cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Neighborhood growth dynamics on the Hamming plane
Creators: name: Gravner, Janko
name: Sivakoff, David
name: Slivken, Erik
Publisher: name: arXiv
Year: 2016
Subjects: subject: Combinatorics (math.CO)
subject: Probability (math.PR)
subject: FOS: Mathematics
subject: 05D99, 60K35

description: We initiate the study of general neighborhood growth dynamics on two dimensional Hamming graphs. The decision to add a point is made by counting the currently occupied points on the horizontal and the vertical line through it, and checking whether the pair of counts lies outside a fixed Young diagram. We focus on two related extremal quantities. The first is the size of the smallest set that eventually occupies the entire plane. The second is the minimum of an energy-entropy functional that comes from the scaling of the probability of eventual full occupation versus the density of the initial product measure within a rectangle. We demonstrate the existence of this scaling and study these quantities for large Young diagrams.
description: 55 pages
On the change of density of states in two-body interactions
Creators: name: Gao, Bo
Publisher: name: arXiv
Year: 2016
Subjects: subject: Atomic Physics (physics.atom-ph)
subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We derive a general relation in two-body scattering theory that more directly relates the change of density of states (DDOS) due to interaction to the shape of the potential. The relation allows us to infer certain global properties of the DDOS from the global properties of the potential. In particular, we show that DDOS is negative at all energies and for all partial waves, for potentials that are more repulsive than $+1/r^2$ everywhere. This behavior represents a different class of global properties of DDOS from that described by the Levinson's theorem.
description: 7 pages, 3 figures
Sonnenfleckenzeichnung Nr. 26001.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 15.09.1980, erstellt von Hans Ulrich Keller
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1980

description: Bleistiftzeichnung mit Tinte und Farbstift überschrieben, erstellt als Projektionsbildzeichnung in der Eidgenössischen Sternwarte Zürich. Instrument: Zeiss Coudé-Refraktor (150/2250 mm).
Die Beobachtungen zu Einzelflecken und zu Sonnenfleckengruppen wurden mit Bleistift auf einem Vordruck eingetragen. Zusätzlich notiert: Tabelle mit den statistischen Angaben, für die Werte g, f sowie Gr (Anzahl g)
Tau flavored dark matter and its impact on tau Yukawa coupling
Creators: name: Chao, Wei
name: Guo, Huai-Ke
name: Li, Hao-Lin
Publisher: name: arXiv
Year: 2016
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: In this paper we preform a systematic study of the tau flavored dark matter model by introducing two kinds of mediators (a scalar doublet and a charged scalar singlet). The electromagnetic properties of the dark matter, as well as their implications in dark matter direct detections, are analyzed in detail. The model turns out contributing a significant radiative correction to the tau lepton mass, in addition to loosing the tension between the measured dark matter relic density and constraints of dark matter direct detections. The loop corrections can be ${\cal O}(10\%)$ of the total tau mass. Signal rates of the Higgs measurements from the LHC in the $h\toττ$ and $h\to γγ$ channels, relative to the Standard Model expectations, can be explained in this model.
description: 18 pages, 7 figures
How to obtain desynchronized network splay states via electrical coupling
Creators: name: Niemeyer, Nelson
name: Hürkey, Silvan
name: Schleimer, Jan-Hendrik
name: Ryglewski, Stefanie
name: Duch, Carsten
name: Schreiber, Susanne
Publisher: name: G-Node
Year: 2023
Subjects: Computational Neuroscience
Single neurons and biophysics

description: Bernstein Conference 2023 abstract. https://bernstein-conference.de
The SHARDDS survey: first resolved image of the HD114082 debris disk in Lower Centaurus Crux with SPHERE
Creators: name: Wahhaj, Zahed
name: Milli, Julien
name: Kennedy, Grant
name: Ertel, Steve
name: Matra, Luca
name: Boccaletti, Anthony
name: del Burgo, Carlos
name: Wyatt, Mark
name: Pinte, Christophe
name: Lagrange, Anne Marie
name: Absil, Olivier
name: Choquet, Elodie
name: Gonzalez, Carlos Gomez
name: Kobayashii, Hiroshi
name: Mawet, Dimitri
name: Mouillet, David
name: Pueyo, Laurent
name: Dent, William R. F.
name: Augereau, Jean-Charles
name: Girard, Julien
Publisher: name: arXiv
Year: 2016
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: We present the first resolved image of the debris disk around the 16+/-8 Myr old star, HD 114082. The observation was made in the H-band using the SPHERE instrument. The star is at a distance of 92+/-6 pc in the Lower Centaurus Crux association. Using a Markov Chain Monte Carlo analysis, we determined that the debris is likely in the form of a dust ring with an inner edge of 27.7+2.8/-3.5 au, position angle -74+0.5/-1.5 deg, and an inclination with respect to the line of sight of 6.7+3.8/-0.4 deg. The disk imaged in scattered light has a surface density declining with radius like ~r^(-4), steeper than expected for grain blowout by radiation pressure. We find only marginal evidence (2 sigma) of eccentricity, and rule out planets more massive than 1.0 Mjup orbiting within 1 au of the ring's inner edge, since such a planet would have disrupted the disk. The disk has roughly the same fractional disk luminosity (Ldisk/L*=3.3x10^(-3)) as HR4796A and Beta Pictoris, however it was not detected by previous instrument facilities most likely because of its small angular size (radius~0.4"), low albedo (~0.2) and low scattering efficiency far from the star due to high scattering anisotropy. With the arrival of extreme adaptive optics systems like SPHERE and GPI, the morphology of smaller, fainter and more distant debris disks are being revealed, providing clues to planet-disk interactions in young protoplanetary systems.
description: 8 pages, 4 figures
title: Формирование международно-правовых стандартов по охране культурного наследия
Creators: name: Цыганков, Евгений
Publisher: name: Новгородский государственный университет имени Ярослава Мудрого (НовГУ)
Year: 2022

description: Данное исследование представляет собой анализ концепции культурного наследия и институционализации его защиты международным правом в различных исторических контекстах вовлеченных государств, т. е. во время мира, конфликта, социального и/или политического кризиса. Кроме того, обсуждается человеческое измерение защиты культурного наследия на международном уровне в рамках международного публичного права. В частности, сначала исследуется, остаются ли государства центральными акторами на национальном и международном уровне в том, что касается защиты культурных ценностей на их территории. Затем исследуется ограничения, накладываемые на диапазон действий государства в связи с первичным и вторичным законодательством международных организаций, в которых участвует государство. Помимо этой формы внешнего давления на юрисдикцию государства, также исследуется, ограничивается ли диапазон действий государства действиями отдельных лиц и групп. Кроме того, исследуется потенциальная роль международного права прав человека в таких ситуациях, взаимозависимость между защитой индивидов и культурных ценностей, а также то, превращается ли индивид в активного субъекта международного права.
Sonnenfleckenzeichnung Nr. 25974.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 14.08.1980, erstellt von Hans Ulrich Keller
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1980

description: Bleistiftzeichnung mit Tinte und Farbstift überschrieben, erstellt als Projektionsbildzeichnung in der Eidgenössischen Sternwarte Zürich. Instrument: Zeiss Coudé-Refraktor (150/2250 mm).
Die Beobachtungen zu Einzelflecken und zu Sonnenfleckengruppen wurden mit Bleistift auf einem Vordruck eingetragen. Zusätzlich notiert: Tabelle mit den statistischen Angaben, für die Werte g, f sowie Gr (Anzahl g)
Sonnenfleckenzeichnung Nr. 25967.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 07.08.1980, erstellt von Hans Ulrich Keller
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1980

description: Bleistiftzeichnung mit Tinte und Farbstift überschrieben, erstellt als Projektionsbildzeichnung in der Eidgenössischen Sternwarte Zürich. Instrument: Zeiss Coudé-Refraktor (150/2250 mm).
Die Beobachtungen zu Einzelflecken und zu Sonnenfleckengruppen wurden mit Bleistift auf einem Vordruck eingetragen. Zusätzlich notiert: Tabelle mit den statistischen Angaben, für die Werte g, f sowie Gr (Anzahl g)
Performance degradation of superlattice MOSFETs due to scattering in the contacts
Creators: name: Long, Pengyu
name: Huang, Jun
name: Jiang, Zhengping
name: Klimeck, Gerhard
name: Rodwell, Mark J. W.
name: Povolotskyi, Michael
Publisher: name: arXiv
Year: 2016
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: Ideal, completely coherent quantum transport calculations had predicted that superlattice MOSFETs may offer steep subthreshold swing performance below 60mV/dec to around 39mV/dec. However, the high carrier density in the superlattice source suggest that scattering may significantly degrade the ideal device performance. Such effects of electron scattering and decoherence in the contacts of superlattice MOSFETs are examined through a multiscale quantum transport model developed in NEMO5. This model couples NEGF-based quantum ballistic transport in the channel to a quantum mechanical density of states dominated reservoir, which is thermalized through strong scattering with local quasi-Fermi levels determined by drift-diffusion transport. The simulations show that scattering increases the electron transmission in the nominally forbidden minigap therefore degrading the subthreshold swing (S.S.) and the ON/OFF DC current ratio. This degradation varies with both the scattering rate and the length of the scattering dominated regions. Different superlattice MOSFET designs are explored to mitigate the effects of such deleterious scattering. Specifically, shortening the spacer region between the superlattice and the channel from 3.5 nm to 0 nm improves the simulated S.S. from 51mV/dec. to 40mV/dec. I. INTRODUCTION
description: 16 pages, 8 figures
Sonnenfleckenzeichnung Nr. 26020.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 06.10.1980, erstellt von Hans Ulrich Keller
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1980

description: Bleistiftzeichnung mit Tinte und Farbstift überschrieben, erstellt als Projektionsbildzeichnung in der Eidgenössischen Sternwarte Zürich. Instrument: Zeiss Coudé-Refraktor (150/2250 mm).
Die Beobachtungen zu Einzelflecken und zu Sonnenfleckengruppen wurden mit Bleistift auf einem Vordruck eingetragen. Zusätzlich notiert: Tabelle mit den statistischen Angaben, für die Werte g, f sowie Gr (Anzahl g)
Anatomical variability explains neuronal response variability of leech T cells, but anatomical subtypes cannot explain systematically different responses
Creators: name: Sandbote, Kevin
name: Arkhypchuk, Ihor
name: Stalf, Katrin
name: Kretzberg, Jutta
Publisher: name: G-Node
Year: 2023
Subjects: Computational Neuroscience
Single neurons and biophysics

description: Bernstein Conference 2023 abstract. https://bernstein-conference.de
Sonnenfleckenzeichnung Nr. 26068.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 23.12.1980, erstellt von Hans Ulrich Keller
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1980

description: Bleistiftzeichnung mit Tinte und Farbstift überschrieben, erstellt als Projektionsbildzeichnung in der Eidgenössischen Sternwarte Zürich. Instrument: Zeiss Coudé-Refraktor (150/2250 mm).
Die Beobachtungen zu Einzelflecken und zu Sonnenfleckengruppen wurden mit Bleistift auf einem Vordruck eingetragen. Zusätzlich notiert: Tabelle mit den statistischen Angaben, für die Werte g, f sowie Gr (Anzahl g)
Sonnenfleckenzeichnung Nr. 25939.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 28.06.1980, erstellt von Hans Ulrich Keller
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1980

description: Bleistiftzeichnung mit Tinte und Farbstift überschrieben, erstellt als Projektionsbildzeichnung in der Eidgenössischen Sternwarte Zürich. Instrument: Zeiss Coudé-Refraktor (150/2250 mm).
Die Beobachtungen zu Einzelflecken und zu Sonnenfleckengruppen wurden mit Bleistift auf einem Vordruck eingetragen. Zusätzlich notiert: Tabelle mit den statistischen Angaben, für die Werte g, f sowie Gr (Anzahl g)
Effect of burst packages on coding by primary sensory afferents in weakly electric fish
Creators: name: Schlungbaum, Maria
name: Barayeu, Alexandra
name: Grewe, Jan
name: Benda, Jan
name: Lindner, Benjamin
Publisher: name: G-Node
Year: 2023
Subjects: Computational Neuroscience
Single neurons and biophysics

description: Bernstein Conference 2023 abstract. https://bernstein-conference.de
Sonnenfleckenzeichnung Nr. 26007.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 21.09.1980, erstellt von Antoine Zelenka
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1980

description: Bleistiftzeichnung mit Tinte und Farbstift überschrieben, erstellt als Projektionsbildzeichnung in der Eidgenössischen Sternwarte Zürich. Instrument: Zeiss Coudé-Refraktor (150/2250 mm).
Die Beobachtungen zu Einzelflecken und zu Sonnenfleckengruppen wurden mit Bleistift auf einem Vordruck eingetragen. Zusätzlich notiert: Tabelle mit den statistischen Angaben, für die Werte g, f sowie Gr (Anzahl g)
Understanding the total width of the $3_{1}^{-}$ state in $\mathrm{^{12}C}$
Creators: name: Li, K. C. W.
name: Neveling, R.
name: Adsley, P.
name: Fujita, H.
name: Papka, P.
name: Smit, F. D.
name: Brümmer, J. W.
name: Donaldson, L. M.
name: Harakeh, M. N.
name: Kokalova, Tz.
name: Nikolskii, E.
name: Paulsen, W.
name: Pellegri, L.
name: Siem, S.
name: Wiedeking, M.
Publisher: name: arXiv
Year: 2023
Subjects: subject: Nuclear Experiment (nucl-ex)
subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: Recent measurements indicate that the previously established upper limit for the $γ$-decay branch of the $3_{1}^{-}$ resonance in $^{12}\textrm{C}$ at $E_{x} = 9.641(5)$ MeV may be incorrect. As a result, the $3_{1}^{-}$ resonance has been suggested as a significant resonance for mediating the triple-$α$ reaction at high temperatures above 2 GK. Accurate estimations of the $3_{1}^{-}$ contribution to the triple-$α$ reaction rate require accurate knowledge of not only the radiative width, but also the total width. In anticipation of future measurements to more accurately determine the $γ$-decay branch of the $3_{1}^{-}$ resonance, the objective of this work is to accurately determine the total width of the $3_{1}^{-}$ resonance. An evaluation was performed on all previous results considered in the current ENSDF average of 46(3) keV for the physical total width (FWHM) of the $3_{1}^{-}$ resonance in $^{12}\textrm{C}$. Significant unaccounted-for uncertainties and a misstated result were discovered in these previous results, leading to an invalid ENSDF average. In this work, the new global \textbf{R}-matrix analysis performed on direct-reaction data yields a formal total width of $Γ(E_{r}) = 46(2)$ keV and an observed total width of $Γ_{\textrm{obs}}(E_{r}) = 38(2)$ keV for the $3_{1}^{-}$ resonance. An observed total width of $Γ_{\textrm{obs}}(E_{r}) = 38(2)$ keV is recommended for the $3_{1}^{-}$ resonance in $\mathrm{^{12}C}$. This observed total width should be employed for future evaluations of the observed total radiative width for the $3_{1}^{-}$ resonance and its contribution to the high-temperature triple-$α$ reaction rate.
Temperature effects on spike counts and spike timing in a mechanoreceptor of a poikilothermic animal
Creators: name: Schultze, Bjarne L.
name: Sandbote, Kevin
name: Scherer, Jens-Steffen
name: Kretzberg, Jutta
Publisher: name: G-Node
Year: 2023
Subjects: Computational Neuroscience
Single neurons and biophysics

description: Bernstein Conference 2023 abstract. https://bernstein-conference.de
VALES: II. The physical conditions of interstellar gas in normal star-forming galaxies up to z=0.2 revealed by ALMA
Creators: name: Hughes, T. M.
name: Ibar, E.
name: Villanueva, V.
name: Aravena, M.
name: Baes, M.
name: Bourne, N.
name: Cooray, A.
name: Dunne, L.
name: Dye, S.
name: Eales, S.
name: Furlanetto, C.
name: Herrera-Camus, R.
name: Ivison, R. J.
name: van Kampen, E.
name: Lara-López, M. A.
name: Maddox, S. J.
name: Michałowski, M. J.
name: Smith, M. W. L.
name: Valiante, E.
name: van der Werf, P.
name: Xue, Y. Q.
Publisher: name: arXiv
Year: 2016
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We use new Band-3 CO(1-0) observations taken with the Atacama Large Millimeter/submillimeter Array (ALMA) to study the physical conditions in the interstellar gas of a sample of 27 dusty main-sequence star-forming galaxies at 0.035$σ$ in 26 sources. We find an average [CII] to CO(1-0) luminosity ratio of 3500$\pm$1200 for our sample that is consistent with previous studies. Using the [CII], CO and FIR measurements as diagnostics of the physical conditions of the interstellar medium, we compare these observations to the predictions of a photodissociation region (PDR) model to determine the gas density, surface temperature, pressure, and the strength of the incident far-ultraviolet (FUV) radiation field, $G_{0}$, normalised to the Habing Field. The majority of our sample exhibit hydrogen densities of 4 < $\log n/\mathrm{cm}^{3}$ < 5.5 and experience an incident FUV radiation field with strengths of 2 < $\log G_0$ < 3 when adopting standard adjustments. A comparison to galaxy samples at different redshifts indicates that the average strength of the FUV radiation field appears constant up to redshift $z\sim$6.4, yet the neutral gas density increases with redshift by a factor of $\sim$100, that persists regardless of various adjustments to our observable quantities. This evolution could provide an explanation for the observed evolution of the star formation rate density with cosmic time, yet could arise from a combination of observational biases when using different suites of emission lines as diagnostic tracers of PDR gas.
description: Accepted for publication in A&A. Abstract abridged for arXiv. 13 pages, including 5 figures and 2 tables
A calcium-based heterosynaptic plasticity rule and its role in synaptic organisation
Creators: name: Tscherniak, Isabel W.
name: Lakhera, Shreya
name: Gjorgjieva, Julijana
Publisher: name: G-Node
Year: 2023
Subjects: Computational Neuroscience
Single neurons and biophysics

description: Bernstein Conference 2023 abstract. https://bernstein-conference.de
A dynamic, data-driven computational model of the GluA2-containing AMPA receptor distribution in dendrites and synapses under basal and plasticity conditions
Creators: name: Wagle, Surbhit
name: Kraynyukova, Nataliya
name: Kracht, Maximilian K.
name: Hafner, Anne-Sophie
name: Acker-Palmer, Amparo
name: Schuman, Erin M.
name: Tchumatchenko, Tatjana
Publisher: name: G-Node
Year: 2023
Subjects: Computational Neuroscience
Single neurons and biophysics

description: Bernstein Conference 2023 abstract. https://bernstein-conference.de
Sonnenfleckenzeichnung Nr. 25954.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 21.07.1980, erstellt von Hans Ulrich Keller
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1980

description: Bleistiftzeichnung mit Tinte und Farbstift überschrieben, erstellt als Projektionsbildzeichnung in der Eidgenössischen Sternwarte Zürich. Instrument: Zeiss Coudé-Refraktor (150/2250 mm).
Die Beobachtungen zu Einzelflecken und zu Sonnenfleckengruppen wurden mit Bleistift auf einem Vordruck eingetragen. Zusätzlich notiert: Tabelle mit den statistischen Angaben, für die Werte g, f sowie Gr (Anzahl g)
Sonnenfleckenzeichnung Nr. 25940.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 30.06.1980, erstellt von Antoine Zelenka
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1980

description: Bleistiftzeichnung mit Tinte und Farbstift überschrieben, erstellt als Projektionsbildzeichnung in der Eidgenössischen Sternwarte Zürich. Instrument: Zeiss Coudé-Refraktor (150/2250 mm).
Die Beobachtungen zu Einzelflecken und zu Sonnenfleckengruppen wurden mit Bleistift auf einem Vordruck eingetragen. Zusätzlich notiert: Tabelle mit den statistischen Angaben, für die Werte g, f sowie Gr (Anzahl g)
Inferring the Neuronal Excitability Type from Noisy Electrophysiological Recordings Using Recurrent Neural Networks
Creators: name: Weerdmeester*, Liz
name: Eberle*, Maren
name: Niemeyer*, Nelson
name: Schleimer, Jan-Hendrik
name: Schreiber, Susanne
Publisher: name: G-Node
Year: 2023
Subjects: Computational Neuroscience
Single neurons and biophysics

description: Bernstein Conference 2023 abstract. https://bernstein-conference.de
Variable Stars in the Quintuplet stellar cluster with the VVV Survey
Creators: name: Molina, C. Navarro
name: Borissova, J.
name: Catelan, M.
name: Alonso-García, J.
name: Kerins, E.
name: Kurtev, R.
name: Lucas, P. W.
name: Medina, N.
name: Minniti, D.
name: Dékány, I.
Publisher: name: arXiv
Year: 2016
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: The Quintuplet cluster is one of the most massive star clusters in the Milky Way, situated very close to the Galactic center. We present a new search for variable stars in the vicinity of the cluster, using the five-year database of the Vista Variables in the Via Lactea (VVV) ESO Public Survey in the near-infrared. A total of 7586 objects were identified in the zone around $2'$ from the cluster center, using 55 $K_S$-band epochs. Thirty-three stars show $K_S$-band variability, 24 of them being previously undiscovered. Most of the variable stars found are slow/semiregular variables, long-period variables of the Mira type, and OH/IR stars. In addition, a good number of our candidates show variations in a rather short timescale. We also propose four Young Stellar Object (YSO) candidates, which could be cluster members.
description: 14 pages, 10 figures. Accepted for publication in MNRAS
Sonnenfleckenzeichnung Nr. 26048.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 22.11.1980, erstellt von Hans Ulrich Keller
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1980

description: Bleistiftzeichnung mit Tinte und Farbstift überschrieben, erstellt als Projektionsbildzeichnung in der Eidgenössischen Sternwarte Zürich. Instrument: Zeiss Coudé-Refraktor (150/2250 mm).
Die Beobachtungen zu Einzelflecken und zu Sonnenfleckengruppen wurden mit Bleistift auf einem Vordruck eingetragen. Zusätzlich notiert: Tabelle mit den statistischen Angaben, für die Werte g, f sowie Gr (Anzahl g)
Decreased neck proprioception and postural stability after induced cervical flexor muscles fatigue
Creators: name: Abdelkader, Nasr Awad
name: Mahmoud, Alaa Yousri
name: Fayaz, Nadia Abdelazim
name: Mahmoud, Lama Saad El-Din
Publisher: name: figshare
Year: 2023
Subjects: Neurology and neuromuscular diseases
Peripheral nervous system

description: J Musculoskelet Neuronal Interact 2020; 20(3):421-428
Sonnenfleckenzeichnung Nr. 26013.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 29.09.1980, erstellt von Antoine Zelenka
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1980

description: Bleistiftzeichnung mit Tinte und Farbstift überschrieben, erstellt als Projektionsbildzeichnung in der Eidgenössischen Sternwarte Zürich. Instrument: Zeiss Coudé-Refraktor (150/2250 mm).
Die Beobachtungen zu Einzelflecken und zu Sonnenfleckengruppen wurden mit Bleistift auf einem Vordruck eingetragen. Zusätzlich notiert: Tabelle mit den statistischen Angaben, für die Werte g, f sowie Gr (Anzahl g)
Study of charm hadronization with prompt $Λ^+_\mathrm{c}$ baryons in proton-proton and lead-lead collisions at $\sqrt{s_\mathrm{NN}}$ = 5.02 TeV
Creators: name: CMS Collaboration
Publisher: name: arXiv
Year: 2023
Subjects: subject: Nuclear Experiment (nucl-ex)
subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: The production of prompt $Λ^+_\mathrm{c}$ baryons is measured via the exclusive decay channel $Λ^+_\mathrm{c}$ $\to$ pK$^-π^+$ at a center-of-mass energy per nucleon pair of 5.02 TeV, using proton-proton (pp) and lead-lead (PbPb) collision data collected by the CMS experiment at the CERN LHC. The pp and PbPb data were obtained in 2017 and 2018 with integrated luminosities of 252 and 0.607 nb$^{-1}$, respectively. The measurements are performed within the $Λ^+_\mathrm{c}$ rapidity interval $\vert y \vert$ $\lt$ 1 with transverse momentum ($p_\mathrm{T}$) ranges of 3-30 and 6-40 GeV/$c$ for pp and PbPb collisions, respectively. Compared to the yields in pp collisions scaled by the expected number of nucleon-nucleon interactions, the observed yields of $Λ^+_\mathrm{c}$ with $p_\mathrm{T}$ $\gt$ 10 GeV/$c$ are strongly suppressed in PbPb collisions. The level of suppression depends significantly on the collision centrality. The $Λ^+_\mathrm{c}$ / D$^0$ production ratio is similar in PbPb and pp collisions at $p_\mathrm{T}$ $\gt$ 10 GeV/$c$, suggesting that the coalescence process does not play a dominant role in prompt $Λ^+_\mathrm{c}$ baryon production at higher $p_\mathrm{T}$.
description: Replaced with the published version. Added the journal reference and the DOI. All the figures and tables can be found at http://cms-results.web.cern.ch/cms-results/public-results/publications/HIN-21-004 (CMS Public Pages)
Numerical evaluation of memory capacity and its dependence on input and output population sparseness, plasticity, and discriminability in binary feed-forward networks
Creators: name: Chen, Lars
name: Auer, Naomi
name: Kempter, Richard
Publisher: name: G-Node
Year: 2023
Subjects: Computational Neuroscience
Learning, plasticity and memory

description: Bernstein Conference 2023 abstract. https://bernstein-conference.de
Behaviourally relevant reorganisation of the hippocampal population code over multiple days of learning
Creators: name: Chiossi, Heloisa S.C.
name: Nardin, Michele
name: Tkačik, Gašper
name: Csicsvari, Jozsef
Publisher: name: G-Node
Year: 2023
Subjects: Computational Neuroscience
Learning, plasticity and memory

description: Bernstein Conference 2023 abstract. https://bernstein-conference.de
Statistics of fractionalized excitations through threshold spectroscopy
Creators: name: Morampudi, Siddhardh C.
name: Turner, Ari M.
name: Pollmann, Frank
name: Wilczek, Frank
Publisher: name: arXiv
Year: 2016
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We show that the anyonic statistics of fractionalized excitations display characteristic signatures in threshold spectroscopic measurements. Drawing motivation from topologically ordered phases such as gapped quantum spin liquids and fractional chern insulators which possess fractionalized excitations, we consider gapped systems with abelian anyonic excitations. The low energy onset of associated correlation functions near the threshold show universal behaviour depending on the statistics of the anyons. This explains some recent theoretical results in spin systems and also provides a route towards detecting statistics in experiments such as neutron scattering and tunneling spectroscopy.
description: 5+1 pages, 4 figures
Neural connectivity structures arising from different types of spike-timing dependent plasticity
Creators: name: Cusseddu, Claudia
name: Festa, Dylan
name: Miehl, Christoph
name: Gjorgjieva, Julijana
Publisher: name: G-Node
Year: 2023
Subjects: Computational Neuroscience
Learning, plasticity and memory

description: Bernstein Conference 2023 abstract. https://bernstein-conference.de
title: Особенности процедуры банкротства физических лиц в Российской Федерации и в зарубежных странах
Creators: name: Чикунова, Анастасия
Publisher: name: Новгородский государственный университет имени Ярослава Мудрого (НовГУ)
Year: 2022

description: В статье проводится анализ осуществления процедуры банкротства физических лиц в Российской Федерации и зарубежных странах; указано нормативное регулирование процедуры банкротства в Российской Федерации; рассматриваются наиболее актуальные вопросы, возникающие при подаче заявления о признании гражданина банкротом; анализируется процедура проведения банкротства в России и в зарубежных странах, в том числе утверждение управляющего с целью реализации имущества, реализация имущества, направленная на погашение кредиторской задолженности с указанием определенного имущества, не подлежащего реализации с целью защиты прав гражданина-должника и последствия признания гражданина банкротом. Автором сделаны выводы и определено значение процедуры банкротства в современном мире, выявлены проблемы российского регулирования процедуры банкротства в контексте зарубежного опыта.
Sonnenfleckenzeichnung Nr. 26037.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 30.10.1980, erstellt von Hans Ulrich Keller
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1980

description: Bleistiftzeichnung mit Tinte und Farbstift überschrieben, erstellt als Projektionsbildzeichnung in der Eidgenössischen Sternwarte Zürich. Instrument: Zeiss Coudé-Refraktor (150/2250 mm).
Die Beobachtungen zu Einzelflecken und zu Sonnenfleckengruppen wurden mit Bleistift auf einem Vordruck eingetragen. Zusätzlich notiert: Tabelle mit den statistischen Angaben, für die Werte g, f sowie Gr (Anzahl g)
Online and memory-driven navigation through neuromodulation-based synaptic plasticity
Creators: name: Danieli, Krubeal
name: Fyhn, Marianne
name: Lepperød, Mikkel E.
Publisher: name: G-Node
Year: 2023
Subjects: Computational Neuroscience
Learning, plasticity and memory

description: Bernstein Conference 2023 abstract. https://bernstein-conference.de
The outflow of gas from the Centaurus A circumnuclear disk: atomic spectral line maps from Herschel-PACS and APEX
Creators: name: Israel, F. P.
name: Guesten, R.
name: Meijerink, R.
name: Requena-Torres, M. A.
name: Stutzki, J.
Publisher: name: arXiv
Year: 2016
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: The physical state of the gas in the central 500 pc of NGC~5128 (the radio galaxy Centaurus A - Cen A), was investigated using the far-infrared fine-structure lines of carbon, oxygen, and nitrogen, as well as the CO(4-3) molecular line. The circumnuclear disk (CND) is traced by emission from dust and the neutral gas ([CI] and CO). A gas outflow with a line-of-sight velocity of 60 km/s is evident in both species. The center of the CND is bright in [OI], [OIII], and [CII]; [OI]63mu emission dominates that of [CII] even though it is absorbed with optical depths of 1.0-1.5. The outflow is well-traced by the [NII] and [NIII] lines and also seen in the [CII] and [OIII] lines that peak in the center. Ionized gas densities are moderate in the CND and low everywhere else. Neutral gas densities range from 4000 per cm3 (outflow, extended thin disk ETD) to 20 000 per cm3 (CND). The CND radiation field is weak compared to the ETD starburst field. The outflow has a much stronger radiation field. The total mass of all the CND gas is 9 x 10^(7) M(o) and the mass of the outflowing gas is only 15%-30% of that. The outflow most likely originates from the shock-dominated CND cavity surrounding the central black hole. With a factor of three uncertainty, the mass outflow rate is about 2 M(o)/yr, a thousand times higher than the accretion rate of the black hole. Without replenishment, the CND will be depleted in 15-120 million years. However, the outflow velocity is well below the escape velocity.
description: 14 pages, 9 figures. Accepted by Astronomy & Astrophysics
Deliverable 3.5: Training activities update
Creators: name: Kohl, Yvonne
name: Gabelova, Alena
name: Bozena Smolkova
name: Siposova, Tatiana
name: Earl, Julie
name: Kataki, Agapi
name: Dusinska, Maria
Publisher: name: Zenodo
Year: 2023
Subjects: Project management
Horizon 2020 projects

description: This deliverable D3.5 is an update on training activities performed within task 3.1 in the second period of the VISION project implementation. Short-term academic stays of early-stage researchers in partners' laboratories allowed the applicants to improve and acquire new scientific and technical skills in various cellular, molecular, and genetic techniques involved in basic and clinical research. Moreover, they had the opportunity to strengthen their personal and professional development in gastrointestinal cancer and nanobiotechnology. The involvement of early-stage researchers in such scientific events enhanced the reputation, credibility, attractiveness, and networking activities of BMC SAV at both international and national levels. Besides BMC SAV, also other VISION partners sent their early-stage scientists for short-term academic stays to partner laboratories.
 The coronavirus pandemic delayed the performance of training activities in 2020. In order to overcome these objective limitations in implementing the planned actions, and if it was possible, the training activities were replaced by theoretical courses and e-lectures (D3.1 Training activities). After the travel restrictions were removed, the first short-term early-stage researchers exchanges started in 2021, and the last academic stay finished in June 2023. At the 2nd Partner Assembly meeting in September 2021, the partners agreed to fully open all in-person training activities since January 2022. In total (2020-2023), 22 in-person training activities have been realized, and 28 early-stage researchers have participated. Some applicants were interested in more than one training.
Asymptotic expansion based equation of state for hard-disk fluids offering accurate virial coefficients
Creators: name: Tian, Jianxiang
name: Gui, Yuanxing
name: Mulero, A.
Publisher: name: arXiv
Year: 2016
Subjects: subject: Chemical Physics (physics.chem-ph)
subject: Soft Condensed Matter (cond-mat.soft)
subject: FOS: Physical sciences

description: Despite the fact that more that more than 30 analytical expressions for the equation of state of hard-disk fluids have been proposed in the literature, none of them is capable of reproducing the currently accepted numeric or estimated values for the first eighteen virial coefficients. Using the asymptotic expansion method, extended to the first ten virial coefficients for hard-disk fluids, fifty-seven new expressions for the equation of state have been studied. Of these, a new equation of state is selected which reproduces accurately all the first eighteen virial coefficients. Comparisons for the compressibility factor with computer simulations show that this new equation is as accurate as other similar expressions with the same number of parameters. Finally, the location of the poles of the 57 new equations shows that there are some particular configurations which could give both the accurate virial coefficients and the correct closest packing fraction in the future when higher virial coefficients than the tenth are numerically calculated.
description: 31 pages, 3 figures, 4 tables
Sets of Priors Reflecting Prior-Data Conflict and Agreement
Creators: name: Walter, Gero
name: Coolen, Frank P. A.
Publisher: name: arXiv
Year: 2016
Subjects: subject: Methodology (stat.ME)
subject: FOS: Computer and information sciences
subject: 62

description: In Bayesian statistics, the choice of prior distribution is often debatable, especially if prior knowledge is limited or data are scarce. In imprecise probability, sets of priors are used to accurately model and reflect prior knowledge. This has the advantage that prior-data conflict sensitivity can be modelled: Ranges of posterior inferences should be larger when prior and data are in conflict. We propose a new method for generating prior sets which, in addition to prior-data conflict sensitivity, allows to reflect strong prior-data agreement by decreased posterior imprecision.
description: 12 pages, 6 figures, In: Paulo Joao Carvalho et al. (eds.), IPMU 2016: Proceedings of the 16th International Conference on Information Processing and Management of Uncertainty in Knowledge-Based Systems, Eindhoven, The Netherlands
Crystal structures and high-temperature superconductivity in molybdenum-hydrogen binary system under high pressure
Creators: name: Yang, Aiqin
name: Tao, Xiangru
name: Quan, Yundi
name: Zhang, Peng
Publisher: name: arXiv
Year: 2023
Subjects: subject: Superconductivity (cond-mat.supr-con)
subject: FOS: Physical sciences

description: Motivated by advances in hydrogen-rich superconductors in the past decades, we conducted variable-composition structural searches in Mo-H binary system at high pressure. A new composition-pressure phase diagram of thermodynamically stable structures has been derived. Besides all previously discovered superconducting molybdenum hydrides, we also identified series of thermodynamically metastable superconducting structures, including I4/mmm-Mo$_3$H$_{14}$, I4cm-MoH$_9$, P4/nmm-MoH$_{10}$ and P42$_1$2-MoH$_{10}$, with the superconducting transition temperatures from 55 to 126 K at 300 GPa. In these superconducting molybdenum hydrides, vibrations of the Mo-atoms contributes significantly to the electron-phonon coupling and the superconducting transition temperature, in complementary to the contributions by the vibrations of the H-atoms. Our works highlight the importance of compounds with non-integer composition ratio and metastable states in material searches, for example the potential high temperature superconductors.
New Virial Equation of State for Hard-Disk Fluids
Creators: name: Tian, Jianxiang
name: Gui, Yuanxing
name: Mulero, A.
Publisher: name: arXiv
Year: 2016
Subjects: subject: Chemical Physics (physics.chem-ph)
subject: Soft Condensed Matter (cond-mat.soft)
subject: FOS: Physical sciences

description: Although many equations of state of hard-disk fluids have been proposed, none is capable of reproducing the currently calculated or estimated values of the first eighteen virial coefficients at the same time as giving very good accuracy when compared with computer simulation values for the compressibility factor over the whole fluid range. A new virial-based expression is here proposed which achieves these aims. For that, we use the fact that the currently accepted estimated values for the highest virial coefficients behave linearly with their order, and also that virial coefficients must have a limiting behaviour that permits the closest packing limit in the compressibility factor to be also adequately reproduced.
description: 21 pages, 3 figures, 2 tables
title: Правовой механизм в области государственного управления при реализации национальных проектов
Creators: name: Шарапова, Надежда
Publisher: name: Новгородский государственный университет имени Ярослава Мудрого (НовГУ)
Year: 2022

description: Национальные проекты являются важнейшей неотъемлемой частью реформы социальной сферы и экономики страны, положившей свое начало в 2018 году, путем издания Президентом Российской Федерации Указа «О национальных целях и стратегических задачах». В рамках действующей правовой системы осуществляется их реализация в области развития отдельных наиболее значимых сфер жизни общества. Однако несмотря на это, не исключается возможность возникновения различных нарушений и проблем правового регулирования, посредством которых допускается риск недостижения целей, обозначенных в разработанных паспортах национальных проектов. Исследование данной проблемы позволит отразить основные «болевые точки», возникающие при реализации национальных проектов. Помимо этого, проведенный анализ позволит проработать и сформировать собственные предложения по их устранению
NREM and REM: cognitive and energetic gains in thalamo-cortical sleeping and awake spiking model
Creators: name: De Luca, Chiara
name: Tonielli, Leonardo
name: Pastorelli, Elena
name: Capone, Cristiano
name: Simula, Francesco
name: Lupo, Cosimo
name: Bernava, Irene
name: Tiddia, Gianmarco
name: De Bonis, Giulia
name: Golosio, Bruno
name: Paolucci, Pier S.
Publisher: name: G-Node
Year: 2023
Subjects: Computational Neuroscience
Learning, plasticity and memory

description: Bernstein Conference 2023 abstract. https://bernstein-conference.de
Sonnenfleckenzeichnung Nr. 25966.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 06.08.1980, erstellt von Hans Ulrich Keller
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1980

description: Bleistiftzeichnung mit Tinte und Farbstift überschrieben, erstellt als Projektionsbildzeichnung in der Eidgenössischen Sternwarte Zürich. Instrument: Zeiss Coudé-Refraktor (150/2250 mm).
Die Beobachtungen zu Einzelflecken und zu Sonnenfleckengruppen wurden mit Bleistift auf einem Vordruck eingetragen. Zusätzlich notiert: Tabelle mit den statistischen Angaben, für die Werte g, f sowie Gr (Anzahl g)
Multi-compartment models with STDP on BrainScaleS-2
Creators: name: Dietrich, Robin
name: Spilger, Philipp
name: Müller, Eric C.
name: Knoll, Alois C.
name: Schemmel, Johannes
Publisher: name: G-Node
Year: 2023
Subjects: Computational Neuroscience
Learning, plasticity and memory

description: Bernstein Conference 2023 abstract. https://bernstein-conference.de
Sonnenfleckenzeichnung Nr. 26051.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 25.11.1980, erstellt von Hans Ulrich Keller
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1980

description: Bleistiftzeichnung mit Tinte und Farbstift überschrieben, erstellt als Projektionsbildzeichnung in der Eidgenössischen Sternwarte Zürich. Instrument: Zeiss Coudé-Refraktor (150/2250 mm).
Die Beobachtungen zu Einzelflecken und zu Sonnenfleckengruppen wurden mit Bleistift auf einem Vordruck eingetragen. Zusätzlich notiert: Tabelle mit den statistischen Angaben, für die Werte g, f sowie Gr (Anzahl g)
NIHAO X: Reconciling the local galaxy velocity function with Cold Dark Matter via mock HI observations
Creators: name: Macciò, Andrea V.
name: Udrescu, Silviu M.
name: Dutton, Aaron A.
name: Obreja, Aura
name: Wang, Liang
name: Stinson, Greg R.
name: Kang, Xi
Publisher: name: arXiv
Year: 2016
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We used 87 high resolution hydrodynamical cosmological simulations from the NIHAO suite to investigate the relation between the maximum circular velocity (Vmax) of a dark matter halo in a collisionless simulation and the velocity width of the HI gas in the same halo in the hydrodynamical simulation. These two quantities are normally used to compare theoretical and observational velocity functions and have led to a possible discrepancy between observations and predictions based on the Cold Dark Matter (CDM) model. We show that below 100 km/s, there is clear bias between HI based velocities and Vmax, that leads to an underestimation of the actual circular velocity of the halo. When this bias is taken into account the CDM model has no trouble in reproducing the observed velocity function and no lack of low velocity galaxies is actually present. Our simulations also reproduce the linewidth - stellar mass (Tully-Fisher) relation and HI sizes, indicating that the HI gas in our simulations is as extended as observed. The physical reason for the lower than expected linewidths is that, in contrast to high mass galaxies, low mass galaxies no longer have extended thin HI rotating disks, as is commonly assumed.
description: 7 pages, 4 figures, minor changes to match the version accepted on MNRAS Letters
Long-term plasticity induces changes in a small, but very specific group of synapses in a biophysically-detailed, large-scale cortical model
Creators: name: Ecker, András
name: Egas Santader, Daniela
name: Bolaños-Puchet, Sirio
name: Isbister, James B.
name: Reimann, Michael W.
Publisher: name: G-Node
Year: 2023
Subjects: Computational Neuroscience
Learning, plasticity and memory

description: Bernstein Conference 2023 abstract. https://bernstein-conference.de
Isophote Shapes of Early-Type Galaxies in Massive Clusters at $z\sim1$ and 0
Creators: name: Mitsuda, Kazuma
name: Doi, Mamoru
name: Morokuma, Tomoki
name: Suzuki, Nao
name: Yasuda, Naoki
name: Perlmutter, Saul
name: Aldering, Greg
name: Meyers, Joshua
Publisher: name: arXiv
Year: 2016
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We compare the isophote shape parameter $a_{4}$ of early-type galaxies (ETGs) between $z\sim1$ and 0 as a proxy for dynamics to investigate the epoch at which the dynamical properties of ETGs are established, using cluster ETG samples with stellar masses of $\log(M_{*}/M_{\odot})\geq10.5$ which have spectroscopic redshifts. We have 130 ETGs from the Hubble Space Telescope Cluster Supernova Survey for $z\sim1$ and 355 ETGs from the Sloan Digital Sky Survey for $z\sim0$. We have developed an isophote shape analysis method which can be used for high-redshift galaxies and has been carefully compared with published results. We have applied the same method for both the $z\sim1$ and $0$ samples. We find similar dependence of the $a_{4}$ parameter on the mass and size at $z\sim1$ and 0; the main population of ETGs changes from disky to boxy at a critical stellar mass of $\log(M_{*}/M_{\odot})\sim11.5$ with the massive end dominated by boxy. The disky ETG fraction decreases with increasing stellar mass both at $z\sim1$ and $0$, and is consistent between these redshifts in all stellar mass bins when the Eddington bias is taken into account. Although uncertainties are large, the results suggest that the isophote shapes and probably dynamical properties of ETGs in massive clusters are already in place at $z>1$ and do not significantly evolve in $z<1$, despite significant size evolution in the same galaxy population. The constant disky fraction favors less violent processes than mergers as a main cause of the size and morphological evolution of intermediate mass ETGs in $z<1$.
description: 22 pages, 21 figures. Accepted for publication in ApJ
Sonnenfleckenzeichnung Nr. 26002.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 16.09.1980, erstellt von Hans Ulrich Keller
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1980

description: Bleistiftzeichnung mit Tinte und Farbstift überschrieben, erstellt als Projektionsbildzeichnung in der Eidgenössischen Sternwarte Zürich. Instrument: Zeiss Coudé-Refraktor (150/2250 mm).
Die Beobachtungen zu Einzelflecken und zu Sonnenfleckengruppen wurden mit Bleistift auf einem Vordruck eingetragen. Zusätzlich notiert: Tabelle mit den statistischen Angaben, für die Werte g, f sowie Gr (Anzahl g)
Near-infrared dual-comb spectroscopy of CO2 and N2O with a discretized highly nonlinear fiber
Creators: name: Malfondet, Alix
name: Deroh, Moise
name: Ahmedou, Sidi-Ely
name: Parriaux, Alexandre
name: Hammani, Kamal
name: Dauliat, Romain
name: Labonté, Laurent
name: Tanzilli, Sébastien
name: Delagnes, Jean-Christophe
name: Roy, Philippe
name: Jamier, Raphaël
name: Millot, Guy
Publisher: name: arXiv
Year: 2023
Subjects: subject: Optics (physics.optics)
subject: FOS: Physical sciences
subject: 78-05

description: In this paper, we introduce an all-fibered dual-comb spectrometer based on a new design of highly nonlinear fiber to efficiently convert frequency combs from 1.55 micron to 2 micron We show that our spectrometer can be used to measure absorption profiles of rovibrational transitions of CO2 and N2O molecules, and especially their collisional self-broadening coefficients. The results show very good agreement with the HITRAN database and thus further measurements have been performed on a mixture CO2 /N2O to measure the broadening of the CO2 absorption lines resulting from the presence of N2O.
description: 26 pages, 11 figure, 1 table