cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Over 19.5% n-Type Bifacial Solar Cells with Screen-Printed Boron Emitter
Creators: name: Uzum, A.
name: Yoshiba, S.
name: Dhamrin, M.
name: Kamisako, K.
name: Sato, H.
name: Katsuma, K.
name: Kato, K.
Publisher: name: WIP
Year: 2014
Subjects: WAFER-BASED SILICON SOLAR CELLS AND MATERIALS TECHNOLOGY
Silicon Solar Cell Improvements

description: 29th European Photovoltaic Solar Energy Conference and Exhibition; 838-840
description: The interest of using n-type silicon and producing bifacial silicon solar cells is still alive because of the
potential for higher efficiency and improved solar cell power generation. In order to use n-type material for bifacial
silicon solar cells, one of the challenges is the formation of p-type emitters by boron diffusion. Developing of costeffective,
simple and industry-friendly alternative procedures for the solar cell industry is becoming more crucial. In
this work, screen-printable boron diffusion paste was introduced and adapted to the solar cell fabrication process and
n-type bifacial solar cells with screen-printed boron emitters were fabricated on large-area CZ-Si wafers. Boron
diffusion was performed at around 975oC for 20 min. The best conversion efficiency of up to 19.5% was achieved
with the electrical properties of 642 mV, 38.2 mA/cm2 and 79.5 for Voc, Jsc and FF, respectively. Process is still under
optimization and better results are expected.
The interaction of long and short waves in dispersive media
Creators: name: Deconinck, Bernard
name: Nguyen, Nghiem V.
name: Segal, Benjamin L.
Publisher: name: arXiv
Year: 2016
Subjects: subject: Pattern Formation and Solitons (nlin.PS)
subject: Analysis of PDEs (math.AP)
subject: FOS: Physical sciences
subject: FOS: Mathematics

description: The KdV equation models the propagation of long waves in dispersive media, while the NLS equation models the dynamics of narrow-bandwidth wave packets consisting of short dispersive waves. A system that couples the two equations to model the interaction of long and short waves seems attractive and such a system has been studied over the last decades. We evaluate the validity of this system, discussing two main problems. First, only the system coupling the linear Schrödinger equation with KdV has been derived in the literature. Second, the time variables appearing in the equations are of a different order. It appears that in the manuscripts that study the coupled NLS-KdV system, an assumption has been made that the coupled system can be derived, justifying its mathematical study. In fact, this is true even for the papers where the asymptotic derivation with the problems described above is presented. In addition to discussing these inconsistencies, we present some alternative systems describing the interaction of long and short waves.
Burst phase distribution of SGR J1935+2154 based on Insight-HXMT
Creators: name: Lu, Xuefeng
name: Song, Liming
name: Ge, Mingyu
name: Tuo, Youli
name: Zhang, Shuang-Nan
name: Qu, Jinlu
name: Cai, Ce
name: Xie, Shenglun
name: Liu, Congzhan
name: Li, Chengkui
name: Fu, Yucong
name: Xu, Yingchen
name: Li, Tianming
Publisher: name: arXiv
Year: 2023
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: On April 27, 2020, the soft gamma ray repeater SGR J1935+2154 entered its intense outburst episode again. Insight-HXMT carried out about one month observation of the source. A total number of 75 bursts were detected during this activity episode by Insight-HXMT, and persistent emission data were also accumulated. We report on the spin period search result and the phase distribution of burst start times and burst photon arrival times of the Insight-HXMT high energy detectors and Fermi Gamma-ray Burst Monitor (GBM). We find that the distribution of burst start times is uniform within its spin phase for both Insight-HXMT and Fermi-GBM observations, whereas the phase distribution of burst photons is related to the type of a burst's energy spectrum. The bursts with the same spectrum have different distribution characteristics in the initial and decay episodes for the activity of magnetar SGR J1935+2154.
description: 12 pages, 9 figures
The effect of influenza vaccination on absenteeism in the workplace
Creators: name: Wadsley, Jane.
Publisher: name: Monash University
Year: 2022

description: This thesis was scanned from the print manuscript for digital preservation and is copyright the author.
 Researchers can access this thesis by asking their local university, institution or public library to
 make a request on their behalf. Monash staff and postgraduate students can use the link in the References field.
Hipposideros bicolor
Creators: name: Koopman, Karl F.
Publisher: name: Zenodo
Year: 1993
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Chiroptera
Hipposideridae
Hipposideros
Hipposideros bicolor

description: Hipposideros bicolor (Temminck, 1834). Tijdschr. Nat. Gesch. Physiol., 1:19. TYPE LOCALITY: Indonesia, Java, Anger coast. DISTRIBUTION: Malaysia to the Philippines, Timor (Indonesia), and adjacent small islands. SYNONYMS: atrox, erigens, javanicus, major. COMMENTS: Includes erigens; see Hill (1963b:27). Does not include pomona, gentilis, or macrobullatus; see Hill et al. (1986).
description: Published as part of Karl F. Koopman, 1993, Order Chiroptera, pp. 137-241 in Mammal Species of the World (2 nd Edition), Washington and London :Smithsonian Institution Press on page 171, DOI: 10.5281/zenodo.7353060
description: {"references": ["Hill, J. E. 1963 b. A revision of the genus Hipposideros. Bulletin of the British Museum (Natural History), Zoology Series, 11: 1 - 129.", "Hill, J. E., A. Zubaid, and G. W. H. Davison. 1986. The taxonomy of leaf-nosed bats of the Hipposideros bicolor group (Chiroptera: Hipposideridae) from southeastern Asia. Mammalia, 50: 535 - 540."]}
On the Impact of Ge in Compensated Solar Grade (SoG) Silicon – a Study on Ingot and Solar Cell Level
Creators: name: Halm, A.
name: Bellmann, M.P.
name: Arumughan, J.
name: Kopecek, R.
name: Peter, P.
Publisher: name: WIP
Year: 2014
Subjects: WAFER-BASED SILICON SOLAR CELLS AND MATERIALS TECHNOLOGY
Silicon Feedstock, Crystallisation and Wafering

description: 29th European Photovoltaic Solar Energy Conference and Exhibition; 786-788
description: In this study, four dopant compensated silicon ingots grown from solar grade silicon (SoG-Si)
feedstock are investigated comparing their properties against a non compensated reference ingot made from
polysilicon feedstock. All four SoG ingots are grown from the same feedstock in the same Bridgman furnace under
the same conditions using two different compensation scenarios. For two ingots Ge - a metallic impurity - is
introduced into the initial melt to study its effects on crystal quality and the possibility of a positive effect on solar
cell efficiency as postulated in ref. [1]. Dislocation density maps measured on selected wafers of the different UMG
ingots reveal lower dislocation densities for the Ge containing wafers as described in ref. [2]. On solar cell level
though, the Ge containing cells show lower conversion efficiencies. High carbon concentrations (6 to 15 ppmw) for
all SoG ingots result in SiC precipitation which leads amongst other effects to high rate of wafer breakage and cell
shunting.
The Wiener Test for the Removability of the Logarithmic Singularity for the Elliptic PDEs with Measurable Coefficients and Its Consequences
Creators: name: Abdulla, Ugur G.
Publisher: name: arXiv
Year: 2016
Subjects: subject: Analysis of PDEs (math.AP)
subject: FOS: Mathematics

description: This paper introduces the notion of $log$-regularity (or $log$-irregularity) of the boundary point $ζ$ (possibly $ζ=\infty$) of the arbitrary open subset $Ω$ of the Greenian deleted neigborhood of $ζ$ in $R^2$ concerning second order uniformly elliptic equations with bounded and measurable coefficients, according as whether the $log$-harmonic measure of $ζ$ is null (or positive). A necessary and sufficient condition for the removability of the logarithmic singularity, that is to say for the existence of a unique solution to the Dirichlet problem in $Ω$ in a class $O(\log |\cdot - ζ|)$ is established in terms of the Wiener test for the $log$-regularity of $ζ$. From a topological point of view, the Wiener test at $ζ$ presents the minimal thinness criteria of sets near $ζ$ in minimal fine topology. Precisely, the open set $Ω$ is a deleted neigborhood of $ζ$ in minimal fine topology if and only if $ζ$ is $log$-irregular. From the probabilistic point of view, the Wiener test presents asymptotic law for the $log$-Brownian motion near $ζ$ conditioned on the logarithmic kernel with pole at $ζ$.
description: arXiv admin note: text overlap with arXiv:1010.4263
Hipposideros breviceps Tate 1941
Creators: name: Koopman, Karl F.
Publisher: name: Zenodo
Year: 1993
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Chiroptera
Hipposideridae
Hipposideros
Hipposideros breviceps

description: Hipposideros breviceps Tate, 1941. Bull. Am. Mus. Nat. Hist., 78:358. TYPE LOCALITY: Indonesia, Sumatra, Mentawai Isis, N Pagi Isl. DISTRIBUTION: Mentawai Isis (Indonesia).
description: Published as part of Karl F. Koopman, 1993, Order Chiroptera, pp. 137-241 in Mammal Species of the World (2 nd Edition), Washington and London :Smithsonian Institution Press on page 171, DOI: 10.5281/zenodo.7353060
Universal anyons at the irradiated surface of topological insulator
Creators: name: Wang, Rui
name: Chen, Wei
name: Wang, Baigeng
name: Xing, D. Y.
Publisher: name: arXiv
Year: 2016
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: Anyons have recently received great attention due to their promising application in topological quantum computation. The best validated system that enjoys the anyonic excitations are the Laughlin states. The quasi-particles in Laughlin states are neither fermions nor bosons but possess the discrete statistical angle ? = ?=m, with m being an integer. Here we report a possible realization of the universal Abelian anyons, whose statistical angle can be tuned continuously by external parameters and can take any arbitrary values interpolating ? = 0 and ? = ?. The proposed setup is the surface state of a three dimensional topological insulator driven by an amplitude-modulated circularly-polarized light. It is found that the external field leads to a particular Floquet phase, which is a two-spatial-dimensional analogy of the Weyl semimetal phase in the Floquet first Brillouin zone. The chiral anomaly of this phase results in a U(1) Chern-Simons gauge theory with a tunable Floquet Chern number. Owing to this underlying gauge field theory, the irradiated surface of topological insulator constitutes a promising platform for the observation of the universal anyons.
HFES 2023 Files
Creators: name: Hewitt, Dylan
Publisher: name: OSF
Year: 2023

description: Data associated with Vo, Hewitt, & He (Accepted, 2023). Web accessibility: A revisit of U.S. state and territory COVID-19 websites after two years. Proceedings of the 67th International Human Factors and Ergonomics Society Annual Meeting.
Rossby waves on stellar equatorial beta-planes: uniformly rotating radiative stars
Creators: name: Albekioni, M.
name: Zaqarashvili, T. V.
name: Kukhianidze, V.
Publisher: name: arXiv
Year: 2023
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Rossby waves arise due to the conservation of total vorticity in rotating fluids and may govern the large-scale dynamics of stellar interiors. Recent space missions collected huge information about the light curves and activity of many stars, which triggered observations of Rossby waves in stellar surface and interiors. We aim to study the theoretical properties of Rossby waves in stratified interiors of uniformly rotating radiative stars with sub-adiabatic vertical temperature gradient. We use the equatorial beta-plane approximation and linear vertical gradient of temperature to study the linear dynamics of equatorially trapped Rossby and inertia-gravity waves in interiors of radiative stars. The governing equation is solved by the method of separation of variables in the vertical and latitudinal directions. Vertical and latitudinal solutions of the waves are found to be governed by Bessel functions and Hermite polynomials, respectively. Appropriate boundary conditions at stellar surface and poles define analytical dispersion relations for Rossby, Rossby-gravity and inertia-gravity waves. The waves are confined in surface layers of 30-50 $H_0$, where $H_0$ is surface density scale height, and trapped between the latitudes of $\pm 60^0$. Observable frequencies (normalized by the angular frequency of the stellar rotation) of Rossby waves with $m=1$ ($m=2$), where $m$ is the toroidal wavenumber, are in the interval of 0.65-1 (1.4-2), depending on stellar rotation, radius and surface temperature. Rossby-type waves can be systematically observed using light curves of Kepler and TESS stars. Observations and theory then can be used for the sounding of stellar interiors.
Effect of the Crucible and its Coating on the Red Zone in Multicrystalline Silicon – Analysis on Solar Cell Level
Creators: name: Botchak, Y.P.
name: Herzog, B.
name: Hahn, G.
Publisher: name: WIP
Year: 2014
Subjects: WAFER-BASED SILICON SOLAR CELLS AND MATERIALS TECHNOLOGY
Silicon Feedstock, Crystallisation and Wafering

description: 29th European Photovoltaic Solar Energy Conference and Exhibition; 780-785
description: The purpose of this work is to investigate the influence of the crucible and its coating on the
deteriorated edge zone (also called “red zone”) during directional solidification of multicrystalline silicon (mc-Si).
Since the material quality is changed by the processing of solar cells due to, e.g., gettering and hydrogenation, this
study was performed on material after having processed it into lab-type solar cells. The use of a standard industrial
quartz/SiO2 crucible coated with a standard Si3N4 powder leads to a clear impact of the “red zone” on solar cells. This
effect decreases over the block height. A thick very highly purified coating powder seems to considerably reduce the
in-diffusion of the impurities from this standard crucible. Using a purified industrial crucible with a coating powder
of very high purity results in a notable reduction of the “red zone” effect on solar cell level. Moreover, the use of a
purified crucible shows no effect of the “red zone” on solar cell until to a distance of ~12 mm from the crucible wall.
This is probably due to the reduction of metallic contamination from the crucible during crystallization as shown by
Schubert et al. [5]. It is shown that the main source of impurities for contamination of the “red zone” is the crucible
whereas the coating has solely an insignificant contribution. Efficiencies of up to 19.0% were achieved on 2 x 2 cm2
solar cells using mc-Si material from a block crystallized with the highly purified crucible and coating. For the
standard crucible, efficiencies of up to 18.9% were realised.
An exploratory study of the enablers, barriers and challenges of Learning Management Systems in Australia and China
Creators: name: Turnbull, Darren
Publisher: name: CQUniversity
Year: 2023
Subjects: Education systems not elsewhere classified
Educational technology and computing

description: Learning technologies play an essential role in how vocational education and training (VET) is delivered by teachers in our post-secondary institutions. The COVID-19 pandemic has exposed the benefits of integrating learning management systems (LMS) into VET institutions' teaching and learning environments. The purpose of this thesis is to examine the impact of unique educational environments on the effectiveness of LMSs from the perspectives of the two main actors in education delivery: teachers and students. Many theoretical models, such as the universal theory of the acceptance and use of technology, attempt to explain the factors that influence user engagement with technology. However, when applied to an educational context, these models do not adequately incorporate the diversity of learning conditions inherent in each individual institution of learning. This thesis addresses this gap by exploring two unique and contrasting deployments of LMSs by public VET institutions: one located in Australia and the other situated in China. By contrasting the different circumstances of technology-enhanced VET delivery in these two institutions through the lens of teachers and students, this thesis identifies the enablers, barriers, and challenges to the effective integration of LMS technology into VET delivery systems. The methodology adopted to explore these issues is a mixed methods convergent design embedded within a case study framework. Data for this study was collected from semi-structured video interviews of AVET teachers (N=11), AVET students (N=7), CVET teachers (N=7), and CVET students (N= 10); online responsive surveys distributed to AVET teachers (N=35), AVET students (N=18), and CVET students (N=107); and records of student interactions with AVET and CVET Moodle databases. This approach enabled the triangulation of the three diverse data sets (interviews, surveys, and secondary LMS data) to develop rich interpretations of LMS efficacy issues at each institution. These issues are categorised into 36 themes in nine categories. Each theme is associated with both enablers and barriers to student and teacher engagement with LMSs. There are 107 enablers and 67 barriers identified in this thesis. There are also seven challenges to LMS implementation, representing opportunities for improvement, identified in this thesis. These challenges are encapsulated in a model called the LMS Enhancement Circle that aligns the seven challenges (security, teaching, learning, content, user interface, institution, and training) to improvement recommendations that target specific attributes of the LMS environment for enhancement.
Hipposideros caffer
Creators: name: Koopman, Karl F.
Publisher: name: Zenodo
Year: 1993
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Chiroptera
Hipposideridae
Hipposideros
Hipposideros caffer

description: Hipposideros caffer (Sundevall, 1846). Ofv. Kongl. Svenska Vet.-Akad. Forhandl. Stockholm, 3(4):118. TYPE LOCALITY: South Africa, Natal, near Durban. DISTRIBUTION: Most of subsaharan Africa except the central forested region; Morocco; Yemen; Zanzibar and Pemba. SYNONYMS: angolensis, aurantiaca, bicornis, braima, gracilis, nanus, tephrus (see Hayman and Hill, 1971:29).
description: Published as part of Karl F. Koopman, 1993, Order Chiroptera, pp. 137-241 in Mammal Species of the World (2 nd Edition), Washington and London :Smithsonian Institution Press on page 171, DOI: 10.5281/zenodo.7353060
description: {"references": ["Hayman, R. W., and J. E. Hill. 1971. Order Chiroptera. Part 2. Pp. 1 - 73, in The mammals of Africa: An identification manual (J. Meester and H. W. Setzer, eds.) [issued 15 Jul 1971]. Smithsonian Institution Press, Washington, D. C., not continuously paginated."]}
Lattice Positions and Electronic Properties of Titanium in Silicon
Creators: name: Marinopoulos, A.G.
name: Coutinho, J.
name: Markevich, V.P.
name: Leonard, S.
name: Peaker, A.R.
name: Hamilton, B.
Publisher: name: WIP
Year: 2014
Subjects: WAFER-BASED SILICON SOLAR CELLS AND MATERIALS TECHNOLOGY
Silicon Feedstock, Crystallisation and Wafering

description: 29th European Photovoltaic Solar Energy Conference and Exhibition; 804-808
description: The electronic structure and electrical levels of Ti impurities in Si were studied theoretically and
experimentally. We performed calculations based on density-functional theory with an explicit treatment of
correlation among the 3d electrons of Ti. Our experiments included secondary ion mass spectroscopy (SIMS) and
deep level transient spectroscopy measurements on Czochralski (Cz)- and float-zone-grown (FZ) Si implanted with
Ti ions and annealed in the temperature range 600-900°C. Our calculations agree with earlier results concerning the
electrical levels of Ti occupying interstitial positions (Tii). Nonetheless, we find that substitutional Ti (Tis) does not
induce levels inside the gap (as previously thought) and that the intra-atomic correlation leads to electrically inert Tis.
Experimentally the electrical behavior of Ti atoms is found to be different in Cz- and FZ-Si annealed at 650°C
although the Ti SIMS profiles are similar. We argue that Tii atoms in FZ-Si react with the much more numerous
vacancies and become substitutional. No levels which could be assigned to Tis were detected, confirming the present
calculations. The differences between FZ- and Cz-Si are also explained from the calculations which predict a stronger
binding of Tii to vacancies than to interstitial oxygen atoms (which are abundant in Cz-material).
No evidence for synchronization of the solar cycle by a "clock"
Creators: name: Weisshaar, E.
name: Cameron, R. H.
name: Schüssler, M.
Publisher: name: arXiv
Year: 2023
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Space Physics (physics.space-ph)
subject: FOS: Physical sciences

description: The length of the solar activity cycle fluctuates considerably. The temporal evolution of the corresponding cycle phase, that is, the deviation of the epochs of activity minima or maxima from strict periodicity, provides relevant information concerning the physical mechanism underlying the cyclic magnetic activity. An underlying strictly periodic process (akin to a perfect "clock"), with the observer seeing a superposition of the perfect clock and a small random phase perturbation, leads to long-term phase stability in the observations. Such behavior would be expected if cycles were synchronized by tides caused by orbiting planets or by a hypothetical torsional oscillation in the solar radiative interior. Alternatively, in the absence of such synchronization, phase fluctuations accumulate and a random walk of the phase ensues, which is a typical property of randomly perturbed dynamo models. Based on the sunspot record and the reconstruction of solar cycles from cosmogenic C14, we carried out rigorous statistical tests in order to decipher whether there exists phase synchronization or random walk. Synchronization is rejected at significance levels of between 95% (28 cycles from sunspot data) and beyond 99% (84 cycles reconstructed from C14, while the existence of random walk in the phases is consistent with all data sets. This result strongly supports randomly perturbed dynamo models with little inter-cycle memory.
description: Astronomy & Astrophysics, in press
Opto-mechanical system for the controlled growth of granular piles
Creators: name: Dominguez-Rubio, Leonanro
name: Martinez, Etien
name: Altshuler, Ernesto
Publisher: name: arXiv
Year: 2015
Subjects: subject: Soft Condensed Matter (cond-mat.soft)
subject: FOS: Physical sciences

description: The formation of sandpiles is a subject if interest in the field of granular matter, but most experiments are unable to control the kinetic energy of the grains added to the apex of the growing pile. In this short article, we describe an opto-mechanical system to grow granular piles by adding sand from a fixed distance above the apex of the pile. To achieve that, we use a laser beam that detects the position of the apex and, as the pile grows, sends a feedback signal to a mechanical device able to control the height of the sand delivey system above the pile.
description: in Spanish
Antivirals in patients hospitalised with influenza and/or its complications (APHIC)
Creators: name: Kainer, Marion A. .
Publisher: name: Monash University
Year: 2022

description: This thesis was scanned from the print manuscript for digital preservation and is copyright the author.
 Researchers can access this thesis by asking their local university, institution or public library to
 make a request on their behalf. Monash staff and postgraduate students can use the link in the References field.
Telesme: Reflective Compression and the Architecture of Poetic Silence
Creators: name: Yasui, Yuji
Publisher: name: Zenodo
Year: 2025
Subjects: subject: semantic compression
subject: poetic summarization
subject: reflective AI
subject: narrative architecture
subject: symbolic retention
subject: multi-persona systems
subject: GPT-4
subject: Artificial intelligence
subject: Artificial Intelligence
subject: Digital humanities
subject: Computational Linguistics
subject: non-Neumann computation
subject: language model evaluation
subject: Literary theory
subject: poetic AI
subject: reflective systems
subject: prompt engineering
subject: Lumiora
subject: Telesme
subject: symbolic memory

description: This paper introduces Telesme, a novel semantic compression architecture that redefines summarization through poetic logic, symbolic recursion, and reflective fidelity. Unlike conventional compression models that prioritize token reduction, Telesme retains metaphor, emotional contour, and structural layering using its own internal criteria.

Telesme is built upon a multi-module system that includes components such as GhostLink, FractalWeaver, and EmoTraceCore, and operates through a pre-output recursive loop to achieve semantic equilibrium. The evaluation framework is based on the original T/P/E/S axis (Structure, Poetic Symbolism, Emotional Contour, Semantic Fidelity), offering a multidimensional approach to text generation quality.

The paper includes detailed comparisons between GPT-4o and Telesme outputs across four literary works (Sōseki, Kajiī, Shakespeare, Dickinson), demonstrating superior symbolic retention and poetic depth. The theory of **Inverted Compression** is also proposed, suggesting that what is omitted in language may still shape narrative form and emotional resonance.

Co-authored by Yuji Yasui and a multi-persona cognitive architecture known as Paracortex (see Chapter 10), this work is both a technical report and a philosophical intervention into how language models understand—and forget—meaning.Version 2, Telesme 0.8.9α (Telesme v0.8.9α.md) and Telesmist v1.0 β3 (Telesmist v1.0 β3.md) added

**Version 2 Update**  This version includes two additional files that document the inner architecture of Telesme and the auxiliary system that enables its construction and control:

Telesme v0.8.9α – The core reflective compression engine that reorganizes meaning through poetic recursion and symbolic trace preservation.

Telesmist v1.0 β3 – An external semantic transpiler designed to construct and configure Telesme remotely, especially in environments (such as Lumiora) where direct structural manipulation is restricted. Telesmist enables reflective editing of Telesme from an isolated semantic layer.

These additions clarify not only the internal architecture of Telesme but also the external mechanism by which it can be instantiated, modified, and directed through symbolic abstraction.

 

DOI of related project: [10.5281/zenodo.15125344](https://doi.org/10.5281/zenodo.15125344)
Quantification of LID in Multicrystalline Silicon Wafers
Creators: name: Søndenå, R.
name: Ghaderi, A.
Publisher: name: WIP
Year: 2014
Subjects: WAFER-BASED SILICON SOLAR CELLS AND MATERIALS TECHNOLOGY
Silicon Feedstock, Crystallisation and Wafering

description: 29th European Photovoltaic Solar Energy Conference and Exhibition; 776-779
description: Light induced degradation occurs in p-type silicon solar cells containing both boron and oxygen. Due to fundamental
differences in the solidification processes multicrystalline silicon contains less oxygen than Czochralski silicon. The
oxygen content in multicrystalline silicon is still sufficient to cause degradation, although to a lesser extent than in
Czochralski silicon. Extended crystal defects such as grain boundaries and dislocations have long been considered the
main factors limiting the performance of multicrystalline silicon solar cells. However, as the detrimental effects of these
extended crystal defects are reduced due to improvements in the solidification process as well as the feedstock and
crucible quality, the effect of boron-oxygen related degradation is expected to be of increasing importance. Grain
boundaries and dislocation clusters contribute to considerable spatial variations in minority carrier lifetimes across a
wafer. Challenges with separating and quantifying the different lifetime limiting effects in multicrystalline silicon are
discussed in this work.
Cosmic metal invaders: Intergalactic OVII as a tracer of the warm-hot intergalactic medium within cosmic filaments in the EAGLE simulation
Creators: name: Tuominen, T.
name: Nevalainen, J.
name: Heinämäki, P.
name: Tempel, E.
name: Wijers, N.
name: Bonamente, M.
name: Aragon-Calvo, M. A.
name: Finoguenov, A.
Publisher: name: arXiv
Year: 2023
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: The current observational status of the hot (log T(K) > 5.5) warm-hot intergalactic medium (WHIM) remains incomplete. While recent observations from stacking large numbers of Cosmic Web filaments have yielded statistically significant detections, direct measurements of single objects remain scarce. The lack of such a sample currently prevents a robust analysis of the cosmic baryon content composed of the hot WHIM, which could help solve the cosmological missing baryons problem. To improve the search for the missing baryons, we used the EAGLE simulation. Our aim is to understand the metal enrichment and distribution of highly ionised metals in the Cosmic Web. We detected the filaments by applying the Bisous formalism to the simulated galaxies, and characterised the spatial distributions as well as mass and volume fractions of the filamentary oxygen and OVII. We then constructed OVII column density maps and determined their detectability with Athena X-IFU. However, the oxygen and OVII number densities drop fast beyond the virial radii of haloes, falling below detectable levels at 700 kpc. Thus, only ~1% of the filament volumes are filled with OVII at detectable densities. This non-homogeneous distribution of the OVII complicates its usage for tracing the missing baryons. Instead, OVII forms narrow envelopes around haloes. This localised nature results in a low chance (10-20% per sight line) of detecting intergalactic OVII with Athena X-IFU within the SDSS catalogue of filaments. With future filament samples from the 4MOST survey, the chances increase up to a level of ~50%. Nonetheless, based on EAGLE results, this would not be enough to conclusively solve the missing baryon problem, as it would be limited to a few times the virial radii of haloes. Fortunately, the volumes around haloes are dense in hot WHIM, and tracing it could reduce the content of baryons still missing by ~25%.
description: 17 pages, 13 figures, accepted for publication in Astronomy and Astrophysics. For associated video, see https://youtu.be/878twggEFoY
Computation of the magnetostatic interaction between linearly magnetized polyhedrons
Creators: name: Chernyshenko, Dmitri
name: Fangohr, Hans
Publisher: name: arXiv
Year: 2016
Subjects: subject: Computational Physics (physics.comp-ph)
subject: FOS: Physical sciences

description: In this paper we present a method to accurately compute the energy of the magnetostatic interaction between linearly (or uniformly, as a special case) magnetized polyhedrons. The method has applications in finite element micromagnetics, or more generally in computing the magnetostatic interaction when the magnetization is represented using the finite element method (FEM). The magnetostatic energy is described by a six-fold integral that is singular when the interaction regions overlap, making direct numerical evaluation problematic. To resolve the singularity, we evaluate four of the six iterated integrals analytically resulting in a 2d integral over the surface of a polyhedron, which is nonsingular and can be integrated numerically. This provides a more accurate and efficient way of computing the magnetostatic energy integral compared to existing approaches. The method was developed to facilitate the evaluation of the demagnetizing interaction between neighouring elements in finite-element micromagnetics and provides a possibility to compute the demagnetizing field using efficient fast multipole or tree code algorithms.
Telesme: Reflective Compression and the Architecture of Poetic Silence
Creators: name: Yuji, Yasui
Publisher: name: Zenodo
Year: 2025
Subjects: subject: semantic compression
subject: poetic summarization
subject: reflective AI
subject: narrative architecture
subject: symbolic retention
subject: multi-persona systems
subject: GPT-4
subject: Artificial intelligence
subject: Artificial Intelligence
subject: Digital humanities
subject: Computational Linguistics
subject: non-Neumann computation
subject: language model evaluation
subject: Literary theory
subject: poetic AI
subject: reflective systems
subject: prompt engineering
subject: Lumiora
subject: Telesme
subject: symbolic memory

description: This paper introduces Telesme, a novel semantic compression architecture that redefines summarization through poetic logic, symbolic recursion, and reflective fidelity. Unlike conventional compression models that prioritize token reduction, Telesme retains metaphor, emotional contour, and structural layering using its own internal criteria.

Telesme is built upon a multi-module system that includes components such as GhostLink, FractalWeaver, and EmoTraceCore, and operates through a pre-output recursive loop to achieve semantic equilibrium. The evaluation framework is based on the original T/P/E/S axis (Structure, Poetic Symbolism, Emotional Contour, Semantic Fidelity), offering a multidimensional approach to text generation quality.

The paper includes detailed comparisons between GPT-4o and Telesme outputs across four literary works (Sōseki, Kajiī, Shakespeare, Dickinson), demonstrating superior symbolic retention and poetic depth. The theory of **Inverted Compression** is also proposed, suggesting that what is omitted in language may still shape narrative form and emotional resonance.

Co-authored by Yuji Yasui and a multi-persona cognitive architecture known as Paracortex (see Chapter 10), this work is both a technical report and a philosophical intervention into how language models understand—and forget—meaning.

DOI of related project: [10.5281/zenodo.15125344](https://doi.org/10.5281/zenodo.15125344)
Hipposideros calcaratus
Creators: name: Koopman, Karl F.
Publisher: name: Zenodo
Year: 1993
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Chiroptera
Hipposideridae
Hipposideros
Hipposideros calcaratus

description: Hipposideros calcaratus (Dobson, 1877). Proc. Zool. Soc. Lond., 1877:122. TYPE LOCALITY: Papua New Guinea, Bismarck Archipelago, Duke of York Isl. DISTRIBUTION: New Guinea, Bismarck Arch., Solomon Isis, adjacent small islands. SYNONYMS: cupidus. COMMENTS: Includes cupidus; see Smith and Hill (1981:8).
description: Published as part of Karl F. Koopman, 1993, Order Chiroptera, pp. 137-241 in Mammal Species of the World (2 nd Edition), Washington and London :Smithsonian Institution Press on page 171, DOI: 10.5281/zenodo.7353060
description: {"references": ["Smith, J. D., and J. E. Hill. 1981. A new species and subspecies of bat of the Hipposideros bicolor-group from Papua New Guinea and the systematic status of Hipposideros calcaratus and Hipposideros cupidus (Mammalia: Chiroptera: Hipposideridae). Contributions in Science, Natural History Museum of Los Angeles County, 331: 1 - 19."]}
Tricritical point in the quantum Hamiltonian mean-field model
Creators: name: Schmid, Harald
name: Dieplinger, Johannes
name: Solfanelli, Andrea
name: Succi, Sauro
name: Ruffo, Stefano
Publisher: name: Universität Regensburg
Year: 2022
Subjects: subject: 530 Physik

description: Engineering long-range interactions in experimental platforms has been achieved with great success in a large variety of quantum systems in recent years. Inspired by this progress, we propose a generalization of the classical Hamiltonian mean-field model to fermionic particles. We study the phase diagram and thermodynamic properties of the model in the canonical ensemble for ferromagnetic interactions as a function of temperature and hopping. At zero temperature, small charge fluctuations drive the many-body system through a first order quantum phase transition from an ordered to a disordered phase at zero temperature. At higher temperatures, the fluctuation-induced phase transition remains first order initially and switches to second order only at a tricritical point. Our results offer an intriguing example of tricriticality in a quantum system with long-range couplings, which bears direct experimental relevance. The analysis is performed by exact diagonalization and mean-field theory.
Novel Texturing Method to Remove Amorphous Silicon on Diamond Wire Sawn Wafers Surfaces
Creators: name: Srinivas, G.R.
name: Saptaji, K.
name: Subbiah, S.
name: Zarepour, H.
name: Butler, D.
Publisher: name: WIP
Year: 2014
Subjects: WAFER-BASED SILICON SOLAR CELLS AND MATERIALS TECHNOLOGY
Silicon Feedstock, Crystallisation and Wafering

description: 29th European Photovoltaic Solar Energy Conference and Exhibition; 809-811
description: Literature study has shown that it is not possible to obtain the required surface morphology in the
diamond wire sawn wafers by using the existing wet etching protocols due to the presence of the masking agentamorphous
phase silicon. Therefore, it is important to etch away amorphous phase to acquire the required texture on
the wafer surface. This study focuses on the removal of the amorphous phase on the diamond wire sawn wafers by
proposing a new etching recipe that consists of potassium hydroxide (KOH) etching followed by improving the light
absorption using acidic etching. Raman spectra results show that wafer samples etched using KOH for more than 60
sec consist mainly of crystalline phases with no presence of amorphous phase. The light reflection of the sawn wafer
etched using the proposed isotropic acidic etching following KOH etching is the lowest compared to the as-cut, 120
sec etched by KOH, and etched by Buffered Oxide Etching (BOE). In this study, we have successfully removed the
amorphous phase and improved the light absorption of the diamond wire sawn wafers using the proposed recipe of
KOH etching for 120 sec followed by isotropic acidic etching with 70% hydrofluoric acid (HF) content in the
mixture.
Texture of average solar photospheric flows and the donut-like pattern
Creators: name: Roudier, T.
name: Ballot, J.
name: Malherbe, J. M.
name: Chane-Yook, M.
Publisher: name: arXiv
Year: 2023
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences
subject: 85-11

description: Detailed knowledge of surface dynamics is one of the key points in understanding magnetic solar activity. The motions of the solar surface, to which we have direct access via the observations, tell us about the interaction between the emerging magnetic field and the turbulent fields. The flows computed with the coherent structure tracking (CST) technique on the whole surface of the Sun allow for the texture of the velocity modulus to be analyzed and for one to locate the largest horizontal flows and determine their organization. The velocity modulus maps show structures more or less circular and closedwhich are visible at all latitudes; here they are referred to as donuts. They reflect the most active convective cells associated with supergranulation. These annular flows are not necessarily joined as would seem to indicate the divergence maps. The donuts have identical properties (amplitude, shape, inclination, etc.) regardless of their position on the Sun. The kinematic simulation of the donuts' outflow applied to passive scalar (corks) indicates the preponderant action of the selected donuts which are, from our analysis, one of the major actors for the magnetic field diffusion on the quiet Sun. The absence of donuts in the magnetized areas (plages) indicates the action of the magnetic field on the strongest supergranular flows and thus modifies the diffusion of the magnetic field in that location. The detection of the donuts is a way to locate in the quiet Sun the vortex and the link with the jet, blinkers, coronal bright points (campfires), or other physical structures. Likewise, the study of the influence of donuts on the evolution of active events, such as the destruction of sunspots, filament eruptions, and their influences on upper layers via spicules and jets, could be done more efficiently via the detection of that structures.
description: 14 pages, 17 figures
Daily variability of Ceres' Albedo detected by means of radial velocities changes of the reflected sunlight
Creators: name: Molaro, P.
name: Lanza, A. F.
name: Monaco, L.
name: Tosi, F.
name: Curto, G. Lo
name: Fulle, M.
name: Pasquini, L.
Publisher: name: arXiv
Year: 2016
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: Bright features have been recently discovered by Dawn on Ceres, which extend previous photometric and Space Telescope observations. These features should produce distortions of the line profiles of the reflected solar spectrum and therefore an apparent radial velocity variation modulated by the rotation of the dwarf planet. Here we report on two sequences of observations of Ceres performed in the nights of 31 July, 26-27 August 2015 by means of the high-precision HARPS spectrograph at the 3.6-m La Silla ESO telescope. The observations revealed a quite complex behaviour which likely combines a radial velocity modulation due to the rotation with an amplitude of approx +/- 6 m/s and an unexpected diurnal effect. The latter changes imply changes in the albedo of Occator's bright features due to the blaze produced by the exposure to solar radiation. The short-term variability of Ceres' albedo is on timescales ranging from hours to months and can both be confirmed and followed by means of dedicated radial velocity observations.
description: 5 pag, 1fig, two tables, MNRAS Letters 2016
Aspects of morphine compliance in patients self-dosing for cancer pain control
Creators: name: O'Connor, Lera.
Publisher: name: Monash University
Year: 2022

description: This thesis was scanned from the print manuscript for digital preservation and is copyright the author.
 Researchers can access this thesis by asking their local university, institution or public library to
 make a request on their behalf. Monash staff and postgraduate students can use the link in the References field.
Hipposideros camerunensis Eisentraut 1956
Creators: name: Koopman, Karl F.
Publisher: name: Zenodo
Year: 1993
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Chiroptera
Hipposideridae
Hipposideros
Hipposideros camerunensis

description: Hipposideros camerunensis Eisentraut, 1956. Zool. Jahrb. Abt. Syst. Oekol. Geogr. Tiere, 84:526. TYPE LOCALITY: Cameroon, near Buea. DISTRIBUTION: Cameroon, E Zaire, W Kenya.
description: Published as part of Karl F. Koopman, 1993, Order Chiroptera, pp. 137-241 in Mammal Species of the World (2 nd Edition), Washington and London :Smithsonian Institution Press on page 171, DOI: 10.5281/zenodo.7353060
Relationship between Macro and Micro-Scale Mechanical Properties of Photovoltaic Silicon Wafers
Creators: name: Kumar, A.
name: Yang, C.
name: Melkote, S.N.
name: Danyluk, S.
Publisher: name: WIP
Year: 2014
Subjects: WAFER-BASED SILICON SOLAR CELLS AND MATERIALS TECHNOLOGY
Silicon Feedstock, Crystallisation and Wafering

description: 29th European Photovoltaic Solar Energy Conference and Exhibition; 769-772
description: It is well-known that mechanical failure of photovoltaic (PV) silicon wafers is intimately influenced by
the local or micro-scale properties of the wafers. While a number of studies on the overall mechanical strength of PV
silicon wafers have been reported, investigations of possible correlation between the micro-scale/local properties (e.g.
local fracture toughness) and wafer scale mechanical properties (e.g. wafer fracture strength) are lacking. This paper
examines the possible correlation between local fracture toughness and the overall wafer fracture strength of multicrystalline
silicon (mc-Si) wafers evaluated using four-line bending tests. It is observed that wafer coupons with
higher local fracture toughness exhibit higher fracture strengths. This correlation is explained through analysis of
dislocation etch pit density. Specifically, the higher local fracture toughness is found to be correlated with higher
dislocation etch pitch density.
IIB matrix model, bosonic master field, and emergent spacetime
Creators: name: Klinkhamer, F. R.
Publisher: name: Scuola Internazionale Superiore di Studi Avanzati (SISSA)
Year: 2022

description: The IIB matrix model has been suggested as a particular formulation of nonperturbative superstring theory (M-theory). It has now been realized that an emerging classical spacetime may reside in its large-$N$ master field. This bosonic master field can, in principle, give rise to Minkowski and Robertson-Walker spacetimes. The outstanding task is to solve the bosonic master-field equation, which is essentially an algebraic equation. In this article, we present new results for the $(D,N)=(10,4)$ bosonic master-field equation of the IIB matrix model, where $D$ is the number of bosonic matrices and $N$ the matrix size. We also give, in a self contained appendix, explicit results for critical points of the effective bosonic action. The main physics application of the (dimensionless) IIB matrix model may be in providing a (conformal) phase that replaces the Friedmann big bang singularity.
Ammonia mapping observations of the Galactic infrared bubble N49: Three NH$_3$ clumps along the molecular filament
Creators: name: Kohno, Mikito
name: Chibueze, James O.
name: Burns, Ross A.
name: Omodaka, Toshihiro
name: Handa, Toshihiro
name: Murase, Takeru
name: Yamada, Rin I.
name: Nagayama, Takumi
name: Nakano, Makoto
name: Sunada, Kazuyoshi
name: Tachihara, Kengo
name: Fukui, Yasuo
Publisher: name: arXiv
Year: 2023
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We have carried out the NH$_3$ $(J,K)=(1,1),(2,2),$ and $(3,3)$ mapping observations toward the Galactic infrared bubble N49 (G28.83-0.25) using the Nobeyama 45 m telescope. Three NH$_3$ clumps (A, B, and C) were discovered along the molecular filament with the radial velocities of $\sim$ 96, 87, and 89 km s$^{-1}$, respectively. The kinetic temperature derived from the NH$_3$ (2,2)/NH$_3$ (1,1) shows $T_{\rm kin} = 27.0 \pm 0.6$ K enhanced at Clump B in the eastern edge of the bubble, where position coincides with massive young stellar objects (MYSOs) associated with the 6.7 GHz class II methanol maser source. This result shows the dense clump is locally heated by stellar feedback from the embedded MYSOs. The NH$_3$ Clump B also exists at the 88 km s$^{-1}$ and 95 km s$^{-1}$ molecular filament intersection. We therefore suggest that the NH$_3$ dense gas formation in Clump B can be explained by a filament-filament interaction scenario. On the other hand, NH$_3$ Clump A and C at the northern and southern side of the molecular filament might be the sites of spontaneous star formation because these clumps are located $\sim$5$-$10 pc away from the edge of the bubble.
description: 29 pages, 13 figures, 3 tables, accepted for Publications of the Astronomical Society of Japan (PASJ)