cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Lacticaseibacillus Zheng & Wittouck & Salvetti & Franz & Harris & Mattarelli & O'Toole & Pot & Vandamme & Walter & Watanabe & Wuyts & Felis & Gänzle & Lebeer 2020, GEN. NOV.
Creators: name: Zheng, Jinshui
name: Wittouck, Stijn
name: Salvetti, Elisa
name: Franz, Charles M. A. P.
name: Harris, Hugh M. B.
name: Mattarelli, Paola
name: O'Toole, Paul W.
name: Pot, Bruno
name: Vandamme, Peter
name: Walter, Jens
name: Watanabe, Koichi
name: Wuyts, Sander
name: Felis, Giovanna E.
name: Gänzle, Michael G.
name: Lebeer, Sarah
Publisher: name: Zenodo
Year: 2020
Subjects: Biodiversity
Taxonomy
Bacteria
Firmicutes
Bacilli
Lactobacillales
Lactobacillaceae
Lacticaseibacillus

description: DESCRIPTIONOF LACTICASEIBACILLUS GEN. NOV.
Lacticaseibacillus (Lac.ti.ca.se.i.ba.cil'lus. L. neut. n. lac milk; L. n. caseus cheese, referring to the casei-group lactobacilli; L. masc. n. bacillus a rod; N.L. masc. n. Lacticaseibacillus a milk-derived rodlet from the [Lactobacillus] casei group).
Strains of Lacticaseibacillus are homofermentative; some but not all species metabolise pentoses via the phosphoketolase pathway. The mol % G+C content of DNA is between 46 and 58.0. The genome size ranges from 1.93 to 3.14 Mbp. Strains are non-motile, oxidase negative, often producing D(−)- and L(+)-lactic acid from glucose. The temperature range for growth is variable, but never below 10 °C and never above 45 °C. One subspecies survives 70 °C for 40 s. Lys–D-Asp is the most common type of the peptidoglycan. The genus has considerable economic importance as it harbours several species thatare used as starter cultures indairy fermentations and as probiotics [58, 59].
Aphylogenetic tree on the basis of 16S rRNA genes of all species in the genus Lacticaseibacillus is provided in Fig. S6F.
The type species is Lacticaseibacillus casei comb. nov.; Lacticaseibacillus was previously referred to as L. casei group.
description: Published as part of Zheng, Jinshui, Wittouck, Stijn, Salvetti, Elisa, Franz, Charles M. A. P., Harris, Hugh M. B., Mattarelli, Paola, O'Toole, Paul W., Pot, Bruno, Vandamme, Peter, Walter, Jens, Watanabe, Koichi, Wuyts, Sander, Felis, Giovanna E., Gänzle, Michael G. & Lebeer, Sarah, 2020, A taxonomic note on the genus Lactobacillus: Description of 23 novel genera, emended description of the genus Lactobacillus Beijerinck 1901, and union of Lactobacillaceae and Leuconostocaceae, pp. 2782-2858 in International Journal of Systematic and Evolutionary Microbiology 70 on page 2811, DOI: 10.1099/ijsem.0.004107, http://zenodo.org/record/4730536
Steatomys jacksoni Hayman 1936
Creators: name: Musser, Guy G.
name: Carleton, Michael D.
Publisher: name: Zenodo
Year: 1993
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Rodentia
Muridae
Steatomys
Steatomys jacksoni

description: Steatomys jacksoni Hayman, 1936. Proc. Zool. Soc. Lond., 1935:930 [1936]. TYPE LOCALITY: Ghana, Ashanti, Wenchi. DISTRIBUTION: Known only from type locality and SW Nigeria. COMMENTS: This species was known only by the holotype, but a few specimens have been recorded from SW Nigeria (Anadu, 1979), and earlier Rosevear (1969) had suggested that two young animals from Wulehe, Togo, might be examples of S. jacksoni. Included in S. pratensis by Coetzee (1977a), but retained as a species by Swanepoel and Schütter (1978), who preferred to recognize it until significance of the diagnostic character (size and shape of interparietal) could be assessed by additional specimens.
description: Published as part of Guy G. Musser & Michael D. Carleton, 1993, Order Rodentia - Family Muridae, pp. 501-755 in Mammal Species of the World (2 nd Edition), Washington and London :Smithsonian Institution Press on page 545, DOI: 10.5281/zenodo.7353098
description: {"references": ["Anadu, P. A. 1979. The occurrence of Steatomys jacksoni Hayman in south-western Nigeria. Acta Theriologica, 24: 513 - 526.", "Rosevear, D. R. 1969. The rodents of West Africa. Trustees of the British Museum (Natural History), London, 677: 1 - 604.", "Coetzee, C. G. 1977 a. Genus Steatomys. Part 6.8. Pp. 1 - 4, in The mammals of Africa: An identification manual (J. Meester and H. W. Setzer, eds.) [issued 22 Aug 1977]. Smithsonian Institution Press, Washington, D. C., not continuously paginated."]}
DEMO Hot Cell and Ex-Vessel Remote Handling
Creators: name: Thomas, Justin
name: Loving, Antony
name: Bachmann, Christian
name: Harman, Jon
Publisher: name: arXiv
Year: 2013
Subjects: subject: Plasma Physics (physics.plasm-ph)
subject: Instrumentation and Detectors (physics.ins-det)
subject: FOS: Physical sciences

description: In Europe the work on the specification and design of a Demonstration Power Plant (DEMO) is being carried out by EFDA in the Power Plant Physics and Technology (PPP&T) programme. DEMO will take fusion from experimental research into showing the potential for commercial power generation. This paper describes the first steps being taken towards the design of the DEMO Hot Cell. It will show a comparison of the current DEMO in-vessel maintenance concepts from a Hot Cell perspective, describe a proposed ex-vessel transport system, and summarize the facilities that have been identified as required within the Hot Cell, examine current RH technology and discuss the identified critical development issues.
description: 4 pages, 7 figures
Synthetic magnetism for solitons in optomechanical array
Creators: name: Djorwé, P.
name: Alphonse, H.
name: Abbagari, S.
name: Doka, S. Y.
name: Engo, S. G. Nana
Publisher: name: arXiv
Year: 2023
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: Optics (physics.optics)
subject: FOS: Physical sciences

description: We propose a synthetic magnetism to generate and to control solitonic waves in $\rm{1D}-$optomechanical array. Each optomechanical cavity in the array couples to its neighbors through photon and phonon coupling. We create the synthetic magnetism by modulating the phonon hopping rate through a modulation frequency, and a modulation phase between resonators at different sites. When the synthetic magnetism effect is not taken into account, the mechanical coupling play a scrucial role of controlling and switching the waves from bright to dark solitons, and it even induces rogue wave-like a shape in the array. For enough mechanical coupling strength, the system enters into a strong coupling regime through splitting/crossing of solitonic waves leading to multiple waves propagation in the array. Under the synthetic magnetism effect, the phase of the modulation enables a good control of the wave propagation, and it also switches soliton shape from bright to dark, and even induces rogue waves as well. Similarly to the mechanical coupling, the synthetic magnetism offers another flexible way to generate plethora of solitonic waves for specific purposes. This work opens new avenues for optomechanical platforms and sheets light on their potentiality of controlling and switching solitonic waves based on synthetic magnetism.
description: 6 pages, 6 figures
Bringing Rubin to the world: Education & Public Outreach and Citizen Science
Creators: name: Higgs, Clare
Publisher: name: Zenodo
Year: 2024

description: Slides presenting the Rubin Education and Public Outreach team's current and planned activities, including a more in depth look at citizen science. I present the resources under developement to support the creation and maintainence of citizen science projects using Rubin data.
A new estimate of the difference among quasi-arithmetic means
Creators: name: Pasteczka, Paweł
Publisher: name: arXiv
Year: 2013
Subjects: subject: Classical Analysis and ODEs (math.CA)
subject: FOS: Mathematics
subject: 26E60, 26D15, 26D07

description: In the 1960s Cargo and Shisha proved some majorizations for the distance among quasi-arithmetic means (defined as f^{-1}(\sum_{i=1}^{n} w_i f(a_i) for any continuous, strictly monotone function f:I->R, where I is an interval, and a=(a_1,...,a_n) is a vector with entries in I, w=(w_1,...,w_n) is a sequence of corresponding weights w_i>0, w_1+...+w_n=1). Nearly thirty years later, in 1991, Pàles presented an iff condition for a sequence of quasi-arithmetic means to converge to another QA mean. It was closely related with the three parameters' operator (f(x)-f(z))/(f(x)-f(y)). The author presented recently an estimate for the distance among such quasi-arithmetic means whose underlying functions satisfy some smoothness conditions. Used was the operator f -> f''/f' introduced in the 1940s by Mikusiński and Łojasiewicz. It is natural to look for similar estimate(s) in the case of the underlying functions not being smooth. For instance, by the way of using Pàles' operator. This is done in the present note. Moreover, the result strengthens author's earlier estimates.
description: 7 pages
Steatomys krebsii Peters 1852
Creators: name: Musser, Guy G.
name: Carleton, Michael D.
Publisher: name: Zenodo
Year: 1993
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Rodentia
Muridae
Steatomys
Steatomys krebsii

description: Steatomys krebsii Peters, 1852. Reise nach Mossambique, Säugethiere, p. 165. TYPE LOCALITY: South Africa, Kaffraria. DISTRIBUTION: S Angola, W Zambia, NE and SE Botswana, Caprivi Strip, and South Africa (W, N, E Cape Province, NW Natal, N Orange Free State, S and SW Transvaal); see map in Skinner and Smithers (1990). SYNONYMS: angolensis, bensoni, bradleyi, chiversi, leucorhynchus, mariae, orangiae, pentonyx, transvaalensis. COMMENTS: Reviewed by Ansell (1978).
description: Published as part of Guy G. Musser & Michael D. Carleton, 1993, Order Rodentia - Family Muridae, pp. 501-755 in Mammal Species of the World (2 nd Edition), Washington and London :Smithsonian Institution Press on pages 545-546, DOI: 10.5281/zenodo.7353098
description: {"references": ["Skinner, J. D., and R. H. N. Smithers. 1990. The mammals of the southern African subregion. Second ed. University of Pretoria, Republic of South Africa, 771 pp.", "Ansell, W. F. H. 1978. The mammals of Zambia. National Parks and Wildlife Service, Chilanga, 126 pp."]}
Application of Coherent Microwave Scattering and Multiphoton Ionization for Diagnostics of Electric Propulsion Systems
Creators: name: Patel, Adam R.
name: Karunarathne, Sashin L. B.
name: Babusis, Nicholas
name: Shashurin, Alexey
Publisher: name: arXiv
Year: 2023
Subjects: subject: Plasma Physics (physics.plasm-ph)
subject: FOS: Physical sciences

description: Nonintrusive measurements of plasma properties are essential to evaluate, and numerically simulate, the in-flight performance of electric propulsion systems. As a logical first step in the development of new diagnostic techniques, this work depicts the implementation of multiphoton ionization and coherent microwave scattering (MPI-CMS) in a gridded-ion accelerator operating on rare gases. Presented studies primarily comprise photoionization spectroscopy of ground and excited state-populations of both neutrals and ions supplemented by optical emission spectroscopy and Langmuir probe derived plume properties. Results suggest the potential of MPI-CMS for non-intrusive measurements of specie number densities.
Steatomys parvus Rhoads 1896
Creators: name: Musser, Guy G.
name: Carleton, Michael D.
Publisher: name: Zenodo
Year: 1993
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Rodentia
Muridae
Steatomys
Steatomys parvus

description: Steatomys parvus Rhoads, 1896. Proc. Acad. Nat. Sci. Philadelphia, p. 529. TYPE LOCALITY: Ethiopia, Lake Rudolf, Rusia. DISTRIBUTION: South Africa (N Natal, Zululand), N Botswana, NW Zimbabwe, N Namibia, Angola, Zambia, Tanzania, Kenya, Uganda, Somalia, S Sudan, and S Ethiopia. SYNONYMS: aquilo, athi, kalaharicus, loveridgei, minutus, swalius, thomasi, tongensis, umbratus. COMMENTS: The single Ethiopian record was listed as S. pratensis by Yalden et al. (1976).
description: Published as part of Guy G. Musser & Michael D. Carleton, 1993, Order Rodentia - Family Muridae, pp. 501-755 in Mammal Species of the World (2 nd Edition), Washington and London :Smithsonian Institution Press on page 546, DOI: 10.5281/zenodo.7353098
description: {"references": ["Yalden, D. W., M. J. Largen, and D. Kock. 1976. Catalogue of the mammals of Ethiopia. 2. Insectivora and Rodentia. Monitore Zoologico Italiano, Supplemento 8 (1): 1 - 118."]}
Growth of $α-Ga_2O_3$ on $Al_2O_3$ by conventional molecular-beam epitaxy and metal-oxide-catalyzed epitaxy
Creators: name: McCandless, J. P.
name: Rowe, D.
name: Pieczulewski, N.
name: Protasenko, V.
name: Alonso-Orts, M.
name: Williams, M. S.
name: Eickhoff, M.
name: Xing, H. G.
name: Muller, D. A.
name: Jena, D.
name: Vogt, P.
Publisher: name: arXiv
Year: 2023
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: We report the growth of $α-Ga_2O_3$ on $m$-plane $Al_2O_3$ by conventional plasma-assisted molecular-beam epitaxy (MBE) and In-mediated metal-oxide-catalyzed epitaxy (MOCATAXY). We report a growth-rate-diagram for $α-Ga_2O_3$ (10-10), and observe (i) a growth rate increase, (ii) an expanded growth window, and (iii) reduced out-of-lane mosaic spread when MOCATAXY is employed for the growth of $α-Ga_2O_3$. Through the use of In-mediated catalysis, growth rates over $0.2\,μ\text{m}\,\text{hr}^{-1}$ and rocking curves with full width at half maxima of $Δω\approx 0.45^{\circ}$ are achieved. Faceting is observed along the $α-Ga_2O_3$ film surface and is explored through scanning transmission electron microscopy.
Polarisation Leakage due to Errors in Track Reconstruction in Gas Pixel Detectors
Creators: name: Bucciantini, N.
name: Di Lalla, N.
name: Romani, R. W. R.
name: Silvestri, S.
name: Negro, M.
name: Baldini, L.
name: Tennant, A. F.
name: Manfreda, A.
Publisher: name: arXiv
Year: 2023
Subjects: subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: X-ray polarimetry, based on Gas Pixel Detectors (GPDs), have reached a high level of maturity with the Imaging X-ray Polarimeter Explorer (IXPE) leading to the first ever spatially resolved polarimetric measures. However, being this a new technique, a few unexpected effect have emerged during in flight operations. In particular it was almost immediately found that on-board unpolarized calibration sources were showing radially polarized halos. The origin of this features was recognized in a correlation between the error in reconstructing the absorption point of the X-ray photon and the direction of its electric field vector. Here we present and discuss in detail this effect, showing that it is possible to provide a simple and robust mathematical formalism to handle it. We further show its role and relevance for the recent IXPE measures, and for the use of GPD-based techniques in general, and illustrate how to model it in the study of extended sources.
description: 19 pages, 10 figures, to be published in A&A
Steatomys pratensis Peters 1846
Creators: name: Musser, Guy G.
name: Carleton, Michael D.
Publisher: name: Zenodo
Year: 1993
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Rodentia
Muridae
Steatomys
Steatomys pratensis

description: Steatomys pratensis Peters, 1846. Bericht Verhandl. K. Preuss. Akad. Wiss. Berlin, 11:258. TYPE LOCALITY: Mozambique, Zambezi River, Tete. DISTRIBUTION: South Africa (Natal, Zululand, Transvaal), Swaziland, Mozambique, Zimbabwe, N Botswana, NE and N Namibia, N Malawi, Zambia, Angola, Zaire, SW Sudan and west to Cameroon. SYNONYMS: bocagei, edulis, gazellae, kasaicus, maunensis, natalensis, nyasae, opimus.
description: Published as part of Guy G. Musser & Michael D. Carleton, 1993, Order Rodentia - Family Muridae, pp. 501-755 in Mammal Species of the World (2 nd Edition), Washington and London :Smithsonian Institution Press on page 546, DOI: 10.5281/zenodo.7353098
Lacticaseibacillus casei Zheng & Wittouck & Salvetti & Franz & Harris & Mattarelli & O'Toole & Pot & Vandamme & Walter & Watanabe & Wuyts & Felis & Gänzle & Lebeer 2020, COMB. NOV.
Creators: name: Zheng, Jinshui
name: Wittouck, Stijn
name: Salvetti, Elisa
name: Franz, Charles M. A. P.
name: Harris, Hugh M. B.
name: Mattarelli, Paola
name: O'Toole, Paul W.
name: Pot, Bruno
name: Vandamme, Peter
name: Walter, Jens
name: Watanabe, Koichi
name: Wuyts, Sander
name: Felis, Giovanna E.
name: Gänzle, Michael G.
name: Lebeer, Sarah
Publisher: name: Zenodo
Year: 2020
Subjects: Biodiversity
Taxonomy
Bacteria
Firmicutes
Bacilli
Lactobacillales
Lactobacillaceae
Lacticaseibacillus
Lacticaseibacillus casei

description: DESCRIPTIONOF LACTICASEIBACILLUS CASEI COMB. NOV.
Lacticaseibacillus casei (ca’se.i. L. gen. n. casei of cheese).
Basonym: Lactobacillus casei (Orla Jensen 1916, Hansen and Lessel 1971, 71 (Approved Lists) (Streptobacterium casei Orla- Jensen 1919, 166).
The species includes strains previously classified as Lactobacillus zeae [155]. Original characteristics of L. casei strains are provided by [2, 156, 157]. L. casei is differentiated from most other lactobacilli by catalase activity [47]. The genome size of the type strain is 2.83 Mbp. The mol% G+C content of DNAis 46.5.
Isolates wereobtained from diversesources including chinese traditional pickle, infant faeces, corn liquor, oat silage, commercial dietary supplements, sputum, nasopharynx [47]. Information on the lifestyle of L. casei is counded by the unclear taxonomy over the past decades; most genomes of designated as L. casei in the NCBI database should be classified as L. paracasei instead [10, 47].
Thetypestrainis 03 [7, IAM 12473, Orland L-323, R.P. Tittsler 303] T =ATCC 393 T =BCRC 10697 T =CCUG 21451 T =CECT 475 T =CIP 103137 T =DSM 20011 T =IAM 12473 T =NBRC 15883 T =JCM 1134 T =KCTC 3109 T =LMG 6904 T =NCIMB 11970 T =NCIMB 11970 T =NRRL B-1922 T.
Genome sequence accession number: BALS00000000.
16S rRNA gene accession number: AF469172.
description: Published as part of Zheng, Jinshui, Wittouck, Stijn, Salvetti, Elisa, Franz, Charles M. A. P., Harris, Hugh M. B., Mattarelli, Paola, O'Toole, Paul W., Pot, Bruno, Vandamme, Peter, Walter, Jens, Watanabe, Koichi, Wuyts, Sander, Felis, Giovanna E., Gänzle, Michael G. & Lebeer, Sarah, 2020, A taxonomic note on the genus Lactobacillus: Description of 23 novel genera, emended description of the genus Lactobacillus Beijerinck 1901, and union of Lactobacillaceae and Leuconostocaceae, pp. 2782-2858 in International Journal of Systematic and Evolutionary Microbiology 70 on page 2811, DOI: 10.1099/ijsem.0.004107, http://zenodo.org/record/4730536
Sub-kiloparsec empirical relations and excitation conditions of HCN and HCO+ J=3-2 in nearby star-forming galaxies
Creators: name: Garcia-Rodriguez, Axel
name: Usero, Antonio
name: Leroy, Adam K.
name: Bigiel, Frank
name: Jimenez-Donaire, Maria Jesus
name: Liu, Daizhong
name: Querejeta, Miguel
name: Saito, Toshiki
name: Schinnerer, Eva
name: Barnes, Ashley
name: Belfiore, Francesco
name: Beslic, Ivana
name: Cao, Yixian
name: Chevance, Melanie
name: Dale, Daniel A.
name: Brok, Jakob S. den
name: Eibensteiner, Cosima
name: Garcia-Burillo, Santiago
name: Glover, Simon C. O.
name: Klessen, Ralf S.
name: Pety, Jerome
name: Puschnig, Johannes
name: Rosolowsky, Erik
name: Sandstrom, Karin
name: Sormani, Mattia C.
name: Teng, Yu-Hsuan
name: Williams, Thomas G.
Publisher: name: arXiv
Year: 2023
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We present new HCN and HCO$^+$ ($J$=3-2) images of the nearby star-forming galaxies (SFGs) NGC 3351, NGC 3627, and NGC 4321. The observations, obtained with the Morita ALMA Compact Array, have a spatial resolution of $\sim$290-440 pc and resolve the inner $R_\textrm{gal} \lesssim$ 0.6-1 kpc of the targets, as well as the southern bar end of NGC 3627. We complement this data set with publicly available images of lower excitation lines of HCN, HCO$^+$, and CO and analyse the behaviour of a representative set of line ratios: HCN(3-2)/HCN(1-0), HCN(3-2)/HCO$^+$(3-2), HCN(1-0)/CO(2-1), and HCN(3-2)/CO(2-1). Most of these ratios peak at the galaxy centres and decrease outwards. We compare the HCN and HCO$^+$ observations with a grid of one-phase, non-local thermodynamic equilibrium (non-LTE) radiative transfer models and find them compatible with models that predict subthermally excited and optically thick lines. We study the systematic variations of the line ratios across the targets as a function of the stellar surface density ($Σ_\textrm{star}$), the intensity-weighted CO(2-1) ($\langle I_\text{CO}\rangle$), and the star formation rate surface density ($Σ_\text{SFR}$). We find no apparent correlation with $Σ_\text{SFR}$, but positive correlations with the other two parameters, which are stronger in the case of $\langle I_\text{CO}\rangle$. The HCN/CO-$\langle I_\text{CO}\rangle$ relations show $\lesssim$0.3 dex galaxy-to-galaxy offsets, with HCN(3-2)/CO(2-1)-$\langle I_\text{CO}\rangle$ being $\sim$2 times steeper than HCN(1-0)/CO(2-1). In contrast, the HCN(3-2)/HCN(1-0)-$\langle I_\text{CO}\rangle$ relation exhibits a tighter alignment between galaxies. We conclude that the overall behaviour of the line ratios cannot be ascribed to variations in a single excitation parameter (e.g. density or temperature).
description: Accepted for publication in A&A. 14 pages, 8 figures
Multiscalar-torsion Cosmology: Exact and Analytic Solutions from Noether Symmetries
Creators: name: Dialektopoulos, Konstantinos F.
name: Leon, Genly
name: Paliathanasis, Andronikos
Publisher: name: arXiv
Year: 2023
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: The Noether symmetry analysis is applied in a multi-scalar field cosmological model in teleparallel gravity. In particular, we consider two scalar fields with interaction in scalar-torsion theory. The field equations have a minisuperspace description, and the evolution of the physical variables depends on the potential function that drives the scalar fields' dynamics. With the requirement for the field equations to admit non-trivial Noether point symmetries and the use of the first theorem of Noether, we constraint all the functional forms for the potential. Finally, we apply symmetry vectors and the corresponding conservation laws to determine exact and analytic solutions in multiscalar-torsion cosmology.
description: 20 pages, no figures
Understanding Community Resilience - A Guide for Companies
Creators: name: Dekker, Rachel
Publisher: name: figshare
Year: 2020
Subjects: subject: 120501 Community Planning
subject: FOS: Social and economic geography
subject: 50101 Ecological Impacts of Climate Change
subject: FOS: Earth and related environmental sciences
subject: 60202 Community Ecology (excl. Invasive Species Ecology)
subject: FOS: Biological sciences

description: The success of a company is directly linked to the resilience ofthe communities where it operates, as well as the resilience of the communities of its workers, its suppliers, and its customers. Increasingly, communities around the world are starting to contemplate their resilience and long-term sustainability. As a result, companies are expected to account for their impacts on community resilience.
This guide helps companies understand why community resilience matters, how communities are beginning to approach resilience, and how companies can explore their role in fostering community resilience.
The kinematics of the magnetised protostellar core IRAS15398-3359
Creators: name: Tabatabaei, Farideh. S.
name: Redaelli, Elena
name: Caselli, Paola
name: Alves, Felipe O.
Publisher: name: arXiv
Year: 2023
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Observations of protostellar envelopes are essential to understand better the process of gravitational collapse toward star and planet formation. From a theoretical perspective, magnetic fields are considered an important factor during the early stages of star formation, especially during the main accretion phase. We aim to study the relation between kinematics and magnetic fields at a very early stage of the star formation process by using data from the Atacama Pathfinder EXperiment (APEX) single dish antenna with the angular resolution of 28". We observed the two molecular lines C18O(2-1) and DCO+(3-2), toward the Class 0 young stellar object IRAS15398-3359. We implement a multi-component Gaussian fitting on the molecular data to study the kinematics. Also, we use previous polarization observations on this source to predict the influence of the magnetic field on the core. The velocity gradient along the central object can be explained as an ongoing outflow motion. We report flowing of material from the filament toward the central object, and of the merging of two velocity components in the C18O (2-1) emission around the protostar position, probably due to the merging of filamentary clouds. Our analysis shows that the large-scale magnetic field line observed previously is preferentially aligned to the rotation axis of the core.
Chemotherapy for a secondary malignancy nearly restores complete chimerism in an SCID-patient after HSCT
Creators: name: Maier, Felix I.
name: Schulz, Ansgar
name: Furlan, Ingrid
name: Felgentreff, Kerstin
name: Jacobsen, Eva-Maria
name: Sirin, Mehtap
name: Schwarz, Klaus
name: Pannicke, Ulrich
name: Stursberg, Jana
name: Debatin, Klaus-Michael
name: Hönig, Manfred
Publisher: name: Universität Ulm
Year: 2024
Subjects: subject: Hematopoietic stem cell transplantation
subject: Inborn errors of immunity
subject: Mixed Chimerism
subject: Secondary malignancy
subject: DDC 610 / Medicine & health

description: For patients with inborn errors of immunity (IEI) and other inborn diseases, mixed donor chimerism is a well-accepted outcome of hematopoietic stem cell transplantation (HSCT). Cytoreductive chemotherapy for a secondary malignancy is a potential challenge for the stability of the graft function after HSCT. We report on a boy with X-SCID who developed Ewing sarcoma ten years after HSCT which was successfully treated with cytoreductive chemotherapy, surgery and local radiation. Surprisingly, this treatment had a positive impact on mixed chimerism with an increase of donor-cell proportions from 40% for neutrophils and 75% for non-T-mononuclear cells (MNCs) to >90% for both. T-cell counts remained stable with 100% of donor origin. This is -to our knowledge- the first report on the impact of cytoreductive chemotherapy on post-HSCT mixed chimerism and provides an important first impression for future patients.
UVIT observations of the Small Magellanic Cloud: Point source catalogue
Creators: name: Devaraj, Ashish
name: Joseph, Prajwel
name: Stalin, C. S.
name: Tandon, Shyam N.
name: Ghosh, Swarna K.
Publisher: name: arXiv
Year: 2023
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Three fields in the outskirts of the Small Magellanic Cloud were observed by the Ultra-Violet Imaging Telescope (UVIT) on board AstroSat, during 31 December 2017 and 01 January 2018. The observations were carried out on a total of seven filters, three in the far ultra-violet (FUV; 1300$-$1800 Å) band and four in the near ultra-violet (NUV; 2000$-$3000 Å) band. We carried out photometry of these observations that have a spatial resolution better than 1.5$^{\prime\prime}$. We present here the first results of this work, which is a matched catalogue of 11,241 sources detected in three FUV and four NUV wavelengths. We make the catalogue available online, which would be of use to the astronomical community to address a wide variety of astrophysical problems. We provide an expression to estimate the total count rate in the full point spread function of UVIT that also incorporate the effect of saturation.
Light vector meson photoproduction in ultraperipheral heavy ion collisions at the LHC within the Reggeometric Pomeron approach
Creators: name: Jenkovszky, László
name: Rocha, Érison S.
name: Machado, Magno V. T.
Publisher: name: arXiv
Year: 2023
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: By using the Reggeometric Pomeron model for vector meson production which successfully describes the high energy lepton-nucleon data, we analyse the light meson production in ultra-peripheral heavy ion collisions at the Large Hadron Collider (LHC). The rapidity distributions for $ρ$ and $ϕ$ photoproduction in lead-lead, xenon-xenon and oxygen-oxygen collisions are investigated.
description: Proceedings IWARA 2022
Ammodillus Thomas 1904
Creators: name: Musser, Guy G.
name: Carleton, Michael D.
Publisher: name: Zenodo
Year: 1993
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Rodentia
Muridae
Ammodillus

description: Ammodillus Thomas, 1904. Ann. Mag. Nat. Hist., ser. 7, 14:102. TYPE SPECIES: Gerbillus imbellis de Winton, 1898. COMMENTS: Reviewed by Pavlinov (1981), who was so impressed with its unique morphological traits that he proposed the monotypic tribe Ammodillini.
description: Published as part of Guy G. Musser & Michael D. Carleton, 1993, Order Rodentia - Family Muridae, pp. 501-755 in Mammal Species of the World (2 nd Edition), Washington and London :Smithsonian Institution Press on page 546, DOI: 10.5281/zenodo.7353098
Entangling gates for trapped-ion quantum computation and quantum simulation
Creators: name: Cai, Zhengyang
name: Luan, Chunyang
name: Ou, Lingfeng
name: Tu, Hengchao
name: Yin, Zihan
name: Zhang, Jing-Ning
name: Kim, Kihwan
Publisher: name: arXiv
Year: 2023
Subjects: subject: Quantum Physics (quant-ph)
subject: Atomic Physics (physics.atom-ph)
subject: FOS: Physical sciences

description: The trapped-ion system has been a leading platform for practical quantum computation and quantum simulation since the first scheme of a quantum gate was proposed by Cirac and Zoller in 1995. Quantum gates with trapped ions have shown the highest fidelity among all physical platforms. Recently, sophisticated schemes of quantum gates such as amplitude, phase, frequency modulation, or multi-frequency application, have been developed to make the gates fast, robust to many types of imperfections, and applicable to multiple qubits. Here, we review the basic principle and recent development of quantum gates with trapped ions.
description: 19 pages, 10 figures. Review paper invited to the Journal of Korean Physical Society (JKPS) special issue commemorating the 30th anniversary of the division of atomic molecular and optical (AMO) physics
Impaired Immune Function in Patients with Chronic Post-Surgical Hypoparathyroidism: Results of the EMPATHY Study. Supplementary Material
Creators: name: Puliani, Giulia
name: Hasenmajer, Valeria
name: Sciarra, Francesca
name: Barbagallo, Federica
name: Sbardella, Emilia
name: Pofi, Riccardo
name: Gianfrilli, Daniele
name: Romagnoli, Elisabetta
name: Venneri, Mary Anna
name: Isidori, Andrea M.
Publisher: name: figshare
Year: 2020
Subjects: subject: 110306 Endocrinology
subject: FOS: Clinical medicine

description: Supplementary materials from: Impaired Immune Function in Patients with Chronic Post-Surgical Hypoparathyroidism: Results of the EMPATHY Study
Investigation of Lower Boundary Conditions of Brominated Very Short-lived Species (VSLS)
Creators: name: Zheng, Siyuan
Publisher: name: Bergische Universität Wuppertal
Year: 2024

description: Photochemical reactions with the reactive halogen atoms Cl and Br mostly cause stratospheric ozone depletion. The chlorine- and bromine-containing very short-lived species (VSLS), which have an atmospheric lifetime of less than six months, play an essential role in stratospheric total bromine loading. However, there is considerable uncertainty about the geographical distribution of their sources, and therefore, it is challenging to reproduce the observations. In order to describe the stratospheric or regional abundance of bromine from VSLS, it is of great importance to quantify the lower boundary conditions of these species. In order to increase our understanding of the role of brominated species in the stratosphere, the Chemical Lagrangian Model of the Stratosphere (CLaMS) has been used to investigate the global surface mixing ratio and lower boundary conditions for the simulation in this thesis. The simulation uses a ‘top-down approach, where atmospheric measurements from aircraft are used in combination with models to quantify and refine the lower boundary emissions. The findings of this thesis reveal that the simulation incorporating a monthly global lower boundary, featuring notable seasonal and zonal variations, exhibits enhanced concordance with observations obtained during the SouthTRAC campaign. However, the elevated mixing ratio of CHBr3 and CH2Br2 in the upper atmosphere was not confirmed by climatological upper tropospheric and stratospheric data, presumably due to slow up- ward transport. Moreover, the exceedingly high values detected in specific regions at the estimated lower boundary are likely attributed to the limited available observations from the SouthTRAC campaign. This underscores the necessity for additional observations during spring and summer, as well as observation data from higher latitudes in the Northern Hemisphere, to comprehensively construct the lower boundary distribution of CHBr3 and CH2Br2.
Lacticaseibacillus baoqingensis BAOQINGENSIS 2020, COMB. NOV.
Creators: name: Zheng, Jinshui
name: Wittouck, Stijn
name: Salvetti, Elisa
name: Franz, Charles M. A. P.
name: Harris, Hugh M. B.
name: Mattarelli, Paola
name: O'Toole, Paul W.
name: Pot, Bruno
name: Vandamme, Peter
name: Walter, Jens
name: Watanabe, Koichi
name: Wuyts, Sander
name: Felis, Giovanna E.
name: Gänzle, Michael G.
name: Lebeer, Sarah
Publisher: name: Zenodo
Year: 2020
Subjects: Biodiversity
Taxonomy
Bacteria
Firmicutes
Bacilli
Lactobacillales
Lactobacillaceae
Lacticaseibacillus
Lacticaseibacillus baoqingensis

description: DESCRIPTIONOF LACTICASEIBACILLUS BAOQINGENSIS COMB. NOV.
Lacticaseibacillus baoqingensis (boa.qing.en’sis. N.L. masc. adj. boaqingensis of Boaqing, from where the type strain was isolated).
Basonym: Lactobacillus baoqingensis Long and Gu 2019, 2347 VP
Original characteristics of L. baoqingensis strains are as provided by Long and Gu [158].
The genome size of the type strain is 2.86 Mbp. The mol% G+C content of DNA is 50.9.
Isolated from a vegetable fermentation.
Thetypestrainis 47–3 T =NCIMB 15165 T =CCM 8903 T =LMG 31064 T.
Genome sequence accession number: RHOI00000000.
16S rRNA gene accession number: MK110840.
description: Published as part of Zheng, Jinshui, Wittouck, Stijn, Salvetti, Elisa, Franz, Charles M. A. P., Harris, Hugh M. B., Mattarelli, Paola, O'Toole, Paul W., Pot, Bruno, Vandamme, Peter, Walter, Jens, Watanabe, Koichi, Wuyts, Sander, Felis, Giovanna E., Gänzle, Michael G. & Lebeer, Sarah, 2020, A taxonomic note on the genus Lactobacillus: Description of 23 novel genera, emended description of the genus Lactobacillus Beijerinck 1901, and union of Lactobacillaceae and Leuconostocaceae, pp. 2782-2858 in International Journal of Systematic and Evolutionary Microbiology 70 on page 2811, DOI: 10.1099/ijsem.0.004107, http://zenodo.org/record/4730536
Insights into Mechanisms of Secondary Organic Aerosol Formation: Approaching Atmospherically Relevant Conditions in an Atmospheric Reaction Chamber
Creators: name: Baker, Yarê
Publisher: name: Bergische Universität Wuppertal
Year: 2024

description: Secondary organic aerosol (SOA) significantly impacts radiative forcing, climate, and human health. A key process in SOA formation is the production of highly oxygenated molecules (HOMs) through the atmospheric oxidation of volatile organic compounds. These HOMs, formed by autoxidation of organic peroxy radicals (RO2), are low in volatility and can condense or nucleate, contributing to SOA. Despite extensive laboratory studies, the formation of HOMs under atmospheric conditions and their role in SOA formation are not yet fully understood. Laboratory conditions often lead to high RO2 concentrations, emphasizing RO2 cross reactions and potentially resulting in overestimated SOA yields. In contrast, atmospheric conditions involve complex mixtures where HOM-RO2 predominantly react with the hydroperoxyl radical (HO2) or nitric oxide (NO).This study investigates HOM formation in the -pinene photooxidation system using steady-state experiments in the SAPHIR-STAR reaction chamber. We shifted the chemical reaction regime from RO2-dominated to more atmospherically relevant conditions by increasing the concentrations of HO2 and NO, both separately and in mixture, while maintaining constant primary -pinene oxidation conditions. Ammonium sulfate particles were added to gain direct insight into the volatility of the HOM product distribution.The atmospheric fate of HOM-RO2 is defined by reactions with RO2, HO2, and NO, and the overall reactivity of their surroundings. Our experiments systematically varied these parameters. The results show that laboratory experiments with dominance of RO2+RO2 cross reactions lead to overestimations of the SOA formation when the according SOA yield is directly transferred to the atmosphere. By mechanistic considerations, we show how the HOM product distribution depends on the HO2 and NO concentrations and explain the reduced SOA formation by chang++
description: es in the HOM products and their volatility.
Ammodillus imbellis
Creators: name: Musser, Guy G.
name: Carleton, Michael D.
Publisher: name: Zenodo
Year: 1993
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Rodentia
Muridae
Ammodillus
Ammodillus imbellis

description: Ammodillus imbellis (de Winton, 1898). Ann. Mag. Nat. Hist., ser. 7, 1:249. TYPE LOCALITY: Somalia, Goodar. DISTRIBUTION: Somalia and E Ethiopia. COMMENTS: Roche and Petter (1968) reviewed the species and mapped its distribution.
description: Published as part of Guy G. Musser & Michael D. Carleton, 1993, Order Rodentia - Family Muridae, pp. 501-755 in Mammal Species of the World (2 nd Edition), Washington and London :Smithsonian Institution Press on page 546, DOI: 10.5281/zenodo.7353098
description: {"references": ["Roche, J., and F. Petter. 1968. Faits nouveaux concernant trois gerbillides mal connus de Somalia: Ammodillus imbellis (De Winton), Microdillus peeli (De Winton), Monodia juliani (Saint Leger). Monitore Zoologico Italiano, n. s., 2 (suppl.): 181 - 198."]}
Spin-orbital order and excitons in magnetoresistive HoBi
Creators: name: Gaudet, J.
name: Yang, H. -Y.
name: Smith, E. M.
name: Halloran, T.
name: Clancy, J. P.
name: Rodriguez-Rivera, J. A.
name: Xu, Guangyong
name: Zhao, Y.
name: Chen, W. C.
name: Sala, G.
name: Aczel, A. A.
name: Gaulin, B. D.
name: Tafti, F.
name: Broholm, C.
Publisher: name: arXiv
Year: 2023
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: The magnetism of the rock-salt $fcc$ rare-earth monopnictide HoBi, a candidate topological material with extreme magnetoresistance, is investigated. From the Ho$^{3+}$ non-Kramers $J$=8 spin-orbital multiplet, the cubic crystal electric field yields six nearly degenerate low-energy levels. These constitute an anisotropic magnetic moment with a Jahn-Teller-like coupling to the lattice. In the cubic phase for $T>T_N~=~5.72(1)~K$, the paramagnetic neutron scattering is centered at $\mathbf{k}=(\frac{1}{2}\frac{1}{2}\frac{1}{2})$ and was fit to dominant antiferromagnetic interactions between Ho spins separated by $\{100\}$ and ferromagnetic interactions between spins displaced by $\{\frac{1}{2}\frac{1}{2}0\}$. For $T
description: 10 pages, 6 figures
Design and characterization of a lumped element single-ended superconducting microwave parametric amplifier with on-chip flux bias line
Creators: name: Mutus, Josh
name: White, Ted
name: Jeffrey, Evan
name: Sank, Daniel
name: Barends, Rami
name: Bochmann, Joerg
name: Chen, Yu
name: Chen, Zijun
name: Chiaro, Ben
name: Dunsworth, Andrew
name: Kelly, Julian
name: Megrant, Anthony
name: Neill, Charles
name: O'Malley, Peter
name: Roushan, Pedram
name: Vainsencher, Amit
name: Wenner, James
name: Siddiqi, Irfan
name: Vijayaraghavan, Rajamani
name: Cleland, Andrew
name: Martinis, John
Publisher: name: arXiv
Year: 2013
Subjects: subject: Superconductivity (cond-mat.supr-con)
subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: We demonstrate a lumped-element Josephson parametric amplifier, using a single-ended design that includes an on-chip, high-bandwidth flux bias line. The amplifier can be pumped into its region of parametric gain through either the input port or through the flux bias line. Broadband amplification is achieved at a tunable frequency $ω/2 π$ between 5 to 7 GHz with quantum-limited noise performance, a gain-bandwidth product greater than 500 MHz, and an input saturation power in excess of -120 dBm. The bias line allows fast frequency tuning of the amplifier, with variations of hundreds of MHz over time scales shorter than 10 ns.
The $z \lesssim 1$ drop of cosmic dust abundance in a semi-analytic framework
Creators: name: Parente, Massimiliano
name: Ragone-Figueroa, Cinthia
name: Granato, Gian Luigi
name: Lapi, Andrea
Publisher: name: arXiv
Year: 2023
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: Observations suggest that the amount of galactic dust in the Universe decreased by a factor $\sim 2-3$ during the last $\sim 8$ Gyr. However, cosmological models of galaxy evolution usually struggle to explain this decrease. Here we use the semi-analytic model (SAM) L-Galaxies2020 to show that this drop may be reproduced assuming standard prescriptions for dust production and evolution. We extend the SAM with i) a state-of-the-art dust model which adopts the two-size approximation and ii) a new disc instability criterion which triggers bulge and central black hole growth. The model reproduces some fundamental properties of the local galaxy population, such as the fraction of spheroid-dominated galaxies and some scaling relations involving dust. Moreover, the model predicts a galactic dust drop from $z \sim 1 \rightarrow 0$, which becomes closer to the observed one when adopting the new treatment of disc instabilities. This result is related to the newly implemented super-massive black hole growth during disc instabilities, which enhances the quenching of massive galaxies. Consequently, these objects feature a lower gas and dust content. We provide a census of the contribution of all the processes affecting the galactic dust content. Accretion is the dominant dust mass growth process. Destruction by supernovae, astration and ejection by winds have all a non-negligible role in decreasing the overall dust content in galaxies below $z \sim 1$. We also discuss predictions concerning extra-galactic dust, confirming that a sputtering efficiency lower than the canonical one is required to match the few available observations.
description: 20 pages, 20 figures, 1 table. Accepted for publication in MNRAS
Development of a Li2MoO4 scintillating bolometer for low background physics
Creators: name: Cardani, L.
name: Casali, N.
name: Nagorny, S.
name: Pattavina, L.
name: Piperno, G.
name: Barinova, O. P.
name: Beeman, J. W.
name: Bellini, F.
name: Danevich, F. A.
name: Di Domizio, S.
name: Gironi, L.
name: Kirsanova, S. V.
name: Orio, F.
name: Pessina, G.
name: Pirro, S.
name: Rusconi, C.
name: Tomei, C.
name: Tretyak, V. I.
name: Vignati, M.
Publisher: name: arXiv
Year: 2013
Subjects: subject: Instrumentation and Detectors (physics.ins-det)
subject: High Energy Physics - Experiment (hep-ex)
subject: Nuclear Experiment (nucl-ex)
subject: FOS: Physical sciences

description: We present the performance of a 33 g Li2MoO4 crystal working as a scintillating bolometer. The crystal was tested for more than 400 h in a dilution refrigerator installed in the underground laboratory of Laboratori Nazionali del Gran Sasso (Italy). This compound shows promising features in the frame of neutron detection, dark matter search (solar axions) and neutrinoless double-beta decay physics. Low temperature scintillating properties were investigated by means of different alpha, beta/gamma and neutron sources, and for the first time the Light Yield for different types of interacting particle is estimated. The detector shows great ability of tagging fast neutron interactions and high intrinsic radiopurity levels (< 90 \muBq/kg for 238-U and < 110 \muBq/kg for 232-Th).
description: revised version
Brachiones Thomas 1925
Creators: name: Musser, Guy G.
name: Carleton, Michael D.
Publisher: name: Zenodo
Year: 1993
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Rodentia
Muridae
Brachiones

description: Brachiones Thomas, 1925. Ann. Mag. Nat. Hist., ser. 9, 16:548. TYPE SPECIES: Gerbillus przewalskii Büchner, 1889. COMMENTS: Placed in the tribe Rhombomyini by Pavlinov et al. (1990); more closely related to Meriones and Sekeetamys than to any other genera.
description: Published as part of Guy G. Musser & Michael D. Carleton, 1993, Order Rodentia - Family Muridae, pp. 501-755 in Mammal Species of the World (2 nd Edition), Washington and London :Smithsonian Institution Press on page 546, DOI: 10.5281/zenodo.7353098
description: {"references": ["Pavlinov, I. Ya., Yu. A. Dubrovsky, O. L. Rossolimo, and E. G. Potapova. 1990. [Gerbils of the world.] Nauka, Moscow, 368 pp. (in Russian)."]}
Brachiones przewalskii
Creators: name: Musser, Guy G.
name: Carleton, Michael D.
Publisher: name: Zenodo
Year: 1993
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Rodentia
Muridae
Brachiones
Brachiones przewalskii

description: Brachiones przewalskii (Büchner, 1889). Wiss. Res. Przewalski Cent.-Asian Reisen., Zool., I:(Säugeth.), p. 51. TYPE LOCALITY: China, Xinjiang (Sinkiang), Lob Nor. DISTRIBUTION: China, deserts from Xinjiang to Gansu. SYNONYMS: arenicolor, callichrous. COMMENTS: Reviewed by Corbet (1978c).
description: Published as part of Guy G. Musser & Michael D. Carleton, 1993, Order Rodentia - Family Muridae, pp. 501-755 in Mammal Species of the World (2 nd Edition), Washington and London :Smithsonian Institution Press on pages 546-547, DOI: 10.5281/zenodo.7353098
description: {"references": ["Corbet, G. B. 1978 c. The mammals of the Palaearctic region: A taxonomic review. British Museum (Natural History), London, 314 pp."]}
Magnetoacoustic waves in a partially ionized two-fluid plasma
Creators: name: Soler, Roberto
name: Carbonell, Marc
name: Ballester, Jose Luis
Publisher: name: arXiv
Year: 2013
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Compressible disturbances propagate in a plasma in the form of magnetoacoustic waves driven by both gas pressure and magnetic forces. In partially ionized plasmas the dynamics of ionized and neutral species are coupled due to ion-neutral collisions. As a consequence, magnetoacoustic waves propagating through a partially ionized medium are affected by the ion-neutral coupling. The degree to which the behavior of the classic waves is modified depends on the physical properties of the various species and on the relative value of the wave frequency compared to the ion-neutral collision frequency. Here, we perform a comprehensive theoretical investigation of magnetoacoustic wave propagation in a partially ionized plasma using the two-fluid formalism. We consider an extensive range of values for the collision frequency, ionization ratio, and plasma $β$, so that the results are applicable to a wide variety of astrophysical plasmas. We determine the modification of the wave frequencies and study the frictional damping due to ion-neutral collisions. Approximate analytic expressions to the frequencies are given in the limit case of strongly coupled ions and neutrals, while numerically obtained dispersion diagrams are provided for arbitrary collision frequencies. In addition, we discuss the presence of cutoffs in the dispersion diagrams that constrain wave propagation for certain combinations of parameters. A specific application to propagation of compressible waves in the solar chromosphere is given.
description: Accepted for publication in ApJ Supplement Series