cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
title: ÐÐ½Ð²Ð°Ð·Ð¸Ñ Ð½Ð¾ÑÐ¼Ð°Ð»ÑÐ½ÑÑ Ð¸ ÑÑÐ°Ð½ÑÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð½ÑÑ ÑÐ¸Ð±ÑÐ¾Ð±Ð»Ð°ÑÑÐ¾Ð² Ð±Ð°ÐºÑÐµÑÐ¸ÑÐ¼Ð¸ S.grimesii
title: Ð¼Ð°Ð³Ð¸ÑÑÐµÑÑÐºÐ°Ñ Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ñ
titleType: Subtitle
Creators: name: ÐÐ²Ð»ÐµÐ², 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: 2017
Subjects: ÐÐ°ÐºÑÐµÑÐ¸Ð¸
Ð¸Ð¼Ð¼Ð¾ÑÑÐ°Ð»Ð¸Ð·Ð¾Ð²Ð°Ð½Ð½ÑÐµ ÐºÐ»ÐµÑÐºÐ¸
Ð±Ð°ÐºÑÐµÑÐ¸Ð°Ð»ÑÐ½Ð°Ñ Ð¸Ð½Ð²Ð°Ð·Ð¸Ñ

description: ÐÐ°Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð¿Ð¾ÑÐ²ÑÑÐµÐ½Ð° Ð¸Ð·ÑÑÐµÐ½Ð¸Ñ Ð²Ð·Ð°Ð¸Ð¼Ð¾Ð´ÐµÐ¹ÑÑÐ²Ð¸Ñ Ð¸Ð¼Ð¼Ð¾ÑÑÐ°Ð»Ð¸Ð·Ð¾Ð²Ð°Ð½Ð½ÑÑ Ð¼ÑÑÐ¸Ð½ÑÑ ÑÐ¸Ð±ÑÐ¾Ð±Ð»Ð°ÑÑÐ¾Ð² 3Ð¢3 Ð¸ Ð¸Ñ in vitro ÑÑÐ°Ð½ÑÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð½ÑÑ Ð°Ð½Ð°Ð»Ð¾Ð³Ð¾Ð² 3Ð¢3-SV40 Ñ ÑÐ°ÐºÑÐ»ÑÑÐ°ÑÐ¸Ð²Ð½ÑÐ¼ Ð¿Ð°ÑÐ¾Ð³ÐµÐ½Ð¾Ð¼ Serratia grimesii Ð¿ÑÐ¸ Ð¸Ñ ÑÐ¾Ð²Ð¼ÐµÑÑÐ½Ð¾Ð¹ Ð¸Ð½ÐºÑÐ±Ð°ÑÐ¸Ð¸ Ð² ÑÑÐ°Ð½Ð´Ð°ÑÑÐ½Ð¾Ð¹ ÑÑÐµÐ´Ðµ Ð¸ ÑÑÐµÐ´Ðµ, ÑÐ¾Ð´ÐµÑÐ¶Ð°ÑÐµÐ¹ 20 Ð¼Ð N-Ð°ÑÐµÑÐ¸Ð»ÑÐ¸ÑÑÐµÐ¸Ð½Ð°. Ð§ÑÐ²ÑÑÐ²Ð¸ÑÐµÐ»ÑÐ½Ð¾ÑÑÑ ÐºÐ»ÐµÑÐ¾Ðº 3Ð¢3 Ðº Ð¸Ð½Ð²Ð°Ð·Ð¸Ð¸ S.grimesii Ð¾ÐºÐ°Ð·Ð°Ð»Ð°ÑÑ Ð² Ð´Ð²Ð° ÑÐ°Ð·Ð° Ð¼ÐµÐ½ÑÑÐµ, ÑÐµÐ¼ ÑÑÐ²ÑÑÐ²Ð¸ÑÐµÐ»ÑÐ½Ð¾ÑÑÑ ÑÑÐ°Ð½ÑÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð½ÑÑ ÐºÐ»ÐµÑÐ¾Ðº 3Ð¢3 SV40 Ðº Ð¸Ð½Ð²Ð°Ð·Ð¸Ð¸Ð¸ S.grimesii. ÐÐ½ÐºÑÐ±Ð°ÑÐ¸Ñ ÐºÐ»ÐµÑÐ¾Ðº 3Ð¢3 Ð¸ 3Ð¢3 SV40 Ð² ÑÐ°ÑÑÐ²Ð¾ÑÐµ Ñ 20 Ð¼Ð N-Ð°ÑÐµÑÐ¸Ð»ÑÐ¸ÑÑÐµÐ¸Ð½Ð° ÑÐ²ÐµÐ»Ð¸ÑÐ¸Ð²Ð°Ð»Ð° ÑÑÐ²ÑÑÐ²Ð¸ÑÐµÐ»ÑÐ½Ð¾ÑÑÑ ÐºÐ»ÐµÑÐ¾Ðº Ðº Ð¸Ð½Ð²Ð°Ð·Ð¸Ð¸ Ð² Ð´Ð²Ð° ÑÐ°Ð·Ð°. ÐÑÐ¸ ÑÐµÑ Ð¶Ðµ ÑÑÐ»Ð¾Ð²Ð¸ÑÑ Ð¸Ð½Ð²Ð°Ð·Ð¸Ñ S.grimesii Ð² ÐºÐ»ÐµÑÐºÐ¸ 3Ð¢3 SV40 ÑÐ²ÐµÐ»Ð¸ÑÐ¸Ð»Ð°ÑÑ Ð² 2.1 ÑÐ°Ð·. Ð­ÑÐ¸ Ð´Ð°Ð½Ð½ÑÐµ Ð¿Ð¾ÐºÐ°Ð·ÑÐ²Ð°ÑÑ, ÑÑÐ¾ ÐºÐ»ÐµÑÐºÐ¸ 3Ð¢3 Ð±Ð¾Ð»ÐµÐµ ÑÐµÐ·Ð¸ÑÑÐµÐ½ÑÐ½Ñ Ðº Ð¸Ð½Ð²Ð°Ð·Ð¸Ð¸ S.grimesii, Ð¿Ð¾ ÑÑÐ°Ð²Ð½ÐµÐ½Ð¸Ñ Ñ ÐºÐ»ÐµÑÐºÐ°Ð¼Ð¸ 3Ð¢3 SV40. Ð¡ÑÐµÐ´Ð¸ Ð²ÑÐµÑ Ð³ÐµÐ½Ð¾Ð², ÑÑÑ ÑÐºÑÐ¿ÑÐµÑÑÐ¸Ñ ÑÐ²ÐµÐ»Ð¸ÑÐ¸Ð²Ð°ÐµÑÑÑ Ð¿Ð¾Ð´ Ð²Ð»Ð¸ÑÐ½Ð¸ÐµÐ¼ NAC, Ð²ÑÐ´ÐµÐ»ÑÐµÑÑÑ Ð-ÐºÐ°Ð´Ð³ÐµÑÐ¸Ð½, ÐºÐ¾ÑÐ¾ÑÑÐ¹ Ð¸Ð³ÑÐ°ÐµÑ Ð¾ÑÐ¾Ð±ÑÑ ÑÐ¾Ð»Ñ Ð¿ÑÐ¸ Ð²Ð·Ð°Ð¸Ð¼Ð¾Ð´ÐµÐ¹ÑÑÐ²Ð¸Ð¸ Ñ Ð¿Ð¾Ð²ÐµÑÑÐ½Ð¾ÑÑÐ½ÑÐ¼Ð¸ Ð±ÐµÐ»ÐºÐ°Ð¼Ð¸ (Ð¸Ð½Ð²Ð°Ð·Ð¸Ð½Ð°Ð¼Ð¸) Ð¿Ð°ÑÐ¾Ð³ÐµÐ½Ð½ÑÑ Ð±Ð°ÐºÑÐµÑÐ¸Ð¹. ÐÐ½ÐºÑÐ±Ð°ÑÐ¸Ñ ÐºÐ»ÐµÑÐ¾Ðº 3Ð¢3 Ð¸ 3Ð¢3 SV40 Ñ NAC Ð¿ÑÐ¸Ð²ÐµÐ»Ð° Ðº ÑÐ²ÐµÐ»Ð¸ÑÐµÐ½Ð¸Ñ ÑÐºÑÐ¿ÑÐµÑÑÐ¸Ð¸ Ð-ÐºÐ°Ð´Ð³ÐµÑÐ¸Ð½Ð°, ÐºÐ¾ÑÐ¾ÑÐ°Ñ ÐºÐ¾ÑÑÐµÐ»Ð¸ÑÑÐµÑ Ñ ÑÐ²ÐµÐ»Ð¸ÑÐµÐ½Ð½Ð¾Ð¹ ÑÑÐ²ÑÑÐ²Ð¸ÑÐµÐ»ÑÐ½Ð¾ÑÑÑÑ ÑÑÐ¸Ñ ÐºÐ»ÐµÑÐ¾Ðº Ðº Ð¸Ð½Ð²Ð°Ð·Ð¸Ð¸. ÐÑÐ¸ Ð¿Ð¾Ð¼Ð¾ÑÐ¸ Ð¼ÐµÑÐ¾Ð´Ð° ÐºÐ¾Ð½ÑÐ¾ÐºÐ°Ð»ÑÐ½Ð¾Ð¹ Ð¼Ð¸ÐºÑÐ¾ÑÐºÐ¾Ð¿Ð¸Ð¸ Ð¿Ð¾ÐºÐ°Ð·Ð°Ð½Ð° ÐºÐ¾Ð»Ð¾ÐºÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ñ S.grimesii Ð¸ Ð-ÐºÐ°Ð´Ð³ÐµÑÐ¸Ð½Ð° ÐºÐ»ÐµÑÐ¾Ðº 3Ð¢3 Ð¸ 3Ð¢3 SV40, ÑÐºÐ°Ð·ÑÐ²Ð°Ñ Ð½Ð° ÑÐ¾, ÑÑÐ¾ Ð-ÐºÐ°Ð´Ð³ÐµÑÐ¸Ð½ Ð²Ð¾Ð²Ð»ÐµÑÐµÐ½ Ð² Ð¸Ð½ÑÐµÑÐ½Ð°Ð»Ð¸Ð·Ð°ÑÐ¸Ñ S.grimesii Ð²Ð½ÑÑÑÑ ÑÑÐºÐ°ÑÐ¸Ð¾ÑÐ¸ÑÐµÑÐºÐ¸Ñ ÐºÐ»ÐµÑÐ¾Ðº.
Probing the Galactic Potential with Next-Generation Observations of Disk Stars
Creators: name: Sumi, T.
name: Johnston, K. V.
name: Tremaine, S.
name: Spergel, D. N.
name: Majewski, S. R.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Near-future surveys promise a dramatic improvement in the number and precision of astrometric, photometric and spectroscopic measurements of stars in the Milky Way's disk. We examine the impact of such surveys on our understanding of the Galaxy by "observing" particle realizations of non-axisymmetric disk distributions orbiting in an axisymmetric halo with appropriate errors and then attempting to recover the underlying potential using a Markov Chain Monte Carlo (MCMC) approach. We demonstrate that the azimuthally averaged gravitational force field in the Galactic plane--and hence, to a lesser extent, the Galactic mass distribution--can be tightly constrained over a large range of radii using a variety of types of surveys so long as the error distribution of the measurements of the parallax, proper motion and radial velocity are well-understood and the disk is surveyed globally. One advantage of our method is that the target stars can be selected non-randomly in real or apparent-magnitude space to ensure just such a global sample without biasing the results. Assuming we can always measure the line-of-sight velocity of a star with at least 1 km/s precision, we demonstrate that the force field can be determined to better than ~1% for Galactocentric radii in the range R=4-20 kpc We conclude that near-future surveys, like SIM Lite, Gaia, and VERA, will provide the first precise mapping of the gravitational force field in the region of the Galactic disk.
description: 41 pages and 10 figures, accepted for publication in ApJ
A Stellar Model-fitting Pipeline for Solar-like Oscillations
Creators: name: Metcalfe, T. S.
name: Creevey, O. L.
name: Christensen-Dalsgaard, J.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Over the past two decades, helioseismology has revolutionized our understanding of the interior structure and dynamics of the Sun. Asteroseismology will soon place this knowledge into a broader context by providing structural data for hundreds of Sun-like stars. Solar-like oscillations have already been detected from the ground in several stars, and NASA's Kepler mission is poised to unleash a flood of stellar pulsation data. Deriving reliable asteroseismic information from these observations demands a significant improvement in our analysis methods. We report the initial results of our efforts to develop an objective stellar model-fitting pipeline for asteroseismic data. The cornerstone of our automated approach is an optimization method using a parallel genetic algorithm. We describe the details of the pipeline and we present the initial application to Sun-as-a-star data, yielding an optimal model that accurately reproduces the known solar properties.
description: 5 pages, 2 figs, Stellar Pulsation: Challenges for Theory and Observation (proceedings to be published by AIP)
Constraining dust and color variations of high-z SNe using NICMOS on Hubble Space Telescope
Creators: name: Nobili, S.
name: Fadeyev, V.
name: Aldering, G.
name: Amanullah, R.
name: Barbary, K.
name: Burns, M. S.
name: Dawson, K. S.
name: Deustua, S. E.
name: Faccioli, L.
name: Fruchter, A. S.
name: Goldhaber, G.
name: Goobar, A.
name: Hook, I.
name: Howell, D. A.
name: Kim, A. G.
name: Knop, R. A.
name: Lidman, C.
name: Meyers, J.
name: Nugent, P. E.
name: Pain, R.
name: Panagia, N.
name: Perlmutter, S.
name: Rubin, D.
name: Spadafora, A. L.
name: Strovink, M.
name: Suzuki, N.
name: Swift, H.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We present data from the Supernova Cosmology Project for five high redshift Type Ia supernovae (SNe Ia) that were obtained using the NICMOS infrared camera on the Hubble Space Telescope. We add two SNe from this sample to a rest-frame I-band Hubble diagram, doubling the number of high redshift supernovae on this diagram. This I-band Hubble diagram is consistent with a flat universe (Omega_Matter, Omega_Lambda= 0.29, 0.71). A homogeneous distribution of large grain dust in the intergalactic medium (replenishing dust) is incompatible with the data and is excluded at the 5 sigma confidence level, if the SN host galaxy reddening is corrected assuming R_V=1.75. We use both optical and infrared observations to compare photometric properties of distant SNe Ia with those of nearby objects. We find generally good agreement with the expected color evolution for all SNe except the highest redshift SN in our sample (SN 1997ek at z=0.863) which shows a peculiar color behavior. We also present spectra obtained from ground based telescopes for type identification and determination of redshift.
description: 30 pages, 10 figures; accepted for publication in ApJ; v2: revised to match the version in the journal
Neutrinoless Double Beta Decay from Lattice QCD: The Short-Distance $π^-\rightarrowπ^+ e^- e^-$ Amplitude
Creators: name: Detmold, William
name: Jay, William I.
name: Murphy, David J.
name: Oare, Patrick R.
name: Shanahan, Phiala E.
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Physics - Lattice (hep-lat)
subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: This work presents a determination of potential short-distance contributions to the unphysical $π^-\rightarrowπ^+ e^- e^-$ decay through lattice QCD calculations. The hadronic contributions to the transition amplitude are described by the pion matrix elements of five Standard Model Effective Field Theory operators, which are computed on five ensembles of domain-wall fermions with $N_f = 2 + 1$ quark flavors with a range of heavier-than-physical values of the light quark masses. The matrix elements are extrapolated to the continuum, physical light-quark mass, and infinite volume limit using a functional form derived in chiral Effective Field Theory ($χ\mathrm{EFT}$). This extrapolation also yields the relevant low-energy constants of $χ\mathrm{EFT}$, which are necessary input for $χ\mathrm{EFT}$ calculations of neutrinoless double beta decay of nuclei.
description: 24 pages, 17 figures
First passage time distribution of active thermal particles in potentials
Creators: name: Walter, Benjamin
name: Pruessner, Gunnar
name: Salbreux, Guillaume
Publisher: name: The Francis Crick Institute
Year: 2021
Subjects: Structural Biology & Biophysics
Computational & Systems Biology

description: We introduce a perturbative method to calculate all moments of the first passage time distribution in stochastic one-dimensional processes which are subject to both white and colored noise. This class of non-Markovian processes is at the center of the study of thermal active matter, that is self-propelled particles subject to diffusion. The perturbation theory about the Markov process considers the effect of self-propulsion to be small compared to that of thermal fluctuations. To illustrate our method, we apply it to the case of active thermal particles (i) in a harmonic trap and (ii) on a ring. For both we calculate the first-order correction of the moment-generating function of first passage times, and thus to all its moments. Our analytical results are compared to numerics.
title: Ð¡Ð¸Ð½ÑÐµÐ· Ð¿Ð»Ð¾ÑÐºÐ¸Ñ ÐºÑÐ»Ð°ÑÐºÐ¾Ð²ÑÑ Ð¼ÐµÑ Ð°Ð½Ð¸Ð·Ð¼Ð¾Ð²
title: Ð¼ÐµÑÐ¾Ð´Ð¸ÑÐµÑÐºÐ¸Ðµ ÑÐºÐ°Ð·Ð°Ð½Ð¸Ñ Ðº ÑÐ°ÑÑÐµÑÐ½Ð¾Ð¼Ñ Ð·Ð°Ð´Ð°Ð½Ð¸Ñ
titleType: Subtitle
Creators: name: ÐÐµÐ»ÑÐµÐ², ÐÐ»ÐµÐ³
Publisher: name: ÐÐÐ Ð¸Ð¼ÐµÐ½Ð¸ Ð. Ð. ÐÐ°Ð»Ð¸Ð½Ð¸Ð½Ð°
Year: 1983
Subjects: ÐÑÐ»Ð°ÑÐºÐ¾Ð²ÑÐµ Ð¼ÐµÑ Ð°Ð½Ð¸Ð·Ð¼Ñ

description: ÐÐµÑÐ¾Ð´Ð¸ÑÐµÑÐºÐ¸Ðµ ÑÐºÐ°Ð·Ð°Ð½Ð¸Ñ Ð¿ÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ñ ÑÑÑÐ´ÐµÐ½ÑÐ°Ð¼ Ð¼ÐµÑÐ°Ð½Ð¸ÑÐµÑÐºÐ¸Ñ ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾ÑÑÐµÐ¹ Ð¿ÑÐ¸ Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¸Ð¸ Ð¸Ð¼Ð¸ ÑÐ°ÑÑÐµÑÐ½Ð¾-Ð³ÑÐ°ÑÐ¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð·Ð°Ð´Ð°Ð½Ð¸Ñ Ð¿Ð¾ Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÐºÑÐ»Ð°ÑÐºÐ¾Ð²Ð¾Ð³Ð¾ Ð¼ÐµÑÐ°Ð½Ð¸Ð·Ð¼Ð° Ð² ÐºÑÑÑÐµ ÑÐµÐ¾ÑÐ¸Ð¸ Ð¼ÐµÑÐ°Ð½Ð¸Ð·Ð¼Ð¾Ð² Ð¸ Ð¼Ð°ÑÐ¸Ð½. Ð¦ÐµÐ»Ñ Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¸Ñ Ð·Ð°Ð´Ð°Ð½Ð¸Ñ Ð·Ð°ÐºÐ»ÑÑÐ°ÐµÑÑÑ Ð² Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ¾Ð¼ Ð¾Ð²Ð»Ð°Ð´ÐµÐ½Ð¸Ð¸ ÑÑÑÐ´ÐµÐ½ÑÐ°Ð¼Ð¸ Ð·Ð½Ð°Ð½Ð¸ÑÐ¼Ð¸ Ð¸ Ð½Ð°Ð²ÑÐºÐ°Ð¼Ð¸ ÑÐ°ÑÑÐµÑÐ°, Ð½ÐµÐ¾Ð±ÑÐ¾Ð´Ð¸Ð¼ÑÐ¼Ð¸ Ð¿ÑÐ¸ Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ð¸ Ð¿Ð»Ð¾ÑÐºÐ¸Ñ ÐºÑÐ»Ð°ÑÐºÐ¾Ð²ÑÑ Ð¼ÐµÑÐ°Ð½Ð¸Ð·Ð¼Ð¾Ð². Ð£ÐºÐ°Ð·Ð°Ð½Ð¸Ñ ÑÐ¾Ð´ÐµÑÐ¶Ð°Ñ Ð¿ÑÐµÐ¸Ð¼ÑÑÐµÑÑÐ²ÐµÐ½Ð½Ð¾ Ð°Ð½Ð°Ð»Ð¸ÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð¼ÐµÑÐ¾Ð´Ñ ÑÐ°ÑÑÐµÑÐ¾Ð². ÐÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ñ Ð² ÑÐ¾ÐºÑÐ°ÑÐµÐ½Ð½Ð¾Ð¼ Ð²Ð¸Ð´Ðµ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ ÑÑÐ°Ð¿Ñ ÑÐ¸Ð½ÑÐµÐ·Ð° Ð´Ð»Ñ ÑÑÐµÑ Ð½Ð°Ð¸Ð±Ð¾Ð»ÐµÐµ ÑÐ°ÑÐ¿ÑÐ¾ÑÑÑÐ°Ð½ÐµÐ½Ð½ÑÑ ÑÑÐµÐ¼ Ð¿Ð»Ð¾ÑÐºÐ¸Ñ ÐºÑÐ»Ð°ÑÐºÐ¾Ð²ÑÑ Ð¼ÐµÑÐ°Ð½Ð¸Ð·Ð¼Ð¾Ð² Ñ ÑÐ¾Ð¾ÑÐ²ÐµÑÑÑÐ²ÑÑÑÐ¸Ð¼Ð¸ Ð¿ÑÐ¸Ð¼ÐµÑÐ°Ð¼Ð¸ ÑÐ°ÑÑÐµÑÐ°. ÐÑÐ¸Ð²ÐµÐ´ÐµÐ½Ð° Ð¾Ð±ÑÐ°Ñ Ð¼ÐµÑÐ¾Ð´Ð¸ÐºÐ° Ð¿ÑÐ¾ÑÐ¸Ð»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÐºÑÐ»Ð°ÑÐºÐ° Ð¸ Ð¿Ð¾Ð»ÑÑÐµÐ½Ñ Ð·Ð°Ð²Ð¸ÑÐ¸Ð¼Ð¾ÑÑÐ¸, Ð¿Ð¾Ð·Ð²Ð¾Ð»ÑÑÑÐ¸Ðµ Ð²ÑÐ¿Ð¾Ð»Ð½ÑÑÑ ÑÐ°ÑÑÐµÑÑ Ñ Ð¿Ð¾Ð¼Ð¾ÑÑÑ ÐºÐ°Ð»ÑÐºÑÐ»ÑÑÐ¾ÑÐ° Ð¸Ð»Ð¸ Ð­Ð¨. ÐÐµÑÐ¾Ð´Ð¸ÑÐµÑÐºÐ¸Ðµ ÑÐºÐ°Ð·Ð°Ð½Ð¸Ñ ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð¾Ð²Ð°Ð½Ñ Ðº Ð¸Ð·Ð´Ð°Ð½Ð¸Ñ Ð¼ÐµÑÐ¾Ð´Ð¸ÑÐµÑÐºÐ¾Ð¹ ÐºÐ¾Ð¼Ð¸ÑÑÐ¸ÐµÐ¹ Ð¼ÐµÑÐ°Ð½Ð¸ÐºÐ¾-Ð¼Ð°ÑÐ¸Ð½Ð¾ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÐ½Ð¾Ð³Ð¾ Ð¤Ð°ÐºÑÐ»ÑÑÐµÑÐ° ÐÐÐ Ð¸Ð¼ÐµÐ½Ð¸ Ð. Ð. ÐÐ°Ð»Ð¸Ð½Ð¸Ð½Ð°.
Fast Online Adaptive Enrichment for Poroelasticity with High Contrast
Creators: name: Su, Xin
name: Pun, Sai-Mang
Publisher: name: arXiv
Year: 2022
Subjects: subject: Numerical Analysis (math.NA)
subject: FOS: Mathematics
subject: 65N30

description: In this work, we develop an online adaptive enrichment method within the framework of the Constraint Energy Minimizing Generalized Multiscale Finite Element Method (CEM-GMsFEM) for solving the linear heterogeneous poroelasticity models with coefficients of high contrast. The proposed method makes use of information of residual-driven error indicators to enrich the multiscale spaces for both the displacement and the pressure variables in the model. Additional online basis functions are constructed in oversampled regions accordingly and are adaptively chosen to reduce the error the most. A complete theoretical analysis of the online enrichment algorithm is provided and justified by thorough numerical experiments.
description: 29 pages, 10 figures, 9 tables. Second round revision of Journal of Computational Physics
Inferring equilibrium transition rates from nonequilibrium protocols
Creators: name: Kuznets-Speck, Benjamin
name: Limmer, David T
Publisher: name: arXiv
Year: 2022
Subjects: subject: Chemical Physics (physics.chem-ph)
subject: Statistical Mechanics (cond-mat.stat-mech)
subject: Biological Physics (physics.bio-ph)
subject: FOS: Physical sciences

description: We develop a theory for inferring equilibrium transition rates from trajectories driven by a time dependent force using results from stochastic thermodynamics. Applying the Kawasaki relation to approximate the nonequilibrium distribution function in terms of the equilibrium distribution function and the excess dissipation, we formulate a nonequilibrium transition state theory to estimate the rate enhancement over the equilibrium rate due to the nonequilibrium protocol. We demonstrate the utility of our theory in examples of pulling of harmonically trapped particles in 1 and 2 dimensions, as well as a semi-flexible polymer with a reactive linker in 3 dimensions. In all cases we find that we are able to infer the transition rates more effectively than phenomenological approaches based on Bell's law. We expect our thermodynamic approach will find use in both molecular simulation and force spectroscopy experiments.
description: 4 pages, 3 figures, comments welcome
Non-Standard Neutrino Self-Interactions Can Cause Neutrino Flavor Equipartition Inside the Supernova Core
Creators: name: Abbar, Sajad
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We show that non-standard neutrino self-interactions can lead to total flavor equipartition in a dense neutrino gas, such as those expected in core-collapse supernovae. In this first investigation of this phenomenon in the multi-angle scenario, we demonstrate that such a flavor equipartition can occur on very short scales, and therefore very deep inside the newly formed proto-neutron star, with a possible significant impact on the physics of core-collapse supernovae. Our findings imply that future galactic core-collapse supernovae can appreciably probe non-standard neutrino self-interactions, for certain cases even when they are many orders of magnitude smaller than the Standard Model terms.
description: 7 pages, 4 figuers
A note on the second moment of automorphic L-functions
Creators: name: Bui, H. M.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Number Theory (math.NT)
subject: FOS: Mathematics

description: We obtain the formula for the twisted harmonic second moment of the $L$-functions associated with primitive Hecke eigenforms of weight 2. A consequence of our mean value theorem is reminiscent of recent results of Conrey and Young on the reciprocity formula for the twisted second moment of Dirichlet $L$-functions.
description: 9 pages
title: Ð¡Ð±Ð¾ÑÐ½Ð¸Ðº Ð·Ð°Ð´Ð°Ð½Ð¸Ð¹ Ð´Ð»Ñ Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ¸Ñ Ð·Ð°Ð½ÑÑÐ¸Ð¹ Ð¸ ÑÐ°Ð¼Ð¾ÑÑÐ¾ÑÑÐµÐ»ÑÐ½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ Ð¿Ð¾ ÐºÑÑÑÑ "Ð£Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ ÑÐµÑÑÑÑÐ½ÑÐ¼ Ð¿Ð¾ÑÐµÐ½ÑÐ¸Ð°Ð»Ð¾Ð¼ Ð² ÑÑÐµÑÐµ ÑÐ¾ÑÐ³Ð¾Ð²Ð»Ð¸ Ð¸ Ð¾Ð±ÑÐµÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¿Ð¸ÑÐ°Ð½Ð¸Ñ"
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ
titleType: Subtitle
Creators: name: ÐÐ»ÑÐ¸Ð½Ð°, ÐÐ»ÑÐ³Ð°
name: Ð¡Ð¾Ð»Ð¾Ð¼Ð°ÑÐ¸Ð½, ÐÐ»ÐµÐºÑÐ°Ð½Ð´Ñ
Publisher: name: Ð¡ÐÐ±Ð¢Ð­Ð
Year: 2011
Subjects: Ð¾Ð±ÑÐµÑÑÐ²ÐµÐ½Ð½Ð¾Ðµ Ð¿Ð¸ÑÐ°Ð½Ð¸Ðµ
ÑÐ¾ÑÐ³Ð¾Ð²Ð»Ñ
ÑÑÐµÐ±Ð½Ð¸ÐºÐ¸ Ð¸ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ñ Ð´Ð»Ñ Ð²ÑÐ·Ð¾Ð²

description: Ð ÑÑÐµÐ±Ð½Ð¾Ð¼ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ð¸ ÑÐ°ÑÐºÑÑÐ²Ð°ÑÑÑÑ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ ÑÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð¿Ð¾Ð½ÑÑÐ¸Ñ Ð¿Ð¾ Ð¾ÑÐµÐ½ÐºÐµ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¸ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ ÑÐµÑÑÑÑÐ½ÑÐ¼ Ð¿Ð¾ÑÐµÐ½ÑÐ¸Ð°Ð»Ð¾Ð¼ ÑÐ¾ÑÐ³Ð¾Ð²Ð¾Ð³Ð¾ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ, Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ñ ÑÐ¾Ð·ÑÐ¹ÑÑÐ²ÐµÐ½Ð½ÑÐµ ÑÐ¸ÑÑÐ°ÑÐ¸Ð¸ Ð´Ð»Ñ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¸Ñ Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ¸Ñ Ð·Ð°Ð½ÑÑÐ¸Ð¹, Ð° ÑÐ°ÐºÐ¶Ðµ Ð¸Ð½Ð´Ð¸Ð²Ð¸Ð´ÑÐ°Ð»ÑÐ½ÑÐµ Ð·Ð°Ð´Ð°Ð½Ð¸Ñ Ð´Ð»Ñ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸ ÑÐ°Ð¼Ð¾ÑÑÐ¾ÑÑÐµÐ»ÑÐ½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ Ð¼Ð°Ð³Ð¸ÑÑÑÐ°Ð½ÑÐ¾Ð². ÐÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¾ Ð´Ð»Ñ Ð¼Ð°Ð³Ð¸ÑÑÑÐ¾Ð², Ð¾Ð±ÑÑÐ°ÑÑÐ¸ÑÑÑ Ð¿Ð¾ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸ÑÐ¼ Â«Ð¢Ð¾ÑÐ³Ð¾Ð²Ð¾Ðµ Ð´ÐµÐ»Ð¾Â» Ð¸ Â«Ð­ÐºÐ¾Ð½Ð¾Ð¼Ð¸ÐºÐ°Â».
XMM-Newton observations of PSR J0554+3107: pulsing thermal emission from a cooling high-mass neutron star
Creators: name: Tanashkin, A. S.
name: Karpova, A. V.
name: Potekhin, A. Y.
name: Shibanov, Y. A.
name: Zyuzin, D. A.
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: XMM-Newton observations of the middle-aged radio-quiet $γ$-ray pulsar J0554+3107 allowed us, for the first time, firmly identify it in X-rays by detection of pulsations with the pulsar period. In the 0.2-2 keV band, the pulse profile shows two peaks separated by about a half of the rotation phase with the pulsed fraction of $25 \pm 6$ per cent. The profile and spectrum in this band can be mainly described by thermal emission from the neutron star with the hydrogen atmosphere, dipole magnetic field of $\sim 10^{13}$ G and non-uniform surface temperature. Non-thermal emission from the pulsar magnetosphere is marginally detected at higher photon energies. The spectral fit with the atmosphere+power law model implies that J0554+3107 is a rather heavy and cool neutron star with the mass of 1.6-2.1 $M_\odot$, the radius of $\approx 13$ km and the redshifted effective temperature of $\approx 50$ eV. The spectrum shows an absorption line of unknown nature at $\approx 350$ eV. Given the extinction-distance relation, the pulsar is located at $\approx 2$ kpc and has the redshifted bolometric thermal luminosity of $\approx 2 \times 10^{32}$ erg s$^{-1}$. We discuss cooling scenarios for J0554+3107 considering plausible equations of state of super-dense matter inside the star, different compositions of the heat-blanketing envelope and various ages.
description: 13 pages, 13 figures. Accepted for publication in MNRAS
X-ray Variations at the Orbital Period from Cygnus X-1 in the High/Soft State
Creators: name: Boroson, Bram
name: Vrtilek, Saeqa Dil
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: Orbital variability has been found in the X-ray hardness of the black hole candidate Cygnus X-1 during the soft/high X-ray state using light curves provided by the Rossi X-ray Timing Explorer's All Sky Monitor. We are able to set broad limits on how the mass-loss rate and X-ray luminosity vary between the hard and soft states. The folded light curve shows diminished flux in the soft X-ray band at phase 0 (defined as the time of of the superior conjunction of the X-ray source). Models of the orbital variability provide slightly superior fits when the absorbing gas is concentrated in neutral clumps and better explain the strong variability in hardness. In combination with the previously established hard/low state dips, our observations give a lower limit to the mass loss rate in the soft state (Mdot<2x10^{-6} Msun/yr) than the limit in the hard state (Mdot<4x10^{-6} Msun/yr). Without a change in the wind structure between X-ray states, the greater mass-loss rate during the low/hard state would be inconsistent with the increased flaring seen during the high-soft state.
description: Accepted for publication in The Astrophysical Journal
Transformation of the Poynting flux into the kinetic energy in relativistic jets
Creators: name: Lyubarsky, Y. E.
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: The acceleration of relativistic jets from the Poynting to the matter dominated stage is considered. The are generally two collimation regimes, which we call equilibrium and non-equilibrium, correspondingly. In the first regime, the jet is efficiently accelerated till the equipartition between the kinetic and electro-magnetic energy. We show that after the equilibrium jet ceases to be Poynting dominated, the ratio of the electro-magnetic to the kinetic energy decreases only logarithmically so that such jets become truly matter dominated only at extremely large distances. Non-equilibrium jets remain generally Poynting dominated till the logarithmically large distances. In the only case when a non-equilibrium jet is accelerated till the equipartition level, we found that the flow is not continued to the infinity but is focused towards the axis at a finite distance from the origin.
description: Submitted to MNRAS Minor changes in the Conclusions
title: Ð¢ÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ð¹ Ð¿ÑÐ¾ÑÐµÑÑ Ð¼ÐµÑ Ð°Ð½Ð¸ÑÐµÑÐºÐ¾Ð¹ Ð¾Ð±ÑÐ°Ð±Ð¾ÑÐºÐ¸ Ð´ÐµÑÐ°Ð»Ð¸ "ÐÐ¾ÑÐ¿ÑÑ"
title: Ð´Ð¸Ð¿Ð»Ð¾Ð¼Ð½ÑÐ¹ Ð¿ÑÐ¾ÐµÐºÑ
titleType: Subtitle
Creators: name: ÐÑÐºÐ¸Ð½, ÐÐ¸ÐºÑÐ¾Ñ
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ÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ð¹ Ð¿ÑÐ¾ÑÐµÑÑ
Ð¼ÐµÑ Ð°Ð½Ð¸ÑÐµÑÐºÐ°Ñ Ð¾Ð±ÑÐ°Ð±Ð¾ÑÐºÐ°
ÑÐ¾ÐºÐ°ÑÐ½ÑÐ¹ ÑÑÐ°Ð½Ð¾Ðº
technological process
machining
lathe machine

description: Ð¢ÐµÐ¼Ð¾Ð¹ Ð´Ð°Ð½Ð½Ð¾Ð³Ð¾ Ð´Ð¸Ð¿Ð»Ð¾Ð¼Ð½Ð¾Ð³Ð¾ Ð¿ÑÐ¾ÐµÐºÑÐ° ÑÐ²Ð»ÑÐµÑÑÑ Â«Ð¢ÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ð¹ Ð¿ÑÐ¾ÑÐµÑÑ Ð¼ÐµÑÐ°Ð½Ð¸ÑÐµÑÐºÐ¾Ð¹ Ð¾Ð±ÑÐ°Ð±Ð¾ÑÐºÐ¸ Ð´ÐµÑÐ°Ð»Ð¸ ÐÐ¾ÑÐ¿ÑÑÂ». Ð¢ÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ°Ñ ÑÐ°ÑÑÑ Ð´Ð°Ð½Ð½Ð¾Ð³Ð¾ Ð´Ð¸Ð¿Ð»Ð¾Ð¼Ð½Ð¾Ð³Ð¾ Ð¿ÑÐ¾ÐµÐºÑÐ° Ð·Ð°ÐºÐ»ÑÑÐ°ÐµÑÑÑ Ð² ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐµ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¿ÑÐ¾ÑÐµÑÑÐ° Ð¸Ð·Ð³Ð¾ÑÐ¾Ð²Ð»ÐµÐ½Ð¸Ñ ÐºÐ¾ÑÐ¿ÑÑÐ°. Ð ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¾ÑÑÐºÐ¾Ð¹ ÑÐ°ÑÑÐ¸ Ð±ÑÐ»Ð¾ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ð¾ ÑÑÑÐ°Ð½Ð¾Ð²Ð¾ÑÐ½Ð¾Ðµ Ð¿ÑÐ¸ÑÐ¿Ð¾ÑÐ¾Ð±Ð»ÐµÐ½Ð¸Ðµ Ð¸ ÐºÐ¾Ð½ÑÑÐ¾Ð»ÑÐ½Ð¾-Ð¸Ð·Ð¼ÐµÑÐ¸ÑÐµÐ»ÑÐ½Ð¾Ðµ Ð¿ÑÐ¸ÑÐ¿Ð¾ÑÐ¾Ð±Ð»ÐµÐ½Ð¸Ðµ. Ð­ÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ°Ñ ÑÐ°ÑÑÑ Ð·Ð°ÐºÐ»ÑÑÐ°Ð»Ð°ÑÑ Ð² Ð¿ÑÐ¾ÑÐ°Ð±Ð¾ÑÐºÐµ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¸Ñ Ð¸ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾-Ð¿Ð»Ð°Ð½Ð¾Ð²ÑÑ Ð²Ð¾Ð¿ÑÐ¾ÑÐ¾Ð² Ð¿ÑÐ¾ÐµÐºÑÐ°. Ð ÑÐ°ÑÑÐ¸ Ð¿Ð¾ Ð±ÐµÐ·Ð¾Ð¿Ð°ÑÐ½Ð¾ÑÑÐ¸ Ð¶Ð¸Ð·Ð½ÐµÐ´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð±ÑÐ» Ð´Ð°Ð½ Ð°Ð½Ð°Ð»Ð¸Ð· Ð²Ð¾Ð·Ð¼Ð¾Ð¶Ð½ÑÑ Ð¾Ð¿Ð°ÑÐ½ÑÑ Ð¸ Ð²ÑÐµÐ´Ð½ÑÑ ÑÐ°ÐºÑÐ¾ÑÐ¾Ð², Ð²Ð¾Ð·Ð½Ð¸ÐºÐ°ÑÑÐ¸Ñ Ð¿ÑÐ¸ ÑÐºÑÐ¿Ð»ÑÐ°ÑÐ°ÑÐ¸Ð¸ Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÑÐµÐ¼Ð¾Ð³Ð¾ Ð¾Ð±ÑÐµÐºÑÐ°, Ð¸ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ñ Ð¼ÐµÑÑ Ð·Ð°ÑÐ¸ÑÑ ÑÐ°Ð±Ð¾ÑÐ°ÑÑÐ¸Ñ.
description: The theme of this diploma project is "technological process of machining parts Housing". The technological part of the diploma project is to develop the technological process of construction of the body. The design of the setting device was designed and test and measurement device.The economic part was exploring the economic, organizational and planning issues of the project.As part of the safety of life was given to the analysis of potentially dangerous and harmful factors arising from the operation of the proposed facility and measures designed to protect workers.
Non-degenerate solutions of universal Whitham hierarchy
Creators: name: Takasaki, Kanehisa
name: Takebe, Takashi
name: Teo, Lee Peng
Publisher: name: arXiv
Year: 2010
Subjects: subject: Mathematical Physics (math-ph)
subject: High Energy Physics - Theory (hep-th)
subject: Exactly Solvable and Integrable Systems (nlin.SI)
subject: FOS: Physical sciences

description: The notion of non-degenerate solutions for the dispersionless Toda hierarchy is generalized to the universal Whitham hierarchy of genus zero with $M+1$ marked points. These solutions are characterized by a Riemann-Hilbert problem (generalized string equations) with respect to two-dimensional canonical transformations, and may be thought of as a kind of general solutions of the hierarchy. The Riemann-Hilbert problem contains $M$ arbitrary functions $H_a(z_0,z_a)$, $a = 1,...,M$, which play the role of generating functions of two-dimensional canonical transformations. The solution of the Riemann-Hilbert problem is described by period maps on the space of $(M+1)$-tuples $(z_α(p) : α= 0,1,...,M)$ of conformal maps from $M$ disks of the Riemann sphere and their complements to the Riemann sphere. The period maps are defined by an infinite number of contour integrals that generalize the notion of harmonic moments. The $F$-function (free energy) of these solutions is also shown to have a contour integral representation.
description: latex2e, using amsmath, amssym and amsthm packages, 32 pages, no figure
Early results from GLASS-JWST XIV: A first morphological atlas of the 1 < z < 5 Universe in the rest-frame optical
Creators: name: Jacobs, Colin
name: Glazebrook, Karl
name: Calabrò, Antonello
name: Treu, Tommaso
name: Nanayakkara, Themiya
name: Jones, Tucker
name: Merlin, Emiliano
name: Abraham, Roberto G.
name: Stevens, Adam R H
name: Vulcani, Benedetta
name: Yang, Lilan
name: Bonchi, Andrea
name: Bradac, Marusa
name: Castellano, Marco
name: Fontana, Adriano
name: Malkan, Matthew A.
name: Mason, Charlotte A
name: Morishita, Takahiro
name: Paris, Diego
name: Trenti, Michele
name: Marchesini, Danilo
name: Wang, Xin
name: Santini, Paola
Publisher: name: arXiv
Year: 2022
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We present a rest-frame optical morphological analysis of galaxies observed with the NIRCam imager on the James Webb Space Telescope (JWST) as part of the GLASS-JWST Early Release Science program. We select 388 sources at redshifts \(0.8 < z < 5.4\) and use the seven 0.9--5\micron\ NIRCam filters to generate rest-frame $gri$ composite color images, and conduct visual morphological classification. Compared to HST-based work we find a higher incidence of disks and bulges than expected at $z>1.5$, revealed by rest frame optical imaging. We detect 123 clear disks (58 at $z>1.5$) of which 76 have bulges. No evolution of bulge fraction with redshift is evident: 61\% at \(z<2\) (\(N=110\)) versus 60\% at \(z\geq2\) (\(N=13\)). A stellar mass dependence is evident, with bulges visible in 80\% of all disk galaxies with mass \(> 10^{9.5}\, {\rm M}_{\odot}\) (\(N=41\)) but only 52\% at \(M < 10^{9.5}\, {\rm M}_{\odot}\) (\(N=82\)). We supplement visual morphologies with non-parametric measurements of Gini and Asymmetry coefficients in the rest-frame $i$-band. Our sources are more asymmetric than local galaxies, with slightly higher Gini values. When compared to high-z rest-frame ultraviolet measurements with Hubble Space Telescope, JWST shows more regular morphological types such as disks, bulges and spiral arms at $z>1.5$, with smoother (i.e. lower Gini) and more symmetrical light distributions.
description: Accepted for publication in ApJ Letters
title: Electrical pre-conditioning of convective clouds
Creators: name: Gilmore, James
Publisher: name: University of Reading
Year: 2019

description: Lightning presents a substantial hazard. Thunderstorm nowcasting requires a lightning strike to have already occurred, so advance warnings of lightning are currently only possible using numerical weather prediction models. This research aims to identify the processes within cumuliform clouds that can distribute charge prior to the first lightning strike. Precipitation can influence the potential gradient measured at the surface, masking the charge residing within an overhead cloud. An increase in negative charge was measured with increasing rain rate that was dependent on changes in surface conditions such as wind speed and surface dryness, but not cloud type. A field campaign was set up at Chilbolton Observatory by installing a field mill and Biral thunderstorm detector. Surface atmospheric electricity measurements were analysed for 653 cumuliform clouds observed over two years using a 35 GHz radar. Mixed-phase clouds with a high ice phase moisture content produced the largest electrification with increases in the size, density, and turbulence of the hydrometeors all increased cloud electrification, findings consistent with the relative diffusional growth rate theory. Ten radiosondes were flown from Reading University Atmospheric Observatory to provide in-situ measurements of charge (up to 550 pC m-3), cloud backscatter, turbulence (up to 10-1 m2 s-3), and supercooled liquid water (up to 2 g m-3) in cumuliform clouds. These measurements yield consistent findings with those from radar observations. The shallow depth of the charge centres within the cumuliform clouds suggests that the charge was typically insufficiently distributed to allow the required potential gradient enhancement for atmospheric breakdown leading to lightning. This is concluded as the fundamental reason cumuliform clouds in the UK are often charged but rarely produce lightning. This research could be used to improve probabilistic lightning forecasts and nowcasts through improvements to lightning parametrisation schemes in forecast models and the identification of potential thunderstorms using real-time existing surface- and satellite-based radar networks.
title: Ð¯Ð·ÑÐºÐ¾Ð²Ð°Ñ ÑÐµÐ¿ÑÐµÐ·ÐµÐ½ÑÐ°ÑÐ¸Ñ ÐºÐ°ÑÐµÐ³Ð¾ÑÐ¸Ð¸ ÑÐ°ÑÐ¿ÐµÐ½ÑÐ° Ð¸ ÑÐ¿Ð¾ÑÐ¾Ð±Ñ ÐµÐµ Ð¿ÐµÑÐµÐ²Ð¾Ð´Ð° (Ð½Ð° Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ðµ Ð¿ÑÐ¾Ð·Ñ Ð. Ð¤. ÐÐ°Ð²ÐºÑÐ°ÑÑÐ°)
title: Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð¼Ð°Ð³Ð¸ÑÑÑÐ°
titleType: Subtitle
Creators: name: ÐÐ½ÑÐ¾Ð½Ð¾Ð², ÐÐ¸ÑÐ¸Ð»Ð»
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2018
Subjects: ÑÐ°ÑÐ¿ÐµÐ½Ñ
ÑÐµÐ¿ÑÐµÐ·ÐµÐ½ÑÐ°ÑÐ¸Ñ
ÑÑÐ¾Ð²Ð½Ð¸ ÑÐµÐºÑÑÐ°
Ð»Ð¸ÑÐµÑÐ°ÑÑÑÐ° ÑÐ¶Ð°ÑÐ¾Ð²

description: Ð Ð°Ð±Ð¾ÑÐ° Ð¿Ð¾ÑÐ²ÑÑÐµÐ½Ð° ÑÑÐµÐ´ÑÑÐ²Ð°Ð¼ ÑÐ·ÑÐºÐ¾Ð²Ð¾Ð¹ ÑÐµÐ¿ÑÐµÐ·ÐµÐ½ÑÐ°ÑÐ¸Ð¸ ÐºÐ°ÑÐµÐ³Ð¾ÑÐ¸Ð¸ ÑÐ°ÑÐ¿ÐµÐ½ÑÐ° Ð² ÑÑÐ´Ð¾Ð¶ÐµÑÑÐ²ÐµÐ½Ð½Ð¾Ð¹ Ð»Ð¸ÑÐµÑÐ°ÑÑÑÐµ, Ð² ÑÐ°ÑÑÐ½Ð¾ÑÑÐ¸ Ð»Ð¸ÑÐµÑÐ°ÑÑÑÐµ ÑÐ¶Ð°ÑÐ¾Ð². ÐÐ½Ð° ÑÐ°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÐµÑÑÑ Ð½Ð° ÑÐ°ÐºÐ¸Ñ ÑÑÐ¾Ð²Ð½ÑÑ ÑÐµÐºÑÑÐ°, ÐºÐ°Ðº ÑÐ¾Ð½ÐµÑÐ¸ÑÐµÑÐºÐ¸Ð¹, Ð³ÑÐ°Ð¼Ð¼Ð°ÑÐ¸ÐºÐ¾-Ð»Ð¸Ð½Ð³Ð²Ð¸ÑÑÐ¸ÑÐµÑÐºÐ¸Ð¹, Ð³ÑÐ°ÑÐ¸ÑÐµÑÐºÐ¸Ð¹ Ð¸ ÑÐ¸Ð½ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ¸Ð¹, ÑÑÐ¸Ð»Ð¸ÑÑÐ¸ÑÐµÑÐºÐ¸Ð¹ Ð¸ ÑÑÐ¾Ð²ÐµÐ½Ñ ÐºÐ¾Ð¼Ð¿Ð¾Ð·Ð¸ÑÐ¸Ð¸. Ð¡ÑÐµÐ´ÑÑÐ²Ð° ÑÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð±ÑÐ»Ð¸ Ð¾Ð±Ð½Ð°ÑÑÐ¶ÐµÐ½Ñ Ð½Ð° Ð²ÑÐµÑ Ð¿ÐµÑÐµÑÐ¸ÑÐ»ÐµÐ½Ð½ÑÑ ÑÑÐ¾Ð²Ð½ÑÑ. ÐÑÐ» Ð¿ÑÐ¾Ð¸Ð·Ð²ÐµÐ´ÐµÐ½ ÑÑÐ°Ð²Ð½Ð¸ÑÐµÐ»ÑÐ½ÑÐ¹ Ð°Ð½Ð°Ð»Ð¸Ð· Ð¿ÐµÑÐµÐ²Ð¾Ð´Ð° Ð¾Ð±Ð½Ð°ÑÑÐ¶ÐµÐ½Ð½ÑÑ ÑÑÐµÐ´ÑÑÐ² Ñ Ð°Ð½Ð³Ð»Ð¸Ð¹ÑÐºÐ¾Ð³Ð¾ Ð½Ð° ÑÑÑÑÐºÐ¸Ð¹ ÑÐ·ÑÐº. ÐÑÐ»Ð¾ Ð¾Ð±Ð½Ð°ÑÑÐ¶ÐµÐ½Ð¾, ÑÑÐ¾ ÑÑÐµÐ´ÑÑÐ² ÑÑÑÑÐºÐ¾Ð³Ð¾ ÑÐ·ÑÐºÐ° Ð´Ð¾ÑÑÐ°ÑÐ¾ÑÐ½Ð¾, ÑÑÐ¾Ð±Ñ ÑÐ¾ÑÑÐ°Ð½Ð¸ÑÑ Ð°Ð²ÑÐ¾ÑÑÐºÐ¸Ð¹ ÑÑÐ¸Ð»Ñ Ð¾ÑÐ¸Ð³Ð¸Ð½Ð°Ð»Ð°.
Electron Scattering in Intrananotube Quantum Dots
Creators: name: Buchs, G.
name: Bercioux, D.
name: Ruffieux, P.
name: Groening, P.
name: Grabert, H.
name: Groening, O.
Publisher: name: arXiv
Year: 2008
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: Disordered Systems and Neural Networks (cond-mat.dis-nn)
subject: FOS: Physical sciences

description: Intratube quantum dots showing particle-in-a-box-like states with level spacings up to 200meV are realized in metallic single-walled carbon nanotubes by means of low dose medium energy Ar irradiation. Fourier transform scanning tunneling spectroscopy compared to results of a Fabry-Perot electron resonator model yields clear signatures for inter- and intra-valley scattering of electrons confined between consecutive irradiation-induced defects (inter-defects distance < 10nm). Effects arising from lifting the degeneracy of the Dirac cones within the first Brillouin zone are also observed.
"Postprint of The Corpus Christi Devotion: Gender, Liturgy and Authority among Dominican Nuns in Castile in the Middle Ages
Creators: name: Pérez Vidal, Mercedes
Publisher: name: Zenodo
Year: 2024

description: This is a digital draft of this article after it has been peer reviewed and accepted for publication, but before it has been typeseet.

Pérez Vidal, Mercedes. “The Corpus Christi Devotion: Gender, Liturgy, and Authority among Dominican Nuns in Castile in the Middle Ages.” Historical Reflections / Réflexions Historiques 42, no. 1 (2016): 35–47. http://www.jstor.org/stable/24720614.
title: ÐÐ½Ð°Ð»Ð¸Ð· Ð¸ Ð¾ÑÐµÐ½ÐºÐ° ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ Ñ Ð¾Ð·ÑÐ¹ÑÑÐ²ÐµÐ½Ð½ÑÑ ÑÐ²ÑÐ·ÐµÐ¹ Ð¼ÐµÐ¶Ð´Ñ ÑÑÐ±ÑÐµÐºÑÐ°Ð¼Ð¸ ÑÐ¾Ð²Ð°ÑÐ½Ð¾Ð³Ð¾ ÑÑÐ½ÐºÐ° (Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ ÐÐÐ Â«ÐÐ°ÐºÑÐ¸Ð´Ð¾Ð¼Â»)
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ÐµÐ¾Ð½ÑÑÐµÐ²Ð°, ÐÐ½Ð°ÑÑÐ°ÑÐ¸Ñ
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2018
Subjects: ÑÐ¾Ð·Ð½Ð¸ÑÐ½Ð°Ñ ÑÐ¾ÑÐ³Ð¾Ð²Ð»Ñ
Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ðµ ÑÐ¾ÑÐ³Ð¾Ð²Ð»Ð¸
ÐºÐ¾Ð½ÐºÑÑÐµÐ½ÑÐ¾ÑÐ¿Ð¾ÑÐ¾Ð±Ð½Ð¾ÑÑÑ
Ð¿Ð¾ÑÑÐ°Ð²ÑÐ¸ÐºÐ¸
Ð¿Ð¾ÑÑÐ°Ð²ÐºÐ¸
Ð°ÑÑÐ¾ÑÑÐ¸Ð¼ÐµÐ½Ñ ÑÐ¾Ð²Ð°ÑÐ¾Ð²

description: ÐÐ±ÑÐµÐºÑÐ¾Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ²Ð»ÑÐµÑÑÑ ÐÐÐ Â«ÐÐ°ÐºÑÐ¸Ð´Ð¾Ð¼Â». Ð¦ÐµÐ»ÑÑ Ð²ÑÐ¿ÑÑÐºÐ½Ð¾Ð¹ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ ÑÐ²Ð»ÑÐµÑÑÑ Ð°Ð½Ð°Ð»Ð¸Ð· Ð¸ Ð¾ÑÐµÐ½ÐºÐ° ÑÑÑÐµÑÑÐ²ÑÑÑÐ¸Ñ ÑÐ¾Ð·ÑÐ¹ÑÑÐ²ÐµÐ½Ð½ÑÑ ÑÐ²ÑÐ·ÐµÐ¹ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ ÐÐÐ Â«ÐÐ°ÐºÑÐ¸Ð´Ð¾Ð¼Â». Ð ÑÐ¾Ð´Ðµ ÑÐ°Ð±Ð¾ÑÑ Ð±ÑÐ» Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ñ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÐµÐºÑÑÐµÐ³Ð¾ ÑÐ¾ÑÑÐ¾ÑÐ½Ð¸Ñ ÑÐ¾ÑÐ³Ð¾Ð²Ð¾Ð³Ð¾ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ Â«ÐÐ°ÐºÑÐ¸Ð´Ð¾Ð¼Â», Ð¿ÑÐ¾Ð°Ð½Ð°Ð»Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ð° Ð¼Ð°ÑÐºÐµÑÐ¸Ð½Ð³Ð¾Ð²Ð°Ñ Ð¼Ð°ÐºÑÐ¾- Ð¸ Ð¼Ð¸ÐºÑÐ¾ÑÑÐµÐ´Ñ, Ð´Ð°Ð½Ð° Ð¾ÑÐµÐ½ÐºÐ° ÐµÐ³Ð¾ ÐºÐ¾Ð½ÐºÑÑÐµÐ½ÑÐ¾ÑÐ¿Ð¾ÑÐ¾Ð±Ð½Ð¾ÑÑÐ¸ Ð¸ Ð´Ð¸Ð½Ð°Ð¼Ð¸ÐºÐ¸ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾-ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¸Ñ Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»ÐµÐ¹, Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¾ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð°ÑÑÐ¾ÑÑÐ¸Ð¼ÐµÐ½ÑÐ° ÑÐ¾ÑÐ³Ð¾Ð²Ð¾Ð³Ð¾ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ Â«ÐÐ°ÐºÑÐ¸Ð´Ð¾Ð¼Â», Ð´Ð°Ð½Ñ Ð°Ð½Ð°Ð»Ð¸Ð· Ð¸ Ð¾ÑÐµÐ½ÐºÐ° ÑÐ¾Ð·ÑÐ¹ÑÑÐ²ÐµÐ½Ð½ÑÑ ÑÐ²ÑÐ·ÐµÐ¹ Ð¿Ð¾ Ð¿Ð¾ÑÑÐ°Ð²ÐºÐ°Ð¼ ÑÐ¾Ð²Ð°ÑÐ¾Ð², Ð° ÑÐ°ÐºÐ¶Ðµ ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð°ÑÐ¸Ð¸ Ð¿Ð¾ Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ñ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ ÑÐ¾Ð·ÑÐ¹ÑÑÐ²ÐµÐ½Ð½ÑÑ ÑÐ²ÑÐ·ÐµÐ¹.
Geometric stabilization of extended S=2 vortices in two-dimensional photonic lattices: theoretical analysis, numerical computation and experimental results
Creators: name: Law, K. J. H.
name: Song, D.
name: Kevrekidis, P. G.
name: Xu, J.
name: Chen, Zhigang
Publisher: name: arXiv
Year: 2009
Subjects: subject: Pattern Formation and Solitons (nlin.PS)
subject: FOS: Physical sciences

description: In this work, we focus our studies on the subject of nonlinear discrete self-trapping of S=2 (doubly-charged) vortices in two-dimensional photonic lattices, including theoretical analysis, numerical computation and experimental demonstration. We revisit earlier findings about S=2 vortices with a discrete model, and find that S=2 vortices extended over eight lattice sites can indeed be stable (or only weakly unstable) under certain conditions, not only for the cubic nonlinearity previously used, but also for a saturable nonlinearity more relevant to our experiment with a biased photorefractive nonlinear crystal. We then use the discrete analysis as a guide towards numerically identifying stable (and unstable) vortex solutions in a more realistic continuum model with a periodic potential. Finally, we present our experimental observation of such geometrically extended S=2 vortex solitons in optically induced lattices under both self-focusing and self-defocusing nonlinearities, and show clearly that the S=2 vortex singularities are preserved during nonlinear propagation.
In-Plane and Out-of-Plane Excitonic Coupling in 2D Molecular Crystals
Creators: name: Kim, Dogyeong
name: Lee, Sol
name: Park, Jiwon
name: Lee, Jinho
name: Choi, Hee Cheul
name: Kim, Kwanpyo
name: Ryu, Sunmin
Publisher: name: arXiv
Year: 2022
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: Understanding the nature of molecular excitons in low-dimensional molecular solids is of paramount importance in fundamental photophysics and various applications such as energy harvesting, switching electronics and display devices. Despite this, the spatial evolution of molecular excitons and their transition dipoles have not been captured in the precision of molecular length scales. Here we show in-plane and out-of-plane excitonic evolution in quasilayered two-dimensional (2D) perylene-3, 4, 9, 10-tetracarboxylic dianhydride (PTCDA) crystals assembly-grown on hexagonal boron nitride (BN) crystals. Complete lattice constants with orientations of two herringbone-configured basis molecules are determined with polarization-resolved spectroscopy and electron diffraction methods. In the truly 2D limit of single layers, two Frenkel emissions Davydov-split by Kasha-type intralayer coupling exhibit energy inversion with decreasing temperature, which enhances excitonic coherence. As the thickness increases, the transition dipole moments of newly emerging charge transfer excitons are reoriented because of mixing with the Frenkel states. The current spatial anatomy of 2D molecular excitons will inspire a deeper understanding and groundbreaking applications of low-dimensional molecular systems.
description: 27 pages, 5 figures
title: ÐÑÑÐ¸ Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ñ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ð¹ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ ÑÐµÐ¿Ð»Ð¾Ð²ÑÑ ÑÐµÑÐµÐ¹
title: Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ°
titleType: Subtitle
Creators: name: ÐÑÐ¸Ð¿Ð¾Ð², Ð¡ÐµÑÐ³ÐµÐ¹
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2018
Subjects: ÑÐµÐ¿Ð»Ð¾Ð²ÑÐµ ÑÐµÑÐ¸
Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ñ ÑÐµÐ¿Ð»Ð¾Ð²ÑÑ ÑÐµÑÐµÐ¹
ÑÐµÐ¿Ð»Ð¾Ð¿Ð¾ÑÐµÑÐ¸ Ð¸Ð·Ð¾Ð»ÑÑÐ¸Ð¸ ÑÑÑÐ±Ð¾Ð¿ÑÐ¾Ð²Ð¾Ð´Ð¾Ð²
ÑÐ½ÐµÑÐ³ÐµÑÐ¸ÑÐµÑÐºÐ°Ñ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÑ

description: ÐÐ±ÑÐµÐºÑÐ¾Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ²Ð»ÑÑÑÑÑ ÑÐµÐ¿Ð»Ð¾Ð²ÑÐµ ÑÐµÑÐ¸.
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 Ð²ÑÑÐ²Ð»ÐµÐ½Ð¸Ðµ Ð¿ÑÑÐµÐ¹ Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ñ ÑÐ½ÐµÑÐ³Ð¾ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ ÑÐµÐ¿Ð»Ð¾Ð²ÑÑ ÑÐµÑÐµÐ¹, Ð°, ÑÐ»ÐµÐ´Ð¾Ð²Ð°ÑÐµÐ»ÑÐ½Ð¾, Ð¸ Ð¸Ñ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ð¹ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸.
Ð Ð°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ñ ÑÑÑÐµÑÑÐ²ÑÑÑÐ¸Ñ ÑÐµÐ¿Ð»Ð¾Ð²ÑÑ ÑÐµÑÐµÐ¹, ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ Ð²Ð¾Ð·Ð¼Ð¾Ð¶Ð½ÑÐµ Ð¿ÑÑÐ¸ Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ñ ÑÐ½ÐµÑÐ³ÐµÑÐ¸ÑÐµÑÐºÐ¾Ð¹ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸, Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· Ð¸ Ð²ÑÐ±ÑÐ°Ð½ ÑÐ¿Ð¾ÑÐ¾Ð± Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ñ ÑÐ½ÐµÑÐ³ÐµÑÐ¸ÑÐµÑÐºÐ¾Ð¹ Ð¸ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ð¹ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ ÑÐµÐ¿Ð»Ð¾Ð²ÑÑ ÑÐµÑÐµÐ¹, Ð¿ÑÐ¾Ð¸Ð·Ð²ÐµÐ´ÐµÐ½Ð° Ð¾ÑÐµÐ½ÐºÐ° ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ð¹ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ ÑÑÑÐ±Ð¾Ð¿ÑÐ¾Ð²Ð¾Ð´Ð¾Ð² Ð² Ð¸Ð·Ð¾Ð»ÑÑÐ¸Ð¸ Ð¸Ð· Ð¼Ð¸Ð½ÐµÑÐ°Ð»ÑÐ½Ð¾Ð¹ Ð²Ð°ÑÑ Ð¸ ÑÐµÐ»ÐµÑÐ¾Ð¾Ð±ÑÐ°Ð·Ð½Ð¾ÑÑÑ Ð¸Ñ Ð·Ð°Ð¼ÐµÐ½Ñ Ð½Ð° ÑÑÑÐ±Ñ Ð² Ð¿ÐµÐ½Ð¾Ð¿Ð¾Ð»Ð¸ÑÑÐµÑÐ°Ð½Ð¾Ð²Ð¾Ð¹ Ð¸Ð·Ð¾Ð»ÑÑÐ¸Ð¸.
SAE Aero Design Competition
Creators: name: Muchla, Grzegorz
Publisher: name: Zenodo
Year: 2020
Subjects: EWADE2020

description: The SAE Aero Design competition is a real-world design challenge designed to compress a typical aircraft development program into one calendar year, taking participants through the system engineering process of breaking down requirements. It exposes participants to the nuances of conceptual design, manufacturing, system integration/test, and sell-off through demonstration. Warsaw University of Technology participated in the SAE Aero Design competition (West) in 2020. Here are a few impressions.
description: http://EWADE.AircraftDesign.org --- http://Presentations2020.AircraftDesign.org
Search for Stable Strange Quark Matter in Lunar Soil using the Mass Spectrometry Technique
Creators: name: Han, Ke
Publisher: name: arXiv
Year: 2008
Subjects: subject: Nuclear Experiment (nucl-ex)
subject: FOS: Physical sciences

description: Strange quark matter is a postulated state which may be the true ground state of cold hadronic matter. Physicists have been searching for strange quark matter in the last several decades but found no definite evidence of its existence. In our experiment, we used the Yale tandem accelerator as a mass spectrometer to identify possible stable strangelets (small chunks of strange quark matter) in lunar soil. The search covers the mass range from A=42 to A=70 amu for nuclear charges 6, 8, and 9. No strangelets are found at sensitivity levels down to $\sim10^{-17}$. The implied limit on strangelet flux in cosmic rays is the most sensitive to date for the covered mass range.
description: Talk given at International Conference on Strangeness in Quark Matter (SQM 2008), Beijing, China, Oct 6-10, 2008
Analytical vectorial structure of non-paraxial four-petal Gaussian beams in the far field
Creators: name: Long, Xuewen
name: Lu, Keqing
name: Zhang, Yuhong
name: Guo, Jianbang
name: Li, Kehao
Publisher: name: arXiv
Year: 2010
Subjects: subject: Optics (physics.optics)
subject: FOS: Physical sciences

description: The analytical vectorial structure of non-paraxial four-petal Gaussian beams(FPGBs) in the far field has been studied based on vector angular spectrum method and stationary phase method. In terms of analytical electromagnetic representations of the TE and TM terms, the energy flux distributions of the TE term, the TM term, and the whole beam are derived in the far field, respectively. According to our investigation, the FPGBs can evolve into a number of small petals in the far field. The number of the petals is determined by the order of input beam. The physical pictures of the FPGBs are well illustrated from the vectorial structure, which is beneficial to strengthen the understanding of vectorial properties of the FPGBs.
Additional file 1 of Dishevelled 2 regulates cancer cell proliferation and T cell mediated immunity in HER2-positive breast cancer
Creators: name: Rasha, Fahmida
name: Boligala, Geetha Priya
name: Yang, Mingxiao V.
name: Martinez-Marin, Dalia
name: Castro-Piedras, Isabel
name: Furr, Kathryn
name: Snitman, Annie
name: Khan, Sonia Y.
name: Brandi, Luis
name: Castro, Maribel
name: Khan, Hafiz
name: Jahan, Nusrat
name: Almodovar, Sharilyn
name: Melkus, Michael W.
name: Pruitt, Kevin
name: Layeequr Rahman, Rakhshanda
Publisher: name: figshare
Year: 2023
Subjects: subject: Medicine
subject: Cell Biology
subject: Molecular Biology
subject: Immunology
subject: FOS: Clinical medicine
subject: Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Cancer
subject: Hematology

description: Additional file 1: Figure S1a. Western blot analysis showing the knockdown of DVL2. Figure S1b. Raw data for western blots in Fig. S1a. Figure S2a. Raw data for western blots in Fig. 2. Figure S2a. Raw data for ChIPdatain Fig. 2. Figure S2b. Raw data for ChIPdatain Fig. 2. Figure S4a. Raw data for western blots in Fig. 4. Figure S4b. Raw data for western blots in Fig. 4.
title: ÐÑÐ½Ð¾Ð²Ñ ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸Ð¸ Ð¼Ð°ÑÐ¸Ð½Ð¾ÑÑÑÐ¾ÐµÐ½Ð¸Ñ. ÐÐ°Ð±Ð¾ÑÐ°ÑÐ¾ÑÐ½ÑÐ¹ Ð¿ÑÐ°ÐºÑÐ¸ÐºÑÐ¼
Creators: name: ÐÑÐºÐ¾Ð², Ð­Ð´ÑÐ°ÑÐ´
name: ÐÐ¾Ð·Ð°ÑÑ, ÐÐ²Ð°Ð½
name: ÐÑÐ±Ð¾Ð¼ÑÐ´ÑÐ¾Ð², Ð¡ÐµÑÐ³ÐµÐ¹
name: Ð¡ÑÐµÐ¿Ð°Ð½Ð¾Ð², Ð¡ÐµÑÐ³ÐµÐ¹
Publisher: name: ÐÐ·Ð´-Ð²Ð¾ ÐÐ¾Ð»Ð¸ÑÐµÑÐ½. ÑÐ½-ÑÐ°
Year: 2015
Subjects: ÐÐ°ÑÐ¸Ð½Ð¾ÑÑÑÐ¾ÐµÐ½Ð¸Ðµ

description: Ð Ð¿Ð¾ÑÐ¾Ð±Ð¸Ð¸ Ð¸Ð·Ð»Ð¾Ð¶ÐµÐ½Ð° Ð¼ÐµÑÐ¾Ð´Ð¸ÐºÐ° Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¸Ñ Ð»Ð°Ð±Ð¾ÑÐ°ÑÐ¾ÑÐ½ÑÑ ÑÐ°Ð±Ð¾Ñ Ð¿Ð¾ Ð´Ð¸ÑÑÐ¸Ð¿Ð»Ð¸Ð½Ð°Ð¼ Â«ÐÑÐ½Ð¾Ð²Ñ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¸ Ð¼Ð°ÑÐ¸Ð½Ð¾ÑÑÑÐ¾ÐµÐ½Ð¸ÑÂ» Ð¸ Â«Ð¢ÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ñ Ð¼Ð°ÑÐ¸Ð½Ð¾ÑÑÑÐ¾ÐµÐ½Ð¸ÑÂ». Ð Ð°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ Ð²Ð¾Ð¿ÑÐ¾ÑÑ Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð¸Ñ Ð¶ÐµÑÑÐºÐ¾ÑÑÐ¸ Ð¼ÐµÑÐ°Ð»Ð»Ð¾ÑÐµÐ¶ÑÑÐ¸Ñ ÑÑÐ°Ð½ÐºÐ¾Ð², ÑÐ°Ð·Ð¼ÐµÑÐ½Ð¾Ð³Ð¾ Ð¸Ð·Ð½Ð¾ÑÐ° ÑÐµÐ¶ÑÑÐµÐ³Ð¾ Ð¸Ð½ÑÑÑÑÐ¼ÐµÐ½ÑÐ°, ÑÐµÐ¿Ð»Ð¾Ð²ÑÑ Ð´ÐµÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¹ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¾Ð¹ ÑÐ¸ÑÑÐµÐ¼Ñ Ð¸ ÑÐ¾ÑÐ½Ð¾ÑÑÐ¸ Ð¾Ð±ÑÐ°Ð±Ð¾ÑÐºÐ¸, Ð² ÑÐ¾Ð¼ ÑÐ¸ÑÐ»Ðµ Ð¿ÑÐ¸ ÑÐ°Ð±Ð¾ÑÐµ Ð½Ð° Ð½Ð°ÑÑÑÐ¾ÐµÐ½Ð½ÑÑ ÑÑÐ°Ð½ÐºÐ°Ñ. ÐÐ¾ÐºÐ°Ð·Ð°Ð½Ð¾ Ð²Ð»Ð¸ÑÐ½Ð¸Ðµ ÑÐµÐ¶Ð¸Ð¼Ð¾Ð² ÑÐµÐ·Ð°Ð½Ð¸Ñ Ð¸ Ð³ÐµÐ¾Ð¼ÐµÑÑÐ¸Ð¸ Ð¸Ð½ÑÑÑÑÐ¼ÐµÐ½ÑÐ° Ð½Ð° Ð¿Ð¾Ð³ÑÐµÑÐ½Ð¾ÑÑÑ ÑÐ¾ÑÐ¼Ñ, ÐºÐ°ÑÐµÑÑÐ²Ð¾ Ð¾Ð±ÑÐ°Ð±Ð¾ÑÐ°Ð½Ð½Ð¾Ð¹ Ð¿Ð¾Ð²ÐµÑÑÐ½Ð¾ÑÑÐ¸, Ð° ÑÐ°ÐºÐ¶Ðµ Ð¸Ð½ÑÐµÐ½ÑÐ¸Ð²Ð½Ð¾ÑÑÑ Ð¸ ÑÐ°ÑÑÐ¾ÑÑ Ð²Ð¸Ð±ÑÐ°ÑÐ¸Ð¸. ÐÐ¿Ð¸ÑÐ°Ð½Ñ ÑÐ¿Ð¾ÑÐ¾Ð±Ñ ÑÐ°Ð·Ð¼ÐµÑÐ½Ð¾Ð¹ Ð½Ð°Ð»Ð°Ð´ÐºÐ¸ ÑÑÐ°Ð½ÐºÐ¾Ð² Ð¸ ÑÐ±Ð¾ÑÐºÐ¸ ÑÐ·Ð»Ð¾Ð² Ð¸ Ð¼ÐµÑÐ°Ð½Ð¸Ð·Ð¼Ð¾Ð². Ð£ÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ Ð¿ÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¾ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² Ð²ÑÐ·Ð¾Ð², Ð¾Ð±ÑÑÐ°ÑÑÐ¸ÑÑÑ Ð¿Ð¾ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸ÑÐ¼ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ Â«Ð¢ÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ðµ Ð¼Ð°ÑÐ¸Ð½Ñ Ð¸ Ð¾Ð±Ð¾ÑÑÐ´Ð¾Ð²Ð°Ð½Ð¸ÐµÂ». ÐÐ½Ð¾ Ð¼Ð¾Ð¶ÐµÑ Ð±ÑÑÑ ÑÐ°ÐºÐ¶Ðµ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¾ Ð¿ÑÐ¸ Ð¾Ð±ÑÑÐµÐ½Ð¸Ð¸ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² Ð¿Ð¾ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸ÑÐ¼ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ Â«ÐÐ¾Ð½ÑÑÑÑÐºÑÐ¾ÑÑÐºÐ¾-ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¾Ðµ Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ðµ Ð¼Ð°ÑÐ¸Ð½Ð¾ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÐ½ÑÑ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²Â» Ð¸ Â«ÐÐ°ÑÐ¸Ð½Ð¾ÑÑÑÐ¾ÐµÐ½Ð¸ÐµÂ», Ð² ÑÐ¸ÑÑÐµÐ¼Ð°Ñ Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¸, Ð² ÑÑÑÐµÐ¶Ð´ÐµÐ½Ð¸ÑÑ Ð´Ð¾Ð¿Ð¾Ð»Ð½Ð¸ÑÐµÐ»ÑÐ½Ð¾Ð³Ð¾ Ð¿ÑÐ¾ÑÐµÑÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½Ð¾Ð³Ð¾ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ñ.
Information entropy of nuclear electromagnetic transitions in AdS/QCD
Creators: name: da Rocha, Roldao
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: Electromagnetic transitions involving nucleons and their resonances are here presented in the fermionic sector of the AdS/QCD soft-wall model, using the differential configurational entropy (DCE) as a measure of information entropy. The DCE is employed to derive adjustable parameters that define the minimal and nonminimal couplings in the nuclear interaction with a gauge vector field, in the nucleonic $γN \to N^*(1535)$ transition. The values obtained comply with phenomenological data with good accuracy.
description: 25 pages, 6 figures