cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Neoseiulus bellottii Moraes & Mesa
Creators: name: Lofego, A. C.
name: De Moraes, G. J.
name: Castro, L. A. S.
Publisher: name: Zenodo
Year: 2004
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Arachnida
Mesostigmata
Phytoseiidae
Neoseiulus
Neoseiulus bellottii

description: Neoseiulus bellottii (Moraes & Mesa)
 Amblyseius bellottii Moraes & Mesa, 1988: 75. Neoseiulus bellottii, Moraes et al., 2004: 108.
 Specimens examined: São Carlos: C. pubescens, I­2000 (8), V­2000 (20); X­2000 (2), I­ 2001 (16), IV­2001 (7), VII­2002 (1), X­2001 (17); M. guianensis, I­2001 (1); P. guajava, IV­2001 (7), X­2001 (1). Pirassununga: C. pubescens, I­2000 (5), V­2000 (32), XI­2000 (16), I­2001 (9), IV­2001 (12), VII­2001 (4), X­2001 (8); M. guianensis, ­ I­2001 (1); P. guajava, IV­2001 (6), X­2001 (1). P.guineense, I­2000 (1), IV­2001 (1). Luiz Antônio: P. guajava, V­2000 (3), I­2001 (1).
 Associated phytophagous mites: Abacarus sp. and O. psidii on P. guajava; Tenuipalpus sp. and Olygonychus sp. on C. pubescens.
 Previous records: Brazil — Bahia; Colombia.
 Remarks: The measurements of 6 adult females collected are similar to those given in the original description, except for j6, J2, Z1 and S5, which are about 25% shorter. The average measurements followed by the respective ranges (in parentheses) are: dorsal shield length 280 (275–285), width 168 (163–180), j1 20 (18–23), j3 30 (28–33), j4 8, j5 8, j6 10, J2 10, J5 7 (6–8), z2 19 (18–20), z4 18 (15–20), z5 7 (5–8), Z1 12 (10–13), Z4 52 (48–58), Z5 68 (65–73), s4 47 (43–50), S2 20 (18–23), S4 14 (13–15), S5 11 (10–13), r3 16 (15–18), R1 13, Sge IV 34 (33–38), Sti IV 18 (18–20), St IV 33 (30–35), St1–St3 56 (55–60), St2–St2 61 (58–65), St5–St5 64 (60–70), length of ventrianal shield 93 (83–98), width at ZV2 level 72 (68–75), width at anus level 65 (63–68), length of calyx of spermatheca 7 (5–8).
The measurements of a single male are: dorsal shield length 220, width 158, j1 15, j3 25, j4 8, j5 8, j6 9, J2 9, J5 5, z2 15, z4 14, z5 8, Z1 10, Z4 40, Z5 45, s4 33, S2 15, S4 10, S5 9, r3 13, R1 11, Sge IV 23, St IV 30, width of ventrianal shield 137 at anterior corners, length of shaft of spermadactyl 13. All measurements are similar to those given in the original description, except for r3 that is ca. 30% shorter.
description: Published as part of Lofego, A. C., De Moraes, G. J. & Castro, L. A. S., 2004, Phytoseiid mites (Acari: Phytoseiidae) on Myrtaceae in the State of São Paulo, Brazil, pp. 1-18 in Zootaxa 516 on pages 7-8, DOI: 10.5281/zenodo.157769
Evolution of the quasi-periodic oscillation frequency in GRO J1655-40 -- Implications for accretion disk dynamics
Creators: name: Chakrabarti, Sandip K.
name: Debnath, Dipak
name: Nandi, Anuj
name: Pal, P. S.
Publisher: name: arXiv
Year: 2008
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Low and intermediate frequency quasi-periodic oscillations (QPOs) are thought to be due to oscillations of Comptonizing regions or hot blobs embedded in Keplerian disks. Any movement of these perturbations is expected systematically to change the QPO frequency. Our goal is to find systems where such a systematic drifts have been observed. We also try to find the real cause of such drifts and whether they shed some light on the accretion disk dynamics. Using archival data of the recent outburst of GRO J1655-40, we report the presence of such systematic drifts not only during the rising phase from the 25th of February 2005 to the 12th March 2005, when the QPO frequency monotonically increased from 82mHz to 17.78Hz but also in the decline phase from the 15th September 2005 to the 5th of October 2005, when the QPO frequency decreased from 13.14Hz to 34mHz. We fitted the frequency drifts with the propagatory oscillating shock solution. In the shock-oscillation solution, the frequency is inversely proportional to the infall time scale from the shock location. We obtained the shock location and strength through such a fit. The astonishing smoothness of the variation of the QPO frequency over a period of weeks directly supports the view that it may due to the drift of an oscillating shock rather than the movements of a blob inside a differentially rotating disk.
description: 8 pages, 3 figures, Astronomy & Astrophysics (accepted)
Renormalization group study of the four-body problem
Creators: name: Schmidt, Richard
name: Moroz, Sergej
Publisher: name: arXiv
Year: 2009
Subjects: subject: Quantum Gases (cond-mat.quant-gas)
subject: Other Condensed Matter (cond-mat.other)
subject: Nuclear Theory (nucl-th)
subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We perform a renormalization group analysis of the non-relativistic four-boson problem by means of a simple model with pointlike three- and four-body interactions. We investigate in particular the unitarity point where the scattering length is infinite and all energies are at the atom threshold. We find that the four-body problem behaves truly universally, independent of any four-body parameter. Our findings confirm the recent conjectures of Platter et al. and von Stecher et al. that the four-body problem is universal, now also from a renormalization group perspective. We calculate the corresponding relations between the four- and three-body bound states, as well as the full bound state spectrum and comment on the influence of effective range corrections.
description: 11 pages, 6 figures; v2: revised and published version
Is leptogenesis falsifiable at LHC?
Creators: name: Frère, J. -M.
name: Hambye, T.
name: Vertongen, G.
Publisher: name: arXiv
Year: 2008
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: It is well known that the leptogenesis mechanism offers an attractive possibility to explain the baryon asymmetry of the universe. Its particular robustness however comes with one major difficulty: it will be very hard if not impossible to test experimentally in a foreseeable future, as most of the mechanics typically takes place at high energy or results from suppressed interactions, without unavoidable low-energy implications. An alternate approach is taken by asking: can it be at least falsified? We show that possible discoveries at current and future colliders, most notably that of right-handed gauge interactions, would indeed forbid at least the "canonical" leptogenesis mechanisms, namely those based on right-handed neutrino decay. General lower bounds for successful leptogenesis on the mass of the right-handed gauge boson W_R are given. Other possibilities to falsify leptogenesis, including from the observation of a Z', are also considered.
description: 22 pages ; v3: discussion about resonant leptogenesis case added ; matches JHEP published version
Pressure induced orientational glass phase in molecular para-hydrogen
Creators: name: Schelkacheva, T. I.
name: Tareyeva, E. E.
name: Chtchelkatchev, N. M.
Publisher: name: arXiv
Year: 2008
Subjects: subject: Disordered Systems and Neural Networks (cond-mat.dis-nn)
subject: Statistical Mechanics (cond-mat.stat-mech)
subject: FOS: Physical sciences

description: We propose a theoretical description of possible orientational glass transition in solid molecular para-hydrogen and ortho-deuterium under pressure supposing that they are mixtures of J=0 and J=2 states of molecules. The theory uses the basic concepts and methods of standard spin-glass theory. We expect our orientational glass to correspond the II' phase of the high pressure hydrogen phase diagram.
A real-time software backend for the GMRT
Creators: name: Roy, Jayanta
name: Gupta, Yashwant
name: Pen, Ue-Li
name: Peterson, Jeffrey B.
name: Kudale, Sanjay
name: Kodilkar, Jitendra
Publisher: name: arXiv
Year: 2009
Subjects: subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: FOS: Physical sciences

description: The new era of software signal processing has a large impact on radio astronomy instrumentation. Our design and implementation of a 32 antennae, 33 MHz, dual polarization, fully real-time software backend for the GMRT, using only off-the-shelf components, is an example of this. We have built a correlator and a beamformer, using PCI-based ADC cards and a Linux cluster of 48 nodes with dual gigabit inter-node connectivity for real-time data transfer requirements. The highly optimized compute pipeline uses cache efficient, multi-threaded parallel code, with the aid of vectorized processing. This backend allows flexibility in final time and frequency resolutions, and the ability to implement algorithms for radio frequency interference rejection. Our approach has allowed relatively rapid development of a fairly sophisticated and flexible backend receiver system for the GMRT, which will greatly enhance the productivity of the telescope. In this paper we describe some of the first lights using this software processing pipeline. We believe this is the first instance of such a real-time observatory backend for an intermediate sized array like the GMRT.
description: 33 pages, 23 figures, 1 table, Published online in Experimental Astronomy
Implementation of a 46-node quantum metropolitan area network
Creators: name: Chen, Teng-Yun
name: Jiang, Xiao
name: Tang, Shi-Biao
name: Zhou, Lei
name: Yuan, Xiao
name: Zhou, Hongyi
name: Wang, Jian
name: Liu, Yang
name: Chen, Luo-Kan
name: Liu, Wei-Yue
name: Zhang, Hong-Fei
name: Cui, Ke
name: Liang, Hao
name: Li, Xiao-Gang
name: Mao, Yingqiu
name: Wang, Liu-Jun
name: Feng, Si-Bo
name: Chen, Qing
name: Zhang, Qiang
name: Li, Li
name: Liu, Nai-Le
name: Peng, Cheng-Zhi
name: Ma, Xiongfeng
name: Zhao, Yong
name: Pan, Jian-Wei
Publisher: name: arXiv
Year: 2021
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: Quantum key distribution (QKD) enables secure key exchanges between two remote users. The ultimate goal of secure communication is to establish a global quantum network. The existing field tests suggest that quantum networks are feasible. To achieve a practical quantum network, we need to overcome several challenges, including realising versatile topologies for large scales, simple network maintenance, extendable configuration, and robustness to node failures. To this end, we present a field operation of a quantum metropolitan-area network with 46 nodes and show that all these challenges can be overcome with cutting-edge quantum technologies. In particular, we realise different topological structures and continuously run the network for 31 months, by employing standard equipment for network maintenance with an extendable configuration. We realise QKD pairing and key management with a sophisticated key control center. In this implementation, the final keys have been used for secure communication such as real-time voice telephone, text messaging, and file transmission with one-time pad encryption, which can support 11 pairs of users to make audio calls simultaneously. Combined with inter-city quantum backbone and ground-satellite links, our metropolitan implementation paves the way toward a global quantum network.
description: 14 pages, 5 figures
F2
Creators: Økonomi- og Indenrigsministeriet (I)
Social- og Indenrigsministeriet
Økonomi- og Indenrigsministeriet (II)
Økonomi- og Indenrigsministeriets Benchmarkingenhed
Publisher: name: Rigsarkivet
Year: 2022

description: Systemet anvendes til intern sagsadministration, varetagelse af ressortområde (ESDH)
Person-thing orientation within an interactional model of leader behavior
Creators: name: Mains, Gordon W.
Publisher: name: University of British Columbia
Year: 2010

description: A simplified interactional model of leader behavior was theoretically developed by reviewing the variety of approaches to the study of leadership and integrating some of the more recent major concerns. The model was conceptualized as including two original independent variable components - the person (leader) and the situation - with a continuous reciprocal influence between them so as to produce a theoretical hybrid interaction variable. The dependent variables consisted of the leader behavior dimensions of Initiating Structure and Consideration. The person component was operationalized by utilizing the construct of Person-Thing orientation from specialization theory and the situation component by creating and categorizing situations in terms of their people-thing nature. The dependent variables were measured by a self-rating behavior checklist. 244 subjects were administered a questionnaire which assessed their Person-Thing orientation, asked for their perceptions of three situations in terms of their nature, and solicited their responses in terms of how they would behave as a leader in each situation. Analysis of the data was carried out (1) to test for the existence of theoretical interaction between the person and situation variables, (2) to test for a significant relationship between Person orientation and Consideration behavior, and, between Thing orientation and Initiating Structure behavior, and (3) to test for differences in behavioral responses as influenced by both a person's specialist orientation and the nature of the situation. The results tended to support the existence of a theoretical interaction effect as conceptually defined between the person and the situation in that both variables had a significant influence on leader behavior. Person orientation and the nature of the situation predicted a Consideration behavior profile between specialties and situations but Thing orientation was not a predictor for Initiating Structure responses. Instead, Initiating Structure was partially predicted by Person orientation. In addition, the two behavior dimensions were found to be highly interdependent. Subsequent analysis discovered the existence of three behavior dimensions: Initiating Structure, Consideration (Being Friendly), and Consideration (Enhancing Participation). The data supported the hypothesized model but resulted in rejecting a connection between Thing orientation and Initiating Structure.
KMD EKJ 19.0.0
Creators: VASUafdeling Nord - Horsens
Horsens Kommune
Publisher: name: Rigsarkivet
Year: 2022

description: Formålet med it-systemet er at samle dokumentation vedr. sagsbehandling, ydelser, intern kommunikation m.v. i forhold til borgere, der modtager ydelser inden for serviceloven, sundhedsloven og dagtilbudsloven. Derudover kunne kommunikere elektronisk med sygehuse, læger, apoteker, andre kommuner i forhold til de gældende sundhedsaftaler. Kunne levere elektronisk data til Danmarks Statistik om borgernes ydelser m.m. samt danne grundlag for styring af økonomi og ressourcer
Public 360 4.1 SP9
Creators: Statens It
Publisher: name: Rigsarkivet
Year: 2022

description: Public 360 er et sags- og dokumenthåndteringssystem (ESDH-system), der har til formål at sikre efterlevelse af journaliseringspligten, identifikation af dokumenter, bevis og dokumentation, arkivering og videndeling.
The Newspaper Portrayal of Mothers Accessing Food Banks in the UK
Creators: name: Ommanney, Sarah
Publisher: name: UH Research Archive
Year: 2021
Subjects: mothers
food bank
identity
help
distress
clinical psychology

description: Aim: This study investigated the newspaper portrayal of mothers’ accessing food banks in the UK. Specifically, how their identities were portrayed, how their experiences were portrayed and how the impact of this was portrayed. Method: Forty-five national online newspaper articles, focusing on mothers’ who had accessed food banks, were analysed from the 1st of October 2019 to the 1st of November 2020. The articles were analysed using Thematic Analysis six-phase framework developed by Braun and Clarke (2006). Results: Three themes were identified following the analysis. The first theme identified was ‘lives stolen by poverty’, subthemes ‘pushed down the ladder by political choices’, ‘narrowing opportunities’, ‘the odds are stacked against them’ and ‘morality’. The second theme was ‘struggling to survive’, followed by subthemes ‘mothering under scarcity’, ‘not knowing where to turn’ and the ‘impact on self-hood’. The third and final theme was ‘struggling to provide’, which was followed by subthemes ‘cycles of love and protection’ and ‘spilling over.’ Considerations and implications: This study placed a psychological lens to the portrayal of mothers’ accessing food banks. Consideration was provided to the implications of newspaper portrayals for mothers’, the support available to them and how these portrayals impact their wellbeing.
KMD EKJ 19.0.0
Creators: Nordfyns Kommune
Publisher: name: Rigsarkivet
Year: 2022

description: Formålet med it-systemet er at samle dokumentation vedr. sagsbehandling, ydelser, intern kommunikation m.v. i forhold til borgere, der modtager ydelser inden for serviceloven, sundhedsloven og dagtilbudsloven. Derudover kunne kommunikere elektronisk med sygehuse, læger, apoteker, andre kommuner i forhold til de gældende sundhedsaftaler. Kunne levere elektronisk data til Danmarks Statistik om borgernes ydelser m.m. samt danne grundlag for styring af økonomi og ressourcer
In vitro kill-time test of disinfectants against Pseudomonas aeruginosa recovered  from water associated with hemodialysis applications
Creators: name: Patamaporn Sukplang And Acharawan Thongmee
Publisher: name: Rangsit University
Year: 2014
Subjects: Pseudomonas aeruginosa, hemodialysis, kill-time

description: 1, 4, Rangsit Journal of Arts and Sciences
Testing the Strong Equivalence Principle. II. Relating the External Field Effect in Galaxy Rotation Curves to the Large-Scale Structure of the Universe
Creators: name: Chae, Kyu-Hyun
name: Desmond, Harry
name: Lelli, Federico
name: McGaugh, Stacy S.
name: Schombert, James M.
Publisher: name: arXiv
Year: 2021
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: Theories of modified gravity generically violate the strong equivalence principle, so that the internal dynamics of a self-gravitating system in free fall depends on the strength of the external gravitational field (the external field effect). We fit rotation curves (RCs) from the SPARC database with a model inspired by Milgromian dynamics (MOND), which relates the outer shape of a RC to the external Newtonian field from the large-scale baryonic matter distribution through a dimensionless parameter $e_{\rm N}$. We obtain a $>4σ$ statistical detection of the external field effect (i.e. $e_{\rm N}>0$ on average), confirming previous results. We then locate the SPARC galaxies in the cosmic web of the nearby Universe and find a striking contrast in the fitted $e_{\rm N}$ {values} for galaxies in underdense versus overdense regions. Galaxies in an underdense region between 22 and 45 Mpc from the celestial axis in the northern sky have RC fits consistent with $e_{\rm N}\simeq0$, while those in overdense regions adjacent to the CfA2 great wall and the Perseus-Pisces supercluster return $e_{\rm N}$ that are a factor of two larger than the median for SPARC galaxies. We also calculate independent estimates of $e_{\rm N}$ from galaxy survey data and find that they agree with the $e_{\rm N}$ inferred from the RCs within the uncertainties, the chief uncertainty being the spatial distribution of baryons not contained in galaxies or clusters.
description: Astrophysical Journal, in press, 13 figures, 3 tables
Tyrsting Herreds tingbog, 1660-1683
Creators: Erik Brejl
Publisher: name: Rigsarkivet
Year: 2022

description: Tingbøger indeholder oplysninger om ejendomme. Hver ejendom har sin egen side, som indeholder oplysninger om ejendommen. Det er oplysninger om datoer for adkomster, servitutter og pantehæftelser. Efterhånden som dokumenterne er blevet tinglyst, er de løbende blevet skrevet ind i skøde- og panteprotokollen.
MPEC 2024-S179 : 2024 SB5
Creators: name: Minor Planet Center Staff
Publisher: name: The Minor Planet Center
Year: 2024
Subjects: subject: Small Solar System bodies
valueUri: http://astrothesaurus.org/uat/1469
subject: 2024 SB5

description: The Minor Planet Electronic Circulars contain information on unusual minor planets, routine data on comets and natural satellites, and occasional editorial announcements.  They are published on behalf of Division F of the International Astronomical Union by the Minor Planet Center, Smithsonian Astrophysical Observatory, Cambridge, MA 02138, U.S.A.
Neoseiulus tunus DeLeon
Creators: name: Lofego, A. C.
name: De Moraes, G. J.
name: Castro, L. A. S.
Publisher: name: Zenodo
Year: 2004
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Arachnida
Mesostigmata
Phytoseiidae
Neoseiulus
Neoseiulus tunus

description: Neoseiulus tunus (DeLeon)
 Typhlodromips tunus DeLeon, 1967: 29; Denmark & Muma, 1973: 253; Moraes et al., 1986: 151. Amblyseius tunus, Feres & Moraes, 1998: 126.
 Neoseiulus tunus, Ferla & Moraes, 2002: 872; Chant & McMurtry; 2003: 21; Moraes et al., 2004:148.
 Specimens examined: Pirassunuga: M. guianensis, I­2000 (2). Luiz Antônio: C. pubescens, V­2000 (3), I­2001 (1).
 Associated phytophagous mites: no phytophagous mites were found associated with this species.
 Previous records: Brazil — Mato Grosso (Ferla & Moraes, 2002), Rio Grande do Sul, São Paulo; Guadeloupe; Jamaica; Marie­Galante; Martinique and Peru.
 Remarks: The measurements of 6 adult females collected are similar to those given in the original description. The average measurements followed by the respective ranges (in parentheses) are: dorsal shield length 277 (258–290), width 176 (168–183), j1 23 (20–25), j3 27 (25–30), j4 13 (13–15), j5 13 (13–15), j6 19 (18–20), J2 20 (18–23), J5 8, z2 21 (20– 23), z4 28 (25–30), z5 15 (13–18), Z1 23 (23–25), Z4 42 (38–45), Z5 67 (63–73), s4 37 (35–40), S2 32 (28–33), S4 19 (15–23), S5 11 (10–13), r3 22 (20–23), R1 15 (13–18), Sge IV 20 (18–23), Sti IV 17 (15–18), St IV 33 (30–35), St1–St3 58 (55–60), St2–St2 63 (60– 68), St5–St5 60 (58–63), length of ventrianal shield 97 (85–103), width at ZV2 level 73 (65–75), width at anus level 58 (53–60), length of calyx of spermatheca 8.
description: Published as part of Lofego, A. C., De Moraes, G. J. & Castro, L. A. S., 2004, Phytoseiid mites (Acari: Phytoseiidae) on Myrtaceae in the State of São Paulo, Brazil, pp. 1-18 in Zootaxa 516 on page 8, DOI: 10.5281/zenodo.157769
Supplementary materials from Chiasmata and the kinetochore component Dam1 are crucial for elimination of erroneous chromosome attachments and centromere oscillation at meiosis I
Creators: name: Wakiya, Misuzu
name: Nishi, Eriko
name: Kawai, Shinnosuke
name: Yamada, Kohei
name: Katsumata, Kazuhiro
name: Hirayasu, Ami
name: Itabashi, Yuta
name: Yamamoto, Ayumu
Publisher: name: The Royal Society
Year: 2021
Subjects: Cell Biology
Molecular Biology

description: Supplementary figures, tables, and legends of the figures and the movies
ATOMIUM: Halide molecules around the S-type AGB star W Aquilae
Creators: name: Danilovich, T.
name: Van de Sande, M.
name: Plane, J. M. C.
name: Millar, T. J.
name: Royer, P.
name: Amor, M. A.
name: Hammami, K.
name: Decock, L.
name: Gottlieb, C. A.
name: Decin, L.
name: Richards, A. M. S.
name: De Beck, E.
name: Baudry, A.
name: Bolte, J.
name: Cannon, E.
name: De Ceuster, F.
name: de Koter, A.
name: Etoka, S.
name: Gobrecht, D.
name: Gray, M.
name: Herpin, F.
name: Homan, W.
name: Jeste, M.
name: Kervella, P.
name: Khouri, T.
name: Lagadec, E.
name: Maes, S.
name: Malfait, J.
name: McDonald, I.
name: Menten, K. M.
name: Montargès, M.
name: Müller, H. S. P.
name: Pimpanuwat, B.
name: Sahai, R.
name: Wallström, S. H. J.
name: Waters, L. B. F. M.
name: Wong, K. T.
name: Yates, J.
name: Zijlstra, A.
Publisher: name: arXiv
Year: 2021
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: S-type asymptotic giant branch (AGB) stars are thought to be intermediates in the evolution of oxygen- to carbon-rich AGB stars. The chemical compositions of their circumstellar envelopes are also intermediate, but have not been studied in as much detail as their carbon- and oxygen-rich counterparts. We aim to determine the abundances of AlCl and AlF from rotational lines, which have been observed for the first time towards an S-type AGB star, W Aql. In combination with models based on PACS observations, we aim to update our chemical kinetics network based on these results. We analyse ALMA observations towards W Aql of AlCl in the ground and first two vibrationally excited states and AlF in the ground vibrational state. Using radiative transfer models, we determine the abundances and spatial abundance distributions of Al$^{35}$Cl, Al$^{37}$Cl, and AlF. We also model HCl and HF emission and compare these models to PACS spectra to constrain the abundances of these species. AlCl is found in clumps very close to the star, with emission confined within 0.1$^{\prime\prime}$ of the star. AlF emission is more extended, with faint emission extending 0.2$^{\prime\prime}$ to 0.6$^{\prime\prime}$ from the continuum peak. We find peak abundances, relative to H$_2$, of $1.7\times 10^{-7}$ for Al$^{35}$Cl, $7\times 10^{-8}$ for Al$^{37}$Cl and $1\times 10^{-7}$ for AlF. From the PACS spectra, we find abundances of $9.7\times 10^{-8}$ and $\leq 10^{-8}$, relative to H$_2$, for HCl and HF, respectively. The AlF abundance exceeds the solar F abundance, indicating that fluorine synthesised in the AGB star has already been dredged up to the surface of the star and ejected into the circumstellar envelope. From our analysis of chemical reactions in the wind, we conclude that AlF may participate in the dust formation process, but we cannot fully explain the rapid depletion of AlCl seen in the wind.
description: Accepted for publication in Astronomy & Astrophysics
Multiphasic FEBio models of transmural transport in the mouse aorta
Creators: name: Wagenseil, Jessica
Publisher: name: figshare
Year: 2024
Subjects: classificationCode: 400399
subject: Biomedical engineering not elsewhere classified
classificationCode: 401799
subject: Mechanical engineering not elsewhere classified

description: This folder contains multiphasic FEBio models and associated outputs to simulate in vitro experiments measuring transmural fluid and solute flux in different cases of aneurysm severity in four different mouse models. Details for the mouse models, FEBio implementation, and limitations of the approach can be found in the associated publication. The README file has a basic description of the models and software version used.
An experimental study of the man-machine interface
Creators: name: Masulis, Paul Stanton
Publisher: name: University of British Columbia
Year: 2010

description: In this thesis, the author pursued two objectives. The first objective was to present a working example of a convenient, "idiot-proof", interactive computer program (designed with the user - not the programmer - in mind). The second objective was to investigate how various types of users interact with the computer, with the intention of reaching some conclusions about which program interfaces were most appropriate and convenient for various user types. In addition, some theories about the effects of various behavioural variables were investigated. The experimental tool used for this research was a simple interactive computer game in which the participants searched for the optimum profit in a three-dimensional space, given a fixed time limit. , Frequent periodic measurements were automatically collected on user performance, attitude, requests for reports, utilization of special features, and other variables; also, the solution protocol of each participant was recorded. The users were cateqorized by coqnitive style (heuristic/analytic), risk attitude, and previous computer experience as determined by a battery of pre-tests and questionnaires. In analyzinq the results, it was found that experience level was the dcminatinq factor on all dimensions: novices were slower, finished less frequently, and were siqnificantly less confident than experienced players. A hiqhly structured proqram interface was found to be more appropriate for these new users., Experience was also the dominating factor in the use of reports, although novices did show a marked learning effect over time - as did all users on most dimensions of performance and behaviour. As previously hypothesized, analytic-types and risk-takers played significantly faster and were more confident than heuristic-types and risk-averters, respectively. Concerning utilization of special program features, it was found that input response defaults influenced users in unfamiliar situations (ones which were new or did not have clear-cut responses), and didn't affect them at all in familiar circumstances. Analytic-types made least use of defaults. Bisk-averters were least likely to abbreviate commands. Also, the extent to which commands were abbreviated depended much upon their length, Finally, in the area of solution protocols, it was indeed found that heuristic-types were much less structured in their approach to solving the problem than analytic-types. .
Disk fragmentation in high-mass star formation. High-resolution observations towards AFGL 2591-VLA 3
Creators: name: Suri, S.
name: Beuther, H.
name: Gieser, C.
name: Ahmadi, A.
name: Sánchez-Monge, Á.
name: Winters, J. M.
name: Linz, H.
name: Henning, Th.
name: Beltrán, M. T.
name: Bosco, F.
name: Cesaroni, R.
name: Csengeri, T.
name: Feng, S.
name: Hoare, M. G.
name: Johnston, K. G.
name: Klaasen, P.
name: Kuiper, R.
name: Leurini, S.
name: Longmore, S.
name: Lumsden, S.
name: Maud, L.
name: Moscadelli, L.
name: Möller, T.
name: Palau, A.
name: Peters, T.
name: Pudritz, R. E.
name: Ragan, S. E.
name: Semenov, D.
name: Schilke, P.
name: Urquhart, J. S.
name: Wyrowski, F.
name: Zinnecker, H.
Publisher: name: arXiv
Year: 2021
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Increasing evidence suggests that, similar to their low-mass counterparts, high-mass stars form through a disk-mediated accretion process. At the same time, formation of high-mass stars still necessitates high accretion rates, and hence, high gas densities, which in turn can cause disks to become unstable against gravitational fragmentation. We study the kinematics and fragmentation of the disk around the high-mass star forming region AFGL 2591-VLA 3 which was hypothesized to be fragmenting based on the observations that show multiple outflow directions. We use a new set of high-resolution (0.19 arcsec) IRAM/NOEMA observations at 843 micron towards VLA 3 which allow us to resolve its disk, characterize the fragmentation, and study its kinematics. In addition to the 843 micron continuum emission, our spectral setup targets warm dense gas and outflow tracers such as HCN, HC$_3$N and SO$_2$, as well as vibrationally excited HCN lines. The high resolution continuum and line emission maps reveal multiple fragments with subsolar masses within the inner 1000 AU of VLA 3. Furthermore, the velocity field of the inner disk observed at 843 micron shows a similar behavior to that of the larger scale velocity field studied in the CORE project at 1.37 mm. We present the first observational evidence for disk fragmentation towards AFGL 2591-VLA 3, a source that was thought to be a single high-mass core. While the fragments themselves are low-mass, the rotation of the disk is dominated by the protostar with a mass of 10.3$\pm 1.8~M_{\odot}$. These data also show that NOEMA Band 4 can obtain the highest currently achievable spatial resolution at (sub-)mm wavelengths in observations of strong northern sources.
description: 16 pages, 11 figures, Accepted for publication in A&A
The solar carbon, nitrogen, and oxygen abundances from a 3D LTE analysis of molecular lines
Creators: name: Amarsi, A. M.
name: Grevesse, N.
name: Asplund, M.
name: Collet, R.
Publisher: name: arXiv
Year: 2021
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Carbon, nitrogen, and oxygen are the fourth, sixth, and third most abundant elements in the Sun. Their abundances remain hotly debated due to the so-called solar modelling problem that has persisted for almost $20$ years. We revisit this issue by presenting a homogeneous analysis of $408$ molecular lines across $12$ diagnostic groups, observed in the solar intensity spectrum. Using a realistic 3D radiative-hydrodynamic model solar photosphere and LTE (local thermodynamic equilibrium) line formation, we find $\logε_{C} = 8.47\pm0.02$, $\logε_{N} = 7.89\pm0.04$, and $\logε_{O} = 8.70\pm0.04$. The stipulated uncertainties mainly reflect the sensitivity of the results to the model atmosphere; this sensitivity is correlated between the different diagnostic groups, which all agree with the mean result to within $0.03$ dex. For carbon and oxygen, the molecular results are in excellent agreement with our 3D non-LTE analyses of atomic lines. For nitrogen, however, the molecular indicators give a $0.12$ dex larger abundance than the atomic indicators, and our best estimate of the solar nitrogen abundance is given by the mean: $7.83$ dex. The solar oxygen abundance advocated here is close to our earlier determination of $8.69$ dex, and so the present results do not significantly alleviate the solar modelling problem.
description: 12 pages, 6 figures, 3 tables; accepted for publication in Astronomy & Astrophysics
title: Global population growth, technology and Malthusian constraints: a quantitative growth theoretic perspective
Creators: name: Lanz, Bruno
name: Dietz, Simon
name: Swanson, Timothy M
Publisher: name: Graduate Institute of International and Development Studies
publisherIdentifier: https://ror.org/007ygn379
publisherIdentifierScheme: ROR
Year: 2016

description: Graduate Institute of International and Development Studies Working Paper ; no. 04/2016
Koldinghus Birks tingbøger, 1748-1761
Creators: Johannes Lind
Publisher: name: Rigsarkivet
Year: 2022

description: Formålet har været at gøre det nemt at følge de enkelte sager i Koldinghus Birketing fra deres start til deres afslutning og i forbindelse dermed at oprette registre over personer, steder og emner.
title: ÐÐ¾Ð´ÐµÐ»Ñ Ð¶Ð¸Ð·Ð½ÐµÐ½Ð½Ð¾Ð³Ð¾ ÑÐ¸ÐºÐ»Ð° Ð¸Ð½Ð½Ð¾Ð²Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð³Ð¾ Ð¿ÑÐ¾ÐµÐºÑÐ°
title: Life cycle model of an innovative project
Creators: name: ÐÐ°ÑÐºÐ¾Ð², ÐÐ²Ð³ÐµÐ½Ð¸Ð¹
name: Ð©ÐµÐ³Ð»Ð¾Ð², ÐÐ¼Ð¸ÑÑÐ¸Ð¹
name: "Ð¡Ð¾Ð²ÑÐµÐ¼ÐµÐ½Ð½Ð¾Ðµ Ð¼Ð°ÑÐ¸Ð½Ð¾ÑÑÑÐ¾ÐµÐ½Ð¸Ðµ: Ð½Ð°ÑÐºÐ° Ð¸ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ðµ", Ð¼ÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½Ð°Ñ Ð½Ð°ÑÑÐ½Ð°Ñ ÐºÐ¾Ð½ÑÐµÑÐµÐ½ÑÐ¸Ñ (13; 2024; Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³)
Publisher: name: ÐÐÐÐÐ¢ÐÐ¥-ÐÐ ÐÐ¡Ð¡
Year: 2024
Subjects: Ð¸Ð½Ð½Ð¾Ð²Ð°ÑÐ¸Ñ
Ð¿ÑÐ¾ÐµÐºÑ
ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ Ð¿ÑÐ¾ÐµÐºÑÐ¾Ð¼
Ð¿ÑÐµÐ´ÑÐ½Ð²ÐµÑÑÐ¸ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð·Ð°
Ð¸Ð½Ð²ÐµÑÑÐ¸ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð·Ð°
Ð¿Ð¾ÑÑÐ¸Ð½Ð²ÐµÑÑÐ¸ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð·Ð°
Ð´Ð¸ÑÑÑÐ·Ð¸Ñ
ÐºÐ¾Ð¼Ð¼ÐµÑÑÐ¸Ð°Ð»Ð¸Ð·Ð°ÑÐ¸Ñ
innovation
project
project management
pre-investment phase
investment phase
post-investment phase
diffusion
commercialization

description: Ð ÑÐ°Ð±Ð¾ÑÐµ Ð¾Ð±Ð¾ÑÐ½Ð¾Ð²ÑÐ²Ð°ÑÑÑÑ Ð³ÑÐ°Ð½Ð¸ÑÑ Ð¸ ÑÑÑÑÐºÑÑÑÐ° Ð¶Ð¸Ð·Ð½ÐµÐ½Ð½Ð¾Ð³Ð¾ ÑÐ¸ÐºÐ»Ð° Ð¸Ð½Ð½Ð¾Ð²Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð³Ð¾ Ð¿ÑÐ¾ÐµÐºÑÐ° Ñ ÑÑÐµÑÐ¾Ð¼ Ð¾ÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÐµÐ¹ Ð¸Ð½Ð½Ð¾Ð²Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð³Ð¾ ÑÐ¸ÐºÐ»Ð° Ð¸ ÑÑÐµÐ±Ð¾Ð²Ð°Ð½Ð¸Ð¹ Ð¿ÑÐ¾ÐµÐºÑÐ½Ð¾Ð³Ð¾ Ð¿Ð¾Ð´ÑÐ¾Ð´Ð°. ÐÑÐµÐ´Ð»Ð°Ð³Ð°ÐµÑÑÑ ÑÐ°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÑÑ Ð¸Ð½Ð½Ð¾Ð²Ð°ÑÐ¸Ð¾Ð½Ð½ÑÐ¹ ÑÐ¸ÐºÐ» Ð² ÑÐ°Ð¼ÐºÐ°Ñ ÑÑÐµÑ ÑÐ°Ð· ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ Ð¸Ð½Ð½Ð¾Ð²Ð°ÑÐ¸Ð¸: Ð¿ÑÐµÐ´ÑÐ½Ð²ÐµÑÑÐ¸ÑÐ¸Ð¾Ð½Ð½Ð°Ñ, Ð¸Ð½Ð²ÐµÑÑÐ¸ÑÐ¸Ð¾Ð½Ð½Ð°Ñ Ð¸ Ð¿Ð¾ÑÑÐ¸Ð½Ð²ÐµÑÑÐ¸ÑÐ¾Ð½Ð½Ð°Ñ. Ð ÑÐ°Ð¼ÐºÐ°Ñ Ð¸Ð½Ð²ÐµÑÑÐ¸ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÑÐ°Ð·Ñ Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ð° Ð¼Ð¾Ð´ÐµÐ»Ñ ÑÑÐµÑÑÐ°Ð·Ð½Ð¾Ð³Ð¾ Ð¶Ð¸Ð·Ð½ÐµÐ½Ð½Ð¾Ð³Ð¾ ÑÐ¸ÐºÐ»Ð° Ð¸Ð½Ð½Ð¾Ð²Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð³Ð¾ Ð¿ÑÐ¾ÐµÐºÑÐ°, Ð²ÐºÐ»ÑÑÐ°ÑÑÐ°Ñ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÑ, Ð²Ð½ÐµÐ´ÑÐµÐ½Ð¸Ðµ Ð¸ Ð´Ð¸ÑÑÑÐ·Ð¸Ñ.
description: The article is devoted the boundaries and structure of the life cycle of an innovative project, taking into account the peculiarities of the innovation cycle and the requirements of the project approach. The proposal is to consider the innovation cycle within the framework of three phases of innovation development: pre-investment, investment, and post-investment. Within the investment phase, a model of a three-phase life cycle of an innovative project including development, implementation, and diffusion is proposed.
Temperature dependence of the properties of open heavy-flavor mesons
Creators: name: Montana, Gloria
name: Ramos, Angels
name: Tolos, Laura
name: Torres-Rincon, Juan M.
Publisher: name: arXiv
Year: 2021
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: We address the modification of open heavy-flavor mesons in a hot medium of light mesons within an effective theory approach consistent with chiral and heavy-quark spin-flavor symmetries and the use of the imaginary time formalism to introduce the non-zero temperature effects to the theory. The unitarized scattering amplitudes, the ground-state self-energies and the corresponding spectral functions are calculated self-consistently. We use the thermal ground-state spectral functions obtained with this methodology to further calculate 1) open-charm meson Euclidean correlators, and 2) off-shell transport coefficients in the hadronic phase.
description: 4 pages, 4 figures, contribution to the proceedings for the 19th International Conference on Strangeness in Quark Matter (SQM 2021), online 17-22 May 2021 (Submission to EPJ)
Tuning the van Hove singularities in AV$_{3}$Sb$_{5}$ (A = K, Rb, Cs) via pressure and doping
Creators: name: LaBollita, Harrison
name: Botana, Antia S.
Publisher: name: arXiv
Year: 2021
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: We investigate the electronic structure of the new family of kagome metals AV$_{3}$Sb$_{5}$ (A = K, Rb, Cs) using first-principles calculations. We analyze systematically the evolution of the van Hove singularities (vHss) across the entire family upon applied pressure and hole doping, specifically focusing on the two vHss closer to the Fermi energy. With pressure, these two saddle points shift away from the Fermi level. At the same time, the Fermi surface undergoes a large reconstruction with respect to the Sb bands while the V bands remain largely unchanged, pointing to the relevant role of the Sb atoms in the electronic structure of these materials. Upon hole doping, we find the opposite trend, where the saddle points move closer to the Fermi level for increasing dopings. All in all, we show how pressure and doping are indeed two mechanisms that can be used to tune the location of the two vHss closer to the Fermi level and can be exploited to tune different Fermi surface instabilities and associated orders.
description: 12 pages, 11 figures, appendix
The importance of thermal torques on the migration of planets growing by pebble accretion
Creators: name: Guilera, O. M.
name: Bertolami, M. M. Miller
name: Masset, F.
name: Cuadra, J.
name: Venturini, J.
name: Ronco, M. P.
Publisher: name: arXiv
Year: 2021
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: A key process in planet formation is the exchange of angular momentum between a growing planet and the protoplanetary disc, which makes the planet migrate through the disc. Several works show that in general low-mass and intermediate-mass planets migrate towards the central star, unless corotation torques become dominant. Recently, a new kind of torque, called the thermal torque, was proposed as a new source that can generate outward migration of low-mass planets. While the Lindblad and corotation torques depend mostly on the properties of the protoplanetary disc and on the planet mass, the thermal torque depends also on the luminosity of the planet, arising mainly from the accretion of solids. Thus, the accretion of solids plays an important role not only in the formation of the planet but also in its migration process. In a previous work, we evaluated the thermal torque effects on planetary growth and migration mainly in the planetesimal accretion paradigm. In this new work, we study the role of the thermal torque within the pebble accretion paradigm. Computations are carried out consistently in the framework of a global model of planet formation that includes disc evolution, dust growth and evolution, and pebble formation. We also incorporate updated prescriptions of the thermal torque derived from high resolution hydrodynamical simulations. Our simulations show that the thermal torque generates extended regions of outward migration in low viscosity discs. This has a significant impact in the formation of the planets.
description: Accepted for publication in MNRAS
Phase gradient protection of stored spatially multimode perfect optical vortex beams in a diffused rubidium vapor
Creators: name: Chen, Yun
name: Wang, Jinwen
name: Wang, Chengyuan
name: Zhang, Shougang
name: Cao, Mingtao
name: Franke-Arnold, Sonja
name: Gao, Hong
name: Li, Fuli
Publisher: name: arXiv
Year: 2021
Subjects: subject: Quantum Physics (quant-ph)
subject: Atomic Physics (physics.atom-ph)
subject: Optics (physics.optics)
subject: FOS: Physical sciences

description: We experimentally investigate the optical storage of perfect optical vortex (POV) and spatially multimode perfect optical vortex (MPOV) beams via electromagnetically induced transparency (EIT) in a hot vapor cell. In particular, we study the role that phase gradients and phase singularities play in reducing the blurring of the retrieved images due to atomic diffusion. Three kinds of manifestations are enumerated to demonstrate such effect. Firstly, the suppression of the ring width broadening is more prominent for POVs with larger orbital angular momentum (OAM). Secondly, the retrieved double-ring MPOV beams' profiles present regular dark singularity distributions that are related to their vortex charge difference. Thirdly, the storage fidelities of the triple-ring MPOVs are substantially improved by designing line phase singularities between multi-ring MPOVs with the same OAM number but $π$ offset phases between adjacent rings. Our experimental demonstration of MPOV storage opens new opportunities for increasing data capacity in quantum memories by spatial multiplexing, as well as the generation and manipulation of complex optical vortex arrays.
Proprioseiopsis neotropicus Ehara
Creators: name: Lofego, A. C.
name: De Moraes, G. J.
name: Castro, L. A. S.
Publisher: name: Zenodo
Year: 2004
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Arachnida
Mesostigmata
Phytoseiidae
Proprioseiopsis
Proprioseiopsis neotropicus

description: Proprioseiopsis neotropicus (Ehara)
 Amblyseius neotropicus Ehara, 1966: 133; Moraes & Mesa, 1988: 79; Moraes et al., 1991: 127.
 Proprioseiopsis neotropicus, Moraes et al., 1986: 119; 2004: 183; Zacarias & Moraes, 2001: 582.
 Specimens examined: Pirassununga: M. venulosa, IV­2001 (1), X­2001 (1).
 Associated phytophagous mites: no phytophagous mites were found associated with this species.
 Previous records: Brazil — Pernambuco, Rio Grande do Sul, São Paulo; Colombia and Equador.
 Remarks: The measurements of 2 adult females collected are similar to those given in the original description, except for j3 and r3, which are ca. 35% longer. The measurements are: dorsal shield length 388–400, width 300–313, j 1 30–35, j3 45–48, j4 3, j5 3–4, j6 3–4, J5 4–5, z 2 23–25, z4 13, z5 3, Z1 5–6, Z4 113–120, Z5 105–110, s4 108–118, S2 8, S4 8, S5 8, r3 25, R1 13, Sge I 30–33, Sge II 33, Sge III 35 –40, Sti III 30, Sge IV 75, Sti IV 55 – 58, St IV 63 –68, St1–St3 63, St2–St2 88–93, St5–St5 110–118, length of ventrianal shield 113–115, width at ZV2 level 118–120, width at anus level 110–113, length of calyx of spermatheca 18–20.
description: Published as part of Lofego, A. C., De Moraes, G. J. & Castro, L. A. S., 2004, Phytoseiid mites (Acari: Phytoseiidae) on Myrtaceae in the State of São Paulo, Brazil, pp. 1-18 in Zootaxa 516 on page 9, DOI: 10.5281/zenodo.157769
Polarization in p-p elastic scattering
Creators: name: Keeler, Richard Kirk
Publisher: name: University of British Columbia
Year: 2010

description: The absolute normalization of the polarization in proton-proton elastic scattering at 24° lab has been determined by a double scattering experiment to an accuracy of ±2% over the energy range 250-520 MeV. The first energy dependant double scattering experiment has been performed at the Triumf variable energy cyclotron. Data were taken at five primary beam energies, 500, 467, 425, 367, and 307 MeV, and for the first time hydrogen was used both as polarizer and analyser.
interTwin D3.1 DTE blueprint architecture, functional specifications and requirements analysis first version
Creators: name: Raul Bardaji Benach
name: Andrea Manzi (EGI)
name: Ivan Rodero (EGI)
Publisher: name: Zenodo
Year: 2023
Subjects: subject: Architecture
subject: FOS: Civil engineering
subject: functional specifications
subject: requirements analysis
subject: Digital Twin Engine

description: This document provides an architectural blueprint for the interTwin Digital Twin Engine, outlining its functional specifications, requirements analysis, and fundamental building blocks.

The blueprint is designed to be utilised by the interTwin project's technical Work Packages (WPs) to align with the requirements of associated subsystems. Additionally, it considers other relevant initiatives and projects to identify potential architectural components that can be incorporated within the interTwin context. The blueprint will ultimately serve as a conceptual model of the Digital Twin Engine, following its planned evolution and iterations through collaborative co-creation during the project.
interTwin D3.1 DTE blueprint architecture, functional specifications and requirements analysis first version
Creators: name: Benach, Raul Bardaji
name: Andrea Manzi (EGI)
name: Ivan Rodero (EGI)
Publisher: name: Zenodo
Year: 2023
Subjects: subject: Architecture
subject: FOS: Civil engineering
subject: functional specifications
subject: requirements analysis
subject: Digital Twin Engine

description: This document provides an architectural blueprint for the interTwin Digital Twin Engine, outlining its functional specifications, requirements analysis, and fundamental building blocks. The blueprint is designed to be utilised by the interTwin project's technical Work Packages (WPs) to align with the requirements of associated subsystems. Additionally, it considers other relevant initiatives and projects to identify potential architectural components that can be incorporated within the interTwin context. The blueprint will ultimately serve as a conceptual model of the Digital Twin Engine, following its planned evolution and iterations through collaborative co-creation during the project.