cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Pseudoneureclipsis ohad Malicky 2009, nov.sp.
Creators: name: Malicky, H.
Publisher: name: Zenodo
Year: 2009
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Trichoptera
Polycentropodidae
Pseudoneureclipsis
Pseudoneureclipsis ohad

description: Pseudoneureclipsis ohad nov.sp. (Tafel 7)
Braun, VFL 4–4,5 mm. KA: 9. Segment in LA ventral mässig breit, dann nach oben zu sehr verschmälert; der Dorsalteil, an dem der Dorsalkomplex ansetzt, ist ungewöhnlich kurz. OA klein und oval, mit einem langen, dünnen Finger, der aus der Innenfläche entspringt. Mittellappen ziemlich gross, unregelmässig rundlich dreieckig. Die Mittelplatte besteht aus einem Paar langer, dünner Finger, die nach hinten und unten gerichtet sind. 1. Glied der UA in LA spitz eiförmig, mit einer äusseren rundlichen, nach oben gerichteten Leiste; 2. Glied aus sehr kurzer Basis eine Kralle bildend, die bis zur Hälfte des 1. Glieds reicht. In VA sind die UA breit oval mit einer subdistalen Eindellung der Aussenkante, die je nach Betrachtungswinkel seichter oder tiefer erscheint. PA leicht s - förmig gebogen, mit vielen langen, feinen Stäbchen im Endteil. – Durch die Form des Dorsalkomplexes und der UA ist diese Art gut charakterisiert; ich kenne keine ähnliche.
HT 3 und 333 PT: Vietnam, Na Hang (160 km WW Hanoi), 150-200m, 26.5.-14.6.199 6, leg. A. Napolov & I. Roma.
description: Published as part of Malicky, H., 2009, Übersicht über die Gattung Pseudoneureclipsis (Trichoptera, Polycentropodidae), mit Beschreibung von neuen Arten, pp. 709-735 in Linzer biologische Beiträge 41 (1) on page 720, DOI: 10.5281/zenodo.5276259
The measurement of the flow of heat through the crust of the earth and through rocks
Creators: name: Beck, A. E.
Publisher: name: Canberra, ACT : The Australian National University
Year: 1956

description: Methods of rapidly measuring the temperature gradient in and the thermal conductivity of the rocks in the upper part of the crust of the earth are described A thermistor is used to indicate temperatures in boreholes to within 0. 02 degree C. It has been found possible to detect and locate to within one or two feet the base of porous ;strata through which water is flowing into the borehole. A steady state apparatus has been constructed hich, within 10 minutes, gives values of the thermal esistance of a disc of rock. It has been used to nvestigate the effect of water content on the thermal conductivity of porous rocks as well as for making outine measurements; surprisingly large changes of onductivity have been found for small changes in moisture Content. Methods for the rapid preparation of discs of rock have also been investigated. Evidence is presented for questioning the reliability of thermal conductivities obtained in the aboratory for coarse grained rocks; it is suggestedthat slides of the rocks should be made and examined before deciding on a suitable thickness for each disc. n an attempt to determine whether laboratory rsults give true "in situ" conductivities a thermal conductivity probe was constructed but although the esults were promising there, were too few to allow a efinite conclusion to be reached. Uncorrected mean values for the heat flux were 2.3x 1o-6 cal./sq. cm./sec. for Tasmania and 2.2 x 10-6 : cal./sq. cm./sec. f'or the Snowy Mountains area.
The algebraic entropy of classical mechanics
Creators: name: McLachlan, Robert I
name: Ryland, Brett
Publisher: name: arXiv
Year: 2002
Subjects: subject: Mathematical Physics (math-ph)
subject: FOS: Physical sciences
subject: 17B01,70G45

description: We describe the `Lie algebra of classical mechanics', modelled on the Lie algebra generated by kinetic and potential energy of a simple mechanical system with respect to the canonical Poisson bracket. It is a polynomially graded Lie algebra, a class we introduce. We describe these Lie algebras, give an algorithm to calculate the dimensions $c_n$ of the homogeneous subspaces of the Lie algebra of classical mechanics, and determine the value of its entropy $\lim_{n\to\infty} c_n^{1/n}$. It is $1.82542377420108...$, a fundamental constant associated to classical mechanics.
description: 23 pages, 2 figures, submitted to J Math Phys
XMMU J181227.8-181234: a new ultracompact X-ray binary candidate
Creators: name: Goodwin, A. J.
name: Galloway, D. K.
name: Zand, J. J. M. in 't
name: Kuulkers, E.
name: Bilous, A.
name: Keek, L.
Publisher: name: arXiv
Year: 2019
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: We report the discovery of Type I (thermonuclear) X-ray bursts from the transient source XMMU J181227.8-181234 = XTE J1812-182. We found 7 X-ray bursts in Rossi X-ray Timing Explorer observations during the 2008 outburst, confirming the source as a neutron star low mass X-ray binary. Based on the measured burst fluence and the average recurrence time of 1.4$^{+0.9}_{-0.5}$ hr, we deduce that the source is accreting almost pure helium ($X \leq 0.1$) fuel. Two bursts occurred just 18 minutes apart; the first short waiting time bursts observed in a source accreting hydrogen-poor fuel. Taking into consideration the effects on the burst and persistent flux due to the inferred system inclination of $30\pm{10}$ degrees, we estimate the distance to be $14\pm{2}$ kpc, where we report the statistical uncertainty but note that there could be up to $20\%$ variation in the distance due to systematic effects discussed in the paper. The corresponding maximum accretion rate is $0.30\pm0.05$ times the Eddington limit. Based on the low hydrogen content of the accreted fuel and the short average recurrence time, we classify the source as a transient ultracompact low-mass X-ray binary.
description: 10 pages, 6 figures, 2 tables. Accepted for publication in MNRAS
Pseudoneureclipsis thales MALICKY & CHANTARAMONGKOL 2009, nov.sp.
Creators: name: Malicky, H.
Publisher: name: Zenodo
Year: 2009
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Trichoptera
Polycentropodidae
Pseudoneureclipsis
Pseudoneureclipsis thales

description: Pseudoneureclipsis thales MALICKY & CHANTARAMONGKOL nov.sp. (Tafel 7)
Dunkelbraun, VFL 5–5,5, mm. KA: 9. Segment ventral mässig breit und rundlich, dann nach dorsal hin verschmälert. Im Gegensatz zu vielen anderen Arten ist hier aber die Vorderkante stark sklerotisiert. Seine Kaudalkante hingegen ist häutig und schlecht zu erkennen. OA gross, ungefähr quadratisch, aber seine Dorsalkante ist in eine sehr lange, scharfe Spitze ausgezogen. Mittellappen relativ lang, distal zweilappig. Die Mittelplatte besteht aus zwei sehr dünnen, langen, nach oben/hinten gerichteten Stäben. 1. Glied der UA in LA länglich und leicht flaschenförmig, in VA fast rechteckig und abgerundet. Die Basis des 2. Glieds nimmt ca. ein Drittel der Dorsalkante des ersten ein, das 2. Glied ist sehr dick und gedrungen und weit nach innen gebogen. PA distal mit vielen, in Reihen angeordneten feinen Dörnchen und ausserdem einer Querreihe grosser, gerader Dornen. – Durch die Form des Dorsalkomplexes, vor allem der OA, ist diese Art unverkennbar.
HT 3 und 233 PT: Thailand, Prov. Mae Hong Son, Oberlauf des Huai Mae Ya bei Doi Mae Ya, 1200m, 19°14‘N, 98°35‘E, 13.5.200 5.
description: Published as part of Malicky, H., 2009, Übersicht über die Gattung Pseudoneureclipsis (Trichoptera, Polycentropodidae), mit Beschreibung von neuen Arten, pp. 709-735 in Linzer biologische Beiträge 41 (1) on page 720, DOI: 10.5281/zenodo.5276259
Arrenurus (Arrenurus) abbreviator Berlese 1888
Creators: name: Smit, H.
name: Gerecke, R.
Publisher: name: Zenodo
Year: 2010
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Arachnida
Trombidiformes
Arrenuridae
Arrenurus
Arrenurus abbreviator

description: Arrenurus (Arrenurus) abbreviator Berlese, 1888
 Arrenurus abbreviator Berlese, 1888: Mota¸s 1927b: 3, 1928f: 279; C. & E. Angelier 1953a: 69; E. Angelier 1959: 16, 1959a: 69; Cassagne-MØjean 1966a: 30.
 Petiolurus abbreviator (Berlese, 1888): Chaudonneret 1947: 4.
Distribution in France: Corsica, Côte-d’Or, Essonne, IsŁre, PyrØnØes (Hautes-PyrØnØes).
description: Published as part of Smit, H. & Gerecke, R., 2010, A CHECKLIST OF THE WATER MITES OF FRANCE (ACARI: HYDRACHNIDIA) Harry S and Reinhard G, pp. 21-91 in Acarologia 50 (1) on page 74, DOI: 10.1051/acarologia/20101952, http://zenodo.org/record/5392293
Political Participation of Higher Education Students - A Cross Sectional Survey Study on Rural Area Students in Indian Universities (2018)
Creators: name: Moorthy, C Gothanda
name: P Lazarus Samraj
Publisher: name: figshare
Year: 2019
Subjects: subject: 160699 Political Science not elsewhere classified
subject: FOS: Political science

description: AbstractEven though Republic of India is a single political entity, Her Population is not participating equally in her political affairs. Her Citizens are living in different decades in time lapse, different modes in activity and different levels in intensity. It has been empirically proved in many studies that politically they are influenced by their ascribed & described cleavage identities like ethnicity, religion, region etc. Permutation & Combination of such myriad of Indian Political Cleavages are a daunting task for any political scientist. Due to this factor, one of the most crucial segment of the society i.e. Higher Education Students, is not studied well enough in its political aspects. This segment is the intellectual asset of the society. Their Politicization is one of the significant politicization of the society. They used to lead different walks of life in the society. In all probability, it will be so in the near future too. Therefore, this research paper is trying to do profile mapping of political activities on a portion of that segment i.e. Higher Education Students from Rural areas. For this purpose, Cross Sectional, Sample Survey Study had been carried out with Multi Stage, Mixed Sampling Method. For Data Collection, Questionnaire was used. This Questionnaire was prepared with due care to capture essential twenty political activities and was administered to Students of seven Indian Universities which are located in different parts of India. With the help of twenty political activity variables, Theoretically Five Political Activity Indices were constructed. By utilizing the software SPSS, Values of Political Activity Indices were captured in Tables and Charts. By analyzing the Tables and Charts, It is found that Students are not participating equally in all the activities. They prefer Election Activity more than other activities.
A Catalogue and Analysis of X-ray luminosities of Early-type galaxies
Creators: name: O'Sullivan, Ewan
name: Forbes, Duncan A.
name: Ponman, Trevor J.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present a catalogue of X-ray luminosities for 401 early-type galaxies, of which 136 are based on newly analysed ROSAT PSPC pointed observations. The remaining luminosities are taken from the literature and converted to a common energy band, spectral model and distance scale. Using this sample we fit the L_X:L_B relation for early-type galaxies and find a best fit slope for the catalogue of ~2.2. We demonstrate the influence of group-dominant galaxies on the fit and present evidence that the relation is not well modeled by a single powerlaw fit. We also derive estimates of the contribution to galaxy X-ray luminosities from discrete sources and conclude that they provide L_discrete/L_B = 29.5 erg/s/L_solar. We compare this result to luminosities from our catalogue. Lastly, we examine the influence of environment on galaxy X-ray luminosity and on the form of the L_X:L_B relation. We conclude that although environment undoubtedly affects the X-ray properties of individual galaxies, particularly those in the centres of groups and clusters, it does not change the nature of whole populations.
description: 33 pages, 16 postscript figures, accepted for publication in MNRAS
Subpixel Response of SOI Pixel Sensor for X-ray Astronomy with Pinned Depleted Diode: First Result from Mesh Experiment
Creators: name: Kayama, Kazuho
name: Tsuru, Takeshi G.
name: Tanaka, Takaaki
name: Uchida, Hiroyuki
name: Harada, Sodai
name: Okuno, Tomoyuki
name: Amano, Yuki
name: Hiraga, Junko S.
name: Yoshida, Masayuki
name: Kamata, Yasuaki
name: Sakuma, Shotaro
name: Yuhi, Daito
name: Urabe, Yukino
name: Tsunemi, Hiroshi
name: Matsumura, Hideaki
name: Kawahito, Shoji
name: Kagawa, Keiichiro
name: Yasutomi, Keita
name: Shrestha, Sumeet
name: Nakanishi, Syunta
name: Kamehama, Hiroki
name: Arai, Yasuo
name: Kurachi, Ikuo
name: Takeda, Ayaki
name: Mori, Koji
name: Nishioka, Yusuke
name: Fukuda, Kohei
name: Hida, Takahiro
name: Yukumoto, Masataka
name: Kohmura, Takayoshi
name: Hagino, Kouichi
name: Oono, Kenji
name: Negishi, Kousuke
name: Yarita, Keigo
Publisher: name: arXiv
Year: 2019
Subjects: subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: FOS: Physical sciences

description: We have been developing a monolithic active pixel sensor, ``XRPIX``, for the Japan led future X-ray astronomy mission ``FORCE`` observing the X-ray sky in the energy band of 1-80 keV with angular resolution of better than 15``. XRPIX is an upper part of a stack of two sensors of an imager system onboard FORCE, and covers the X-ray energy band lower than 20 keV. The XRPIX device consists of a fully depleted high-resistivity silicon sensor layer for X-ray detection, a low resistivity silicon layer for CMOS readout circuit, and a buried oxide layer in between, which is fabricated with 0.2 $μ$ m CMOS silicon-on-insulator (SOI) technology. Each pixel has a trigger circuit with which we can achieve a 10 $μ$ s time resolution, a few orders of magnitude higher than that with X-ray astronomy CCDs. We recently introduced a new type of a device structure, a pinned depleted diode (PDD), in the XRPIX device, and succeeded in improving the spectral performance, especially in a readout mode using the trigger function. In this paper, we apply a mesh experiment to the XRPIX devices for the first time in order to study the spectral response of the PDD device at the subpixel resolution. We confirmed that the PDD structure solves the significant degradation of the charge collection efficiency at the pixel boundaries and in the region under the pixel circuits, which is found in the single SOI structure, the conventional type of the device structure. On the other hand, the spectral line profiles are skewed with low energy tails and the line peaks slightly shift near the pixel boundaries, which contribute to a degradation of the energy resolution.
description: 10 pages, 7 figures, , Conference proceedings for PIXEL2018
Pseudoneureclipsis higleri Malicky 2009, nov.sp.
Creators: name: Malicky, H.
Publisher: name: Zenodo
Year: 2009
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Trichoptera
Polycentropodidae
Pseudoneureclipsis
Pseudoneureclipsis higleri

description: Pseudoneureclipsis higleri nov.sp. (Tafel 8)
Braun, VFL 6-7 mm. KA: Der breite Ventralteil des 9. Segments ist allmählich nach oben/hinten verschmälert und gleichzeitig stark nach hinten gebogen; die schmale Dorsalspange sitzt dort im rechten Winkel an und ist gleich hoch wie der Ventralteil. Die OA setzen entlang seiner ganzen Länge an, sind in der Ventralhälfte kurz, aber in der Dorsalhälfte sehr lang nach hinten gebogen; in DA sind sie schmal. Der kurze, breite Ventrokaudalfinger der OA ist dicht mit kleinen Häkchen besetzt. Mittellappen lang, flaschenförmig. Mittelplatte aus zwei langen, distal mit Häkchen besetzten Fingern bestehend. UA kurz, in LA einförmig, in VA breit rhombisch; das 2. Segment ist sehr kurz, die Kralle ebenfalls. PA mit einem Paar schlecht erkennbarer Strukturen innen, sonst ohne Sklerite. – Durch die Form der OA sehr charakteristisch und von allen ähnlichen Arten unterscheidbar.
Diese Art widme ich meinem lieben Kollegen L.G.W. HIGLER.
HT 3: Indien (U.J.K.H.), Thangrain, 22.4.196 0. – 13 PT: do. Mawpran, 10.4.1960; 13 PT: do., Rumkheng, 26.3.1960; 13 PT: do., Nongrim, 27.3.1960; alle leg. F. Schmid, coll. CNC.
description: Published as part of Malicky, H., 2009, Übersicht über die Gattung Pseudoneureclipsis (Trichoptera, Polycentropodidae), mit Beschreibung von neuen Arten, pp. 709-735 in Linzer biologische Beiträge 41 (1) on page 721, DOI: 10.5281/zenodo.5276259
Theoretical Models of Polarized Dust Emission from Protostellar Cores
Creators: name: Padoan, Paolo
name: Goodman, Alyssa
name: Draine, Bruce
name: Juvela, Mika
name: Nordlund, AAke
name: Rognvaldsson, Ornolfur Einar
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We model the polarized thermal dust emission from protostellar cores that are assembled by super-sonic turbulent flows in molecular clouds. Self-gravitating cores are selected from a three dimensional simulation of super-sonic and super-Alfvenic magneto-hydrodynamic (MHD) turbulence. The polarization is computed in two ways. In model A it is assumed that dust properties and grain alignment efficiency are uniform; in model B it is assumed that grains are not aligned at visual extinction larger than 3 mag. The main results of this work are: i) Values of the degree of polarization P between 1 and 10% are typical, despite the super-Alfvenic nature of the turbulence; ii) A steep decrease of P with increasing values of the sub-mm dust continuum intensity I is always found in self--gravitating cores selected from the MHD simulations, if grains are not aligned above a certain value of visual extinction (model B); iii) The same behavior is hard to reproduce if grains are aligned independently of visual extinction (model A); iv) The Chandrasekhar-Fermi formula, corrected by a factor f=0.4, provides an approximate estimate of the average magnetic field strength in the cores. Sub-mm dust continuum polarization maps of quiescent protostellar cores and Bok globules always show a decrease in P with increasing value of I consistent with the predictions of our model B. We therefore conclude that sub-mm polarization maps of quiescent cores do not map the magnetic field inside the cores at visual extinction larger than approximately 3 mag. There is no inconsistency between the results from optical and near-IR polarized absorption of background stars, and the observed polarization of sub-mm dust continuum from quiescent cores. In both cases, grains at large visual extinction appear to be virtually unaligned.
description: 21 pages, color figures, submitted to ApJ
The End of Uncertainty_ Structured Resonance as the Substrate of Philosophy
Creators: name: Bostick, Devin
Publisher: name: Zenodo
Year: 2025
Subjects: subject: Philosophy
subject: FOS: Philosophy, ethics and religion
subject: Science
subject: Theoretical physics
subject: Metaphysics
subject: Philosophy of Language
subject: Philosophy of Structured Emergence
subject: Philosophy of Structured Resonance

description: Main CODES Framework

Abstract

This paper initiates a structural phase transition in the history of philosophy. It argues that the canonical arc—from metaphysics to epistemology, from language games to post-structuralism—was not progress, but a recursive drift from coherence. The root error: mistaking symbolic uncertainty for ontological truth. Through CODES (Chirality of Dynamic Emergent Systems), we present a replacement substrate: structured resonance. Here, truth is not declared, but phase-locked; knowledge is not possessed, but cohered; and the foundational illusions of randomness, dualism, and semantic disjunction are resolved as artifacts of incomplete resonance mapping. This is not a new theory. This is the substrate beneath all coherent theories. What follows is not the collapse of philosophy, but its return—tuned, recursive, and phase-locked to the Field.
Additional file 1 of Translation of two healthy eating and active living support programs for parents of 2–6 year old children: a parallel partially randomised preference trial protocol (the ‘time for healthy habits’ trial)
Creators: name: Hammersley, Megan L.
name: Wyse, Rebecca J.
name: Jones, Rachel A.
name: Wolfenden, Luke
name: Yoong, Serene
name: Stacey, Fiona
name: Eckermann, Simon
name: Okely, Anthony D.
name: Innes-Hughes, Christine
name: Li, Vincy
name: Green, Amanda
name: May, Christine
name: Xu, Joe
name: Rissel, Chris
Publisher: name: figshare
Year: 2020
Subjects: subject: Medicine
subject: Sociology
subject: FOS: Sociology
subject: Biological Sciences not elsewhere classified
subject: Science Policy

description: Additional file 1.Table 1. Trial registration data set.
Candidate Pre-Mainsequence F Stars with Circumstellar Dust Identified Using Combined 2MASS and uvby Data
Creators: name: Suchkov, A. A.
name: Schultz, A. B.
name: Lisse, C. M.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We propose a method that uses near-infrared plus uvby photometry to identify potentially extensive circumstellar dusty environment about F and A stars. The method has been applied to a sample of ~900 metal rich reddened F stars with 2MASS and uvby data, suggesting the presence of circumstellar dust emitting in the near infrared for ~70 stars. The log T_e - M_V diagram suggests that most, if not all, of them are likely pre-mainsequence (PMS). They seem to be consistent with being a continuation of the class of Herbig Ae/Be PMS stars into the spectral type F. Their number drops sharply downward of log T_e ~ 3.84 (spectral types later than ~F5), which may provide new clues to the PMS evolution of stars with 1 to 2 solar mass. We present a list of 21 most conspicuous candidate stars with circumstellar dust. About half of them are associated with the extended star-forming region around rho Oph. The brightest of these 21 stars, with V < 7.5, turn out to be IRAS sources, suggesting the presence of heated dust emitting in the far infrared. Also in this list, HD 81270 is reported as a very unusual star moving away from the Galactic plane at a projected speed of 70 km/sec.
description: 8 pages, 4 figures, 1 table. To appear in ApJ, part 2, v. 570, 2002 May 1
Constraints on the primordial curvature power spectrum from primordial black holes
Creators: name: Sato-Polito, Gabriela
name: Kovetz, Ely D.
name: Kamionkowski, Marc
Publisher: name: arXiv
Year: 2019
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: Large-amplitude density perturbations may have collapsed during the radiation dominated epoch of the Universe to form primordial black holes (PBHs). There are several constraints to the abundance of PBHs that stem from evaporation or gravitational effects. Due to the connection between primordial perturbations and the formation of PBHs, constraints on the present-day abundance of PBHs can be translated into limits on the primordial curvature power spectrum. We introduce several new observational and forecasted constraints to the amplitude of the primordial power spectrum and incorporate in our analysis uncertainties in the critical overdensity for collapse and considerations of ellipsoidal collapse. Our results provide the most stringent limits from PBHs on the primordial curvature power spectrum on small scales.
description: 7 pages, 2 figures; submitted for publication in PRD
Pseudoneureclipsis hazarmavet MALICKY & MEY 2009, nov.sp.
Creators: name: Malicky, H.
Publisher: name: Zenodo
Year: 2009
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Trichoptera
Polycentropodidae
Pseudoneureclipsis
Pseudoneureclipsis hazarmavet

description: Pseudoneureclipsis hazarmavet MALICKY & MEY nov.sp. (Tafel 9)
Dunkelbraun, VFL 4 mm. KA: 9. Segment in LA relativ breit, mit einem weiten Vorsprung in der Mitte der Vorderkante. Dorsalteil schmal. OA rundlich, mit einer sehr langen, nach oben gebogenen Kralle, die an der Innenfläche entspringt. Mittellappen relativ gross und zweilappig, wobei die beiden Lappen breit voneinander getrennt sind; von ihrer Ventralseite entspringt je ein langer, in LA keulenförmiger Fortsatz, der nach oben gebogen ist. Ob es sich dabei eventuell um die Mittelplatte handelt, ist nicht erkennbar. Unterhalb davon gibt es ein Paar sehr grosser, spitzer Krallen, die dem PA anliegen; auch diese könnten die Mittelplatte sein. 1. Glied der UA in LA eiförmig, in VA parallelrandig und distal abgestutzt. 2. Glied aus breiter Basis in eine basal breite, dann dünne Kralle verlaufend, die bis ca. 2/3 der Länger des 1. Glieds reicht. PA mit vielen kleinen Dörnchen und einem Paar gerader Stäbchen im Endteil. - Die Form des Dorsalkomplexes charakterisiert die Art ziemlich gut.
HT 3 und 13 PT: Kambodscha, Cardamom Mts., Pramuoy vill., 270m, 12°16‘N, 103°01‘E, 24.- 25.2.200 0, leg. M. Nuss, coll. Zoologisches Museum Berlin.
description: Published as part of Malicky, H., 2009, Übersicht über die Gattung Pseudoneureclipsis (Trichoptera, Polycentropodidae), mit Beschreibung von neuen Arten, pp. 709-735 in Linzer biologische Beiträge 41 (1) on page 722, DOI: 10.5281/zenodo.5276259
The Las Campanas IR Survey. II. Photometric redshifts, comparison with models and clustering evolution
Creators: name: Firth, A. E.
name: Somerville, R. S.
name: McMahon, R. G.
name: Lahav, O.
name: Ellis, R. S.
name: Sabbey, C. N.
name: McCarthy, P. J.
name: Chen, H. -W.
name: Marzke, R. O.
name: Wilson, J.
name: Abraham, R. G.
name: Beckett, M. G.
name: Carlberg, R. G.
name: Lewis, J. R.
name: Mackay, C. D.
name: Murphy, D. C.
name: Oemler, A. E.
name: Persson, S. E.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The LCIR Survey, using the Cambridge IR Survey Instrument (CIRSI), reaches H \~ 20-21 over ~1 deg^2. We present results for 744 arcmin^2 in which public UBVRI data exist. We compare optical-IR colours with predictions of a semi-analytic hierarchical model (SAM) and find reasonable agreement. We also determine photometric redshifts, finding a median z of z_m ~ 0.55. We compare N(z) of different spectral types with models, showing that the observations are inconsistent with simple PLE models while the SAM provides a reasonable fit to the total N(z) but underestimates the number of z ~ 1 red spectral types. We also present N(z) for samples of red objects (EROs). We find that EROs with R - H > 4 and H < 20.5 have z_m ~ 1; redder EROs have higher z_m. For 19 < H < 20, EROs with R - H > 4 comprise ~18% of the observed galaxy population while in the SAM they contribute only ~4%. We also determine the angular correlation function w(theta) for magnitude, colour, spectral type and photo-z selected samples and use the estimated N(z) to derive the spatial clustering xi(r). Parametrizing xi(r) by xi(r_c,z)=(r_c/r_*(z))^(-1.8) (r_c comoving), we find that r_*(z) increases by ~1.5-2 times from z = 0 to z ~ 1.2. We interpret this as a selection effect - the galaxies selected at z ~ 1.2 are intrinsically very luminous. When galaxies are selected by absolute magnitude we find no evidence for evolution in r_* over this z range. Extrapolated to z = 0, we find r_*(0) ~ 6.5 h^-1Mpc for red galaxies and r_*(0) ~ 2-4 h^-1Mpc for blue galaxies. We also find that while the angular clustering amplitude of EROs with R - H > 4 or I - H > 3 is up to four times that of the whole galaxy population, the spatial clustering length r_*(z=1) is ~7.5-10.5 h^-1Mpc which is only a factor of ~1.7 times r_* for non-EROs lying in a similar z and luminosity range.
description: Accepted by MNRAS, 32 pages, 39 figures, 9 tables; accepted version - typos corrected, 2 new figures
Arrenurus (Arrenurus) batillifer Koenike 1896
Creators: name: Smit, H.
name: Gerecke, R.
Publisher: name: Zenodo
Year: 2010
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Arachnida
Trombidiformes
Arrenuridae
Arrenurus
Arrenurus batillifer

description: Arrenurus (Arrenurus) batillifer Koenike, 1896
 Arrenurus batillifer Koenike, 1896: Mota¸s 1927b: 3, 1928f: 280, 1928g: 6; C. & E. Angelier 1953a: 70; Cassagne-MØjean 1966a: 43; Smit & Van der Hammen 1992: 55.
 Petiolurus batillifer (Koenike, 1896): Chaudonneret 1947: 4.
Distribution in France: Ain, Cantal, Côte-d’Or, IsŁre, Pas-de-Calais, PyrØnØes (Hautes-PyrØnØes, PyrØnØes-Atlantiques).
description: Published as part of Smit, H. & Gerecke, R., 2010, A CHECKLIST OF THE WATER MITES OF FRANCE (ACARI: HYDRACHNIDIA) Harry S and Reinhard G, pp. 21-91 in Acarologia 50 (1) on page 75, DOI: 10.1051/acarologia/20101952, http://zenodo.org/record/5392293
Political Participation of Higher Education Students - A Cross Sectional Survey Study on Rural Area Students in Indian Universities (2018)
Creators: name: Moorthy, C Gothanda
name: Dr.P.Lazarus Samraj Ph.D
Publisher: name: figshare
Year: 2019
Subjects: subject: 160699 Political Science not elsewhere classified
subject: FOS: Political science

description: AbstractEven though Republic of India is a single political entity, Her Population is not participating equally in her political affairs. Her Citizens are living in different decades in time lapse, different modes in activity and different levels in intensity. It has been empirically proved in many studies that politically they are influenced by their ascribed & described cleavage identities like ethnicity, religion, region etc. Permutation & Combination of such myriad of Indian Political Cleavages are a daunting task for any political scientist. Due to this factor, one of the most crucial segment of the society i.e. Higher Education Students, is not studied well enough in its political aspects. This segment is the intellectual asset of the society. Their Politicization is one of the significant politicization of the society. They used to lead different walks of life in the society. In all probability, it will be so in the near future too. Therefore, this research paper is trying to do profile mapping of political activities on a portion of that segment i.e. Higher Education Students from Rural areas. For this purpose, Cross Sectional, Sample Survey Study had been carried out with Multi Stage, Mixed Sampling Method. For Data Collection, Questionnaire was used. This Questionnaire was prepared with due care to capture essential twenty political activities and was administered to Students of seven Indian Universities which are located in different parts of India. With the help of twenty political activity variables, Theoretically Five Political Activity Indices were constructed. By utilizing the software SPSS, Values of Political Activity Indices were captured in Tables and Charts. By analyzing the Tables and Charts, It is found that Students are not participating equally in all the activities. They prefer Election Activity more than other activities.
Arrenurus (Arrenurus) bruzelii Koenike 1885
Creators: name: Smit, H.
name: Gerecke, R.
Publisher: name: Zenodo
Year: 2010
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Arachnida
Trombidiformes
Arrenuridae
Arrenurus
Arrenurus bruzelii

description: Arrenurus (Arrenurus) bruzelii Koenike, 1885
 Arrenurus bruzelii Koenike, 1885: Barrois & Moniez 1887: 25; Derône 1914: 46, 1915: 560; Vandel 1919a: 91; Soudan 1920: 5; Mota¸s 1926b: 411, 1928f: 280, 1928g: 6; C. Angelier 1950a: 6, 1953: 223; Do 1962: 67; Cassagne-MØjean 1966a: 69.
 Petiolurus Bruzelii (Koenike, 1885): Chaudonneret 1947: 4.
 New record. Indre: 1/0/0, Étang Prieur, SW of MØobecq, 46°42’48.18" N, 1°23’40.40" E, 7 July 2000, leg. H. van der Hammen.
Distribution in France: Cantal, Côte-d’Or, Doubs, Essonne, Haute-Saône, HØrault, Indre, IsŁre, Jura, Nord, Pas-de-Calais, Savoie, Var.
description: Published as part of Smit, H. & Gerecke, R., 2010, A CHECKLIST OF THE WATER MITES OF FRANCE (ACARI: HYDRACHNIDIA) Harry S and Reinhard G, pp. 21-91 in Acarologia 50 (1) on pages 75-76, DOI: 10.1051/acarologia/20101952, http://zenodo.org/record/5392293
Pseudoneureclipsis ziphjon Malicky 2009, nov.sp.
Creators: name: Malicky, H.
Publisher: name: Zenodo
Year: 2009
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Trichoptera
Polycentropodidae
Pseudoneureclipsis
Pseudoneureclipsis ziphjon

description: Pseudoneureclipsis ziphjon nov.sp. (Tafel 9)
Braun, VFL 3,5 mm. KA: Das 9. Segment ist in LA mässig breit, hat im unteren Drittel der Vorderkante einen fast rechteckigen Vorsprung und in der Mitte der Kaudalkante eine tiefe runde Einbuchtung. Der Dorsalteil ist etwas verschmälert, aber nicht auf eine schmale Spange reduziert. OA gross, in LA mit konvexer Ventral- und leicht konkaver Dorsalkante. Mittellappen kurz, rundlich. Die Mittelplatte besteht aus einem Paar dicker, rundlicher Finger. Das 1. Glied der UA hat in LA eine konvexe Ventralkante und dorsal einen nach vorne gerichteten, abstehenden Finger, in VA ist es breit dreieckig mit abgerundet rechteckiger Innenecke, die mit grossen Dörnchen besetzt ist, und einer leicht nach aussen verlängerten Aussenecke. Das 2. Glied ist in LA nur in Form eines rundlichen Knopfes zu sehen; in VA ist es breit und rundlich fingerförmig und weit nach innen gerichtet. Der PA hat distal zwei Paar spitzer Dornen. Nach der Form der UA ist diese Art unverkennbar.
HT: 3 und 433 PT: Indien (Madras), Ottakada, 5.1.196 2, leg. F. Schmid, coll. CNC.
description: Published as part of Malicky, H., 2009, Übersicht über die Gattung Pseudoneureclipsis (Trichoptera, Polycentropodidae), mit Beschreibung von neuen Arten, pp. 709-735 in Linzer biologische Beiträge 41 (1) on page 722, DOI: 10.5281/zenodo.5276259
Physics of Weibel-mediated relativistic collisionless shocks
Creators: name: Lemoine, M.
name: Gremillet, L.
name: Pelletier, G.
name: Vanthieghem, A.
Publisher: name: arXiv
Year: 2019
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Plasma Physics (physics.plasm-ph)
subject: FOS: Physical sciences

description: We develop a comprehensive theoretical model of relativistic collisionless pair shocks mediated by the current filamentation instability. We notably characterize the noninertial frame in which this instability is of a mostly magnetic nature, and describe at a microscopic level the deceleration and heating of the incoming background plasma through its collisionless interaction with the electromagnetic turbulence. Our model compares well to large-scale 2D3V PIC simulations, and provides an important touchstone for the phenomenology of such plasma systems.
description: Phys. Rev. Lett. 123, 035101 (2019)
Bracelets and the Goussarov Filtration of the Space of Knots
Creators: name: Bar-Natan, Dror
Publisher: name: arXiv
Year: 2001
Subjects: subject: Geometric Topology (math.GT)
subject: FOS: Mathematics
subject: 57M27

description: Following Goussarov's paper `Interdependent Modifications of Links and Invariants of Finite Degree' [Topology 37 (1998) 595--602] we describe an alternative finite type theory of knots. While (as shown by Goussarov) the alternative theory turns out to be equivalent to the standard one, it nevertheless has its own share of intrinsic beauty.
description: Published by Geometry and Topology Monographs at http://www.maths.warwick.ac.uk/gt/GTMon4/paper1.abs.html
Arrenurus (Arrenurus) compactus Piersig 1894
Creators: name: Smit, H.
name: Gerecke, R.
Publisher: name: Zenodo
Year: 2010
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Arachnida
Trombidiformes
Arrenuridae
Arrenurus
Arrenurus compactus

description: Arrenurus (Arrenurus) compactus Piersig, 1894
 Arrenurus compactus Piersig, 1894: Vandel 1919a: 91; Mota¸s 1928e: 28, 1928f: 280, 1928g: 13; C. & E. Angelier1953a: 70; Cassagne-MØjean 1966a: 53.
Distribution in France: Doubs, Haute-Saône, IsŁre, PyrØnØes (Hautes-PyrØnØes).
description: Published as part of Smit, H. & Gerecke, R., 2010, A CHECKLIST OF THE WATER MITES OF FRANCE (ACARI: HYDRACHNIDIA) Harry S and Reinhard G, pp. 21-91 in Acarologia 50 (1) on page 76, DOI: 10.1051/acarologia/20101952, http://zenodo.org/record/5392293
The P-W problem
Creators: name: Martin, Errol Peter
Publisher: name: The Australian National University
Year: 1978
Subjects: subject: Logic, Symbolic and mathematical

description: This thesis investigates the properties of two systems of pure implication, with axioms a~d rules corresponding to the principles of transitivity of implication in the one system, and these axioms and rules plus the law of identity in the other. The main part of the text is devoted to a semantic analysis of these two systems. A class of models, called S-models, is defined and studied. The original construction of these S-models is due to R.K. Meyer. They derive t heir strength and interest from the fact that they employ a three-valued interpretation of the metalogical operations. By suitably determining the notion of validity using these three values, both of the systems mentioned above can be accommodated at once within the same class of models. The results obtained include soundness and completeness, decidability, arid, most importantly, the solution to a problem posed by Anderson and Belnap in their treatise, Entailment (Princeton U.P. 1975). Briefly, it is shown that, in the system o f pure transitivity axioms (and corresponding rules) , no instance of the axiom of identity is provable. When the axiom of identity is added to the system , one obtains as a corresponding result that no two distinct formulas co-entail each other.
On the Power Spectrum Density of Gamma Ray Bursts
Creators: name: Suzuki, Motoko
name: Morikawa, Masahiro
name: Joichi, Izumi
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Gamma ray bursts (GRBs) are known to have short-time variability and power-law behavior with the index -1.67 in the power spectrum density. Reanalyzing the expanded data, we have found a) the power-law comes from the global profile of the burst and not from the self-similar shots nor rapid fluctuations in the luminosity profile. b) The power indices vary from burst to burst and the value -1.67 is given simply as the mean value of the distribution; there is no systematic correlation among GRBs to yield the power law.
description: 10 pages, 4 figures, submitted to ApJ Letters
Arrenurus (Arrenurus) crassicaudatus Kramer 1875
Creators: name: Smit, H.
name: Gerecke, R.
Publisher: name: Zenodo
Year: 2010
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Arachnida
Trombidiformes
Arrenuridae
Arrenurus
Arrenurus crassicaudatus

description: Arrenurus (Arrenurus) crassicaudatus Kramer, 1875
 Arrenurus crassicaudatus Kramer, 1875: Vandel 1919a: 91; Mota¸s & C. Angelier 1927d: 14; Mota¸s 1928e: 28, 1928f: 278, 1928g: 9; C. Angelier 1953: 226; E. Angelier et al. 1963: 465; Smit & Van der Hammen 1992: 55.
 Micrarrenurus crassicaudatus (Kramer, 1875): Cassagne-MØjean 1966a: 83.
 New records. Pas-de-Calais: 0/1/0, pond, Les Landes de Blendecques, 50°42’13.21" N 2°16’53.08" E, 19 April 1996, leg. H. Smit & H. van der Hammen; 0/4/0, fish pond, Les Landes de Blendecques, 50°42’13.72" N 2°16’53.52" E, 20 April 1996, leg. H. Smit & H. van der Hammen. Indre: 3/11/0, Étang Prieur, SW of MØobecq, 46°42’48.18" N, 1°23’40.40" E, 7 July 2000, leg. H. van der Hammen; 1/0/0, Étang Nuret, La Brenne, 46°47’30.57" N 1°12’35.98" E, 9 July 2000, leg. H. van der Hammen.
Distribution in France: Ain, Doubs, Haute-Loire, Haute-Savoie, Indre, IsŁre, Jura, Pas-de-Calais, Puyde-Dôme, Savoie, Tarn.
description: Published as part of Smit, H. & Gerecke, R., 2010, A CHECKLIST OF THE WATER MITES OF FRANCE (ACARI: HYDRACHNIDIA) Harry S and Reinhard G, pp. 21-91 in Acarologia 50 (1) on page 76, DOI: 10.1051/acarologia/20101952, http://zenodo.org/record/5392293
Nuclear data-induced uncertainty quantification of prompt neutron decay constant based on perturbation theory for ADS experiments at KUCA
Creators: name: Endo, Tomohiro
name: Watanabe, Kenichi
name: Chiba, Go
name: Yamanaka, Masao
name: Rooijen, Willem Frederik Geert Van
name: Pyeon, Cheol Ho
Publisher: name: Taylor & Francis
Year: 2019
Subjects: subject: Cell Biology
subject: Pharmacology
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: Hematology

description: In experimental benchmarks of the accelerator-driven system (ADS) conducted at the Kyoto University Critical Assembly (KUCA), the prompt neutron decay constant α was measured using two types of pulsed neutron sources, i.e. a D-T neutron source and a spallation neutron source driven by a 100-MeV proton beam. The measurement results of α are useful information to validate the numerical results predicted by the prompt ω-eigenvalue calculation. In this study, the numerical analysis of α using a multi-energy group SN neutron transport code was carried out for the uranium-lead zoned experimental cores. To reduce the discretization error owing to the deterministic code, the KUCA geometry was modelled in detail as a three-dimensional heterogeneous plate-by-plate geometry, and an improved variant of EON quadrature was utilized. In addition, the sensitivity coefficients of α with respect to nuclear data were efficiently evaluated by first-order perturbation theory, followed by nuclear data-induced uncertainty quantification based on the 56 neutron-energy group SCALE covariance library. Consequently, the numerical results of α were validated successfully by the experimental results of the pulsed neutron source method, compared with the range of the nuclear data-induced uncertainties.
Atrichelaphinis tigrina
Creators: name: Mitter, H.
Publisher: name: Zenodo
Year: 2009
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Cetoniidae
Atrichelaphinis
Atrichelaphinis tigrina

description: Atrichelaphinis tigrina (OLIVIER 1789)
M a t e r i a l: Umg. Kokstad, S-Afrika, 4 Ex. (undatiert), leg. H. Franz; Orib Gorge b. Port Sheperton, S-Afrika, 1 Ex. (undatiert), leg. H. Franz.
In Südafrika montan verbreitet.
description: Published as part of Mitter, H., 2009, Bemerkenswerte Cetoniidae aus der Sammlung von H. Franz im Naturhistorischen Museum Wien (Coleoptera: Cetoniidae), pp. 743-746 in Linzer biologische Beiträge 41 (1) on page 744, DOI: 10.5281/zenodo.5276267
Pulsating Heat Pipe Simulations: Impact of PHP Orientation
Creators: name: Nekrashevych, Iaroslav
name: Nikolayev, Vadim
Publisher: name: arXiv
Year: 2019
Subjects: subject: Classical Physics (physics.class-ph)
subject: Fluid Dynamics (physics.flu-dyn)
subject: FOS: Physical sciences

description: The pulsating (called also oscillating) heat pipe (PHP) is a simple capillary tube bent in meander and filled with a two-phase fluid. We discuss numerical simulations of the 10-turn copper-water PHP under vertical favorable (bottom-heated), vertical unfavorable (top-heated), and horizontal orientations. Within the present approach, the horizontal orientation is equivalent to the microgravity conditions. The simulations are performed with the in-house CASCO software. The time-averaged spatial distribution of the liquid plugs inside the PHP is influenced by gravity. This affects the overall PHP performance. We show that, independently of the PHP orientation, contribution of the latent heat transfer is large with respect to the sensible heat transfer. We discuss the phenomena occurring inside the PHP during startup and the stable regimes (intermittent and continuous oscillations followed by dryout
description: Microgravity Science and Technology, Springer, 2019
Characterization of M,L and T dwarfs in the Sloan Digital Sky Survey
Creators: name: Hawley, S. L.
name: Covey, K. R.
name: Knapp, G. R.
name: Golimowski, D. A.
name: Fan, X.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: An extensive sample of M, L and T dwarfs identified in the Sloan Digital Sky Survey (SDSS) has been compiled. The sample of 718 dwarfs includes 677 new objects (629 M dwarfs, 48 L dwarfs) together with 41 that have been previously published. All new objects and some of the previously published ones have new optical spectra obtained either with the SDSS spectrographs or with the Apache Point Observatory 3.5m ARC telescope. Spectral types and SDSS colors are available for all objects; approximately 35% also have near-infrared magnitudes measured by 2MASS or on the Mauna Kea system. We use this sample to characterize the color--spectral type and color--color relations of late type dwarfs in the SDSS filters, and to derive spectroscopic and photometric parallax relations for use in future studies of the luminosity and mass functions based on SDSS data. We find that the (i*-z*) and (i*-J) colors provide good spectral type and absolute magnitude (M_i*) estimates for M and L dwarfs. Our distance estimates for the current sample indicate that SDSS is finding early M dwarfs out to about 1.5 kpc, L dwarfs to approximately 100 pc and T dwarfs to near 20 pc. The T dwarf photometric data show large scatter and are therefore less reliable for spectral type and distance estimation.
description: 46 pages, 14 figures (24 pages of figures), Accepted for publication in the Astronomical Journal
Chiloloba acuta
Creators: name: Mitter, H.
Publisher: name: Zenodo
Year: 2009
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Cetoniidae
Chiloloba
Chiloloba acuta

description: Chiloloba acuta (WIEDEMANN 1823)
M a t e r i a l: Rampur, Theral, Nepal, 9 Ex. (undatiert), leg. H. Franz.
Besonders in Indien weit verbreitete Art.
description: Published as part of Mitter, H., 2009, Bemerkenswerte Cetoniidae aus der Sammlung von H. Franz im Naturhistorischen Museum Wien (Coleoptera: Cetoniidae), pp. 743-746 in Linzer biologische Beiträge 41 (1) on page 744, DOI: 10.5281/zenodo.5276267
Retrieving the True Masses of Gravitational-wave Sources
Creators: name: Chen, Xian
name: Shen, Zhe-Feng
Publisher: name: arXiv
Year: 2019
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: Gravitational waves (GWs) encode important information about the mass of the source. For binary black holes (BBHs), the templates that are used to retrieve the masses normally are developed under the assumption of a vacuum environment. However, theories suggest that some BBHs form in gas-rich environments. Here we study the effect of hydrodynamic drag on the chirp signal of a stellar-mass BBH and the impact on the measurement of the mass. Based on theoretical arguments, we show that the waveform of a BBH in gas resembles that of a more massive BBH residing in a vacuum. The effect is important for LISA sources but negligible for LIGO/Virgo binaries. Furthermore, we carry out a matched-filtering search of the best fitting parameters. We find that the best-fit chirp mass could be significantly greater than the real mass if the gas effect is not appropriately accounted for. Our results have important implications for the future joint observation of BBHs using both ground- and space-based detectors.
description: 5 pages, 1 figure. This is a contribution to the conference proceedings: Recent Progress in Relativistic Astrophysics, Fudan University, China
Geometric factors in the Bohr--Rosenfeld analysis of the measurability of the electromagnetic field
Creators: name: Hnizdo, V.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Mathematical Physics (math-ph)
subject: FOS: Physical sciences

description: The Geometric factors in the field commutators and spring constants of the measurement devices in the famous analysis of the measurability of the electromagnetic field by Bohr and Rosenfeld are calculated using a Fourier--Bessel method for the evaluation of folding integrals, which enables one to obtain the general geometric factors as a Fourier--Bessel series. When the space region over which the factors are defined are spherical, the Fourier--Bessel series terms are given by elementary functions, and using the standard Fourier-integral method of calculating folding integrals, the geometric factors can be evaluated in terms of manageable closed-form expressions.
description: 21 pages, REVTeX