cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
A complete 12CO 2--1 map of M51 with HERA: II. Total gas surface densities and gravitational stability
Creators: name: Hitschfeld, M.
name: Kramer, C.
name: Schuster, K. F.
name: Garcia-Burillo, S.
name: Stutzki, J.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: To date the onset of large-scale star formation in galaxies and its link to gravitational stability of the galactic disk have not been fully understood. The nearby face-on spiral galaxy M51 is an ideal target for studying this subject. This paper combines CO, dust, HI, and stellar maps of M51 and its companion galaxy to study the H2/HI transition, the gas-to-dust ratios, and the stability of the disk against gravitational collapse. We combine maps of the molecular gas using 12CO 2--1 map HERA/IRAM-30m data and HI VLA data to study the total gas surface density and the phase transition of atomic to molecular gas. The total gas surface density is compared to the dust surface density from 850 micron SCUBA data. Taking into account the velocity dispersions of the molecular and atomic gas, and the stellar surface densities derived from the 2MASS K-band survey, we derive the total Toomre Q parameter of the disk. The gas surface density in the spiral arms is approximately 2-3 higher compared to that of the interarm regions. The ratio of molecular to atomic surface density shows a nearly power-law dependence on the hydrostatic pressure P_hydro. The gas surface density distribution in M51 shows an underlying exponential distribution with a scale length of h_gas=7.6 kpc representing 55% of the total gas mass, comparable to the properties of the exponential dust disk. In contrast to the velocity widths observed in HI, the CO velocity dispersion shows enhanced line widths in the spiral arms compared to the interarm regions. The contribution of the stellar component in the Toomre Q-parameter analysis is significant and lowers the combined Q-parameter Q_tot by up to 70% towards the threshold for gravitational instability. The value of Q_tot varies from 1.5-3 in radial averages. A map of Q_tot shows values around 1 on the spiral arms.
description: 15 pages, 15 figures, accepted by A&A for publication
Lorentz violation in three-family neutrino oscillation
Creators: name: Yang, Shimin
name: Ma, Bo-Qiang
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We analyze the consequences of Lorentz violation (LV) to three-generation neutrino oscillation in the massless neutrino sector. We present a general formalism of three-family neutrino oscillation with neutrino flavor states being mixing states of energy eigenstates. It is also found that the mixing parts could strongly depend on neutrino energy by special choices of Lorentz violation parameters. By confronting with the existing experimental data on neutrino oscillation, the upper bounds on LV parameters are derived. Because the oscillation amplitude could vary with the neutrino energy, neutrino experiments with energy dependence may test and constrain the Lorentz violation scenario for neutrino oscillation.
description: 15 latex pages, 5 figures, final version for journal publication
Entropy production and the arrow of time
Creators: name: Parrondo, Juan M. R.
name: Broeck, Christian van den
name: Kawai, Ryoichi
Publisher: name: arXiv
Year: 2009
Subjects: subject: Statistical Mechanics (cond-mat.stat-mech)
subject: FOS: Physical sciences

description: We present an exact relationship between the entropy production and the distinguishability of a process from its time-reverse, quantified by the relative entropy between forward and backward states. The relationship is shown to remain valid for a wide family of initial conditions, such as canonical, constrained canonical, multi-canonical and grand canonical distributions, as well as both for classical and quantum systems.
description: 15 pages, no figures
The Relationship Between Religious Centers and Urban Development: Evidence from Ghana
Creators: name: Eshtiyagh, Javad
Publisher: name: University of Chicago
Year: 2023
Subjects: subject: urban
subject: machine learning
subject: satellite images
subject: religious centers

description: A large number of churches and mosques have been recently established in Ghana. Local policymakers and foreign philanthropists politically and financially support establishing these houses of worship due to their assumption regarding a causal relationship between religious centers and neighborhood development. The current study aims to test whether the assumption regarding a causal link holds by extracting and analyzing features from satellite images and conducting a spatial clustering analysis. The results indicate that religious centers are more likely to be constructed in fast-growing neighborhoods with certain characteristics. However, there are no signs of them changing temporal trends in urban development. Religious centers are more likely to be established in middle-class neighborhoods with high population density and above-average rates of illiteracy and unemployment. In addition to testing the mentioned assumption, the results shed some light on the influence of demand-and-supply factors versus socioeconomic and accessibility variables on the spatial distribution of religious centers.
Big Bang Nucleosynthesis with long-lived strongly interacting relic particles
Creators: name: Kusakabe, Motohiko
name: Kajino, Toshitaka
name: Yoshida, Takashi
name: Mathews, Grant J.
Publisher: name: arXiv
Year: 2010
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We study effects of relic long-lived strongly interacting massive particles (X particles) on big bang nucleosynthesis (BBN). The X particle is assumed to have existed during the BBN epoch, but decayed long before detected. The interaction strength between an X and a nucleon is assumed to be similar to that between nucleons. Rates of nuclear reactions and beta decay of X-nuclei are calculated, and the BBN in the presence of neutral charged X^0 particles is calculated taking account of captures of X^0 by nuclei. As a result, the X^0 particles form bound states with normal nuclei during a relatively early epoch of BBN leading to the production of heavy elements. Constraints on the abundance of X^0 are derived from observations of primordial light element abundances. Particle models which predict long-lived colored particles with lifetimes longer than about 200 s are rejected. This scenario prefers the production of 9Be and 10B. There might, therefore, remain a signature of the X particle on primordial abundances of those elements. Possible signatures left on light element abundances expected in four different models are summarized.
description: 6 pages, 2 figures, to appear in the Proceedings of IAU Symposium 268: Light elements in the Universe (C. Charbonnel, M. Tosi, F. Primas, C. Chiappini, eds.; Cambridge Univ. Press)
Lusztig limit of quantum sl(2) at root of unity and fusion of (1,p) Virasoro logarithmic minimal models
Creators: name: Bushlanov, P. V.
name: Feigin, B. L.
name: Gainutdinov, A. M.
name: Tipunin, I. Yu.
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We introduce a Kazhdan--Lusztig-dual quantum group for (1,p) Virasoro logarithmic minimal models as the Lusztig limit of the quantum sl(2) at pth root of unity and show that this limit is a Hopf algebra. We calculate tensor products of irreducible and projective representations of the quantum group and show that these tensor products coincide with the fusion of irreducible and logarithmic modules in the (1,p) Virasoro logarithmic minimal models.
description: 19 pages
A HR-like diagram for galaxies: the M_BH versus M_G sigma^2 relation
Creators: name: Feoli, Antonio
name: Mancini, Luigi
Publisher: name: arXiv
Year: 2009
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We show that the relation between the mass of supermassive black holes located in the center of the host galaxies and the kinetic energy of random motions of the corresponding bulges is a useful tool to study the evolution of galaxies. In the form log[M_BH] = b + m log[M_G sigma^2/c^2], the best-fitting results for a sample of 64 galaxies of various morphological types are the slope m=0.80 and the normalization b=4.53. We note that, in analogy with the H-R diagram for stars, each morphological type of galaxy generally occupies a different area in the M_BH - (M_G sigma^2)/c^2 plane. In particular, we find elliptical galaxies in the upper part of the line of best fit, the lenticular galaxies in the middle part, and the late-type galaxies in the lower part, the mass of the central black hole giving an estimate of the age, whereas the kinetic energy of the stellar bulges is directly connected with the temperature of each galactic system. Finally, the values of the linear correlation coefficient, the intrinsic scatter, and the chi^2 obtained by using the M_BH - M_G sigma^2 relation are better than the corresponding ones obtained from the M_BH - sigma or M_BH - M_G relation.
description: ApJ, in press
ILAMBv2.5 benchmarking results comparing E3SMv1.1 CMIP6 historical simulations with multi-model CMIP5 historical simulations
Creators: name: Burrows, Susannah
name: Maltrud, Mathew
name: Yang, Xiaojuan
name: Zhu, Qing
name: Jeffery, Nicole
name: Shi, Xiaoying
name: Ricciuto, Daniel
name: Wang, Shanlin
name: Bisht, Gautam
name: Tang, Jinyun
name: Wolfe, Jon
name: Harrop, Bryce E.
name: Singh, Balwinder
name: Brent, Lee
name: Baldwin, Sterling
name: Zhou, Tian
name: Cameron-Smith, Philip J.
name: Keen, Noel
name: Collier, Nathan
name: Xu, Min
name: Hunke, E. C.
name: M. Elliott, Scott
name: K. Turner, Andrew
name: Li, H.
name: Wang, H.
name: Golaz, Jean‐Christophe
name: Bond-lamberty, Ben
name: Hoffman, Forrest M.
name: Riley, William J.
name: Thornton, Peter E.
name: Calvin, Kate
name: Leung, L. Ruby
Publisher: name: figshare
Year: 2020
Subjects: classificationCode: 419999
subject: Other environmental sciences not elsewhere classified
classificationCode: 370799
subject: Hydrology not elsewhere classified
classificationCode: 370699
subject: Geophysics not elsewhere classified
classificationCode: 370202
subject: Climatology
classificationCode: 310908
subject: Animal physiology - biophysics
classificationCode: 310909
subject: Animal physiology - cell
classificationCode: 310910
subject: Animal physiology - systems
classificationCode: 310899
subject: Plant biology not elsewhere classified

description: These are the land model benchmarking results for the Energy
Exascale Earth System Model version 1.1 (E3SMv1.1) coupled
biogeochemistry outputs from CMIP6 historical simulations compared
with multi-model CMIP5 historical simulations. The benchmarking
results were generated using the International Land Model
Benchmarking package version 2.5 (ILAMBv2.5). While the CMIP5 model
results were obtained from the Earth System Grid Federation (ESGF),
the E3SMv1.1 model results included in this analysis were produced
from the raw model output using the workflow script at https://github.com/rubisco-sfa/elm2ilamb_wkflow. The script includes the functions of time serialization, conservative regridding and cmorization. The Earth System Modeling Framework (ESMF) "ESMF_RegridWeightGen" tool was used for generating weights for interpolating from the E3SM's cubed sphere grid to a regular lat/lon grid.

The web interface for the benchmarking results can be found at
https://www.ilamb.org/ELM/ilamb_e3sm_cbgcv1/

The ILAMB software can be obtained from
https://github.com/rubisco-sfa/ILAMB
Dissemination and Communication
Creators: name: FUDGE-5G Partners
Publisher: name: Zenodo
Year: 2021

description: The present document reports the dissemination and communication activities in the scope of the FUDGE-5G project, entailing both the project communication channels and dissemination activities in relevant events. It encompasses the methodology and procedures that FUDGE-5G has put in place to generate the communication and dissemination content, which include deliverables, news, scientific publications and presentations. The document also covers the initial communication and dissemination strategy. Moreover, the document lists all produced contents and presents a statistical overview of the performance of the established communication channels. This is the first version of Deliverable D5.2, reporting the activities conducted so far (up to Month 12). A final version of this deliverable is planned for Month 30, reporting all the dissemination and communication activities conducted in the scope of the project. Finally, it should be noted that this first version of Deliverable D5.2 was originally planned for Month 15, being anticipated to Month 12 to better align with the midterm review of the project.
Occurrence of Tachyonic Preheating in the Mixed Higgs-$R^2$ Model
Creators: name: He, Minxi
name: Jinno, Ryusuke
name: Kamada, Kohei
name: Starobinsky, Alexei A.
name: Yokoyama, Jun'ichi
Publisher: name: Deutsches Elektronen-Synchrotron, DESY, Hamburg
Year: 2020
Subjects: coupling: nonminimal
tachyon: stability
inflation: model
preheating
efficiency
scalaron

description: It has recently been suggested that at the post-inflationary stage of the mixed Higgs-$R^2$ model of inflation there can arise an efficient particle production from the tachyonic instability of the Higgs field. It might complete the preheating of the Universe, if appropriate conditions are satisfied, especially in the Higgs-like regime. In this paper, we study this behavior in more depth, including the conditions of occurrence, analytical estimates for the maximal efficiency, and the necessary degree of fine-tuning of model parameters to complete preheating by this effect. We find that the parameter sets that cause the most efficient tachyonic instabilities obey simple laws in both the Higgs-like regime and $R^2$-like regime, respectively. We then estimate the efficiency of this instability. In particular, even in the deep $R^2$-like regime with a small non-minimal coupling, this effect is strong enough to complete preheating although a severe fine-tuning is required among the model parameters. We also estimate how much fine-tuning is needed to complete preheating by this effect. It is shown that the fine-tuning of parameters for the sufficient particle production is at least $ < \mathcal{O}(0.1) $ in the deep Higgs-like regime with a large scalaron mass, while it is more severe $\sim {\cal O}(10^{-4})-{\cal O}(10^{-5})$ in the $R^2$-like regime with a small non-minimal coupling.
The Generation of Promoter-Mediated Transcriptional Noise in Bacteria
Creators: name: Mitarai, Namiko
name: Dodd, Ian B.
name: Crooks, Michael T.
name: Sneppen, Kim
Publisher: name: arXiv
Year: 2008
Subjects: subject: Molecular Networks (q-bio.MN)
subject: Quantitative Methods (q-bio.QM)
subject: FOS: Biological sciences

description: Noise in the expression of a gene produces fluctuations in the concentration of the gene product. These fluctuations can interfere with optimal function or can be exploited to generate beneficial diversity between cells; gene expression noise is therefore expected to be subject to evolutionary pressure. Shifts between modes of high and low rates of transcription initiation at a promoter appear to contribute to this noise both in eukaryotes and prokaryotes. However, models invoked for eukaryotic promoter noise such as stable activation scaffolds or persistent nucleosome alterations seem unlikely to apply to prokaryotic promoters. We consider the relative importance of the steps required for transcription initiation. The 3-step transcription initiation model of McClure is extended into a mathematical model that can be used to predict consequences of additional promoter properties. We show in principle that the transcriptional bursting observed at an E. coli promoter by Golding et al. (2005) can be explained by stimulation of initiation by the negative supercoiling behind a transcribing RNA polymerase (RNAP) or by the formation of moribund or dead-end RNAP-promoter complexes. Both mechanisms are tunable by the alteration of promoter kinetics and therefore allow the optimization of promoter mediated noise.
description: 4 figures, 1 table. Supplemental materials are also included
Local structure of liquid carbon controls diamond nucleation
Creators: name: Ghiringhelli, L. M.
name: Valeriani, C.
name: Meijer, E. J.
name: Frenkel, D.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Soft Condensed Matter (cond-mat.soft)
subject: FOS: Physical sciences

description: Diamonds melt at temperatures above 4000 K. There are no measurements of the steady-state rate of the reverse process: diamond nucleation from the melt, because experiments are difficult at these extreme temperatures and pressures. Using numerical simulations, we estimate the diamond nucleation rate and find that it increases by many orders of magnitude when the pressure is increased at constant supersaturation. The reason is that an increase in pressure changes the local coordination of carbon atoms from three-fold to four-fold. It turns out to be much easier to nucleate diamond in a four-fold coordinated liquid than in a liquid with three-fold coordination, because in the latter case the free-energy cost to create a diamond-liquid interface is higher. We speculate that this mechanism for nucleation control is relevant for crystallization in many network-forming liquids. On the basis of our calculations, we conclude that homogeneous diamond nucleation is likely in carbon-rich stars and unlikely in gaseous planets.
Additional file 2 of Hsa_circ_0003258 promotes prostate cancer metastasis by complexing with IGF2BP3 and sponging miR-653-5p
Creators: name: Yu, Yu-Zhong
name: Lv, Dao-Jun
name: Wang, Chong
name: Song, Xian-Lu
name: Xie, Tao
name: Wang, Tao
name: Li, Zhi-Min
name: Guo, Jia-Ding
name: Fu, Du-Jiang
name: Li, Kang-Jin
name: Wu, Ding-Lan
name: Chan, Franky Leung
name: Feng, Ning-Han
name: Chen, Zhe-Sheng
name: Zhao, Shan-Chao
Publisher: name: figshare
Year: 2022
Subjects: subject: Biophysics
subject: Biochemistry
subject: Medicine
subject: Cell Biology
subject: Molecular Biology
subject: Biological Sciences not elsewhere classified
subject: Cancer
subject: Statistics
subject: FOS: Mathematics

description: Additional file 2: Supplementary Table S1. Oligos used in the study.
Social Science education in Aotearoa New Zealand
Creators: name: Wood, Bronwyn
name: Oliveira, Genaro
Publisher: name: Open Access Te Herenga Waka-Victoria University of Wellington
Year: 2023
Subjects: Uncategorized

description: Prior to colonization, tangata whenua (people of the land) in Aotearoa (New Zealand) developed robust knowledge traditions. Formal social sciences education in New Zealand began with the schooling system introduced by European settlers in the late 19th century. It has been subject to recurrent review and reform since its foundation. The Education Act of 1877 led to the first formal national curriculum that introduced geography and history teaching in primary schools. During the first half of the 20th century, social sciences education in New Zealand saw a greater emphasis on citizenship education due to increasing migration and geopolitical changes resulting from the two world wars. Enduring and contentious curricular changes would follow the recommendations of the Thomas Report (1944), which introduced social studies in secondary schools as a new integrated school subject to promote learning across the social sciences. Since the 1990s, the social sciences have been named as one of New Zealand’s eight curriculum learning areas. Social studies (junior social sciences) remain as a core integrated subject taught compulsorily from years 1 to 10 (primary, intermediate, and junior secondary years), while a suite of discrete social sciences disciplines is optional for students at senior secondary levels (years 11–13). For almost 80 years, social sciences curricula have been the primary vehicle for citizenship education. The most recent curricular reforms have emphasized the importance of Mātauranga Māori (indigenous knowledge) to promote culturally-responsive social sciences learning in commitment to Aotearoa New Zealand’s bicultural foundations.
MPEC 2023-Y45 : 2023 YQ
Creators: name: Minor Planet Center Staff
Publisher: name: The Minor Planet Center
Year: 2023
Subjects: subject: Small Solar System bodies
valueUri: http://astrothesaurus.org/uat/1469
subject: 2023 YQ

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.
Backward-angle photoproduction of eta meson from protons at E_gamma = 1.6 - 2.4 GeV
Creators: name: Sumihama, M.
name: Ahn, D. S.
name: Ahn, J. K.
name: Akimune, H.
name: Asano, Y.
name: Chang, W. C.
name: Date, S.
name: Ejiri, H.
name: Fujimura, H.
name: Fujiwara, M.
name: Fukui, S.
name: Hasegawa, S.
name: Hicks, K.
name: Hotta, T.
name: Imai, K.
name: Ishikawa, 0 T.
name: Iwata, T.
name: Kato, Y.
name: Kawai, H.
name: Kino, K.
name: Kohri, H.
name: Kumagai, N.
name: Matsuda, T.
name: Matsumura, T.
name: Mibe, T.
name: Miyabe, M.
name: Muramatsu, N.
name: Nakano, T.
name: Niiyama, M.
name: Nomachi, M.
name: Ohashi, Y.
name: Ohkuma, H.
name: Ooba, T.
name: Oshuev, D. S.
name: Rangacharyulu, C.
name: Sakaguchi, 0 A.
name: Shagin, P. M.
name: Shiino, Y.
name: Shimizu, A.
name: Shimizu, H.
name: Sugaya, Y.
name: Toi, Y.
name: Toyokawa, H.
name: Wakai, A.
name: Wang, C. W.
name: Wang, S. C.
name: Yonehara, K.
name: Yorita, T.
name: Yoshimura, M.
name: Yosoi, M.
name: Zegers, R. G. T.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Nuclear Experiment (nucl-ex)
subject: FOS: Physical sciences

description: Differential cross sections for eta photoproduction off protons have been measured at E_gamma = 1.6 - 2.4 GeV in the backward direction. A bump structure has been observed above 2.0 GeV in the total energy. No such bump is observed in cross sections for eta', omega and pi0 photoproductions. It is inferred that this unique structure in eta photoproduction is due to a baryon resonance with a large portion of ss-bar strongly coupled to the etaN channel.
description: 3 figures, Submitted to PRL
Subsurface Circulations within Active Regions
Creators: name: Hindman, Bradley W.
name: Haber, Deborah A.
name: Toomre, Juri
Publisher: name: arXiv
Year: 2009
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Using high-resolution ring analysis (HRRA) we deduce subsurface flows within magnetic active regions and within quiet sun. With this procedure we are capable of measuring flows with a horizontal spatial resolution of 2 degrees in heliographic angle (or roughly 20 Mm). From the resulting flow fields we deduce mean inflow rates into active regions, mean circulation speeds around active regions, and probability density functions (PDFs) of properties of the flow field. These analyses indicate that active regions have a zonal velocity that exceeds that of quiet sun at the same latitude by 20 m/s, yet active regions advect poleward at the same rate as quiet sun. We also find that almost all active regions possess a mean inflow (20-30 m/s) and a cyclonic circulation (~5 m/s) at their peripheries, whereas their cores, where the sunspots are located, are zones of strong anticyclonic outflow (~50 m/s). From the PDFs, we find that active regions modify the structure of convection with a scale greater than that of supergranulation. Instead of possessing an asymmetry between inflows and outflows (with a larger percentage of the surface occupied by outflows), as is seen in quiet sun, active regions possess symmetric distributions.
description: 34 pages, 12 figures, submitted to the Astrophysical Journal
Current-conserving nonlinear response theory in driven systems
Creators: name: Peralta-Ramos, J.
name: Calzetta, E.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Other Condensed Matter (cond-mat.other)
subject: FOS: Physical sciences

description: Employing the closed-time path 2PI effective action (CTP 2PI EA) approach, we study the response of an open interacting electronic system to time-dependent external electromagnetic fields. We show that the 2PI EA provides a systematic way of calculating the propagator and response functions of the system. Due to the invariance of the 2PI EA under external gauge transformations, the response functions calculated from it are such that the Ward-Takahashi hierarchy, that ensures current conservation beyond the expectation value level, is satisfied. These findings may be useful in the study of interacting electronic pumping devices, and serve to clarify the connection between current conservation (beyond the mean value level) and real-time nonlinear response theory.
description: 9 pages. To appear in Proceedings of FCM 2008. v2: Acknowledgements added
Blowing dusty bubbles into the CGM: The contribution of dust-enshrouded starbursts to the baryon cycle
Creators: name: Kamieneski, Patrick
Publisher: name: Zenodo
Year: 2024

description: Maximal starbursts form stars at a sufficient rate to disrupt the collapse of molecular clouds through stellar feedback. Capturing their prevalence is critical to understanding the quenching of star formation after Cosmic Noon. Dusty star-forming galaxies (DSFGs) are considered the best candidates, as they are optically thick not just to UV radiation from massive stars, but even to dust-reprocessed IR light. This creates significant radiation pressure, capable of ejecting dust and gas from the plane of the disk and into the circumgalactic medium (CGM). To better understand this, we focus on some of the most luminous known DSFGs. Our sample of 30 gravitationally-lensed objects includes hyperluminous IR galaxies with SFRs ~ 300-3000 Msun/yr. Using 0.1”-resolution ALMA observations, and taking advantage of lensing magnification, we aim to identify ~100pc-scale regions forming stars at super-Eddington rates, from where galactic winds are likely to be launched. Such measurements are nearly impossible without lensing, as they would require ~10 milliarcsec resolution. JWST is now adding valuable insight to this picture, peering through the thick shrouds of dust and allowing for spatially-resolved SED fitting of DSFGs on similar scales. Through NIRCam, we find widespread distributions of star formation, but also a significant presence of dust in front of more quiescent regions. This may be further evidence of our proposed scenario of dust being transported into the intervening CGM.
THE DEVELOPMENT OF SIGN LANGUAGE COMMUNICATION WITH THE EMOTIONAL FEELINGS IN DEAF CHILD
Creators: name: Absamatova, Gulkhayo
Publisher: name: Zenodo
Year: 2023

description: This article is devoted to the social situation in which a child with hearing impairment finds himself is of great importance in the emergence of his peculiarities in the development of emotions and the formation of certain personality traits. The development of the emotional sphere of deaf children is influenced by certain unfavorable factors. Violation of verbal communication partially isolates a deaf person from the speaking people around him, which creates difficulties in assimilating social experience.
REACH Story of Change: Monitoring and modelling river water quality to protect Dhaka’s river system
Creators: name: REACH
Publisher: name: University of Oxford
Year: 2024

description: The Ready Made Garment (RGM) industry in Bangladesh is one source of pollution into Dhaka’s heavily contaminated rivers. Industrial pollution together with domestic waste damages rivers, estuaries and coastal waters with serious impact on the health and livelihoods of people who live nearby. REACH has created river system models to evaluate domestic and industrial effluents in rivers, and contributed to the development of a new water quality monitoring network in Dhaka. The models have also been used to assess mitigation measures for river clean-up, both for a government-led USD 20 billion mitigation scheme in Dhaka, and for industry, to inform potential investment in water treatment measures. Since 2019, Primark, the Alliance for Water Stewardship (AWS) and the Partnership for Cleaner Textiles (PaCT) representing many of the major international RMG companies, have been collaborating with the REACH programme to understand and respond to pollution from their factories.
Three-body break-up in deuteron-deuteron scattering at 65 MeV/nucleon
Creators: name: Ramazani-Moghaddam-Arani, A.
name: Amir-Ahmadi, H. R.
name: Bacher, A. D.
name: Bailey, C. D.
name: Biegun, A.
name: Eslami-Kalantari, M.
name: Gašparić, I.
name: Joulaeizadeh, L.
name: Kalantar-Nayestanaki, N.
name: Kistryn, St.
name: Kozela, A.
name: Mardanpour, H.
name: Messchendorp, J. G.
name: Micherdzinska, A. M.
name: Moeini, H.
name: Shende, S. V.
name: Stephan, E.
name: Stephenson, E. J.
name: Sworst, R.
Publisher: name: arXiv
Year: 2010
Subjects: subject: Nuclear Experiment (nucl-ex)
subject: FOS: Physical sciences

description: We successfully identified a few final states in deuteron-deuteron scattering at 65 MeV/nucleon at KVI using a unique and advanced detection system called BINA. This facility enabled us to perform cross sections and polarization measurements with an excellent statistical and systematical precision. The analysis procedure and part of the results of the three-body break-up channel in deuteron-deuteron scattering at 65 MeV/nucleon are presented in this paper.
description: proceedings of the 19th International IUPAP Conference on Few-Body Problems in Physics, Bonn University, 31.08 - 05.09.2009, Bonn, GERMANY
השפעת מקור גורמי הסבל על רמת החמלה העצמית
Creators: name: Cohen, Gili Pattir
name: Novoselsky, Asaf
name: Cohen, Neta
name: TAU Experimental Psychology Team
Publisher: name: Open Science Framework
Year: 2023
Subjects: subject: Social and Behavioral Sciences
subject: Psychology
subject: FOS: Psychology

description: זוהי ההרשמה מראש למחקר שלנו, במסגרת קורס פסיכולוגיה ניסויית באוניברסיטת תל אביב.
Transitivity vs. Intransitivity in decision making process. (An example in quantum game theory)
Creators: name: Makowski, Marcin
Publisher: name: arXiv
Year: 2009
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We compare two different ways of quantization a simple sequential game Cat's Dilemma in the context of the debate on intransitive and transitive preferences. This kind of analysis can have essential meaning for the research on the artificial intelligence (some possibilities are discussed). Nature has both properties transitive and intransitive and maybe quantum models can be more able to capture this dualism than classical one. We also present electoral interpretation of the game.
description: 18 pages, 3 figures
Überprüfung der Interrater-Reliabilität der Jugendversion des Diagnostischen Interviews bei Psychischen Störungen (J-DIPS) mit Fokus auf die DSM-5 Forschungsdiagnosen „Nichtsuizidale Selbstverletzungen“ und „Suizidale Verhaltensstörung“
Creators: name: Theobald, Louisa
Publisher: name: Open Science Framework
Year: 2023
Subjects: subject: Psychiatry and Psychology
subject: Mental Disorders
subject: Medicine and Health Sciences

description: Nichtsuizidales Selbstverletzendes Verhalten und die Suizidale Verhaltensstörung bilden im Jugendalter prävalente Störungsbilder ab. Bisher können diese Forschungsdiagnosen des DSM-5 mit gängigen klinischen Interviews nicht adäquat erfasst werden. Zur Diagnostik dieser Forschungsdiagnosen kann das Diagnostische Interview bei Psychischen Störungen (J-DIPS) verwendet werden. Um das J-DIPS in der Forschung sowie in der klinischen Praxis anwendbar zu machen, werden in dieser Arbeit die im J-DIPS enthaltenen Forschungsdiagnosen auf ihr Interrater-Reliabilität hin überprüft.
A widely tunable laser frequency offset lock with digital counting
Creators: name: Hughes, Joshua
name: Fertig, Chad
Publisher: name: arXiv
Year: 2009
Subjects: subject: Instrumentation and Detectors (physics.ins-det)
subject: Atomic Physics (physics.atom-ph)
subject: FOS: Physical sciences

description: We demonstrate a hybrid analog+digital electronic lock to stabilize a dynamically tunable rf offset between two lasers. Our method features an 80 MHz capture range, +/- 7 GHz tuning range, frequency agility of 1 MHz/microsecond, and low (<30 ppm) drift in the absolute optical frequency difference after ~1000 s. With this scheme, multiple slave lasers can easily be referenced to one stable master laser, while each remains rapidly and accurately tunable over the wide frequency ranges encountered in typical laser cooling and trapping experiments.
description: 8 pages, 8 figures
Lorentz Boosted Nucleon-Nucleon T-matrix and the Triton Binding Energy
Creators: name: Kamada, H.
name: Gloeckle, W.
name: Witala, H.
name: Golak, J.
name: Skibinski, R.
name: Polyzou, W.
name: Elster, Ch.
Publisher: name: arXiv
Year: 2008
Subjects: subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: The phase equivalent relativistic NN potential, which is related by a nonlinear equation to the original nonrelativistic potential, is used to construct the mass operator (rest Hamiltonian) of the 3-nucleon system. Employing the CD Bonn NN potential, the solution of the relativistic 3N Faddeev equation for $^3$H shows slightly less binding energy than the corresponding nonrelativistic result. The effect of the Wigner spin rotation on the binding is very small.
description: 6 pages, 2 figures, Asia Pacific Few-Body Conference 2008 in Indonesia, submitted to Modern Physics Letters A
CO Line Excitation and Molecular Gas Conditions in Nearby Galaxies
Creators: name: Keenan, Ryan Patrick
Publisher: name: Zenodo
Year: 2024

description: The CO(1-0) line has been carefully calibrated as a tracer of molecular gas mass. However, recent studies often favor higher J CO transitions which are brighter and accessible for redshift ranges where CO(1-0) is not. These lines are not perfect analogues for CO(1-0), owing to their more stringent excitation conditions, and must be calibrated for use as molecular gas tracers. Conversely, observations of multiple CO lines in a single target can constrain additional gas properties beyond mass. I will present the Arizona Molecular ISM Survey with the SMT (AMISS), a multi-CO line survey of z<0.05 galaxies conducted with the CO(1-0), CO(2-1) and CO(3-2) lines. The project targeted a representative sample of 10^9 Msun < M* < 10^11.5 Msun galaxies. The final survey includes CO(2-1) spectra of 176 galaxies and CO(3-2) spectra for a subset of 45 supplemented by new and archival CO(1-0) spectra for all targets. I will present the results of our study of CO luminosity ratios, showing that CO(2-1) and CO(3-2) are systematically fainter relative to CO(1-0) in galaxies with less star formation activity. These results provide a reference for comparison to ongoing high-redshift gas excitation studies with ALMA, as well as a tool for converting between CO lines in studies of nearby galaxies.
Simultaneous Arithmetic Progressions on Algebraic Curves
Creators: name: Schwartz, Ryan
name: Solymosi, József
name: de Zeeuw, Frank
Publisher: name: arXiv
Year: 2009
Subjects: subject: Number Theory (math.NT)
subject: Combinatorics (math.CO)
subject: FOS: Mathematics
subject: 11P21

description: A simultaneous arithmetic progression (s.a.p.) of length k consists of k points (x_i, y_σ(i)), where x_i and y_i are arithmetic progressions and σis a permutation. Garcia-Selfa and Tornero asked whether there is a bound on the length of an s.a.p. on an elliptic curve in Weierstrass form over Q. We show that 4319 is such a bound for curves over R. This is done by considering translates of the curve in a grid as a graph. A simple upper bound is found for the number of crossings and the 'crossing inequality' gives a lower bound. Together these bound the length of an s.a.p. on the curve. We then use a similar method to extend the result to arbitrary real algebraic curves. Instead of considering s.a.p.'s we consider k^2/3 points in a grid. The number of crossings is bounded by Bezout's Theorem. We then give another proof using a result of Jarnik bounding the number of grid points on a convex curve. This result applies as any real algebraic curve can be broken up into convex and concave parts, the number of which depend on the degree. Lastly, these results are extended to complex algebraic curves.
description: 11 pages, 6 figures, order of email addresses corrected 12 pages, closing remarks, a reference and an acknowledgment added
Physiotherapy Provision and Practice: A EuropeAn Intensive CarE Unit (ICU) Survey (PEAiCE)
Creators: name: Lewko, Agnieszka
name: Nydahl, Peter
name: Grossenbacher, Sabrina
name: McWilliams, David
Publisher: name: Open Science Framework
Year: 2023
Subjects: subject: Medicine and Health Sciences
subject: physiotherapy practice
subject: respiratory physiotherapy
subject: Intensive Care
subject: ICU rehabilitation
subject: ICU
subject: physiotherapy practice internationally
subject: physiotherapy

description: Physiotherapists are experts in early mobilisation and respiratory techniques, assisting patients in their recovery from critical illness in the Intensive Care Unit (ICU). However, current provision of physiotherapyand practice delivered across Europe is varied and inconsistent. This project will utalise a large-scale survey design to identify physiotherapy practices in ICU across Europe and will allow development of targeted education packages and inform physiotherapy curricula, which will benefit patients in the long-term to receive the best and evidence-informed care across the whole continent.
Supplementary Materials
Creators: name: Büscher, Thies Henning
name: Petersen, Dennis
name: Bijma, Nienke N.
name: Bäumler, Fabian
name: Pirk, Christian W. W.
name: Büsse, Sebastian
name: Heepe, Lars
name: Gorb, Stanislav N.
Publisher: name: figshare
Year: 2021
Subjects: subject: Zoology
subject: FOS: Biological sciences

description: Supplementary Materials for the acticle "The exceptional attachment ability of the ectoparasitic bee louse Braula coeca (Diptera, Braulidae) on the honeybee" in Physiological Entomology
Exact Coupling Coefficient Distribution in the Doorway Mechanism
Creators: name: Kohler, Heiner
name: Guhr, Thomas
name: Aberg, Sven
Publisher: name: arXiv
Year: 2010
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: In many--body and other systems, the physics situation often allows one to interpret certain, distinct states by means of a simple picture. In this interpretation, the distinct states are not eigenstates of the full Hamiltonian. Hence, there is an interaction which makes the distinct states act as doorways into background states which are modeled statistically. The crucial quantities are the overlaps between the eigenstates of the full Hamiltonian and the doorway states, that is, the coupling coefficients occuring in the expansion of true eigenstates in the simple model basis. Recently, the distribution of the maximum coupling coefficients was introduced as a new, highly sensitive statistical observable. In the particularly important regime of weak interactions, this distribution is very well approximated by the fidelity distribution, defined as the distribution of the overlap between the doorway states with interaction and without interaction. Using a random matrix model, we calculate the latter distribution exactly for regular and chaotic background states in the cases of preserved and fully broken time--reversal invariance. We also perform numerical simulations and find excellent agreement with our analytical results.
description: 22 pages, 4 figures
An exercise program for people with visual impairment in Taiwan: An occupational perspective (Protocol)
Creators: name: Thomacos, Nikos
name: Lalor, Aislinn
name: Chang, Chun-Wei
name: Chen, Ming-De
Publisher: name: Open Science Framework
Year: 2023
Subjects: subject: Health Services Research
subject: Sociology
subject: FOS: Sociology
subject: Public Health
subject: Medicine and Health Sciences
subject: Health Services Administration
subject: Social and Behavioral Sciences
subject: occupational engagement
subject: blindness
subject: low vision
subject: physical activity

description: People with visual impairment have reduced access to participate in exercise due to factors related to their impaired vision. Individuals with visual impairment in Taiwan similarly have lower participation rates in exercise than those without visual impairment. Consequently, people with visual impairment in Taiwan are at increased risk of poorer health. In recent years, some social welfare organisations that provide services to people with visual impairment have become aware of this issue, and have commenced provision of exercise programs within their service. However, little is known about the impact these exercise programs have for people with visual impairment in Taiwan. The consideration of applicability, suitability, and the occupational meaning of exercise programs for people with visual impairment are also limited. This research will investigate the influence of a purposely-designed exercise program for people with visual impairment in Taiwan.
Axion quality from the (anti)symmetric of SU(N)
Creators: name: Ardu, Marco
name: Di Luzio, Luca
name: Landini, Giacomo
name: Strumia, Alessandro
name: Teresi, Daniele
name: Wang, Jin-Wei
Publisher: name: Deutsches Elektronen-Synchrotron, DESY, Hamburg
Year: 2020
Subjects: model: scalar
symmetry: Peccei-Quinn
interaction: gauge
symmetry: global
strong interaction: CP
axion
dark matter
quality
spontaneous symmetry breaking
bound state
inflation
monopole
thermal
SU(N)
U(1)

description: We propose two models where a U(1) Peccei-Quinn global symmetry arises accidentally and is respected up to high-dimensional operators, so that the axion solution to the strong CP problem is successful even in the presence of Planck-suppressed operators. One model is SU$(N)$ gauge interactions with fermions in the fundamental and a scalar in the symmetric. The axion arises from spontaneous symmetry breaking to SO$(N)$, that confines at a lower energy scale. Axion quality in the model needs $N \gtrsim 10$. SO bound states and possibly monopoles provide extra Dark Matter candidates beyond the axion. In the second model the scalar is in the anti-symmetric: SU$(N)$ broken to Sp$(N)$ needs even $N \gtrsim 20$. The cosmological DM abundance, consisting of axions and/or super-heavy relics, can be reproduced if the PQ symmetry is broken before inflation (Boltzmann-suppressed production of super-heavy relics) or after (super-heavy relics in thermal equilibrium get partially diluted by dark glue-ball decays).
The implications from CANGAROO-III observations of TeV blazar PKS 2155-304
Creators: name: Nishijima, K.
name: Sakamoto, Y.
name: Kushida, J.
name: Saito, K.
Publisher: name: arXiv
Year: 2008
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We have observed the high-frequency-peaked BL Lacertae object PKS2155-304 in 2004, 2005 and 2006 with the CANGAROO-III imaging atmospheric Cherenkov telescope, and have detected a signal above 660 GeV at the 4.8/sigma level during the 2006 outburst period. Intranight flux variability on time scale of half an hour is observed. From this variability time scale, the size of the TeV gamma-ray emission region is restricted to 5x10^13δcm, and the super massive black hole mass is estimated to be less than 1.9x10^8δM_{Solar}, where δis the beaming factor. The differential energy spectrum is obtained, and an upper limit of the extragalactic infrared background light (EBL) flux is derived under some assumption. We also fit a synchrotron self Compton (SSC) model to the spectral energy distribution (SED) and derive the beaming factor and magnetic field strength.
description: 4 pages, 5 figures, proceedings of the "4th Heidelberg International Symposium on High Energy Gamma-Ray Astronomy" July 7-11, 2008, Heidelberg, Germany
Phantom dark energy with varying-mass dark matter particles: acceleration and cosmic coincidence problem
Creators: name: Leon, Genly
name: Saridakis, Emmanuel N.
Publisher: name: arXiv
Year: 2009
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We investigate several varying-mass dark-matter particle models in the framework of phantom cosmology. We examine whether there exist late-time cosmological solutions, corresponding to an accelerating universe and possessing dark energy and dark matter densities of the same order. Imposing exponential or power-law potentials and exponential or power-law mass dependence, we conclude that the coincidence problem cannot be solved or even alleviated. Thus, if dark energy is attributed to the phantom paradigm, varying-mass dark matter models cannot fulfill the basic requirement that led to their construction.
description: 11 pages, 5 figures
Analyzing on Adverse Side Effects of COVID-19 Vaccines
Creators: name: Oroy, Kurez
Publisher: name: Open Science Framework
Year: 2023
Subjects: subject: Education

description: Since the roll-out of COVID-19 vaccines, there have been reports of allergic reactions in some individuals. The Centers for Disease Control and Prevention (CDC) has stated that severe allergic reactions to COVID-19 vaccines are rare, but it is important to understand the nature and causes of these reactions in order to minimize the risk and address concerns.
Solar Radiation Pressure and Deviations from Keplerian Orbits
Creators: name: Kezerashvili, Roman Ya.
name: Vazquez-Poritz, Justin F.
Publisher: name: arXiv
Year: 2009
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: Space Physics (physics.space-ph)
subject: FOS: Physical sciences

description: Newtonian gravity and general relativity give exactly the same expression for the period of an object in circular orbit around a static central mass. However, when the effects of the curvature of spacetime and solar radiation pressure are considered simultaneously for a solar sail propelled satellite, there is a deviation from Kepler's third law. It is shown that solar radiation pressure affects the period of this satellite in two ways: by effectively decreasing the solar mass, thereby increasing the period, and by enhancing the effects of other phenomena, rendering some of them detectable. In particular, we consider deviations from Keplerian orbits due to spacetime curvature, frame dragging from the rotation of the sun, the oblateness of the sun, a possible net electric charge of the sun, and a very small positive cosmological constant.
description: 4 pages, minor typo corrected, additional comments
USO DE COMPOSTOS CANABINÓIDES EM SAÚDE
Creators: name: Maritsa Carla De Bortoli
name: Da Silva, Letícia Aparecida Lopes Bezerra
name: De Freitas Oliveira, Cintia
name: De Melo, Roberta Crevelário
name: De Araujo, Bruna Carolina
Publisher: name: Open Science Framework
Year: 2023
Subjects: subject: Medicine and Health Sciences

description: O presente estudo tem como objetivo identificar e sumarizar as melhores evidências científicas disponíveis sobre o uso medicinal dos compostos canabinóides.
Data Management Plan
Creators: name: Project Partners
Publisher: name: Zenodo
Year: 2021

description: The present document covers the underlying issues related to data management in FUDGE- 5G, both for qualitative and quantitative data generated during the project. It encompasses the methodology and procedures that FUDGE-5G has put in place to generate, store and publish results, which include deliverables, open-source contributions, scientific publications and datasets. Furthermore, the document covers ethics and privacy issues, describing how the project follows GDPR principles and how personal data is handled during the project.