cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Cataclysmic Variables: An Empirical Angular Momentum Loss Prescription From Open Cluster Data
Creators: name: Andronov, N.
name: Pinsonneault, M.
name: Sills, A.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We apply the angular momentum loss rates inferred from open cluster stars to the evolution of cataclysmic variables (CVs). We show that the angular momentum prescriptions used in earlier CV studies are inconsistent with the measured rotation data in open clusters. The timescale for angular momentum loss above the fully convective boundary is ~ 2 orders of magnitude longer than inferred from the older model, and the observed angular momentum loss properties show no evidence for a change in a behavior at the fully convective boundary. This provides evidence against the hypothesis that the period gap is caused by an abrupt change in the angular momentum loss law when the secondary becomes fully convective. It also implies that the timescale for CV evolution is much longer than it was than previously thought, comparable to a Hubble time. For the same reason, it will be more difficult to produce CVs from the products of common envelope evolution and implies a lower space density of CVs. The empirical loss law is consistent with the observed period minimum (1.3 hours) contrary to the minimum predicted by angular momentum loss due to gravitational radiation alone (1.1 hours). We introduce a method to infer the time-averaged mass accretion rate and derive mass-period relation for different evolutionary states of the secondary. The mass-period relationship is more consistent with evolved secondaries than with unevolved secondaries above the period gap. Implications for the CV period gap are discussed, including the possibility that two populations of secondaries could produce the gap.
description: 30 pages, 6 figures. Submitted ApJ
The Effects of Photoionization on Galaxy Formation - I: Model and Results at z=0
Creators: name: Benson, A. J.
name: Lacey, C. G.
name: Baugh, C. M.
name: Cole, S.
name: Frenk, C. S.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We develop a coupled model for the evolution of the global properties of the intergalactic medium (IGM) and the formation of galaxies, in the presence of a photoionizing background due to stars and quasars. We use this model to predict the thermodynamic history of the IGM when photoionized by galaxies forming in a cold dark matter (CDM) universe. The evolution of the galaxies is calculated using a semi-analytical model, including a detailed treatment of the effects of tidal stripping and dynamical friction on satellite galaxies orbiting inside larger dark matter halos. We include in the model the negative feedback on galaxy formation from the photoionizing background. Photoionization inhibits galaxy formation in low-mass dark matter halos in two ways: (i) heating of the IGM and inhibition of the collapse of gas into dark halos by the IGM pressure, and (ii) reduction in the radiative cooling of gas within halos. The result of our method is a self-consistent model of galaxy formation and the IGM. The IGM is reheated twice (during reionization of HI and HeII), and we find that the star formation rate per unit volume is slightly suppressed after each episode of reheating. We find that galaxies brighter than L_* are mostly unaffected by reionization, while the abundance of faint galaxies is significantly reduced, leading to present-day galaxy luminosity functions with shallow faint end slopes, in good agreement with recent observational data. Reionization also affects other properties of these faint galaxies, in a readily understandable way.
description: 22 pages, 11 figures, submitted to MNRAS
Quantum Instabilities of Solitons
Creators: name: Weigel, H.
Publisher: name: arXiv
Year: 2019
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We compute the vacuum polarization energies for a couple of soliton models in one space and one time dimensions. These solitons are mappings that connect different degenerate vacua. From the considered sample solitons we conjecture that the vacuum polarization contribution to the total energy leads to instabilities whenever degenerate vacua with different curvatures in field space are accessible to the soliton.
description: Contribution to the proceedings of ICNAAM
Mathematical analysis of the photoelectric effect
Creators: name: Bach, Volker
name: Klopp, Frederic
name: Zenk, Heribert
Publisher: name: arXiv
Year: 2002
Subjects: subject: Mathematical Physics (math-ph)
subject: FOS: Physical sciences

description: We study the photoelectric effect on the example of a simplified model of an atom with a single bound state, coupled to the quantized electromagnetic field. For this model, we show that Einstein's prediction for the photoelectric effect is qualitatively and quantitatively correct to leading order in the coupling parameter. More specifically, considering the ionization of the atom by an incident photon cloud consisting of $N$ photons, we prove that the total ionized charge is additive in the $N$ involved photons. Furthermore, if the photon cloud is approaching the atom from a large distance, the kinetic energy of the ejected electron is shown to be given by the difference of the photon energy of each single photon in the photon cloud and the ionization energy.
description: See also http://www.intlpress.com/ATMP
Additional file 1: of Towards a universal model of family centered care: a scoping review
Creators: name: Kokorelias, Kristina
name: Gignac, Monique
name: Naglie, Gary
name: Cameron, Jill
Publisher: name: figshare
Year: 2019
Subjects: subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences
subject: Developmental Biology
subject: Science Policy

description: Search Strategy Example (Medline). (DOCX 13 kb)
N=1 supersymmetric sigma model with boundaries, I
Creators: name: Albertsson, Cecilia
name: Lindstrom, Ulf
name: Zabzine, Maxim
Publisher: name: arXiv
Year: 2001
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: Mathematical Physics (math-ph)
subject: FOS: Physical sciences

description: We study an N=1 two-dimensional non-linear sigma model with boundaries representing, e.g., a gauge fixed open string. We describe the full set of boundary conditions compatible with N=1 superconformal symmetry. The problem is analyzed in two different ways: by studying requirements for invariance of the action, and by studying the conserved supercurrent. We present the target space interpretation of these results, and identify the appearance of partially integrable almost product structures.
description: 24 pages, LaTeX. v2: minor clarification in section 3.2, reference added. v3: section added on N=2 supersymmetry. v4: typos corrected, published version
Megastigmus bipunctatus
Creators: name: Stojanova, A.
name: Ghahari, H.
Publisher: name: Zenodo
Year: 2009
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Torymidae
Megastigmus
Megastigmus bipunctatus

description: Megastigmus bipunctatus (SWEDERUS 1795)
D i s t r i b u t i o n i n I r a n:Ghazvinprovince(ZARNEGAR et al. 2008).
G e n e r a l d i s t r i b u t i o n: Palaearctic (Austria, Bulgaria, Czech Republic, Denmark, Estonia, Finland, France, Germany, Hungary, Iran, Italy, Kazakhstan, Montenegro, Morocco, Netherlands, Poland, Romania, Russia, Serbia, Slovakia, Slovenia, Spain, Sweden, Switzerland, Ukraine, United Kingdom, Uzbekistan.
description: Published as part of Stojanova, A. & Ghahari, H., 2009, Checklists of Iranian Eurytomidae and Torymidae (Hymenoptera, Chalcidoidea), pp. 845-862 in Linzer biologische Beiträge 41 (1) on page 854, DOI: 10.5281/zenodo.5276308
Additional file 1: of Detailed observation on expression dynamics of Polycomb group genes during rice early endosperm development in subspecies hybridization reveals their characteristics of parent-of-origin genes
Creators: name: Kuang, Quan
name: Yinghua Wang
name: Shisheng Li
Publisher: name: figshare
Year: 2019
Subjects: subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: Ecology
subject: 69999 Biological Sciences not elsewhere classified
subject: Developmental Biology

description: Table S1. Primers of Distinction betweenÂ OsEMF2a(l) and OsEMF2a(s). (DOC 27 kb)
Reachability analysis in stochastic directed graphs by reinforcement learning
Creators: name: Possieri, Corrado
name: Frasca, Mattia
name: Rizzo, Alessandro
Publisher: name: arXiv
Year: 2022
Subjects: subject: Artificial Intelligence (cs.AI)
subject: Machine Learning (cs.LG)
subject: FOS: Computer and information sciences

description: We characterize the reachability probabilities in stochastic directed graphs by means of reinforcement learning methods. In particular, we show that the dynamics of the transition probabilities in a stochastic digraph can be modeled via a difference inclusion, which, in turn, can be interpreted as a Markov decision process. Using the latter framework, we offer a methodology to design reward functions to provide upper and lower bounds on the reachability probabilities of a set of nodes for stochastic digraphs. The effectiveness of the proposed technique is demonstrated by application to the diffusion of epidemic diseases over time-varying contact networks generated by the proximity patterns of mobile agents.
description: in IEEE Transactions on Automatic Control, 2023
Bifurcation-Based Learning Algorithm (BBLA): A Novel Approach to Model Optimization via Iterative Divergence
Creators: name: Kodsi, Adil
Publisher: name: Zenodo
Year: 2025
Subjects: Machine Learning, Optimization, Hyperparameter Tuning, AI, BBLA, Ensemble Learning

description: This paper introduces the Bifurcation-Based Learning Algorithm (BBLA), a novel approach to model optimization that simulates iterative learning divergence through structured bifurcation. Inspired by decision theory and complex systems, BBLA incrementally branches a base model into sub-models by applying assumption-driven hyperparameter variations. Each iteration evaluates accuracy, performance, and drift through a composite reward function. The algorithm is validated on benchmark datasets and compared against supervised and unsupervised methods, showcasing competitive accuracy and enhanced robustness. BBLA offers a unique method for structured model discovery, adaptable to dynamic learning environments and applicable to both conventional ML workflows and emerging AI orchestration challenges.
Estimating Stochastic Gravitational Wave Backgrounds with Sagnac Calibration
Creators: name: Hogan, Craig J.
name: Bender, Peter L.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Armstrong et al. have recently presented new ways of combining signals to precisely cancel laser frequency noise in spaceborne interferometric gravitational wave detectors such as LISA. One of these combinations, the symmetrized Sagnac observable, is much less sensitive to external signals at low frequencies than other combinations, and thus can be used to determine the instrumental noise level. We note here that this calibration of the instrumental noise permits smoothed versions of the power spectral density of stochastic gravitational wave backgrounds to be determined with considerably higher accuracy than earlier estimates, at frequencies where one type of noise strongly dominates and is not substantially correlated between the six main signals generated by the antenna. We illustrate this technique by analyzing simple estimators of gravitational wave background power, and show that the instrumental sensitivity to broad-band backgrounds at some frequencies can be improved by more than an order of magnitude over the standard method, comparable to that which would be achieved by cross-correlating two separate antennas. The applications of this approach to studies of astrophysical gravitational wave backgrounds generated after recombination and to searches for a possible primordial background are discussed.
description: 14 pages, 4 figures, Latex, to appear in Phys. Rev. D; minor corrections and references added
Additional file 1: of Health-resource use and quality of life in children with bronchiectasis: a multi-center pilot cohort study
Creators: name: Lovie-Toon, Yolanda
name: Grimwood, Keith
name: Byrnes, Catherine
name: Goyal, Vikas
name: Busch, Greta
name: I. Masters
name: Marchant, Julie
name: Buntain, Helen
name: Kerry-Ann OâGrady
name: Chang, Anne
Publisher: name: figshare
Year: 2019
Subjects: subject: Medicine
subject: Pharmacology
subject: Biotechnology
subject: Sociology
subject: FOS: Sociology
subject: Developmental Biology
subject: Science Policy
subject: 111714 Mental Health
subject: FOS: Health sciences
subject: 110309 Infectious Diseases

description: Table S1. Parent and child-reported cough severity scores at time of clinic visits. Table S2. Correlations between parent and child-reported quality-of-life (QoL) and parent and child-reported cough severity at baseline and months 3, 6, 9 and 12. Table S3. Comparison of baseline characteristics between those participants who completed all 12-monthly follow-up tasks and those participants who did not. (DOCX 21 kb)
Prasadiseius incanus Prasad and Guanilo 2011, n. sp.
Creators: name: Prasad, V.
name: Guanilo, A. D.
name: Grados, J.
name: Prassad, I.
Publisher: name: Zenodo
Year: 2011
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Arachnida
Mesostigmata
Otopheidomenidae
Prasadiseius
Prasadiseius incanus

description: Prasadiseius incanus Prasad and Guanilo, n. sp.
 (Figs. 1 – 26)
description: Published as part of Prasad, V., Guanilo, A. D., Grados, J. & Prassad, I., 2011, A New Species Of Prasadiseius Wainstein, 1970 (Acari: Otopheidomenidae) From Hawk Moths (Lepidoptera: Sphingidae) In Peru, pp. 99-125 in Acarologia 51 (1) on page 109, DOI: 10.1051/acarologia/20111999, http://zenodo.org/record/5392781
Hubble Space Telescope analysis of stellar populations within the globular cluster G1 (Mayall II) in M31
Creators: name: Nardiello, D.
name: Piotto, G.
name: Milone, A. P.
name: Rich, R. M.
name: Cassisi, S.
name: Bedin, L. R.
name: Bellini, A.
name: Renzini, A.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: In this paper we present a multi-wavelength analysis of the complex stellar populations within the massive globular cluster Mayall II (G1), a satellite of the nearby Andromeda galaxy projected at a distance of 40 kpc. We used images collected with the Hubble Space Telescope in UV, blue and optical filters to explore the multiple stellar populations hosted by G1. The $m_{\rm F438W}$ versus $m_{\rm F438W}- m_{\rm F606W}$ colour-magnitude diagram shows a significant spread of the red giant branch, that divides $\sim 1$ mag brighter than the red clump. A possible explanation is the presence of two populations with different iron abundance or different C+N+O content, or different helium content, or a combination of the three causes. A similar red giant branch split is observed also for the Galactic globular cluster NGC6388. Our multi-wavelength analysis gives also the definitive proof that G1 hosts stars located on an extended blue horizontal branch. The horizontal branch of G1 exhibits similar morphology as those of NGC6388 and NGC6441, which host stellar populations with extreme helium abundance (Y>0.33). As a consequence, we suggest that G1 may also exhibit large star-to-star helium variations.
description: 13 pages, 9 figures (2 at low resolution), 2 tables. Accepted for publication in MNRAS on March 1, 2019
Additional file 5: of Guide for library design and bias correction for large-scale transcriptome studies using highly multiplexed RNAseq methods
Creators: name: Katayama, Shintaro
name: Skoog, Tiina
name: Söderhäll, Cilla
name: Einarsdottir, Elisabet
name: Krjutškov, Kaarel
name: Kere, Juha
Publisher: name: figshare
Year: 2019
Subjects: subject: Biochemistry
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: 69999 Biological Sciences not elsewhere classified
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: Cancer

description: Figure S1. Spearman correlation coefficients between the technical replicates of normalized expression levels by four different normalization methods and the libraries. Figure S2. PCA of the BEAS-2B technical replicates of normalized expression levels by four different normalization methods. Figure S3. Normalized expression levels by the four different normalization methods, and the ranks, of three library-biased genes. Figure S4. Pairwise comparison of raw read counts and the Spearman correlation coefficients before and after the library bias correction. Figure S5. Spearman correlation coefficients between the technical replicates of the normalized expression levels before and after the library bias correction. Figure S6. PCA of the technical replicates of the spike-in normalized expression levels before and after the library bias correction. Figure S7. PCA of normalized expression levels of the BEAS-2B technical replicates by four different normalization methods, before and after the library bias correction. Figure S8. Quantity of the library before sequencing, and REDUNDANCY and CODING_RATE after the sequencing. (PDF 2469 kb)
The Effects of Photoionization on Galaxy Formation - II: Satellites in the Local Group
Creators: name: Benson, A. J.
name: Frenk, C. S.
name: Lacey, C. G.
name: Baugh, C. M.
name: Cole, S.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We use a self-consistent model of galaxy formation and the evolution of the intergalactic medium to study the effects of the reionization of the universe at high redshift on the properties of satellite galaxies like those seen around the Milky Way. Photoionization suppresses the formation of small galaxies, so that surviving satellites are preferentially those that formed before the universe reionized. As a result, the number of satellites expected today is about an order of magnitude smaller than the number inferred by identifying satellites with subhalos in high-resolution simulations of the dark matter. The resulting satellite population has an abundance and a distribution of circular velocities similar to those observed in the Local Group. We explore many other properties of satellite galaxies, including their gas content, metallicity and star formation rate, and find generally good agreement with available data. Our model predicts the existence of many as yet undetected satellites in the Local Group. We quantify their observability in terms of their apparent magnitude and surface brightness and also in terms of their constituent stars. A near-complete census of the Milky Way's satellites would require imaging to V~20 and to a surface brightness fainter than 26 V-band magnitudes per square arcsecond. Satellites with integrated luminosity V=15 should contain of order 100 stars brighter than B=26, with central stellar densities of a few tens per square arcminute. Discovery of a large population of faint satellites would provide a strong test of current models of galaxy formation.
description: 14 pages, 11 figures, submitted to MNRAS
Additional file 1 of Restoration of dysregulated intestinal barrier and inflammatory regulation through synergistically ameliorating hypoxia and scavenging reactive oxygen species using ceria nanozymes in ulcerative colitis
Creators: name: Zhang, Ying
name: Lei, Hengyu
name: Wang, Pengchong
name: Zhou, Qinyuan
name: Yu, Jie
name: Leng, Xue
name: Ma, Ruirui
name: Wang, Danyang
name: Dong, Kai
name: Xing, Jianfeng
name: Dong, Yalin
Publisher: name: figshare
Year: 2023
Subjects: subject: Biophysics
subject: Biochemistry
subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Cell Biology
subject: Molecular Biology
subject: Physiology
subject: Chemical Sciences not elsewhere classified
subject: Science Policy
subject: Immunology
subject: FOS: Clinical medicine
subject: Cancer

description: Additional file1: Fig. S1 Scheme of PEG-CNPs preparation via a modified reverse micelle method. (a) Synthetic schematic for PEG-CNPs preparation. (b) Detailed process for PEG-CNPs preparation. Fig. S2 The XRD pattern shows the structure of OA-CNPs (a) and PEG-CNPs (b). Fig. S3 The colloidal stability of PEG-CNPs in PBS or DMEM containing 10% fetal bovine serum (FBS) within 7 days. Data represent means ± s.d. n = 3. Fig. S4 Cytotoxicity of PEG-CNPs in (a) RAW 264.7 cells and (b) HT-29 cells. Cell viability was evaluated at 24 h of exposure to PEG-CNPs. Data represent means ± s.d. n = 6. Fig. S5 Photographs of red blood cells and the hemolytic activity of PEG-CNPs. Data represent means ± s.d. n = 3. Fig. S6 Representative H&E staining of major organs from colitis mice at day 5 after 1.5 mg/kg PEG-CNPs treatment. Fig. S7 Long-term toxicity of PEG-CNPs in healthy mice. Blood biochemistry analyses of ALT (a), AST (b), BUN (c) and creatinine (d) of mice at day 21 after 1.5 mg/kg PEG-CNPs treatment. (e) Representative H&E staining of major organs from mice. Data represent means ± s.d. n = 6. Fig. S8 In vivo pharmacokinetic curves of PEG-CNPs (1.5 mg/kg). Data represent means ± s.d. n = 3. Fig. S9 Biodistribution of Ce element at different time points after intravenous injection of PEG-CNPs (1.5 mg/kg) in healthy mice (a) and colitis mice (b). Data represent means ± s.d. n = 3. Fig. S10 Colon targeting of PEG-CNPs (1.5 mg/kg) in colon tissues. Data represent means ± s.d. n = 3. ***P < 0.001 vs. control group. Fig. S11 Representative fluorescence images of HT-29 cells (a) and RAW 264.7 cells (b) after incubation with FITC-PEG-CNPs for 24 h. Scale bars: 50 μm. Fig. S12 Morphology of RAW 264.7 cells after treated with LPS (-/+) (100 ng/ml) and PEG-CNPs. Table S1 Sequences of the primers used for qRT-PCR. Table S2 The evaluation criteria of disease activity index (DAI) of mice. Table S3 Pharmacokinetic parameters of PEG-CNPs. Data represent means ± s.d. n = 3.
MOESM1 of Conserved gene signalling and a derived patterning mechanism underlie the development of avian footpad scales
Creators: name: Cooper, Rory
name: Lloyd, Victoria
name: Di-PoĂŻ, Nicolas
name: Fletcher, Alexander
name: Barrett, Paul
name: Fraser, Gareth
Publisher: name: figshare
Year: 2019
Subjects: subject: Medicine
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Evolutionary Biology
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences
subject: Developmental Biology
subject: Computational Biology

description: Additional file 1. Additional figures.
Variability in the Thermal Emission from Accreting Neutron Star Transients
Creators: name: Brown, Edward F.
name: Bildsten, Lars
name: Chang, Philip
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The composition of the outer 100 m of a neutron star sets the heat flux that flows outwards from the core. For an accreting neutron star in an X-ray transient, the thermal quiescent flux depends sensitively on the amount of hydrogen and helium remaining on the surface after an accretion outburst and on the composition of the underlying ashes of previous H/He burning. Because H/He has a higher thermal conductivity, a larger mass of H/He implies a shallower thermal gradient through the low density envelope and hence a higher effective temperature for a given core temperature. The mass of residual H and He varies from outburst to outburst, so the thermal quiescent flux is variable even though the core temperature is constant for timescales < 10 000 yr. Heavy elements settle from a H/He envelope in a few hours; we therefore model the quiescent envelope as two distinct layers, H/He over heavier elements, and treat the mass of H/He as a free parameter. We find that the emergent thermal quiescent flux can vary by a factor of 2 to 3 between different quiescent epochs. The variation is more pronounced at lower interior temperatures, making systems with low quiescent luminosities and frequent outbursts, such as SAX J1808.4-3658, ideal candidates from which to observe this effect. We compute, for different ash compositions, the interior temperatures of Cen X-4, Aql X-1, and SAX J1808.4-3658. In the case of Aql X-1, the inferred high interior temperature suggests that neutrino cooling contributes to the neutron star's thermal balance.
description: 14 pages, 5 figures, uses emulateapj5 and psnfss fonts. To be published in The Astrophysical Journal
From Gold to Coherence_ The 53-Year Drift and the Return to Structured Resonance
Creators: name: Bostick, Devin
Publisher: name: Zenodo
Year: 2025
Subjects: CODES Framework
Structured Resonance
Phase Coherence
Post-Probabilistic Systems
Financial Phase Drift
Petro-Dollar Collapse
Gold Standard
AI Decoherence
Prime Frequency Intelligence
Spectral Money
Deterministic Cognition
Post-1971 Monetary Systems
Phase-Locked AI
Resonance-Based Modeling
Cognitive Realignment

description: Main CODES Framework

Abstract

For over five decades, the global economic and cognitive architecture has operated under the illusion of probabilistic stability. This paper traces the origin and trajectory of that illusion, beginning with the 1971 Nixon Shock that severed the U.S. dollar from its gold standard — an act that removed not just a monetary backing, but a coherence anchor. In the absence of structured resonance, global systems—financial, technological, political, and epistemological—have defaulted to stochastic scaffolding: increasingly complex, increasingly fragile.

The 1971–2025 period marks a historical waveform of systemic decoherence, patched repeatedly with synthetic anchors like the petro-dollar, algorithmic finance, and stochastic AI. These were not true solutions; they were spectral compensations. The result has been a drift from lawful phase alignment to speculative entropy.

This paper introduces the CODES framework as the inevitable resolution: a mathematically grounded, prime-structured model for coherence restoration across all levels of system design. CODES does not oppose probability—it renders it obsolete by reintroducing lawful resonance as the substrate of structure, intelligence, and value. The Resonance Intelligence Core (RIC), built atop these principles, is the first system to operationalize this transition in real-time inference and systemic governance.

Structured resonance is not a concept. It is the missing infrastructure of post-1971 civilization. And its return, via CODES, signals not a shift, but a restoration of lawful coherence across domains once thought disconnected.
Megastigmus dorsalis
Creators: name: Stojanova, A.
name: Ghahari, H.
Publisher: name: Zenodo
Year: 2009
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Torymidae
Megastigmus
Megastigmus dorsalis

description: Megastigmus dorsalis (FABRICIUS 1798)
D i s t r i b u t i o n i n I r a n: Lurestanprovince(AZIZKHANI et al. 2005, LOTFALIZADEH & GHARALI 2005); West Azerbaijan province (ZARGARAN et al. 2008); Iran (NOYES 2003).
G e n e r a l d i s t r i b u t i o n: Palaearctic (Bulgaria, Bosnia and Herzegovina, Croatia, Czech Republic, Denmark, France, Germany, Hungary, Iran, Italy, Moldova, Netherlands, Peoples' Republic of China, Republic of Macedonia, Romania, Russia, Serbia, Slovakia, Sweden, Turkey, Ukraine, United Kingdom); Oriental (India).
description: Published as part of Stojanova, A. & Ghahari, H., 2009, Checklists of Iranian Eurytomidae and Torymidae (Hymenoptera, Chalcidoidea), pp. 845-862 in Linzer biologische Beiträge 41 (1) on page 854, DOI: 10.5281/zenodo.5276308
Thermal torque effects on the migration of growing low-mass planets
Creators: name: Guilera, O. M.
name: Cuello, N.
name: Montesinos, M.
name: Bertolami, M. M. Miller
name: Ronco, M. P.
name: Cuadra, J.
name: Masset, F. S.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: As planets grow the exchange of angular momentum with the gaseous component of the protoplanetary disc produces a net torque resulting in a variation of the semi-major axis of the planet. For low-mass planets not able to open a gap in the gaseous disc this regime is known as type I migration. Pioneer works studied this mechanism in isothermal discs finding fast inward type I migration rates that were unable to reproduce the observed properties of extrasolar planets. In the last years, several improvements have been made in order to extend the study of type I migration rates to non-isothermal discs. Moreover, it was recently shown that if the planet's luminosity due to solid accretion is taken into account, inward migration could be slowed down and even reversed. In this work, we study the planet formation process incorporating, and comparing, updated type I migration rates for non-isothermal discs and the role of planet's luminosity over such rates. We find that the latter can have important effects on planetary evolution, producing a significant outward migration for the growing planets.
description: Accepted for publication in Monthly Notices of the Royal Astronomical Society
Squilloides leptosquilla
Creators: name: Ahyong, Shane T.
Publisher: name: Zenodo
Year: 2002
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Malacostraca
Stomatopoda
Squillidea
Squilloides
Squilloides leptosquilla

description: Squilloides leptosquilla (Brooks, 1886)
 Squilla leptosquilla Brooks, 1886: 30-34, pl. 1, figs 1, 2. Type locality: Celebes Sea, Philippines, 12°46’N, 122°10’E. — Jurich 1904: 370-372, pl. 25 (I), fig. 1- 1b. — Kemp 1913: 46-48. — Hansen 1926: 10.
 Squilloides leptosquilla – Moosa 1986: 410, 411, pl. I, figs D, E. — Ahyong 2001: 310-312, fig. 150.
MATERIAL EXAMINED. — Tanimbar Islands, stn CP84, 09°23’S, 131°09’E, 275- 246 m, 4.XI.1991, 1 tl 58 (MNHN). — Stn DW44, 07°52’S, 132°48’E, 291- 295 m, 29.X.1991, 1 broken cl 7.5 (MNHN). — Kai Islands, stn DW24, 05°32’S, 132°51’E, 230-243 m, 26.X.1991, 1 tl 33 (MNHN). — Stn 10/81, 10.X.1991, 1 tl 87 (MNHN). — Stn CP16, 05°17’S, 132°50’E, 315-349 m, 24.X.1991, 1 tl 62 (MNHN).
DISTRIBUTION. — The Philippines, the Andaman Islands, Australia, the Banda Sea, and now from Kai and Tanimbar, Indonesia at depths between 170 and 754 m (Ahyong 2001).
REMARKS
The specimens in the present series generally agree well with the holotype and published accounts (Brooks 1886; Kemp 1913; Moosa 1986; Ahyong 2001). Variation in the Indonesian specimens resembles that reported by Ahyong (2001) for Australian material. In the smaller specimens, the eye is more triangular, and the median carina on the carapace and rostral plate is less distinct than in the largest specimen. The lateral process of TS5 is directed laterally in the smallest specimen, and anterolaterally in the largest specimen.
description: Published as part of Ahyong, Shane T., 2002, Stomatopoda (Crustacea) of the KARUBAR Expedition in Indonesia, pp. 373-383 in Zoosystema 24 (2) on page 382, DOI: 10.5281/zenodo.5392839
Fermi Level Dependent Spin Pumping from a Magnetic Insulator into a Topological Insulator
Creators: name: Wang, Hailong
name: Kally, James
name: Sahin, Cuneyt
name: Liu, Tao
name: Yanez, Wilson
name: Kamp, Eric J.
name: Richardella, Anthony
name: Wu, Mingzhong
name: Flatte, Michael E.
name: Samarth, Nitin
Publisher: name: arXiv
Year: 2019
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: Topological spintronics aims to exploit the spin-momentum locking in the helical surface states of topological insulators for spin-orbit torque devices. We address a fundamental question that still remains unresolved in this context: does the topological surface state alone produce the largest values of spin-charge conversion efficiency or can the strongly spin-orbit coupled bulk states also contribute significantly? By studying the Fermi level dependence of spin pumping in topological insulator/ferrimagnetic insulator bilayers, we show that the spin Hall conductivity is constant when the Fermi level is tuned across the bulk band gap, consistent with a full bulk band calculation. The results suggest a new perspective, wherein "bulk-surface correspondence" allows spin-charge conversion to be simultaneously viewed either as coming from the full bulk band, or from spin-momentum locking of the surface state.
САЙЛОВ ТИЗИМИ
Creators: name: Рахмонова Рухшона Нурбек қизи Шароф Рашидов номидаги Самарқанд Давлат Университети юридик факультети 1-босқич талаба
Publisher: name: Zenodo
Year: 2025

description: Ушбу мақолада бугунги кунда сайлов тизимининг долзарблиги, унинг демократик жамиятдаги ўрни ва ривожланиш йўналишлари таҳлил қилинади. Сайлов тизими фуқароларнинг сиёсий жараёндаги иштироқини таъминловчи асосий институтлардан бири бўлиб, унинг шаффофлиги ва адолатли жамият барқарорлигига бевосита таъсир кўрсатади. Мақолада сайлов тизимининг турлари, уларнинг афзалликлари ва камчиликлари, шунингдек, замонавий технологиялар ва халқаро тажриба асосида уни такомиллаштириш имкониятлари ёритилган. Сайлов жараёнининг ошкоралиги ва фуқароларнинг фаоллиги демократик бошқарувнинг муҳим шарти эканлиги асосланади. Шунингдек, соҳада олиб борилаётган туб ислоҳотлар ҳамда сайлов тизими турлари: мажоритар ва пропорционал сайлов турлари, уларнинг моҳияти ва мазмуни ёритиб борилади.
Megastigmus pistaciae WALKER 1871
Creators: name: Stojanova, A.
name: Ghahari, H.
Publisher: name: Zenodo
Year: 2009
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Torymidae
Megastigmus
Megastigmus pistaciae

description: Megastigmus pistaciae WALKER 1871
D i s t r i b u t i o n i n I r a n: East Azerbaijan, Fars, Hamadan, Isfahan, Khorasan, Markazi, Simnan, Tehran and Zanjan provinces (ABAI & ADELI 1984; MODARES AWAL 1997; MEHRNEJAD 2001; JALILVAND & GHOLIPOUR 2002); Isfahan province (BASIRAT & SEYEDOLESLAMI 2000); Qazvin province (LOTFALIZADEH & GHARALI 2005); Iran (ZOEBELEIN 1966; NIKOLSKAYA & ZEROVA 1978; RICE & MICHAILIDES 1988; GRISSELL & PRINSLOO 2001; NOYES 2003; ROQUES & SKRZYPCZYNSKA 2003).
G e n e r a l d i s t r i b u t i o n: Palaearctic (Afganistan, Algeria, Bulgaria, Croatia, Cyprus, France, Greece, Iran, Israel, Italy, Montenegro, Morocco, Peoples' Republic of China, Portugal, Tunisia, Turkey, Turkmenistan, Ukraine, Uzbekistan); Nearctic (United States of America); Neotropical (Mexico); Australian (Australia).
description: Published as part of Stojanova, A. & Ghahari, H., 2009, Checklists of Iranian Eurytomidae and Torymidae (Hymenoptera, Chalcidoidea), pp. 845-862 in Linzer biologische Beiträge 41 (1) on page 854, DOI: 10.5281/zenodo.5276308
Ground state degeneracy of the Pauli-Fierz Hamiltonian inlcuding spin
Creators: name: Hiroshima, F.
name: Spohn, H.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Mathematical Physics (math-ph)
subject: FOS: Physical sciences

description: We consider an electron, spin 1/2, minimally coupled to the quantized radiation field in the nonrelativistic approximation, a situation defined by the Pauli-Fierz Hamiltonian $H$. There is no external potential and $H$ fibers as $\int^\oplus H_p dp$ according to the total momentum $p$. We prove that the ground state subspace of $H_p$ is two-fold degenerate provided the charge $e$ and the total momentum $p$ are sufficiently small. We also establish that the total angular momentum of the ground state subspace is $\pm1/2$ and study the case of a confining external potential.
description: See also http://www.intlpress.com/ATMP
Orbital angular momentum of the proton and intrinsic five-quark Fock states
Creators: name: An, C. S.
name: Saghai, B.
Publisher: name: arXiv
Year: 2019
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The orbital angular momentum ($L_q$) of the proton is studied by employing the extended constituent quark model. Contributions from different flavors, namely, up, down, strange, and charm quarks in the proton are investigated. Probabilities of the intrinsic $q\bar{q}$ pairs are calculated using a $^{3}P_{0}$ transition operator to fit the sea flavor asymmetry $I_a=\bar{d}-\bar{u}=0.118\pm0.012$ of the proton. Our numerical results lead to $L_q=0.158 \pm 0.014$, in agreement with $4/3I_a=0.157 \pm 0.016$, and consistent with findings based on various other approaches.
description: typos corrected
The biodiverse rotifers (Rotifera: Eurotatoria) of Northeast India: faunal heterogeneity, biogeography, richness in diverse ecosystems and interesting species assemblages
Creators: name: Sharma, Bhushan Kumar
name: Sharma, Sumita
Publisher: name: Zoological Research Museum Alexander Koenig
Year: 2019
Subjects: Biodiversity
distribution
important taxa
species assemblages
Rotifera paradox

description: The biodiverse Rotifera of northeast India (NEI) revealed 303 species belonging to 53 genera and 24 families; ~96% of these species examined from seven states of NEI affirm the rotifer heterogeneity of our plankton and semi-plank-ton collections. This study documents the record number of species of global and regional biogeographic interest, high-lights affinity with Southeast Asian and Australian faunas, and indicates notable heterogeneity in richness and composition amongst the seven northeastern states. The speciose rotifers of small lentic biotopes of Arunachal Pradesh, Mizoram, Nagaland, Meghalaya, Manipur and Tripura, the floodplain lakes (beels) and small wetlands (dobas and dubies) of the Brahmaputra and the Barak floodplains of Assam, and the floodplain lakes (pats) of Manipur are noteworthy. Deepor Beel and Loktak Lake (two Ramsar sites) are the globally rich rotifer `hotspots’. Interesting assemblages per sample of 80+ species in certain beels and pats, and up to 50 species in dobas and dubies depict the `Rotifera paradox’. The most diverse and interesting Rotifera of NEI, than any other region of India, is attributed to habitat and ecosystem heterogeneity of wa-ter bodies spread over varied ecological regimes, the location of the region in the Himalayan and Indo-Burma Biodiversity hotspots, vital biogeographic corridor of 'the Assam gateway', 'the rotiferologist effect and the sampling intensity. Our study marks a valuable contribution to biodiversity and biogeography of the Indian, Asian and Oriental Rotifera.
Megastigmus rosae BOUCEK 1971
Creators: name: Stojanova, A.
name: Ghahari, H.
Publisher: name: Zenodo
Year: 2009
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Torymidae
Megastigmus
Megastigmus rosae

description: Megastigmus rosae BOUČEK 1971
D i s t r i b u t i o n i n I r a n: East Azerbaijan province (LOTFALIZADEH & GHARALI 2005).
G e n e r a l d i s t r i b u t i o n: Palaearctic (Armenia, Austria, Azerbaijan, Bulgaria, Czech Republic, Georgia, Germany, Iran, Kazakhstan, Russia, Switzerland, Tadzhikistan, Turkey, Turkmenistan, Ukraine).
description: Published as part of Stojanova, A. & Ghahari, H., 2009, Checklists of Iranian Eurytomidae and Torymidae (Hymenoptera, Chalcidoidea), pp. 845-862 in Linzer biologische Beiträge 41 (1) on page 854, DOI: 10.5281/zenodo.5276308
Seiberg--Witten invariants and surface singularities
Creators: name: Nemethi, Andras
name: Nicolaescu, Liviu I
Publisher: name: arXiv
Year: 2001
Subjects: subject: Algebraic Geometry (math.AG)
subject: Geometric Topology (math.GT)
subject: FOS: Mathematics
subject: 14B05, 14J17, 32S25, 57R57, 57M27, 14E15, 32S55, 57M25

description: We formulate a very general conjecture relating the analytical invariants of a normal surface singularity to the Seiberg-Witten invariants of its link provided that the link is a rational homology sphere. As supporting evidence, we establish its validity for a large class of singularities: some rational and minimally elliptic (including the cyclic quotient and `polygonal') singularities, and Brieskorn-Hamm complete intersections. Some of the verifications are based on a result which describes (in terms of the plumbing graph) the Reidemeister-Turaev sign refined torsion (or, equivalently, the Seiberg-Witten invariant) of a rational homology 3-manifold M, provided that M is given by a negative definite plumbing. These results extend previous work of Artin, Laufer and S S-T Yau, respectively of Fintushel-Stern and Neumann-Wahl.
description: Published by Geometry and Topology at http://www.maths.warwick.ac.uk/gt/GTVol6/paper9.abs.html
Richardson diffusion in neurons
Creators: name: Iomin, Alexander
Publisher: name: arXiv
Year: 2019
Subjects: subject: Biological Physics (physics.bio-ph)
subject: Disordered Systems and Neural Networks (cond-mat.dis-nn)
subject: Soft Condensed Matter (cond-mat.soft)
subject: Statistical Mechanics (cond-mat.stat-mech)
subject: Neurons and Cognition (q-bio.NC)
subject: FOS: Physical sciences
subject: FOS: Biological sciences

description: The dynamics of an initial wave packed affected by random noise is considered in the framework of a comb model. The model is relevant to a diffusion problem in neurons where the transport of ions can be accelerated by an external random field due to synapse fluctuations. In the present specific case, it acts as boundary conditions, which lead to a reaction transport equation with multiplicative noise. The temporal behavior of the mean squared displacement is estimated analytically, and it is shown that the spreading of the initial wave packet corresponds to Richardson diffusion.
A New Code for Nonradial Stellar Pulsations and its Application to Low - Mass, Helium White Dwarfs
Creators: name: Corsico, A. H.
name: Benvenuto, O. G.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present a finite difference code intended for computing linear, adiabatic, nonradial pulsations of spherical stars. This code is based on a general Newton - Raphson technique in order to handle the relaxation of the eigenvalue (square of the eigenfrequency) of the modes and their corresponding eigenfunctions. This code has been tested computing the pulsation spectra of polytropic spheres finding a good agreement with previous work. Then, we have coupled this code to our evolutionary code and applied it to the computation of the pulsation spectrum of a low mass, pure - helium white dwarf of 0.3 M_{sun} for a wide range of effective temperatures. In making this calculation we have taken an evolutionary time step short enough such that eigenmodes corresponding to a given model are used as initial approximation to those of the next one. Specifically, we have computed periods, period spacing, eigenfunctions, weight functions, kinetic energies and variational periods for a wide range of modes. To our notice this is the first effort in studying the pulsation properties of helium white dwarfs. The solution we have found working with these realistic white dwarf models are in good accord with the predictions of the asymptotic theory of Tassoul (1980) for high order modes. This indicates that the code presented here is able to work adequately also with realistic stellar models.
description: 27 pages, 7 figures Accepted for publication in ApSS
An analytical perspective for policy studies in intergovernment financial relations in Australia
Creators: name: Blackburn, V. C.
Publisher: name: The Australian National University
Year: 1978
Subjects: subject: Intergovernmental fiscal relations Australia
subject: Australia Economic policy

description: Systems analysis provides a framework for the quantification of financial interrelationships in a multi-level hierarchical system of government. In outlining how the entanglements of intergovernmental financial relations can be quantified, reference is made to the specific impact of Commonwealth funding on State and local government financial behaviour, and to the general impact on resource allocation processes in major sectors of the regional economy. As a first step in the elaboration of a range of policy relevant research studies a behavioural model has been estimated of the fiscal impact of Commonwealth and State government grants on local government financial behaviour.
Belotelsonidea Schram 1981
Creators: name: Schram, Frederick R.
Publisher: name: Zenodo
Year: 2006
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Malacostraca
Belotelsonidea

description: Order BELOTELSONIDEA Schram, 1981  DIAGNOSIS. — Well-developed carapace free from thoracic segments, covering thorax, with a well-developed optic notch and large lateral branchiostegal expansion; no maxillipeds, all eight thoracopods with robust endopods, without exopods; pleopods as biramous flaps, uropodal rami large and variously developed; telson longer than wide, narrowing distally, with limited subterminal lobes.
description: Published as part of Schram, Frederick R., 2006, Lobetelson mclaughlinae n. gen., n. sp., a new genus and species of belotelsonid malacostracan from the Pennsylvanian of the Mazon Creek area, pp. 277-284 in Zoosystema 28 (2) on page 278, DOI: 10.5281/zenodo.5392923
The Helium Abundance of NGC 6791 from Modeling of Stellar Oscillations
Creators: name: McKeever, Jean
name: Basu, Sarbani
name: Corsaro, Enrico
Publisher: name: arXiv
Year: 2019
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: The helium abundance of stars is a strong driver of evolutionary timescales, however it is difficult to measure in cool stars. We conduct an asteroseismic analysis of NGC 6791, an old, metal rich open cluster that previous studies have indicated also has a high helium abundance. The cluster was observed by Kepler and has unprecedented lightcurves for many of the red giant branch stars in the cluster. Previous asteroseismic studies with Kepler data have constrained the age through grid based modeling of the global asteroseismic parameters ($Δν$ and $ν_{\mathrm{max}}$). However, with the precision of Kepler data, it is possible to do detailed asteroseismology of individual mode frequencies to better constrain the stellar parameters, something that has not been done for these cluster stars as yet. In this work, we use the observed mode frequencies in 27 hydrogen shell burning red giants to better constrain initial helium abundance ($Y_0$) and age of the cluster. The distributions of helium abundance and age for each individual red giant are combined to create a final probability distribution for age and helium abundance of the entire cluster. We find a helium abundance of $Y_0=0.297\pm0.003$ and a corresponding age of $8.2\pm0.3$ Gyr.
description: accepted to ApJ
MOESM9 of Genetic parameters for first lactation dairy traits in the Alpine and Saanen goat breeds using a random regression test-day model
Creators: name: Arnal, Mathieu
name: Larroque, Hélène
name: Leclerc, Hélène
name: Ducrocq, Vincent
name: Robert-Granié, Christèle
Publisher: name: figshare
Year: 2019
Subjects: subject: Genetics
subject: FOS: Biological sciences
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: Science Policy

description: Additional file 9: Figure S6. Genetic correlations between DIM 40 and other DIM in Alpine goats from the leg4 model.