final Diagnosis: Patent cardiac foramen ovale with permanent shunt right-left shunt.
title: ÐÐ¾Ð´Ð±Ð¾Ñ ÑÐµÐ¿Ð»Ð¾Ð¸Ð·Ð¾Ð»ÑÑÐ¸Ð¾Ð½Ð½ÑÑ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ð¾Ð² Ð¾Ð³ÑÐ°Ð¶Ð´Ð°ÑÑÐ¸Ñ ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð¹ Ð¾Ð±ÑÐµÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð·Ð´Ð°Ð½Ð¸Ñ
title: Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ°
titleType: Subtitle
Creators: name: Ð¨ÐµÑÐ¾Ð²ÑÐ¾Ð², ÐÐ»ÐµÐºÑÐ°Ð½Ð´Ñ
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2018
Subjects: ÑÐµÐ¿Ð»Ð¾ÑÐ°ÑÑÐµÑ
ÑÐµÐ¿Ð»Ð¾Ð¸Ð·Ð¾Ð»ÑÑÐ¸Ñ
Ð¾Ð³ÑÐ°Ð¶Ð´Ð°ÑÑÐ¸Ðµ ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð¸
Ð¾Ð±ÑÐµÑÑÐ²ÐµÐ½Ð½Ð¾Ðµ Ð·Ð´Ð°Ð½Ð¸Ðµ

description: Ð ÑÐ°Ð¼ÐºÐ°Ñ Ð½Ð°ÑÑÐ½Ð¾Ð¹ ÑÐ°ÑÑÐ¸ Ð´Ð¸Ð¿Ð»Ð¾Ð¼Ð½Ð¾Ð³Ð¾ Ð¿ÑÐ¾ÐµÐºÑÐ° Ð±ÑÐ» Ð¿ÑÐ¾Ð¸Ð·Ð²ÐµÐ´ÐµÐ½ Ð¿Ð¾Ð´Ð±Ð¾Ñ ÑÐµÐ¿Ð»Ð¾Ð¸Ð·Ð¾Ð»ÑÑÐ¸Ð¾Ð½Ð½ÑÑ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ð¾Ð² Ð¾Ð³ÑÐ°Ð¶Ð´Ð°ÑÑÐ¸Ñ ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð¹ Ð¾Ð±ÑÐµÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð·Ð´Ð°Ð½Ð¸Ñ. Ð Ð°ÑÐ¿Ð¾Ð»Ð¾Ð¶ÐµÐ½Ð¸Ðµ ÑÐµÐ¿Ð»Ð¾Ð¸Ð·Ð¾Ð»ÑÑÐ¸Ð¾Ð½Ð½Ð¾Ð³Ð¾ ÑÐ»Ð¾Ñ Ñ Ð½Ð°ÑÑÐ¶Ð½Ð¾Ð¹ ÑÑÐ¾ÑÐ¾Ð½Ñ ÑÑÐµÐ½Ñ Ð² Ð²ÐµÐ½ÑÐ¸Ð»Ð¸ÑÑÐµÐ¼Ð¾Ð¼ ÑÐ°ÑÐ°Ð´Ðµ Ð¾Ð±Ð»Ð°Ð´Ð°ÐµÑ ÑÑÐ´Ð¾Ð¼ Ð¿ÑÐµÐ¸Ð¼ÑÑÐµÑÑÐ² Ñ ÑÐµÐ¿Ð»Ð¾ÑÐ¸Ð·Ð¸ÑÐµÑÐºÐ¾Ð¹ ÑÐ¾ÑÐºÐ¸ Ð·ÑÐµÐ½Ð¸Ñ. Ð ÑÐ°ÑÑÐ½Ð¾ÑÑÐ¸, Ð¸ÑÐºÐ»ÑÑÐ°ÐµÑÑÑ Ð²Ð»Ð¸ÑÐ½Ð¸Ðµ Ð¿Ð¾ÑÑÐ¸ Ð²ÑÐµÑ ÑÐµÐ¿Ð»Ð¾Ð¿ÑÐ¾Ð²Ð¾Ð´Ð½ÑÑ Ð²ÐºÐ»ÑÑÐµÐ½Ð¸Ð¹ (Ð¼Ð¾ÑÑÐ¸ÐºÐ¾Ð² ÑÐ¾Ð»Ð¾Ð´Ð°), ÐºÐ¾ÑÐ¾ÑÑÐµ Ð¾Ð±ÑÑÐ½Ð¾ Ð¿ÑÐ¸ÑÑÑÑÑÐ²ÑÑÑ Ð² ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸ÑÑ. ÐÐ´Ð½Ð°ÐºÐ¾ Ð¾Ð³ÑÐ°Ð¶Ð´Ð°ÑÑÐ¸Ðµ ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð¸ Ñ ÑÐµÐ¿Ð»Ð¾Ð¸Ð·Ð¾Ð»ÑÑÐ¸Ð¾Ð½Ð½ÑÐ¼Ð¸ Ð²ÐµÐ½ÑÐ¸Ð»Ð¸ÑÑÐµÐ¼ÑÐ¼Ð¸ ÑÐ°ÑÐ°Ð´Ð°Ð¼Ð¸ Ð²ÑÐµ Ð¶Ðµ Ð¾Ð±Ð»Ð°Ð´Ð°ÑÑ ÑÐµÐ¿Ð»Ð¾Ð¿ÑÐ¾Ð²Ð¾Ð´Ð½ÑÐ¼Ð¸ Ð²ÐºÐ»ÑÑÐµÐ½Ð¸ÑÐ¼Ð¸, ÐºÐ¾ÑÐ¾ÑÑÐµ ÑÑÑÐµÑÑÐ²ÐµÐ½Ð½Ð¾ ÑÐ½Ð¸Ð¶Ð°ÑÑ ÐºÐ¾ÑÑÑÐ¸ÑÐ¸ÐµÐ½Ñ ÑÐµÐ¿Ð»Ð¾ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¾Ð¹ Ð¾Ð´Ð½Ð¾ÑÐ¾Ð´Ð½Ð¾ÑÑÐ¸ Ð¸ Ð¿ÑÐ¸Ð²ÐµÐ´ÐµÐ½Ð½Ð¾Ðµ ÑÐ¾Ð¿ÑÐ¾ÑÐ¸Ð²Ð»ÐµÐ½Ð¸Ðµ ÑÐµÐ¿Ð»Ð¾Ð¿ÐµÑÐµÐ´Ð°ÑÐµ. Ð ÑÐ°Ð±Ð¾ÑÐµ Ð¿ÑÐ¸Ð½ÑÑ ÑÐ°ÑÑÐ½ÑÐ¹ ÑÐ»ÑÑÐ°Ð¹ Ð¿Ð»Ð¾ÑÐºÐ¾ÑÑÐ¸ Ð¾Ð³ÑÐ°Ð¶Ð´Ð°ÑÑÐµÐ¹ ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð¸, Ð³Ð´Ðµ ÑÐµÐ¿Ð»Ð¾Ð¿Ð¾ÑÐµÑÐ¸ Ð¿ÑÐ¾Ð¸ÑÑÐ¾Ð´ÑÑ ÑÐ¾Ð»ÑÐºÐ¾ ÑÐµÑÐµÐ· Ð´ÑÐ±ÐµÐ»Ñ, ÐºÑÐµÐ¿ÑÑÐ¸Ðµ ÑÑÐµÐ¿Ð»Ð¸ÑÐµÐ»Ñ Ðº ÑÑÐµÐ½Ðµ. Ð¢Ð°ÐºÐ¶Ðµ ÑÐ°Ð±Ð¾ÑÐµ Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð° Ð¿ÑÐ¾Ð²ÐµÑÐºÐ° Ð½ÐµÐ¾Ð±ÑÐ¾Ð´Ð¸Ð¼Ð¾ÑÑÐ¸ ÑÑÐµÐ¿Ð»ÐµÐ½Ð¸Ñ Ð¾Ð³ÑÐ°Ð¶Ð´Ð°ÑÑÐ¸Ñ ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð¹ Ð½Ð° Ð²ÑÑ Ð²ÑÑÐ¾ÑÑ Ð¿Ð¾Ð´Ð·ÐµÐ¼Ð½ÑÑ ÑÑÐ°Ð¶ÐµÐ¹ Ð¾Ð±ÑÐµÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð·Ð´Ð°Ð½Ð¸Ñ.
title: Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð¼ÐµÑÐ¾Ð´Ð¸ÐºÐ¸ ÑÐ°ÑÑÐµÑÐ° ÑÐ¸Ð» ÑÐµÐ·Ð°Ð½Ð¸Ñ Ð¿ÑÐ¸ ÑÐ°ÑÐ¾Ð½Ð½Ð¾Ð¼ ÑÑÐµÐ·ÐµÑÐ¾Ð²Ð°Ð½Ð¸Ð¸ Ð¿ÑÐ¸ Ð¾Ð±ÑÐ°Ð±Ð¾ÑÐºÐµ Ð´ÐµÑÐ°Ð»Ð¸ Â«Ð¨Ð°ÑÑÐ½ Ð¿ÑÐ¸ÑÐµÐ¿Ð½Ð¾Ð¹Â»
title: Ð¼Ð°Ð³Ð¸ÑÑÐµÑÑÐºÐ°Ñ Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ñ
titleType: Subtitle
Creators: name: Ð§Ð²ÑÐºÐ¾Ð², ÐÐ½Ð´ÑÐµÐ¹
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2016
Subjects: Ð¤ÑÐµÐ·ÐµÑÐ¾Ð²Ð°Ð½Ð¸Ðµ Ð¼ÐµÑÐ°Ð»Ð»Ð¾Ð² ÑÐ°ÑÐ¾Ð½Ð½Ð¾Ðµ
Ð ÐµÐ·Ð°Ð½Ð¸Ðµ Ð¼ÐµÑÐ°Ð»Ð»Ð¾Ð²
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Early Results from GLASS-JWST. XIX: A High Density of Bright Galaxies at $z\approx10$ in the Abell 2744 Region
Creators: name: Castellano, Marco
name: Fontana, Adriano
name: Treu, Tommaso
name: Merlin, Emiliano
name: Santini, Paola
name: Bergamini, Pietro
name: Grillo, Claudio
name: Rosati, Piero
name: Acebron, Ana
name: Leethochawalit, Nicha
name: Paris, Diego
name: Bonchi, Andrea
name: Belfiori, Davide
name: Calabrò, Antonello
name: Correnti, Matteo
name: Nonino, Mario
name: Polenta, Gianluca
name: Trenti, Michele
name: Boyett, Kristan
name: Brammer, G.
name: Broadhurst, Tom
name: Caminha, Gabriel B.
name: Chen, Wenlei
name: Filippenko, Alexei V.
name: Fortuni, Flaminia
name: Glazebrook, Karl
name: Mascia, Sara
name: Mason, Charlotte A.
name: Menci, Nicola
name: Meneghetti, Massimo
name: Mercurio, Amata
name: Metha, Benjamin
name: Morishita, Takahiro
name: Nanayakkara, Themiya
name: Pentericci, Laura
name: Roberts-Borsani, Guido
name: Roy, Namrata
name: Vanzella, Eros
name: Vulcani, Benedetta
name: Yang, Lilan
name: Wang, Xin
Publisher: name: arXiv
Year: 2022
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We report the detection of a high density of redshift $z\approx 10$ galaxies behind the foreground cluster Abell 2744, selected from imaging data obtained recently with NIRCam onboard {\it JWST} by three programs -- GLASS-JWST, UNCOVER, and DDT\#2756. To ensure robust estimates of the lensing magnification $μ$, we use an improved version of our model that exploits the first epoch of NIRCam images and newly obtained MUSE spectra, and avoids regions with $μ>5$ where the uncertainty may be higher. We detect seven bright $z\approx 10$ galaxies with demagnified rest-frame $-22 \lesssim M_{\rm UV}\lesssim -19$ mag, over an area of $\sim37$ sq. arcmin. Taking into account photometric incompleteness and the effects of lensing on luminosity and cosmological volume, we find that the density of $z\approx 10$ galaxies in the field is about $10\times$ ($3\times$) larger than the average at $M_{UV}\approx -21~ (-20)$ mag reported so far. The density is even higher when considering only the GLASS-JWST data, which are the deepest and the least affected by magnification and incompleteness. The GLASS-JWST field contains 5 out of 7 galaxies, distributed along an apparent filamentary structure of 2 Mpc in projected length, and includes a close pair of candidates with $M_{\rm UV}< -20$ mag having a projected separation of only 16 kpc. These findings suggest the presence of a $z\approx 10$ overdensity in the field. In addition to providing excellent targets for efficient spectroscopic follow-up observations, our study confirms the high density of bright galaxies observed in early {\it JWST} observations, but calls for multiple surveys along independent lines of sight to achieve an unbiased estimate of their average density and a first estimate of their clustering.
description: Accepted for publication in ApJL, 13 pages, 4 figures
Head-Tail Modes for Strong Space Charge
Creators: name: Burov, Alexey
Publisher: name: arXiv
Year: 2008
Subjects: subject: Accelerator Physics (physics.acc-ph)
subject: FOS: Physical sciences

description: The head-tail modes are described for the space charge tune shift significantly exceeding the synchrotron tune. A general equation for the modes is derived. The spatial shapes of the modes, their frequencies, and coherent growth rates are explored. The Landau damping rates are also found. The suppression of the transverse mode coupling instability by the space charge is explained.
description: 11 pages, 7 figures, submitted to Phys. Rev. ST-Accel. Beams
Note on inconsistency of unitarity saturation and maximal odderon
Creators: name: Troshin, S. M.
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: It is shown that regime of elastic scattering with maximal odderon contribution is not compatible with unitarity and black disk limits saturation.
description: 5 pages, revised version, text modified, reference added, results unchanged
Non-abelian gauge structure in neutrino mixing
Creators: name: Blasone, Massimo
name: Di Mauro, Marco
name: Vitiello, Giuseppe
Publisher: name: arXiv
Year: 2010
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We discuss the existence of a non-abelian gauge structure associated with flavor mixing. In the specific case of two flavor mixing of Dirac neutrino fields, we show that this reformulation allows to define flavor neutrino states which preserve the Poincaré structure. Phenomenological consequences of our analysis are explored.
description: 13 pages, 2 figures
Additional file 1 of The collateral activity of RfxCas13d can induce lethality in a RfxCas13d knock-in mouse model
Creators: name: Li, Yunfei
name: Xu, Junjie
name: Guo, Xuefei
name: Li, Zhiwei
name: Cao, Lili
name: Liu, Shengde
name: Guo, Ying
name: Wang, Guodong
name: Luo, Yujie
name: Zhang, Zeming
name: Wei, Xuemei
name: Zhao, Yingchi
name: Liu, Tongtong
name: Wang, Xiao
name: Xia, Huawei
name: Kuang, Ming
name: Guo, Qirui
name: Li, Junhong
name: Chen, Luoying
name: Wang, Yibing
name: Li, Qi
name: Wang, Fengchao
name: Liu, Qinghua
name: You, Fuping
Publisher: name: figshare
Year: 2023
Subjects: subject: Biophysics
subject: Biochemistry
subject: Microbiology
subject: FOS: Biological sciences
subject: Cell Biology
subject: Genetics
subject: Molecular Biology
subject: Neuroscience
subject: Biological Sciences not elsewhere classified
subject: Cancer
subject: Mental Health

description: Additional file 1. Supplementary figures.
Exploring the Emission Mechanisms of Mrk 180 with long term X-ray and $γ$-ray data
Creators: name: Mondal, Sandeep Kumar
name: Das, Saikat
name: Gupta, Nayantara
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: Markarian (Mrk) 180 is a BL Lacertae (BL Lac) object located at a redshift of 0.045 and a potential candidate for high-energy cosmic ray acceleration. We have analyzed the Fermi Large Area Telescope (\textit{Fermi}-LAT) $γ$-ray data of Mrk 180 collected over a period of 12.8 years and found no significant enhancement in the flux from the long-term $γ$-ray light curve. We have also analyzed Swift X-ray, ultraviolet \& optical, and X-ray Multi-Mirror Mission (XMM-Newton) data to construct the multi-wavelength spectral energy distribution (SED). The SED has been modeled with one-zone pure leptonic and lepto-hadronic scenarios to explain the underlying physics of multi-wavelength emission. The pure leptonic model and the two lepto-hadronic models, viz., (i) line-of-sight interactions of ultrahigh-energy cosmic rays (UHECR; $E\gtrsim 10^{17}$ eV) with the cosmic background radiation and (ii) the interactions of relativistic protons with the cold protons in the jet, have been compared in our work. Moreover, an earlier study has associated Mrk 180 with the Telescope Array (TA) hotspot of UHECRs at $E>57$ EeV. This speculation motivates us to check whether ultrahigh energy protons and iron nuclei can reach the earth from Mrk 180. After comparing the results of our simulation with the current observational data, we find that Mrk 180 is unlikely to be a source of the UHECR events contributing to the TA hotspot for conservative strengths of extragalactic magnetic fields.
description: 12 pages, 4 figures, 1 table; Accepted for publication in ApJ
Comparing Symbiotic Nebulae and Planetary Nebulae Luminosity Functions
Creators: name: Frankowski, Adam
name: Soker, Noam
Publisher: name: arXiv
Year: 2009
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We compare the observed symbiotic nebulae (SyN) luminosity function (SyNLF) in the [O III] 5007A line to the planetary nebulae (PN) luminosity function (PNLF) and find that the intrinsic SyNLF (ISyNLF) of galactic SyNs has - within its uncertainty of 0.5-0.8mag - very similar cutoff luminosity and general shape to those of the PNLF. The [O III]/(Halpha+[N II]) line ratios of SyNs and PNs are shown to be also related. Possible implications of these results for the universality of the PNLF are briefly outlined.
description: Accepted by ApJ Letters
Mitigating the impact of the CIB on galaxy cluster SZ detection with spectrally constrained matched filters
Creators: name: Zubeldia, Íñigo
name: Chluba, Jens
name: Battye, Richard
Publisher: name: arXiv
Year: 2022
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: Galaxy clusters detected through the thermal Sunyaev-Zeldovich (tSZ) effect are a powerful cosmological probe from which constraints on cosmological parameters such as $Ω_{\mathrm{m}}$ and $σ_8$ can be derived. The measured cluster tSZ signal can be, however, contaminated by Cosmic Infrared Background (CIB) emission, as the CIB is spatially correlated with the cluster tSZ field. We quantify the extent of this contamination by applying the iterative multi-frequency matched filter (iMMF) cluster-finding method to mock Planck-like data from the Websky simulation. We find a significant bias in the retrieved cluster tSZ observables (signal-to-noise and Compton-$y$ amplitude), at the level of about $0.5\, σ$ per cluster. This CIB-induced bias translates into about $20$% fewer detections than expected if all the Planck HFI channels are used in the analysis, which can potentially bias derived cosmological constraints. We introduce a spectrally constrained iMMF, or sciMMF, which proves to be highly effective at suppressing this CIB-induced bias from the tSZ cluster observables by spectrally deprojecting the cluster-correlated CIB at the expense of a small signal-to-noise penalty. Our sciMMF is also robust to modelling uncertainties, namely to the choice of deprojection spectral energy distribution. With it, CIB-free cluster catalogues can be constructed and used for cosmological inference. We provide a publicly available implementation of our sciMMF as part of the SZiFi package.
description: 21 pages, submitted to MNRAS, comments welcome