cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Orbital degree of freedom in artificial electron lattices on metal surface
Creators: name: Ma, Liang
name: Qiu, Wen-Xuan
name: Lü, Jing-Tao
name: Gao, Jin-Hua
Publisher: name: arXiv
Year: 2017
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: Orbital degree of freedom plays a fundamental role in condensed matter physics. Recently, a new kind of artificial electron lattice has been realized in experiments by confining the metal surface electrons with adsorbed molecular lattice. A most recent example is the Lieb lattice realized by CO adsorption on Cu(111) surface [M. R. Slot, et al., Nat. Phys. 13, 672(2017)]. The Lieb lattice is of special interest due to its flat band physics. Here, by first-principles calculations, muffin-tin potential model and tight binding model, we demonstrate that, the high energy states observed in the experiment actually correspond to the artificial $p$-orbitals of the electron lattice. Our numerical results, together with the experimental observation, show that artificial $p$-orbital fermionic lattice has already been realized in solid state system. This opens a new avenue to investigate the orbital degree of freedom in a controllable way.
description: 6 pages, 4 figures
title: Lily :
title: Guidelines for the Conduct of Tests for Distinctness, Uniformity and Stability.
titleType: Subtitle
Creators: name: (:Unas)
Publisher: name: Unknown
Year: 2011

description: The purpose of these guidelines (“Test Guidelines”) is to elaborate the principles contained in the General Introduction (document TG/1/3), and its associated TGP documents, into detailed practical guidance for the harmonized examination of distinctness, uniformity and stability (DUS) and, in particular, to identify appropriate characteristics for the examination of DUS and production of harmonized variety descriptions.
Pennaria Goldfuss 1820
Creators: name: Calder, Dale R.
Publisher: name: Zenodo
Year: 2010
Subjects: Biodiversity
Taxonomy
Animalia
Cnidaria
Hydrozoa
Anthoathecata
Pennariidae
Pennaria

description: Genus Pennaria Goldfuss, 1820
 Pennaria Goldfuss, 1820: 89.
 Type species. Pennaria disticha Goldfuss, 1820, by subsequent designation by Bedot (1901).
 Diagnosis. Capitate Hydrozoa having characters of the family Pennariidae.
 Remarks. Confusion over the taxonomic status of the name Pennaria, the authorship of which is now attributed to Goldfuss (1820), was clarified by Gibbons & Ryland (1989). Halocordyle Stechow, 1921a is thus regarded as a junior synonym. Other issues surrounding the taxonomy and nomenclature of the genus were discussed by Calder (1988).
 Numbers of species currently recognized worldwide in the genus Pennaria vary from eight (Bouillon et al. 2006; Schuchert 2009) to two (Daly et al. 2007), the latter estimate presumably referring to the hydroid stage only.
description: Published as part of Calder, Dale R., 2010, Some anthoathecate hydroids and limnopolyps (Cnidaria, Hydrozoa) from the Hawaiian archipelago 2590, pp. 1-91 in Zootaxa 2590 (1) on page 63, DOI: 10.11646/zootaxa.2590.1.1, http://zenodo.org/record/10834110
Entanglement and Extreme Spin Squeezing
Creators: name: Sorensen, Anders
name: Molmer, Klaus
Publisher: name: arXiv
Year: 2000
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: For any mean value of a cartesian component of a spin vector we identify the smallest possible uncertainty in any of the orthogonal components. The corresponding states are optimal for spectroscopy and atomic clocks. We show that the results for different spin J can be used to identify entanglement and to quantity the depth of entanglement in systems with many particles. With the procedure developed in this letter, collective spin measurements on an ensemble of particles can be used as an experimental proof of multi-particle entanglement
description: 4 pages, 2 figures, minor changes in the presentation
Soft pion theorem, asymptotic symmetry and new memory effect
Creators: name: Hamada, Yuta
name: Sugishita, Sotaro
Publisher: name: arXiv
Year: 2017
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: It is known that soft photon and graviton theorems can be regarded as the Ward-Takahashi identities of asymptotic symmetries. In this paper, we consider soft theorem for pions, i.e., Nambu-Goldstone bosons associated with a spontaneously broken axial symmetry. The soft pion theorem is written as the Ward-Takahashi identities of the $S$-matrix under asymptotic transformations. We investigate the asymptotic dynamics, and find that the conservation of charges generating the asymptotic transformations can be interpreted as a pion memory effect.
description: 25 pages, 2 figures, v2: references and discussions added
Sphaerocorynidae Prevot 1959
Creators: name: Calder, Dale R.
Publisher: name: Zenodo
Year: 2010
Subjects: Biodiversity
Taxonomy
Animalia
Cnidaria
Hydrozoa
Anthoathecata
Sphaerocorynidae

description: Family Sphaerocorynidae Prévot, 1959  Sphaerocorynidae Prévot, 1959: 108.
 Diagnosis. Capitate hydroids almost always stolonal with terminal hydranths; stems monosiphonic, arising from a creeping hydrorhiza. Perisarc covering hydrorhiza, hydrocaulus, and hydrocladia (if present), terminating at hydranth base. Hydranths pyriform, with bulbous base and elongate, proboscis-like hypostome; tentacles all capitate, solid, either simple or with both simple and trifid ones present, arranged in a narrow band around broadest part of hydranth.
Gonophores eumedusoids or free medusae, arising on hydranth among or just distal to tentacles. Medusae, when present, with bell-shaped umbrella; exumbrellar nematocyst tracks present or absent; manubrium flaskshaped in juveniles, becoming quadrate to cruciform in cross-section in adults, not extending beyond velar opening; radial canals four; marginal tentacles two or four, with intermediate wart-like clusters or spiral rings of nematocysts, terminating in an oval capitulum armed with nematocysts; marginal bulbs large, adhering to exumbrella, expanded adaxially; abaxial ocelli present. Gonads confluent on perradii of manubrium.
 Remarks. Prévot (1959) established Sphaerocorynidae for Sphaerocoryne Pictet, 1893, a genus previously included in Corynidae Johnston, 1836. The concept of the family adopted here is as proposed by Petersen (1990), who referred two genera to it (Sphaerocoryne and Heterocoryne Wedler & Larson, 1986). The principal difference distinguishing them is the presence of both trifid and simple capitate tentacles in Heterocoryne, and simple capitate tentacles only in Sphaerocoryne. Where known, gonophores are free medusae in Sphaerocoryne and eumedusoids in Heterocoryne. Although Petersen (1990) suggested that the two genera “could be merged,” he treated them both as valid. Petersen’s classification of the group has been followed by authors including Cairns et al. (2002), Bouillon et al. (2006), Daly et al. (2007), and Schuchert (2009).
 As discussed below, Sphaerocoryne sensu Petersen (1990) is divided into two genera here, Sphaerocoryne sensu stricto and Corynetes Haeckel, 1879.
The cnidome in Sphaerocorynidae comprises both desmonemes and stenoteles. Five species are currently assigned to the family (Schuchert 2009).
description: Published as part of Calder, Dale R., 2010, Some anthoathecate hydroids and limnopolyps (Cnidaria, Hydrozoa) from the Hawaiian archipelago 2590, pp. 1-91 in Zootaxa 2590 (1) on page 66, DOI: 10.11646/zootaxa.2590.1.1, http://zenodo.org/record/10834110
Additional file 1: of Can metamorphosis survival during larval development in spiny lobster Sagmariasus verreauxi be improved through quantitative genetic inheritance?
Creators: name: Nguyen Nguyen
name: Fitzgibbon, Quinn
name: Quinn, Jane
name: Smith, Greg
name: Battaglene, Stephen
name: Knibb, Wayne
Publisher: name: figshare
Year: 2018
Subjects: subject: Genetics
subject: FOS: Biological sciences
subject: Ecology
subject: 69999 Biological Sciences not elsewhere classified
subject: Developmental Biology

description: Table S1. Characterization of microsatellite loci (DOCX 16Â kb)
A Centralized Reputation Management Scheme for Isolating Malicious Controller(s) in Distributed Software-Defined Networks
Creators: name: Mughal, Bilal Karim
name: Hameed, Sufian
name: Shaikh, Ghulam Muhammad
Publisher: name: arXiv
Year: 2017
Subjects: subject: Networking and Internet Architecture (cs.NI)
subject: Cryptography and Security (cs.CR)
subject: Distributed, Parallel, and Cluster Computing (cs.DC)
subject: FOS: Computer and information sciences

description: Software-Defined Networks have seen an increasing in their deployment because they offer better network manageability compared to traditional networks. Despite their immense success and popularity, various security issues in SDN remain open problems for research. Particularly, the problem of securing the controllers in distributed environment is still short of any solutions. This paper proposes a scheme to identify any rogue/malicious controller(s) in a distributed environment. Our scheme is based on trust and reputation system which is centrally managed. As such, our scheme identifies any controllers acting maliciously by comparing the state of installed flows/policies with policies that should be installed. Controllers rate each other on this basis and report the results to a central entity, which reports it to the network administrator.
description: 6 pages, 4 figures
Additional file 9: of Homoeolog expression bias in allopolyploid oleaginous marine diatom Fistulifera solaris
Creators: name: Nomaguchi, Tatsuhiro
name: Maeda, Yoshiaki
name: Yoshino, Tomoko
name: Asahi, Toru
name: Tirichine, Leila
name: Bowler, Chris
name: Tanaka, Tsuyoshi
Publisher: name: figshare
Year: 2018
Subjects: subject: Biochemistry
subject: Microbiology
subject: FOS: Biological sciences
subject: Genetics
subject: Molecular Biology
subject: Physiology
subject: Ecology
subject: 69999 Biological Sciences not elsewhere classified
subject: Marine Biology
subject: Computational Biology

description: Figure S8. Range of homoeolog expression bias in metabolic pathways. Box plot of log2 showing the expression ratio of homoeologous gene pairs in each metabolic pathway. Red dotted line indicates the equal ratio log2. Black dotted line indicates the threshold of expression ratio where the homoeologous gene pair is defined as biased (log2FCâ >â 1). The orange and blue colors of the box indicate the direction of homoeolog expression bias, towards Fso_h and Fso_l, respectively. (PDF 37 kb)
Self-reproduction in k-inflation
Creators: name: Helmer, Ferdinand
name: Winitzki, Sergei
Publisher: name: arXiv
Year: 2006
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: Astrophysics (astro-ph)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We study cosmological self-reproduction in models of inflation driven by a scalar field $ϕ$ with a noncanonical kinetic term ($k$-inflation). We develop a general criterion for the existence of attractors and establish conditions selecting a class of $k$-inflation models that admit a unique attractor solution. We then consider quantum fluctuations on the attractor background. We show that the correlation length of the fluctuations is of order $c_{s}H^{-1}$, where $c_{s}$ is the speed of sound. By computing the magnitude of field fluctuations, we determine the coefficients of Fokker-Planck equations describing the probability distribution of the spatially averaged field $ϕ$. The field fluctuations are generally large in the inflationary attractor regime; hence, eternal self-reproduction is a generic feature of $k$-inflation. This is established more formally by demonstrating the existence of stationary solutions of the relevant FP equations. We also show that there exists a (model-dependent) range $ϕ_{R}
description: RevTeX 4, 17 pages, 1 figure
La storia letteraria come romanzo familiare
Creators: name: Castoldi, Alberto
Publisher: name: SigMa - Rivista di Letterature comparate, Teatro e Arti dello spettacolo
Year: 2019

description: Il presente contributo era stato pubblicato nel volume Il giudizio di valore e il canone letterario, a cura di L. Innocenti, Roma, Bulzoni, 2000, pp. 101-117 («I libri dell’Associazione Sigismondo Malatesta. Studi di letteratura comparata e teatro», XVI).
description: SigMa - Rivista di Letterature comparate, Teatro e Arti dello spettacolo, N. 3 (2019)
ALMA Observations of SMM11 Reveal an Extremely Young Protostar in Serpens Main Cluster
Creators: name: Aso, Yusuke
name: Ohashi, Nagayoshi
name: Aikawa, Yuri
name: Machida, Masahiro N.
name: Saigo, Kazuya
name: Saito, Masao
name: Takakuwa, Shigehisa
name: Tomida, Kengo
name: Tomisaka, Kohji
name: Yen, Hsi-Wei
name: Williams, Jonathan P.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We report the discovery of an extremely young protostar, SMM11, located in the associated submillimeter condensation SMM11 in the Serpens Main cluster using the Atacama Large Millimeter/submillimeter Array (ALMA) during its Cycle 3 at 1.3 mm and an angular resolution of ~0.5"~210 AU. SMM11 is a Class 0 protostar without any counterpart at 70 um or shorter wavelengths. The ALMA observations show 1.3 mm continuum emission associated with a collimated 12CO bipolar outflow. Spitzer and Herschel data show that SMM11 is extremely cold (T_bol=26 K) and faint (L_bol
description: 8 pages, 4 figures, accepted by ApJL
Porpita Lamarck 1801
Creators: name: Calder, Dale R.
Publisher: name: Zenodo
Year: 2010
Subjects: Biodiversity
Taxonomy
Animalia
Cnidaria
Hydrozoa
Anthoathecata
Porpitidae
Porpita

description: Genus Porpita Lamarck, 1801
 Porpita Lamarck, 1801: 355.
 Type species. Porpita indica Lamarck, 1801, a junior subjective synonym of Medusa porpita Linnaeus, 1758 [Porpita porpita], by monotypy.
 Diagnosis. Porpitid hydroids with disc-shaped mantle and internal float; upper surface nearly flat or with central bulge, sail absent. Dactylozooids with capitate tentacles in three vertical rows.
Porpitid medusae with eight radial canals when mature; adults with one or two slender capitate marginal tentacles, young medusae lacking tentacles; algal symbionts usually present, aggregated in endodermal cells bordering radial canals.
 Remarks. The widely used name Porpita Lamarck, 1801 (Hydrozoa) is a junior homonym of Porpita Soldani, 1789 (Protozoa), as noted in an earlier work (Calder 1988). Reversal of Precedence can be applied in this case under provisions of the current code (ICZN Art. 23.9), with Porpita Lamarck, 1801 being designated as both valid and a nomen protectum and Porpita Soldani, 1789 being relegated to a nomen oblitum. First, the senior homonym has not been used as a valid name in zoology after 1899 to my knowledge (ICZN Art. 23.9.1.1). Second, Porpita Lamarck, 1801 has been used in at least 25 works by more than 10 authors in the past 50 years (ICZN Art. 23.9.1.2) (Brinckmann-Voss 1970, 1987; Herring 1971; Bouillon 1974, 1984b, 1985; Eldredge & Devaney 1977; Calder 1988, 1993; Petersen 1990; Cairns et al. 1991, 2002; Medel & López-González 1996; Schuchert 1996; Kelmo & Santa-Isabel 1998; Hoover 1998; Bullard & Hay 2002; Kirkendale & Calder 2003; Anderson et al. 2004; Oiso et al. 2005; Dunn et al. 2005; Shimabukuro et al. 2006; Bouillon et al. 2006; Gravier-Bonnet 2007; Daly et al. 2007).
 More than 20 nominal species have been assigned at various times to this genus worldwide (Calder 1988). Over the past century, most authors have recognized no more than three of these as valid: Porpita porpita (Linnaeus, 1758) from the Indian Ocean, P. umbella (O.F. Müller, 1776b) from the Atlantic Ocean, and P. pacifica Lesson, 1826 from the Pacific Ocean. Moser (1925) and Totton (1954) have been followed here in regarding these three as conspecific, with the name P. porpita having priority. For reviews of the taxonomy and nomenclature of this genus, see Bigelow (1911) and Calder (1988).
description: Published as part of Calder, Dale R., 2010, Some anthoathecate hydroids and limnopolyps (Cnidaria, Hydrozoa) from the Hawaiian archipelago 2590, pp. 1-91 in Zootaxa 2590 (1) on pages 69-70, DOI: 10.11646/zootaxa.2590.1.1, http://zenodo.org/record/10834110
Low frequency radio and X-ray properties of core-collapse supernovae
Creators: name: Ray, A.
name: Chandra, P.
name: Sutaria, F.
name: Bhatnagar, S.
Publisher: name: arXiv
Year: 2003
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Radio and X-ray studies of young supernovae probe the interaction between the supernova shock waves and the surrounding medium and give clues to the nature and past of the progenitor star. Here we discuss the early emission from type Ic SN 2002ap and argue that repeated Compton boosting of optical photons by hot electrons presents the most natural explanation of the prompt X-ray emission. We describe the radio spectrum of another type Ic SN 2003dh (GRB030329) obtained with combined GMRT and VLA data. We report on the low frequency radio monitoring of SN 1995N and our objectives of distinguishing between competing models of X-ray emission from this SN and the nature of its progenitor by X-ray spectroscopy. Radio studies on SN 2001gd, SN 2001ig and SN 2002hh are mentioned.
description: 5 pages, 4 figures. Uses svmult.cls. To appear in proceedings of IAU Colloquium 192 "Supernovae (10 years of SN 1993J)", April 2003, Valencia, Spain, eds. J. M. Marcaide and K. W. Weiler
Joseph Conrad: tanti paesaggi, un unico spazio
Creators: name: Serpieri, Alessandro
Publisher: name: SigMa - Rivista di Letterature comparate, Teatro e Arti dello spettacolo
Year: 2019

description: Il presente contributo era stato pubblicato nel volume Raccontare e descrivere. Lo spazio nel romanzo dell’Ottocento, a cura di F. Fiorentino, Bulzoni, Roma 1997, pp. 193-209 («I libri dell’Associazione Sigismondo Malatesta. Studi di letteratura comparata e teatro», IX).
description: SigMa - Rivista di Letterature comparate, Teatro e Arti dello spettacolo, N. 3 (2019)
title: A computational model for full or partial damage of single or multiple adjacent columns in disproportionate collapse analysis via linear programming
Creators: name: Gerasimidis, Simos
name: Bisbos, C.
name: Baniotopoulos, C.
Publisher: name: University of Massachusetts Amherst
Year: 2013
Subjects: subject: disproportionate collapse analysis;
subject: progressive collapse
subject: alternate load path method
subject: limit analysis
subject: damaged steel frames
subject: partial damage concept
subject: Civil and Environmental Engineering
subject: Engineering

description: The evaluation of the sensitivity or insensitivity of structures to local damage has been a major research field during the last decades, mainly provoked due to the series of aging structures and infrastructures. Many researchers have described this property as redundancy, others as the resistance to disproportionate collapse or robustness and still others as the ability of structural systems to display alternate load paths in case of a local damage. In any case, the problem for the evaluation of this property is increasingly alarming since many systems experience similar collapses (American Society of Civil Engineers (2009). Proceedings of Structures Congress on the first international symposium on disproportionate collapse. ASCE, Austin, TX). This paper presents the numerical assessment of disproportionate collapse analysis introducing the concept of partial damage of structural elements. Global robustness measures are proposed also for the case of multiple partial losses of adjacent elements. The measures are computed on the basis of a mathematical optimization problem using collapse load analysis of steel frames with pre-existing damage. Results comparing the cases of partial losses with the full column lossesare presented and discussed.
NH_3(1_0-0_0) in the pre-stellar core L1544
Creators: name: Caselli, P.
name: Bizzocchi, L.
name: Keto, E.
name: Sipila, O.
name: Tafalla, M.
name: Pagani, L.
name: Kristensen, L. E.
name: van der Tak, F. F. S.
name: Walmsley, C. M.
name: Codella, C.
name: Nisini, B.
name: Aikawa, Y.
name: Faure, A.
name: van Dishoeck, E. F.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Pre-stellar cores represent the initial conditions in the process of star and planet formation, therefore it is important to study their physical and chemical structure. Because of their volatility, nitrogen-bearing molecules are key to study the dense and cold gas present in pre-stellar cores. The NH_3 rotational transition detected with Herschel-HIFI provides a unique combination of sensitivity and spectral resolution to further investigate physical and chemical processes in pre-stellar cores. Here we present the velocity-resolved Herschel-HIFI observations of the ortho-NH_3(1_0-0_0) line at 572 GHz and study the abundance profile of ammonia across the pre-stellar core L1544 to test current theories of its physical and chemical structure. Recently calculated collisional coefficients have been included in our non-LTE radiative transfer code to reproduce Herschel observations. A gas-grain chemical model, including spin-state chemistry and applied to the (static) physical structure of L1544 is also used to infer the abundance profile of ortho-NH_3 . The hyperfine structure of ortho-NH_3(1_0-0_0) is resolved for the first time in space. All the hyperfine components are strongly self-absorbed. The profile can be reproduced if the core is contracting in quasi-equilibrium, consistent with previous work, and if the NH_3 abundance is slightly rising toward the core centre, as deduced from previous interferometric observations of para-NH_3(1,1). The chemical model overestimates the NH_3 abundance at radii between ~ 4000 and 15000 AU by about two orders of magnitude and underestimates the abundance toward the core centre by more than one order of magnitude. Our observations show that chemical models applied to static clouds have problems in reproducing NH_3 observations.
description: accepted for publication in A&A Letters
Quantum information theory
Creators: name: Nielsen, M. A.
Publisher: name: arXiv
Year: 2000
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: Quantum information theory is the study of the achievable limits of information processing within quantum mechanics. Many different types of information can be accommodated within quantum mechanics, including classical information, coherent quantum information, and entanglement. Exploring the rich variety of capabilities allowed by these types of information is the subject of quantum information theory, and of this Dissertation. In particular, I demonstrate several novel limits to the information processing ability of quantum mechanics. Results of especial interest include: the demonstration of limitations to the class of measurements which may be performed in quantum mechanics; a capacity theorem giving achievable limits to the transmission of classical information through a two-way noiseless quantum channel; resource bounds on distributed quantum computation; a new proof of the quantum noiseless channel coding theorem; an information-theoretic characterization of the conditions under which quantum error-correction may be achieved; an analysis of the thermodynamic limits to quantum error-correction, and new bounds on channel capacity for noisy quantum channels.
description: 259 pages, reformatted version of Dissertation submitted for the Doctor of Philosophy in Physics at the University of New Mexico, August 1998
Porpita porpita porpita (Linnaeus 1758
Creators: name: Calder, Dale R.
Publisher: name: Zenodo
Year: 2010
Subjects: Biodiversity
Taxonomy
Animalia
Cnidaria
Hydrozoa
Anthoathecata
Porpitidae
Porpita
Porpita porpita

description: Porpita porpita (Linnaeus, 1758)
Fig. 46
 Medusa porpita Linnaeus, 1758: 659.
 Porpita pacifica.— Eldredge & Devaney, 1977: 107, fig. 2.— Hoover, 1998: 23, fig.; 2006: 23, fig.
 Type locality. “Habitat in India ” (Indian Ocean) (Linnaeus 1758).
 Material examined. Oahu: Lanikai Beach, shore, 22.vi.1972, low tide, one colony, 2.6 cm in diameter, coll. Frances Frazier, BPBM D452.
 Description. Hydroid colony pleustonic, polymorphic, with disc-shaped mantle overlying a chitinous float. Upper surface of mantle and float slightly concave, with scattered hollow papillae, central pore and peripheral stigmata indistinct; lower surface with one short, broad central gastrozooid, a medial ring of gonozooids, and a peripheral ring of dactylozooids, with most gonozooids and dactylozooids missing in present material. Gonozooids vermiform to club-shaped, with nematocyst knobs scattered over body and arranged in a whorl at distal end. Dactylozooids club-shaped, somewhat triangular in cross-section distally, with short capitate tentacles in three vertical rows over body and arranged in a whorl at distal end. Nematocyst reservoir disc-shaped, internal, between gastrozooid and float.
Gonophores free medusae, arising in clusters from base of gonozooids.
 Remarks. The taxonomy of this hydrozoan was thoroughly reviewed by Bigelow (1911). While he recognized Porpita pacifica Lesson, 1826 as the valid name for the species in the Pacific Ocean, Moser (1925) and Totton (1954) have been followed here in considering it synonymous with P. porpita (Linnaeus, 1758). An account of the cnidome has been given in a previous report (Calder 1988). Additional information on the species is given by Schuchert (2010).
 The hydroid stage of Porpita porpita is a component of the open ocean pleuston, and specimens occasionally wash ashore in Hawaii (Eldredge & Devaney 1977; Hoover 1998, 2006). Colonies are deep blue in colour when alive. Besides hydroid and medusa, the life cycle includes several juvenile stages, including a rataria “larva” and a young pleustonic hydroid stage.
 Recorded distribution. Hawaii. Oahu: off the windward coast (Eldredge & Devaney 1977, as Porpita pacifica). Maui: Molokini Islet (Hoover 1998, 2006, as Porpita pacifica).
Worldwide. Circumglobal, tropical and temperate waters; pleustonic (Calder 1988; Schuchert 2010).
description: Published as part of Calder, Dale R., 2010, Some anthoathecate hydroids and limnopolyps (Cnidaria, Hydrozoa) from the Hawaiian archipelago 2590, pp. 1-91 in Zootaxa 2590 (1) on pages 70-71, DOI: 10.11646/zootaxa.2590.1.1, http://zenodo.org/record/10834110
Additional file 1: of The Xylella fastidosa RTX operons: evidence for the evolution of protein mosaics through novel genetic exchanges
Creators: name: Gambetta, Gregory
name: Matthews, Mark
name: Syvanen, Michael
Publisher: name: figshare
Year: 2018
Subjects: subject: Microbiology
subject: FOS: Biological sciences
subject: Genetics
subject: Molecular Biology
subject: Evolutionary Biology
subject: Developmental Biology
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: 60506 Virology

description: Table S1. Gene name, NCBI protein accession number, and NCBI gene locus tag for the Xylella fastidiosa RTXs. Figure S1 and S2. Complete DNA-DNA dot plots (created with the Dotter software) of RTX operon comparisons between Xf (Temecula) and itself, other Xf strains Dixon, 9a5c, and Ann1, and in the case of the RTX4 operon Ralstonia solanacearum. Putative open reading frames are designated by arrows, orthologues are like colored, and mutations resulting in premature stop codons or frame shifts (FS) are noted. Figure S3. ClustalW multiple nucleotide sequence alignment of the Xf (Temecula) RTX3 operon N-terminal repeats (sequences 1-6) and the RTX3 N-terminus (sequence 7). N-terminal repeat sequences contain a large inverted repeat region (arrows and shading). (PDF 809 kb)
Massless spinning test particles in vacuum algebraically special spacetimes
Creators: name: Bini, Donato
name: Cherubini, Christian
name: Andrea, Geralico
name: Jantzen, Robert T.
Publisher: name: arXiv
Year: 2006
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: The motion of massless spinning test particles is investigated using the Newman-Penrose formalism within the Mathisson-Papapetrou model extended to massless particles by Mashhoon and supplemented by the Pirani condition. When the "multipole reduction world line" lies along a principal null direction of an algebraically special vacuum spacetime, the equations of motion can be explicitly integrated. Examples are given for some familiar spacetimes of this type in the interest of shedding some light on the consequences of this model.
description: Slightly modified version with respect to the published one [ International Journal of Modern Physics D, Vol. 15 pp. 737-758 (2006)] which unfortunately contains few (unespected) misprints
Gravitational Microlensing: A Tool for Detecting and Characterizing Free-Floating Planets
Creators: name: Han, Cheongho
name: Chung, Sun-Ju
name: Kim, Doeon
name: Park, Byeong-Gon
name: Ryu, Yoon-Hyun
name: Kang, Sangjun
name: Lee, Dong Wook
Publisher: name: arXiv
Year: 2003
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Various methods have been proposed to search for extrasolar planets. Compared to the other methods, microlensing has unique applicabilities to the detections of Earth-mass and free-floating planets. However, the microlensing method is seriously flawed by the fact that the masses of the detected planets cannot be uniquely determined. Recently, Gould, Gaudi, & Han introduced an observational setup that enables one to resolve the mass degeneracy of the Earth-mass planets. The setup requires a modest adjustment to the orbit of an already proposed Microlensing planet-finder satellite combined with ground-based observations. In this paper, we show that a similar observational setup can also be used for the mass determinations of free-floating planets with masses ranging from ~0.1 M_J to several Jupiter masses. If the proposed observational setup is realized, the future lensing surveys will play important roles in the studies of Earth-mass and free-floating planets, which are the populations of planets that have not been previously probed.
description: total 8 pages, including 3 figures, ApJ, in press (Mar 1, 2004)
Formalization of the fundamental group in untyped set theory using auto2
Creators: name: Zhan, Bohua
Publisher: name: arXiv
Year: 2017
Subjects: subject: Logic in Computer Science (cs.LO)
subject: FOS: Computer and information sciences

description: We present a new framework for formalizing mathematics in untyped set theory using auto2. Using this framework, we formalize in Isabelle/FOL the entire chain of development from the axioms of set theory to the definition of the fundamental group for an arbitrary topological space. The auto2 prover is used as the sole automation tool, and enables succinct proof scripts throughout the project.
description: 17 pages, accepted for ITP 2017
An expectation value expansion of Hermitian operators in a discrete Hilbert space
Creators: name: Asplund, Roberth
name: Bjork, Gunnar
name: Bourenanne, Mohamed
Publisher: name: arXiv
Year: 2000
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We discuss a real-valued expansion of any Hermitian operator defined in a Hilbert space of finite dimension N, where N is a prime number, or an integer power of a prime. The expansion has a direct interpretation in terms of the operator expectation values for a set of complementary bases. The expansion can be said to be the complement of the discrete Wigner function. We expect the expansion to be of use in quantum information applications since qubits typically are represented by a discrete, and finite-dimensional physical system of dimension N=2^p, where p is the number of qubits involved. As a particular example we use the expansion to prove that an intermediate measurement basis (a Breidbart basis) cannot be found if the Hilbert space dimension is 3 or 4.
description: A mild update. In particular, I. D. Ivanovic's earlier derivation of the expansion is properly acknowledged. 16 pages, one PS figure, 1 table, written in RevTeX
Velella Lamarck 1801
Creators: name: Calder, Dale R.
Publisher: name: Zenodo
Year: 2010
Subjects: Biodiversity
Taxonomy
Animalia
Cnidaria
Hydrozoa
Anthoathecata
Porpitidae
Velella

description: Genus Velella Lamarck, 1801
 Velella Lamarck, 1801: 355.
 Type species. Medusa velella Linnaeus, 1758 [Velella velella], by absolute tautonymy.
 Diagnosis. Porpitid hydroids with mantle and internal float oval in shape; upper surface with erect, triangular sail oriented diagonally to long axis of float. Dactylozooids with bands and patches of nematocysts; tentacles lacking.
Porpitid medusae with four radial canals; tentacle bulbs four, one opposite pair lacking tentacles and the other pair with 1–2 capitate tentacles each; algal symbionts usually present, aggregated near radial canals and ring canal.
 Remarks. Many nominal species of this genus have been described from tropical and temperate oceans worldwide. At present, however, all are believed referable to one species, Velella velella (Linnaeus, 1758) (Calder 1988; Bouillon et al. 2006; Schuchert 2010).
description: Published as part of Calder, Dale R., 2010, Some anthoathecate hydroids and limnopolyps (Cnidaria, Hydrozoa) from the Hawaiian archipelago 2590, pp. 1-91 in Zootaxa 2590 (1) on page 71, DOI: 10.11646/zootaxa.2590.1.1, http://zenodo.org/record/10834110
Robust, open-source removal of systematics in Kepler data
Creators: name: Aigrain, S.
name: Parviainen, H.
name: Roberts, S.
name: Reece, S.
name: Evans, T.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We present ARC2 (Astrophysically Robust Correction 2), an open-source Python-based systematics-correction pipeline to correct for the Kepler prime mission long cadence light curves. The ARC2 pipeline identifies and corrects any isolated discontinuities in the light curves, then removes trends common to many light curves. These trends are modelled using the publicly available co-trending basis vectors, within an (approximate) Bayesian framework with `shrinkage' priors to minimise the risk of over-fitting and the injection of any additional noise into the corrected light curves, while keeping any astrophysical signals intact. We show that the ARC2 pipeline's performance matches that of the standard Kepler PDC-MAP data products using standard noise metrics, and demonstrate its ability to preserve astrophysical signals using injection tests with simulated stellar rotation and planetary transit signals. Although it is not identical, the ARC2 pipeline can thus be used as an open source alternative to PDC-MAP, whenever the ability to model the impact of the systematics removal process on other kinds of signal is important.
description: 13 pages, 10 figures, accepted for publication in MNRAS
MOESM1 of Sewage sludge for sustainable agriculture: contaminantsâ contents and potential use as fertilizer
Creators: name: Lamastra, Lucrezia
name: Suciu, Nicoleta
name: Trevisan, Marco
Publisher: name: figshare
Year: 2018
Subjects: subject: Biochemistry
subject: Space Science
subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Pharmacology
subject: Biotechnology
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Ecology
subject: Immunology
subject: FOS: Clinical medicine
subject: 69999 Biological Sciences not elsewhere classified
subject: Inorganic Chemistry
subject: 60506 Virology

description: Additional file 1. NP, NP1EO, NP2EO, DEHP range (min, max values) and median concentration in sewage sludge during the present study (2013-2014).
Gravitomagnetic Effects in a Conductor in an Applied Magnetic Field
Creators: name: Ahmedov, B. J.
name: Karim, M.
Publisher: name: arXiv
Year: 2006
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The electromagnetic measurements of general relativistic gravitomagnetic effects which can be performed within a conductor embedded in the space-time of slow rotating gravitational object in the presence of magnetic field are proposed.
description: 5 pages
Additional file 1 of A first insight into the genomic background of Ilex pubescens (Aquifoliaceae) by flow cytometry and genome survey sequencing
Creators: name: Zhou, Peng
name: Zhang, Qiang
name: Li, Jiao
name: Li, Fei
name: Huang, Jing
name: Zhang, Min
Publisher: name: figshare
Year: 2023
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Additional file 1.
Additional file 8: of Homoeolog expression bias in allopolyploid oleaginous marine diatom Fistulifera solaris
Creators: name: Nomaguchi, Tatsuhiro
name: Maeda, Yoshiaki
name: Yoshino, Tomoko
name: Asahi, Toru
name: Tirichine, Leila
name: Bowler, Chris
name: Tanaka, Tsuyoshi
Publisher: name: figshare
Year: 2018
Subjects: subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Physiology
subject: Ecology
subject: 69999 Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Marine Biology
subject: 111714 Mental Health
subject: FOS: Health sciences
subject: Hematology

description: Figure S7. Expression and functional differences depending on existence of motif TABASTA in promoter region. (A) Figure shows the mean number of homoeologous gene pairs which showing homoeolog expression bias towards Fso_h or Fso_l (n = 3, ±S.D.). Bars were separated into three groups depend on whether the motif exist in promoter region of both gene of the pair, only Fso_h gene of the pair or only Fso_l gene of the pair. Asterisk show significant differences (p
Canonical Analysis of Non-Relativistic Particle and Superparticle
Creators: name: Kluson, J.
Publisher: name: arXiv
Year: 2017
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We perform canonical analysis of non-relativistic particle in Newton-Cartan Background. Then we extend this analysis to the case of non-relativistic superparticle in the same background. We determine constraints structure of this theory and find generator of κ-symmetry.
description: 17 pages, references added
Finite volume effects for non-Gaussian multi-field inflationary models
Creators: name: Bernardeau, Francis
name: Uzan, Jean-Philippe
Publisher: name: arXiv
Year: 2003
Subjects: subject: Astrophysics (astro-ph)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Models of multi-field inflation exhibiting primordial non-Gaussianity have recently been introduced. This is the case in particular if the fluctuations of a light field scalar field, transverse to the inflaton direction, with quartic coupling can be transferred to the metric fluctuations. So far in those calculations only the ensemble statistical properties have been considered. We explore here how finite volume effects could affect those properties. We show that the expected non-Gaussian properties survive at a similar level when the finite volume effects are taken into account and also find that they can skew the metric distribution even though the ensemble distribution is symmetric.
description: 13 pages, 2 figures
Remarks on Papapetrou Class of Vacuum Solutions of Einstein Equations
Creators: name: Ahmedov, B. J.
name: Khugaev, A. V.
Publisher: name: arXiv
Year: 2006
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Class of axially symmetric solutions of vacuum Einstein field equations including the Papapetrou solution as particular case has been found. It has been shown that the derived solution describes the external axial symmetric gravitational field of the source with nonvanishing mass. The general solution is obtained for this class of functions. As an example of physical application, the spacetime metric outside a line gravitomagnetic monopole has been obtained from Papapetrou solution of vacuum equations of gravitational field.
description: 8 pages
Additional file 7: of Overexpression of the protein disulfide isomerase AtCYO1 in chloroplasts slows dark-induced senescence in Arabidopsis
Creators: name: Tominaga, Jun
name: Nakahara, Yasutoshi
name: Horikawa, Daisuke
name: Tanaka, Ayumi
name: Kondo, Maki
name: Kamei, Yasuhiro
name: Takami, Tsuneaki
name: Sakamoto, Wataru
name: Unno, Kazutoshi
name: Sakamoto, Atsushi
name: Shimada, Hiroshi
Publisher: name: figshare
Year: 2018
Subjects: subject: Biochemistry
subject: Cell Biology
subject: Molecular Biology
subject: Sociology
subject: FOS: Sociology
subject: Developmental Biology
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: Plant Biology
subject: FOS: Biological sciences
subject: Computational Biology

description: Figure S4. Maintenance of RBC-L and LHCP at 10 DDI as indicated by Coomassie staining following SDS-PAGE. (PDF 586Â kb)
Comment on "Foundations of quantum mechanics: Connection with stochastic processes"
Creators: name: Alonso, D.
name: Muga, J. G.
name: Mayato, R. Sala
Publisher: name: arXiv
Year: 2000
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: Recently, Olavo has proposed several derivations of the Schrodinger equation from different sets of hypothesis ("axiomatizations") [Phys. Rev. A 61, 052109 (2000)]. One of them is based on the infinitesimal inverse Weyl transform of a classically evolved phase space density. We show however that the Schrodinger equation can only be obtained in that manner for linear or quadratic potential functions.
description: 3 pages, no figures
Pre-Hawking radiation cannot prevent the formation of apparent horizon
Creators: name: Chen, Pisin
name: Unruh, William G.
name: Wu, Chih-Hung
name: Yeom, Dong-han
Publisher: name: arXiv
Year: 2017
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: As an attempt to solve the black hole information loss paradox, recently there has been the suggestion that, due to semi-classical effects, a pre-Hawking radiation must exist during the gravitational collapse of matter, which in turn prevents the apparent horizon from forming. Assuming the pre-Hawking radiation does exist, here we argue the opposite. First we note that the stress energy tensor near the horizon for the pre-Hawking radiation is far too small to do anything to the motion of a collapsing shell. Thus the shell will always cross the apparent horizon within a finite proper time. Moreovall, the amount of energy that can be radiated must be less than half of the total initial energy (if the particle starts at rest at infinity) before the shell becomes a null shell and cannot radiate any more without becoming tachyonic. We conclude that for any gravitational collapsing process within Einstein gravity and semi-classical quantum field theory, the formation of the apparent horizon is inevitable. Pre-Hawking radiation is therefore not a valid solution to the information paradox.
description: 6 pages, 2 figures
Trachylina Haeckel 1879
Creators: name: Calder, Dale R.
Publisher: name: Zenodo
Year: 2010
Subjects: Biodiversity
Taxonomy
Animalia
Cnidaria
Hydrozoa
Trachylina

description: Subclass Trachylina Haeckel, 1879  Trachylinae Haeckel, 1879: 2.
 Remarks. Trachylina Haeckel, 1879 encompasses the hydrozoan orders Actinulida Swedmark & Teissier, 1959, Limnomedusae Kramp, 1938, Narcomedusae Haeckel, 1879, and Trachymedusae Haeckel, 1879 (Collins 2000; Daly et al. 2007; Collins et al. 2008). Details on the phylogeny of the group are provided in Collins et al. (2008).
description: Published as part of Calder, Dale R., 2010, Some anthoathecate hydroids and limnopolyps (Cnidaria, Hydrozoa) from the Hawaiian archipelago 2590, pp. 1-91 in Zootaxa 2590 (1) on page 72, DOI: 10.11646/zootaxa.2590.1.1, http://zenodo.org/record/10834110
Einselection and Decoherence from an Information Theory Perspective
Creators: name: Zurek, W. H.
Publisher: name: arXiv
Year: 2000
Subjects: subject: Quantum Physics (quant-ph)
subject: Statistical Mechanics (cond-mat.stat-mech)
subject: FOS: Physical sciences

description: We introduce and investigate a simple model of conditional quantum dynamics. It allows for a discussion of the information-theoretic aspects of quantum measurements, decoherence, and environment-induced superselection (einselection).
description: Proceedings of the Planck constant centenary meeting. Uses annalen.cls and fleqn.sty
Observability of Forming Planets and their Circumplanetary Disks I. -- Parameter Study for ALMA
Creators: name: Szulágyi, J.
name: van der Plas, G.
name: Meyer, M. R.
name: Pohl, A.
name: Quanz, S. P.
name: Mayer, L.
name: Daemgen, S.
name: Tamburello, V.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: We present mock observations of forming planets with ALMA. The possible detections of circumplanetary disks (CPDs) were investigated around planets of Saturn, 1, 3, 5, and 10 Jupiter-masses that are placed at 5.2 AU from their star. The radiative, three dimensional hydrodynamic simulations were then post-processed with RADMC3D and the ALMA Observation Simulator. We found that even though the CPDs are too small to be resolved, they are hot due to the accreting planet in the optically thick limit, therefore the best chance to detect them with continuum observations in this case is at the shortest ALMA wavelengths, such as Band 9 (440 microns). Similar fluxes were found in the case of Saturn and Jupiter-mass planets, as for the 10 $\mathrm{M_{Jup}}$ gas-giant, due to temperature weighted optical depth effects: when no deep gap is carved, the planet region is blanketed by the optically thick circumstellar disk leading to a less efficient cooling there. A test was made for a 52 AU orbital separation, showed that optically thin CPDs are also detectable in band 7 but they need longer integration times ($>$5hrs). Comparing the gap profiles of the same simulation at various ALMA bands and the hydro simulation confirmed that they change significantly, first because the gap is wider at longer wavelengths due to decreasing optical depth; second, the beam convolution makes the gap shallower and at least 25% narrower. Therefore, caution has to be made when estimating planet masses based on ALMA continuum observations of gaps.
description: Accepted for publication at MNRAS. Typos are corrected since previous version. 11 pages, 5 tables, 4 figures