cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
title: Alexandri Aphrodisiensis maximi Peripatetici, In Qvatvor Libros Meteorologicorvm Aristotelis, Commentatio lucidissima; 1561
title: Quæ omnia nuper maxima sunt diligentia castigata: Addito Indice Etiam Eorvm, quæ in commentatione Alexandri obseruatione digna annotatu sunt
titleType: Subtitle
Creators: name: Alexander Aphrodisiensis
name: Piccolomini, Alessandro
name: Aristoteles
name: Piccolomini, Alessandro
Publisher: name: Universitätsbibliothek der Ludwig-Maximilians-Universität München
Year: 2013

description: Bibliogr. Nachweis: Edit 16 CNCE 1073. - Vorlageform des Erscheinungsvermerks: Venetijs, Apud Hieronymum Scottum. M D LXI. - Einheitssacht. des komm. Werkes: Meteorologica
Ad Homeri Stvdiosos Adolescentes Abrahami Loescheri elegia, in qua summa librorum Homericorum continetur; [ca. 1560]
Creators: name: Lüttringhaus, Arthur
Publisher: name: Universitätsbibliothek der Ludwig-Maximilians-Universität München
Year: 2013

description: Text teils griech., teils lat.
The eclipse of the V773 Tau B circumbinary disk
Creators: name: Kenworthy, M. A.
name: Picos, D. González
name: Elizondo, E.
name: Martin, R. G.
name: van Dam, D. M.
name: Rodriguez, J. E.
name: Kennedy, G. M.
name: Ginski, C.
name: Mugrauer, M.
name: Vogt, N.
name: Adam, C.
name: Oelkers, R. J.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: A deep (~70%) and extended (~150 days) eclipse was seen towards the young multiple stellar system V773 Tau in 2010. We interpret it as due to the passage of a circumbinary disk around the B components moving in front of the A components. Our aim is to characterise the orientation and structure of the disk, to refine the orbits of the subcomponents, and to predict when the next eclipse will occur. We combine the photometry from several ground based surveys, construct a model for the light curve of the eclipse, and use high angular resolution imaging to refine the orbits of the three components of the system, A, B and C. Frequency analysis of the light curves, including from the TESS satellite, enables characterisation of the rotational periods of the Aa and Ab stars. A toy model of the circumbinary disk shows that it extends out to approximately 5 au around the B binary and has an inclination of 73 degrees with respect to the orbital plane of AB, where the lower bound of the radius of the disk is constrained by the geometry of the AB orbit and the upper bound is set by the stability of the disk. We identify several frequencies in the photometric data that we attribute to rotational modulation of the Aa and Ab stellar companions. We produce the first determination of the orbit of the more distant C component around the AB system and limit its inclination to 93 degrees. The high inclination and large diameter of the disk, together with the match from theory suggest that B is an almost equal mass, moderately eccentric binary. We identify the rotational periods of the Aa and Ab stars, identify a third frequency in the light curve that we attribute to the orbital period of the stars in the B binary. We predict that the next eclipse will be around 2037, during which both detailed photometric and spectroscopic monitoring will characterise the disk in greater detail.
description: 13 pages, 15 figures, 5 tables, A&A in press. All data and reduction scripts available at https://github.com/mkenworthy/V773TauBdisk
Anguis graeca Bedriaga 1881
Creators: name: Sindaco, Roberto
name: Rossi, Roberta
Publisher: name: Zenodo
Year: 2020
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Reptilia
Squamata
Anguidae
Anguis
Anguis graeca

description: Anguis graeca Bedriaga, 1881
The only record of the Greek Slow Worm from Lefkada is due to Werner (1894: 232). Its occurrence on the island is confirmed after over a century by a citizen science record from near Vasiliki (10/11/2019), where a dead specimen was photographed.
description: Published as part of Sindaco, Roberto & Rossi, Roberta, 2020, Annotated checklist of the herpetofauna (Amphibia, Reptilia) of Lefkada Island (Ionian Islands, Greece), pp. 57-68 in Natural History Sciences 7 (2) on page 60, DOI: 10.4081/nhs.2020.480, http://zenodo.org/record/12753965
The fundamental theorem of cubical small cancellation theory
Creators: name: Jankiewicz, Kasia
Publisher: name: arXiv
Year: 2014
Subjects: subject: Group Theory (math.GR)
subject: FOS: Mathematics

description: We give a new proof of the main theorem in the theory of C(6) small cancellation complexes. We prove the fundamental theorem of cubical small cancellation theory for C(9) cubical small cancellation complexes.
description: 35 pages
Epixerus Thomas 1909
Creators: name: Honacki, James H.
name: Kinman, Kenneth E.
name: Koeppl, James W.
Publisher: name: Zenodo
Year: 1982
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Rodentia
Sciuridae
Epixerus

description: Epixerus Thomas, 1909. Ann. Mag. Nat. Hist., 8 (3):472. ISIS NUMBER: 5301410002006000000.
description: Published as part of James H. Honacki, Kenneth E. Kinman & James W. Koeppl, 1982, Order Rodentia (Part 1), pp. 345-382 in Mammal Species of the World (1 st Edition), Lawrence, Kansas, USA :Alien Press, Inc. & The Association of Systematics Collections on page 349, DOI: 10.5281/zenodo.7353023
Analysis of $Ω(2012)$ as a molecule in the chiral quark model
Creators: name: Hu, Xiaohuang
name: Ping, Jialun
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: Inspired by the updated information on $Ω(2012)$ by the Belle Collaboration, we conduct a study of all possible $S$-wave pentaquark systems with quark contents $sssq\bar{q},q=u,d$ in a chiral quark model with the help of Gaussian expansion method. Channel coupling is also considered. The real-scaling method (stabilization method) is employed to identify and check the bound states and the genuine resonances. In addition, the decay widths of all resonances are given. The results show that $Ω(2012)$ can be interpreted as a $Ξ^*K$ molecular state with quantum number of $IJ^P=0(\frac{3}{2})^-$. Other resonances are obtained: $Ξ^* K^*$ with $IJ^P=0(\frac{1}{2})^-$ and$0(\frac{3}{2})^-$, $Ωπ$ with $IJ^P=1(\frac{3}{2})^-$. These pentaquark states is expected to be further verified in future experiments.
description: 10 pages, 5 figures. arXiv admin note: text overlap with arXiv:2109.09972
title: The LIBERATOR Archive, October 2019
title: Official Publication of the Liberal Arts Council
titleType: AlternativeTitle
Creators: name: University Of Texas At Austin
Publisher: name: University of Texas at Austin
Year: 2019
Subjects: Liberal Arts
railway
midsommar
fashion
disney
Diwali
music
television
vignette
Chernobyl
air condition

description: Contents: October 3, 2019 Train of Thought: Laowai Reflections on the Railway // by Varun Hukeri -- October 5, 2019 The Power of Weakness, Womanhood, and Empathy in Midsommar // by Michaela Lavelle -- October 15, 2019 Trash Makeover Challenge Inspires Local Artists to Create Sustainable Fashion // by Alyssa Hiarker -- October 17, 2019 Movement // by Kate Diller -- October 20, 2019 Bad Disney Channel Movies – The UTea Podcast Episode 1 // by Allison McCarty, Elena Edwards, Mariah Sanchez, and Valeria Colunga -- October 21, 2019 Diwali: Christmas in October // by Rohin Balkundi -- October 23, 2019 Malleable Metal // by Harrison Fernelius -- October 26, 2019 Techno-Paranoia and the Allure of Black Mirror // by Hayle Chen -- October 27, 2019 Dueling Vignettes // by Cameron Waltz -- October 27, 2019 Chernobyl Part One – The UTea Podcast Episode 2 // by Allison McCarty, Hubert Ning, Rohin Balkundi, and Terrane Ansley -- October 30, 2019 “Bleed Orange, Live Green”…Waste AC Energy? // by Morgan Jeitler -- October 31, 2019 You Can’t Kill the Undead: The Twilight Renaissance in 2019 // by Frida Silva
Enumeration Schemes for Words Avoiding Patterns With Repeated Letters
Creators: name: Pudwell, Laura
Publisher: name: Zenodo
Year: 2008

description: We discuss the enumeration of words avoiding patterns with repeated letters. More specifically, we find enumeration schemes (i.e., recurrences) to count pattern-avoiding words using a divide-and-conquer technique, breaking up a set of words based on the pattern formed by the smallest letters of each word. We apply this method to the counting of words avoiding patterns of length 3 and words avoiding any monotone pattern.
Pseudopus apodus subsp. thracius Obst 1978
Creators: name: Sindaco, Roberto
name: Rossi, Roberta
Publisher: name: Zenodo
Year: 2020
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Reptilia
Squamata
Anguidae
Pseudopus
Pseudopus apodus
Pseudopus apodus thracius obst, 1978

description: Pseudopus apodus thracius Obst, 1978
Available records of the Glass Lizard on Lefkada are scarce, both in literature (Werner, 1929: 474; Schmid, 2019: 72) and in the web: Ligia (17/6/2019) and Vasiliki (30/4/2019).
We found this species at several places: Agios Petros (17/5/2019), Komilio (23/5/2019), Livadia (24/5/2019), between Asprogerakata and Apolpaina (24/5/2019), Poros (25/5/2019), and Spanochori (26/5/2019; Fig. 2F).
description: Published as part of Sindaco, Roberto & Rossi, Roberta, 2020, Annotated checklist of the herpetofauna (Amphibia, Reptilia) of Lefkada Island (Ionian Islands, Greece), pp. 57-68 in Natural History Sciences 7 (2) on page 60, DOI: 10.4081/nhs.2020.480, http://zenodo.org/record/12753965
Documenting is not enough : an example of collaborative work in a French Research Infrastructure
Creators: name: Petorin, Elodie
name: Chmilevschi, Ada
Publisher: name: Zenodo
Year: 2020

description: The question of data access has become an increasingly important topic in scientific research: the FAIR principle, the Research Data Alliance, the Open Science Cloud, etc... As a matter of fact, the challenge of data and metadata findable, accessible, interoperable and reusable (FAIR) is becoming more and more important in the scientific community these days. But yet, how can we produce FAIR data? Also, how to disseminate them? The Large Research Infrastructure Progedo has set up a network of university data platform, each of these skills platforms aims to provide real supports which form the necessary link between digital platforms and users. Furthermore, the interest of working upstream the data production, in collaboration with the researchers, allows us to obtain detailed documentation consisting in document of context as well as metadata. Moreover, downstream the chain of data, the national archive of data from official statistics (ADISP), a service of Progedo, documents those metadata to the DDI standard and disseminate it to the European scientific community. To conclude, the purpose of this presentation will be to highlight the betterment of this collaborative work between Adisp and the university data platform in the data life cycle and the interest of it.
Constraints on primordial magnetic fields from CMB distortions in the axiverse
Creators: name: Tashiro, Hiroyuki
name: Silk, Joseph
name: Marsh, David J. E.
Publisher: name: arXiv
Year: 2013
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Measuring spectral distortions of the cosmic microwave background (CMB) is attracting considerable attention as a probe of high energy particle physics in the cosmological context, since PIXIE and PRISM have recently been proposed. In this paper, CMB distortions due to resonant conversions between CMB photons and light axion like particles (ALPs) are investigated, motivated by the string axiverse scenario which suggests the presence of a plenitude of light axion particles. Since these resonant conversions depend on the strength of primordial magnetic fields, constraints on CMB distortions can provide an upper limit on the product of the photon-ALP coupling constant g and the comoving strength of primordial magnetic fields B. Potentially feasible constraints from PIXIE/PRISM can set a limit g B < 10^{-16} GeV^{-1} nG for ALP mass, m_ϕ< 10^{-14} eV. Although this result is not a direct constraint on g and B, it is significantly tighter than the product of the current upper limits on g and B.
description: 8 pages, 3 figures
Epixerus ebii
Creators: name: Honacki, James H.
name: Kinman, Kenneth E.
name: Koeppl, James W.
Publisher: name: Zenodo
Year: 1982
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Rodentia
Sciuridae
Epixerus
Epixerus ebii

description: Epixerus ebii (Temminck, 1853). Esquisses Zool. sur la Cote de Guine, p. 129. TYPE LOCALITY: Ghana. DISTRIBUTION: Sierra Leone to Ghana. COMMENT: Includes jonesi; formerly included wilsoni; see Robbins and Schütter, 1977, Saugetierk. Mitt., 25:22-23. PROTECTED STATUS: CITES - Appendix III (Ghana). ISIS NUMBER: 5301410002006001001.
description: Published as part of James H. Honacki, Kenneth E. Kinman & James W. Koeppl, 1982, Order Rodentia (Part 1), pp. 345-382 in Mammal Species of the World (1 st Edition), Lawrence, Kansas, USA :Alien Press, Inc. & The Association of Systematics Collections on page 349, DOI: 10.5281/zenodo.7353023
A Propound Method for the Improvement of Cluster Quality
Creators: name: Bhatia, Shveta Kundra
name: Dixit, V. S.
Publisher: name: arXiv
Year: 2013
Subjects: subject: Machine Learning (cs.LG)
subject: FOS: Computer and information sciences

description: In this paper Knockout Refinement Algorithm (KRA) is proposed to refine original clusters obtained by applying SOM and K-Means clustering algorithms. KRA Algorithm is based on Contingency Table concepts. Metrics are computed for the Original and Refined Clusters. Quality of Original and Refined Clusters are compared in terms of metrics. The proposed algorithm (KRA) is tested in the educational domain and results show that it generates better quality clusters in terms of improved metric values.
A multi-simulation study of relativistic SZ temperature scalings in galaxy clusters and groups
Creators: name: Lee, Elizabeth
name: Anbajagane, Dhayaa
name: Singh, Priyanka
name: Chluba, Jens
name: Nagai, Daisuke
name: Kay, Scott T.
name: Cui, Weiguang
name: Dolag, Klaus
name: Yepes, Gustavo
Publisher: name: arXiv
Year: 2022
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: The Sunyaev-Zeldovich (SZ) effect is a powerful tool in modern cosmology. With future observations promising ever improving SZ measurements, the relativistic corrections to the SZ signals from galaxy groups and clusters are increasingly relevant. As such, it is important to understand the differences between three temperature measures: (a) the average relativistic SZ (rSZ) temperature, (b) the mass-weighted temperature relevant for the thermal SZ (tSZ) effect, and (c) the X-ray spectroscopic temperature. In this work, we compare these cluster temperatures, as predicted by the {\sc Bahamas} \& {\sc Macsis}, {\sc Illustris-TNG}, {\sc Magneticum}, and {\sc The Three Hundred Project} simulations. Despite the wide range of simulation parameters, we find the SZ temperatures are consistent across the simulations. We estimate a $\simeq 10\%$ level correction from rSZ to clusters with $Y\simeq10^{-4}$~Mpc$^{-2}$. Our analysis confirms a systematic offset between the three temperature measures; with the rSZ temperature $\simeq 20\%$ larger than the other measures, and diverging further at higher redshifts. We demonstrate that these measures depart from simple self-similar evolution and explore how they vary with the defined radius of haloes. We investigate how different feedback prescriptions and resolution affect the observed temperatures, and discover the SZ temperatures are rather insensitive to these details. The agreement between simulations indicates an exciting avenue for observational and theoretical exploration, determining the extent of relativistic SZ corrections. We provide multiple simulation-based fits to the scaling relations for use in future SZ modelling.
description: Accepted by MNRAS
THE INFLUENCE OF PRACTICAL WORK IN SCHOOLS ON THE FORMATION OF TEACHERS' ERUDITION
Creators: name: Jo`rayeva Gulshodaxon
Publisher: name: Zenodo
Year: 2024

description: Abstract: The article examines the influence of practical work in the school environment on the development of teachers' erudition. The study was conducted in order to identify how the active involvement of teachers in practical activities within the school contributes to their professional growth and knowledge expansion. The author analyzes various methods of working with teachers, such as seminars, master classes, training courses and pedagogical practice. Special attention is paid to how these forms of practical work contribute to the deepening of teachers' knowledge in the field of the subject, pedagogical techniques, as well as to improving their professional competence. The results of the study can be useful both for teachers seeking self-development and for the school administration when planning professional development programs for staff.

Keywords: practical work in schools, formation of teacher erudition, educational process, teaching methods, professional development, pedagogical practice, curricula, integration of knowledge, pedagogical competencies, learning environment, educational effectiveness.
title: The LIBERATOR Archive, October 2020
title: Official Publication of the Liberal Arts Council
titleType: AlternativeTitle
Creators: name: University Of Texas At Austin
Publisher: name: University of Texas at Austin
Year: 2020
Subjects: Liberal Arts
poem
horror
film

description: Contents: October 25, 2020 Poems // by Aryan Bhalla -- October 31, 2020 The Only Thing to Fear Is Fear Itself: Horror Movies and the Social Consciousness // by Alyssa Hiarker
An estimation of local bulk flow with the maximum-likelihood method
Creators: name: Ma, Yin-Zhe
name: Pan, Jun
Publisher: name: arXiv
Year: 2013
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: A maximum-likelihood method, tested as an unbiased estimator from numerical simulations, is used to estimate cosmic bulk flow from peculiar velocity surveys. The likelihood function is applied to four observational catalogues (ENEAR, SFI++, A1SN and SC) constructed from galaxy peculiar velocity surveys and Type-Ia supernovae data at low redshift ($z \leq 0.03$). We find that the Spiral Field {\it I}-band catalogue constrains the bulk flow to be $V=290 \pm 30 {\,{\rm km}\,{\rm s}^{-1}}$ towards $l=281^{\circ} \pm 7^{\circ}$, $b=8^{\circ +6^{\circ}}_{-5^{\circ}}$ on effective scales of $ 58 {\,{h^{-1} {\rm Mpc}}}$, which is the tightest constraints achievable at the present time. By comparing the amplitudes of our estimated bulk flows with theoretical prediction, we find excellent agreement between the two. In addition, directions of estimated bulk flows are also consistent with measurements in other studies.
description: 10 pages, 15 figures, and table 4, 2013, MNRAS, doi: 10.1093
"param_card.SM.C1C1.SlepSnu.dat" of "Search for electroweak production of supersymmetric particles in final states with two or three leptons at $\sqrt{s}=13\,$TeV with the ATLAS detector"
Creators: name: ATLAS Collaboration
Publisher: name: HEPData
Year: 2018

description: SLHA file for benchmark signal
description: No description provided.
A study of the NGC 1193 and NGC 1798 open clusters using CCD UBV photometric and Gaia EDR3 data
Creators: name: Yontan, T.
name: Cakmak, H.
name: Bilir, S.
name: Banks, T.
name: Raul, M.
name: Canbay, R.
name: Koc, S.
name: Tasdemir, S.
name: Ercay, H.
name: Ozturk, B. Tanik
name: Dursun, D. C.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We present photometric, astrometric, and kinematic studies of the old open star clusters NGC 1193 and NGC 1798. Both of the clusters are investigated by combining data sets from Gaia EDR3 and CCD UBV observational data. Analysis of the radial distribution of stars through the cluster regions indicates that the cluster limit radii are $r_{\rm lim}=8'$ for both of the clusters. We determine the membership probabilities of stars considering Gaia EDR3 proper motion and trigonometric parallax data, resulting in 361 stars in NGC 1193 and 428 in NGC 1798 being identified as most likely cluster members, having membership probabilities greater than P>0.5. Mean proper motion components are estimated as ($μ_α\cos δ$, $μ_δ) = (-0.207(0.009), -0.431(0.008)$) for NGC 1193 and ($μ_α\cos δ$, $μ_δ)=(0.793(0.006), -0.373(0.005)$) mas/yr for NGC 1798. E(B-V) color excesses were derived for NGC 1193 as $0.150(0.037)$ and for NGC 1798 as 0.505(0.100) mag through the use of two-color diagrams. Photometric metallicities are also determined from two-color diagrams with the results of [Fe/H] = -0.30(0.06) dex for NGC 1193 and [Fe/H]=-0.20(0.07) dex for NGC 1798. The isochrone fitting distance and age of NGC 1193 are 5562(381) pc and 4.6(1) Gyr, respectively. For NGC 1798, these parameters are 4451(728) pc and 1.3(0.2) Gyr. These ages indicate that NGC 1193 and NGC 1798 are old open clusters. The overall present-day mass function slopes for main-sequence stars are found as 1.38(2.16) for NGC 1193 and 1.30(0.21) for NGC 1798, which are in fair agreement with the value of Salpeter (1955). Kinematic and dynamic orbital calculations indicate that NGC 1193 and NGC 1798 belong to the thick-disk and thin-disk populations, respectively. In addition, both of the clusters were born outside the solar circle, and both orbit in the metal-poor region of the Galactic disk.
description: Comments: 29 pages, including 13 figures and 4 tables, accepted for publication in the Revista Mexicana de Astronom\'ia y Astrof\'isica
Transition states and thermal collapse of dipolar Bose-Einstein condensates
Creators: name: Junginger, Andrej
name: Kreibich, Manuel
name: Main, Jörg
name: Wunner, Günter
Publisher: name: arXiv
Year: 2013
Subjects: subject: Quantum Gases (cond-mat.quant-gas)
subject: Chaotic Dynamics (nlin.CD)
subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We investigate thermally excited, dipolar Bose-Einstein condensates. Quasi-particle excitations of the atomic cloud cause density fluctuations which can induce the collapse of the condensate if the inter-particle interaction is attractive. Within a variational approach, we identify the collectively excited stationary states of the gas which form transition states on the way to the BEC's collapse. We analyze transition states with different $m$-fold rotational symmetry and identify the one which mediates the collapse. The latter's symmetry depends on the trap aspect ratio of the external trapping potential which determines the shape of the BEC. Moreover, we present the collapse dynamics of the BEC and calculate the corresponding decay rate using transition state theory. We observe that the thermally induced collapse mechanism is important near the critical scattering length, where the lifetime of the condensate can be significantly reduced. Our results are valid for an arbitrary strength of the dipole-dipole interaction. Specific applications are discussed for the elements $^{52}$Cr, $^{164}$Dy and $^{168}$Er with which dipolar BECs have been experimentally realized.
description: 10 pages, 6 figures
Tunable electronic correlation effects in nanotube-light interactions
Creators: name: Miyauchi, Yuhei
name: Zhang, Zhengyi
name: Takekoshi, Mitsuhide
name: Tomio, Yuh
name: Suzuura, Hidekatsu
name: Perebeinos, Vasili
name: Deshpande, Vikram V.
name: Lu, Chenguang
name: Berciaud, Stéphane
name: Kim, Philip
name: Hone, James
name: Heinz, Tony F.
Publisher: name: arXiv
Year: 2013
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: Electronic many-body correlation effects in one-dimensional (1D) systems such as carbon nanotubes have been predicted to modify strongly the nature of photoexcited states. Here we directly probe this effect using broadband elastic light scattering from individual suspended carbon nanotubes under electrostatic gating conditions. We observe significant shifts in optical transition energies, as well as line broadening, as the carrier density is increased. The results demonstrate the differing role of screening of many-body electronic interactions on the macroscopic and microscopic length scales, a feature inherent to quasi-1D systems. Our findings further demonstrate the possibility of electrical tuning of optical transitions and provide a basis for understanding of various optical phenomena in carbon nanotubes and other quasi-1D systems in the presence of charge carrier doping.
description: 18 pages, 4 figures, plus supplemental material of 11 pages and 3 figures
Quantum many-body scars of spinless fermions with density-assisted hopping in higher dimensions
Creators: name: Tamura, Kensuke
name: Katsura, Hosho
Publisher: name: arXiv
Year: 2022
Subjects: subject: Quantum Physics (quant-ph)
subject: Statistical Mechanics (cond-mat.stat-mech)
subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: We introduce a class of spinless fermion models that exhibit quantum many-body scars (QMBS) originating from kinetic constraints in the form of density-assisted hopping. The models can be defined on any lattice in any dimension and allow for spatially varying interactions. We construct a tower of exact eigenstates with finite energy density, and we demonstrate that these QMBS are responsible for the nonthermal nature of the system by studying the entanglement entropy and correlation functions. The quench dynamics from certain initial states is also investigated, and it is confirmed that the QMBS induce nonthermalizing dynamics. As another characterization of the QMBS, we give a parent Hamiltonian for which the QMBS are unique ground states. We also prove the uniqueness rigorously.
description: 12 pages, 8 figures, v3: minor corrections, Appendix C added, one figure removed
Toward a Population Synthesis of Disks and Planets I. Evolution of Dust with Entrainment in Winds and Radiation Pressure
Creators: name: Burn, Remo
name: Emsenhuber, Alexandre
name: Weder, Jesse
name: Völkel, Oliver
name: Klahr, Hubert
name: Birnstiel, Til
name: Ercolano, Barbara
name: Mordasini, Christoph
Publisher: name: arXiv
Year: 2022
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: Millimeter astronomy provides valuable information on the birthplaces of planetary systems. In order to compare theoretical models with observations, the dust component has to be carefully calculated. Here, we aim to study the effects of dust entrainment in photoevaporative winds and the ejection and drag of dust due to effects caused by radiation from the central star. We improved and extended the existing implementation of a two-population dust and pebble description in the global Bern/Heidelberg planet formation and evolution model. Modern prescriptions for photoevaporative winds were used and we account for settling and advection of dust when calculating entrainment rates. In order to prepare for future population studies with varying conditions, we explore a wide range of disk-, photoevaporation-, and dust-parameters. We find that if dust can grow to pebble sizes, that is, if they are resistant to fragmentation or turbulence is weak, drift dominates and the entrained mass is small but larger than under the assumption of no vertical advection of grains with the gas flow. For the case of fragile dust shattering at velocities of 1 m/s - as indicated in laboratory experiments -, an order of magnitude more dust is entrained which becomes the main dust removal process. Radiation pressure effects disperse massive, dusty disks on timescales of a few 100 Myr. These results highlight the importance of dust entrainment in winds as a solid mass removal process. Furthermore, this model extension lies the basis for future statistical studies of planet formation in their birth environment.
description: Accepted for publication in A&A
On Thompson's group T and algebraic K-theory
Creators: name: Geoghegan, Ross
name: Varisco, Marco
Publisher: name: arXiv
Year: 2014
Subjects: subject: Geometric Topology (math.GT)
subject: K-Theory and Homology (math.KT)
subject: FOS: Mathematics
subject: 19B28, 57M07, 20F65

description: Using a theorem of Lück-Reich-Rognes-Varisco, we show that the Whitehead group of Thompson's group T is infinitely generated, even when tensored with the rationals. To this end we describe the structure of the centralizers and normalizers of the finite cyclic subgroups of T, via a direct geometric approach based on rotation numbers. This also leads to an explicit computation of the source of the Farrell-Jones assembly map for the rationalized higher algebraic K-theory of the integral group ring of T.
description: Final version, 12 pages
Epixerus wilsoni du Chaillu 1860
Creators: name: Honacki, James H.
name: Kinman, Kenneth E.
name: Koeppl, James W.
Publisher: name: Zenodo
Year: 1982
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Rodentia
Sciuridae
Epixerus
Epixerus wilsoni

description: Epixerus wilsoni du Chaillu, 1860. Proc. Boston Soc. Nat. Hist., 7:364. TYPE LOCALITY: Gabon. DISTRIBUTION: Cameroun to Gabon. COMMENT: Amtmann, 1975, Part 6.1:6-7, included wilsoni with ebii, but Robbins and Schlitter, 1977, Saugetierk. Mitt., 25:22-23, recognized wilsoni as a distinct species. ISIS NUMBER: 5301410002006002001.
description: Published as part of James H. Honacki, Kenneth E. Kinman & James W. Koeppl, 1982, Order Rodentia (Part 1), pp. 345-382 in Mammal Species of the World (1 st Edition), Lawrence, Kansas, USA :Alien Press, Inc. & The Association of Systematics Collections on page 349, DOI: 10.5281/zenodo.7353023
description: {"references": ["Amtmann, E. 1975. Family Sciuridae. Part 6. 1. Pp. 1 - 12, in The mammals of Africa: An identification manual (J. Meester and H. W. Setzer, eds.) [issued 10 Dec 1975]. Smithsonian Institution Press, Washington, D. C., not continuously paginated."]}
Imaging in Reflecting Spheres
Creators: name: Eckmann, Jean-Pierre
name: Gunaratne, Gemunu H.
name: Shulman, Jason
name: Wood, Lowell T.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Optics (physics.optics)
subject: Mathematical Physics (math-ph)
subject: FOS: Physical sciences

description: We study the formation of images in a reflective sphere in three configurations using caustics of the field of light rays. The optical wavefront emerging from a source point reaching a subject following passage through the optical system is, in general, a Gaussian surface with partial focus along the two principal directions of the Gaussian surface; i.e. there are two images of the source point, each with partial focus. As the source point moves, the images move on two surfaces, referred to as \emph{viewable surfaces}. In our systems, one viewable surface consists of points with radial focus and the other consists of points with azimuthal focus. The problems we study are (1) imaging of a parallel beam of light, (2) imaging of the infinite viewed from a location outside the sphere, and (3) imaging of a planar object viewed through the point of its intersection with the radial line normal to the plane. We verify the existence of two images experimentally and show that the distance between them agrees with the computations.
Stellar Energetic Particle Transport in the Turbulent and CME-disrupted Stellar Wind of AU~Microscopii
Creators: name: Fraschetti, F.
name: Alvarado-Gómez, J. D.
name: Drake, J. J.
name: CoheN, O.
name: Garraffo, C.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Space Physics (physics.space-ph)
subject: FOS: Physical sciences

description: Energetic particles emitted by active stars are likely to propagate in astrospheric magnetized plasma turbulent and disrupted by the prior passage of energetic Coronal Mass Ejections (CMEs). We carried out test-particle simulations of $\sim$ GeV protons produced at a variety of distances from the M1Ve star AU~Microscopii by coronal flares or travelling shocks. Particles are propagated within the large-scale quiescent three-dimensional magnetic field and stellar wind reconstructed from measured magnetograms, and { within the same stellar environment following passage of a $10^{36}$~erg kinetic energy CME}. In both cases, magnetic fluctuations with an isotropic power spectrum are overlayed onto the large scale stellar magnetic field and particle propagation out to the two innnermost confirmed planets is examined. In the quiescent case, the magnetic field concentrates the particles onto two regions near the ecliptic plane. After the passage of the CME, the closed field lines remain inflated and the re-shuffled magnetic field remains highly compressed, shrinking the scattering mean free path of the particles. In the direction of propagation of the CME-lobes the subsequent EP flux is suppressed. Even for a CME front propagating out of the ecliptic plane, the EP flux along the planetary orbits highly fluctuates and peaks at $\sim 2 -3$ orders of magnitude higher than the average solar value at Earth, both in the quiescent and the post-CME cases.
description: 19 pages, 14 figures, submitted
Ferromagnetic Quantum Criticality Studied by Hall Effect Measurements in UCoAl
Creators: name: Combier, Tristan
name: Aoki, Dai
name: Knebel, Georg
name: Flouquet, Jacques
Publisher: name: arXiv
Year: 2013
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: Hall effect measurements were performed under pressure and magnetic field up to 2.2 GPa and 16 T on a single crystal of UCoAl. At ambient pressure, the system undergoes a first order metamagnetic transition at the critical field B_m = 0.7 T from a paramagnetic ground state to a field-induced ferromagnetic state. The Hall signal is linear at low field and shows a step-like anomaly at the transition, with only little change of the Hall coefficient. The anomaly is sharpest at the temperature of the critical end point T_0 = 12 K above which the first order metamagnetic transition becomes a crossover. Under pressure B_m increases and T_0 decreases. The step-like anomaly in the Hall effect disappears at P_M ~= 1.3 GPa and the metamagnetic transition is not detected above the quantum critical end point (QCEP) at P_Delta ~= 1.7 GPa, B_m ~= 7 T. Using magnetization data, we analyse our Hall resistivity data at ambient pressure in order to quantitatively account for both ordinary and anomalous contributions to the Hall effect. Under pressure, a drastic change in the field dependence of the Hall coefficient is found on crossing the QCEP. A possible Fermi surface change at B_m remains an open question.
description: 7 pages, 10 figures, accepted for publication in the Journal of the Physical Society of Japan manuscript number 66092
Trisunius cultellatus ASSING 2011
Creators: name: Assing, Volker
Publisher: name: Zenodo
Year: 2015
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Staphylinidae
Trisunius
Trisunius cultellatus

description: Trisunius cultellatus ASSING, 2011(Map 3) M a t e r i a l e x a m i n e d: China Y u n n a n: 13, 1♀, mountains NW Dongchuan, 26°10'N, 103°04'E, 2350 m, trail margin, litter and soil between herbs sifted, 8.VIII.2014, leg. Assing (cAss); 233, 2♀♀, 3 exs., E Kunming, Xiaobailong Forest Park, 24°56'N, 103°05'E, 2110 m, secondary pine forest, pine litter and litter at trail margin sifted, 10.VIII.2014, leg. Assing & Schülke (cAss, cSch); 1 3, mountains W Dongchuan, Sedan Snow Mountain Scenic Resort, 26°06'N, 102°55'E, 2620 m, secondary pine forest, litter, moss, and roots of herbs sifted, 14.VIII.2014, leg. Assing (cAss); 1♀, mountain W Xundian, 25°35' N, 103°09'E, 2200 m, mixed forest with alder and pine, bark of rotting pine trunk with termites sifted, 15.VIII.2014, leg. Assing (cAss). Vietnam: 13, 7 km NW Sa Pa, 22°22'N, 103°47'E, 1840 m, steep moist stream valley with bushes and trees, litter and roots of herbs sifted, 30.VII.2013, leg. Wunderle (cAss); 13, pass 8 km WNW Sa Pa, 22°21'N, 103°46'E, 2010 m, secondary d eciduous forest with bamboo, forest margin with bushes, litter, moss, and roots sifted, 5.VIII.2013, leg. Assing (cAss); 1 ♀, same data, but 6.VIII.2013 (cWun); 333, 5♀♀, pass 8 km NW Sa Pa, 22°21'N, 103°46'E, 2030 m, margin of secondary deciduous forest with bushes, bamboo, and herbs, litter, roots, and moss sifted, 9.VIII.2013, leg. Assing & Wunderle (cAss, cWun); 1 ♀, same data, but 10.VIII.2013, leg. Assing (cAss). C o m m e n t: This wing-dimorphic species is the most widespread representative of the genus in China, where it has been recorded from numerous localities in Yunnan and Shaanxi (ASSING 2011, 2013, 2014). The above material represents the first records from eastern Yunnan and Vietnam (Map 3). All the exam ined specimens from Vietnam are micropterous.
description: Published as part of Assing, Volker, 2015, A revision of Trisunius V. Three new species and additional records, including the first records of the genus from Vietnam (Coleoptera: Staphylinidae: Paederinae), pp. 1179-1190 in Linzer biologische Beiträge 47 (2) on page 1182, DOI: 10.5281/zenodo.5184218
description: {"references": ["ASSING V. (2011): Trisunius gen. nov. from the southern East Palaearctic and the Oriental regions (Coleoptera: Staphy linidae: Paederinae: Medonina). - Linzer Biologische Beitrage 43 (1): 195 - 220.", "ASSING V. (2013): A revision of Trisunius III. Three new species from North India and Nepal, and additional records (Coleoptera: Staphylinidae: Paederinae). - Linzer Biologis che Beitrage 45 (2): 1531 - 1540.", "ASSING V. (2014): A revision of Trisunius IV. Two new species and additional records from China (Coleoptera: S taphylinidae: Paederinae). - Linzer Biologische Beitrage 46 (1): 443 - 448."]}
Challenges for QCD theory - some personal reflections -
Creators: name: Sjöstrand, T.
Publisher: name: arXiv
Year: 2013
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: At the LHC all processes are QCD ones, whether "signal" or "background". In this review the frontiers of current QCD research are addressed, towards increased understanding, improved calculational precision, and role in potential future discoveries. Issues raised include the limits of perturbative QCD calculations and parton distribution usage, the nature of multiparton interactions, the impact of colour reconnection on physical observables, the need for progress on hadronization modelling, the improvements of parton showers and their combination with the matrix-element description, the use of QCD concepts in Beyond-the-Standard-Model scenarios, and the key position of event generators and other software in the successful exploration of LHC physics. On the way, several questions are posed, where further studies are needed.
description: 14 pages, to appear in the proceedings of the Nobel Symposium on LHC results, Uppsala, Sweden, 13 -- 17 May 2013
Eupetaurus Thomas 1888
Creators: name: Honacki, James H.
name: Kinman, Kenneth E.
name: Koeppl, James W.
Publisher: name: Zenodo
Year: 1982
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Rodentia
Sciuridae
Eupetaurus

description: Eupetaurus Thomas, 1888. J. Asiat. Soc. Bengal, 57:256. ISIS NUMBER: 5301410002042000000.
description: Published as part of James H. Honacki, Kenneth E. Kinman & James W. Koeppl, 1982, Order Rodentia (Part 1), pp. 345-382 in Mammal Species of the World (1 st Edition), Lawrence, Kansas, USA :Alien Press, Inc. & The Association of Systematics Collections on page 349, DOI: 10.5281/zenodo.7353023
Algyroides nigropunctatus
Creators: name: Sindaco, Roberto
name: Rossi, Roberta
Publisher: name: Zenodo
Year: 2020
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Reptilia
Squamata
Lacertidae
Algyroides
Algyroides nigropunctatus

description: Algyroides nigropunctatus (Duméril and Bibron, 1839)
Algyroides nigropunctatus kephallithacius Keymar, 1986
The occurrence of the Dalmatian Algyroides in Lefkada is well known (Werner, 1894: 230; Werner, 1929: 477; Schmid, 2019: 73). We found this lizard at several localities: Marantochori (17/5/2019), Sivros (19/5/2019), Nydri waterfalls (19/5/2019, Fig. 2G), between Maranthochori and Kastri bay (23/5/2019), Fterno (23/5/2019), between Chortata and Kalamitsi (25/5/2019), Lefkada town (18/5/2019), Sivros (19/5/2019), Agios Ilias (19/5/2019), Agios Nikitas (24/5/2019), between Spanochori and Lefkas town (24/5/2019 and 26/5/2019), between Khortata and Kalamitsi (25/5/2019). Moreover, several citizen science records are available: Athani (18/9/2019, Frini (22/5/2019), Kariotes (2/6/2019), Karya (20/6/2019), Lefkada town (14/4/2019), Ligia (23 and 30/6/2019), Marantochori (24/7/2019), Sivros (2/6/2019), Vasiliki (28/8/2017, 8/3/2019, 2/4/2019, 6/5/2019).
description: Published as part of Sindaco, Roberto & Rossi, Roberta, 2020, Annotated checklist of the herpetofauna (Amphibia, Reptilia) of Lefkada Island (Ionian Islands, Greece), pp. 57-68 in Natural History Sciences 7 (2) on page 60, DOI: 10.4081/nhs.2020.480, http://zenodo.org/record/12753965
Trisunius iaculatus ASSING 2011
Creators: name: Assing, Volker
Publisher: name: Zenodo
Year: 2015
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Staphylinidae
Trisunius
Trisunius iaculatus

description: Trisunius iaculatus ASSING, 2011(Map 4) M a t e r i a l e x a m i n e d: Thailand: 233, Doi Inthanon, Kew Mae Pan, 18°33'N, 98°29'E, 2100 m, along stream, leaf litter sifted, 19.XII.2013, leg. Ob (cAss); 1 ♀, Doi Inthanon, summit (Ang Ka), 18°35'N, 98°29'E, 2555 m, peat bog, in reeds, 10. XII.2013, leg. Ob (cAss); 1 3, Doi Inthanon, summit, 18°35'N, 98°29'E, 2530 m, along stream bank, 11.XII.2013, leg. Ob (cAss); 233, 2♀♀, Doi Inthanon, summit, 18°35'N, 98°29'E, 2530 m, leaf litter sifted, 11.XII.2013, leg. Ob (cAss); 1♀, Doi Inthanon, 18°35'N, 98°29'E, 2440 m, peat bog, litter in swampy area, 14.I.2014, leg. Ob (cAss); 1 ♀, Doi Inthanon, Kew Mae Pan Waterfall, 18°33'N, 98°29'E, 2190 m, litter sifted, 15.I.2014, leg. Ob (cAss). C o m m e n t: The previously known distribution of T. iaculatus was confined to West Yunnan (ASSING 2013). The above specim ens represent the first records from Thailand (Map 4).
description: Published as part of Assing, Volker, 2015, A revision of Trisunius V. Three new species and additional records, including the first records of the genus from Vietnam (Coleoptera: Staphylinidae: Paederinae), pp. 1179-1190 in Linzer biologische Beiträge 47 (2) on page 1183, DOI: 10.5281/zenodo.5184218
description: {"references": ["ASSING V. (2011): Trisunius gen. nov. from the southern East Palaearctic and the Oriental regions (Coleoptera: Staphy linidae: Paederinae: Medonina). - Linzer Biologische Beitrage 43 (1): 195 - 220.", "ASSING V. (2013): A revision of Trisunius III. Three new species from North India and Nepal, and additional records (Coleoptera: Staphylinidae: Paederinae). - Linzer Biologis che Beitrage 45 (2): 1531 - 1540."]}
Complicial structures in the nerves of omega-categories
Creators: name: Steiner, Richard
Publisher: name: arXiv
Year: 2013
Subjects: subject: Category Theory (math.CT)
subject: FOS: Mathematics
subject: 18D05

description: It is known that strict omega-categories are equivalent through the nerve functor to complicial sets and to sets with complicial identities. It follows that complicial sets are equivalent to sets with complicial identities. We discuss these equivalences. In particular we give a conceptual proof that the nerves of omega-categories are complicial sets, and a direct proof that complicial sets are sets with complicial identities.
description: 25 pages. Version 2 has updated reference in bibliography. Paper has been published
Roughness of molecular property landscapes and its impact on modellability
Creators: name: Aldeghi, Matteo
name: Graff, David E.
name: Frey, Nathan
name: Morrone, Joseph A.
name: Pyzer-Knapp, Edward O.
name: Jordan, Kirk E.
name: Coley, Connor W.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Quantitative Methods (q-bio.QM)
subject: FOS: Biological sciences

description: In molecular discovery and drug design, structure-property relationships and activity landscapes are often qualitatively or quantitatively analyzed to guide the navigation of chemical space. The roughness (or smoothness) of these molecular property landscapes is one of their most studied geometric attributes, as it can characterize the presence of activity cliffs, with rougher landscapes generally expected to pose tougher optimization challenges. Here, we introduce a general, quantitative measure for describing the roughness of molecular property landscapes. The proposed roughness index (ROGI) is loosely inspired by the concept of fractal dimension and strongly correlates with the out-of-sample error achieved by machine learning models on numerous regression tasks.
description: 17 pages, 6 figures, 2 tables (SI with 17 pages, 16 figures)
ΜΟΧΕ: «Εφραθά», τόμ. 7, σ. 428.
Creators: name: Vasileiadis, Pavlos D.
Publisher: name: Zenodo
Year: 2014
Subjects: Παύλος Βασιλειάδης
Pavlos Vasileiadis
Ephrath
Εφραθά

description: English title: “Ephrath” (Ephrathah), Encyclopedia ΜΟΧΕ vol. 7, p. 428.
Temperature-dependent critical spin-orbit field for orthogonal switching in antiferromagnets
Creators: name: Rama-Eiroa, R.
name: Otxoa, R. M.
name: Atxitia, U.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: Applied Physics (physics.app-ph)
subject: FOS: Physical sciences

description: The discovery of current-induced spin-orbit torque (SOT) orthogonal reorientation, also known as orthogonal switching, of metallic Mn$_2$Au and CuMnAs has opened the door for ultrafast writing of an antiferromagnet (AFM). Phenomenological theory predicts that the minimum field necessary for SOT switching -- critical field -- for ultrashort pulses increases inversely proportional to the pulse duration, thereby limiting the use of ultrafast stimulus as driving force for switching. We explore the possibility that by varying the working temperature the critical field reduces enabling orthogonal switching in response to ultrashort pulses. To do so, we extend previous theory to finite temperature and show that the critical field for an orthogonal switching strongly depends on temperature. We determine how the temperature dependence of the critical field varies as a function of the pulse duration. While for long pulses, the temperature dependence of the critical field is determined by the anisotropy field, for ultrashort pulses, it is determined by the characteristic frequency of the AFM. We show that the short and long pulse duration limits for the critical field can be connected by an analytical expression.