Miracle-dz/UniFAR-FTUs huggingface dataset:
A Study on Prevalence of Diarrhoeal Diseases among under five Children in Kanchipuram Town

Aim and Background: In the present study was to investigate that the study on prevalence of Diarrhoel disease among under five children in Kanchipuram town. Diarrhoeal diseases are a major cause of hospitalizations and child deaths globally. Together they account for approximately one in six deaths among children younger than five years. In India more than 2.3 million annual deaths among children, about 334 000 are attributable to diarrhoeal diseases. Materials and Methods: This is a cross sectional study was conducted to know the prevalence of diarrhoeal diseases among under the age of five Years children in Kanchipuram town. This study was carried out in 10 wards of kanchipuram town. In the present study mullti stage sampling system were used. Results: The total sample studied was 1138 under five children. In which 601 (52.8%) were male children and 537 (47.2%) were female children. It was observed in the study that diarrhoea in children is higher in joint family (33.0%) when compared the nuclear family (22.2%). The association was found to be statistically significant. Conclusion: In the present study we conclude that diarrhoeal diseases have been on an increase in families with young mothers, overcrowding and poor immunization. Hence it is advisable exclusive breast feeding for minimum of 6 months.
White Button Mushroom (Agaricus bisporus) Supplementation Ameliorates Spatial Memory Deficits and Plaque Formation in an Amyloid Precursor Protein Mouse Model of Alzheimer’s Disease

Alzheimer’s Disease (AD) is characterized by cognitive impairment and the presence of amyloid-β (Aβ) plaques and tau tangles. This study was conducted to assess the effects of white button mushroom (WBM) supplementation on spatial memory and plaque formation in mice with mutations in amyloid (Aβ). Mice with amyloid precursor protein (hAPP) mutations and their wildtype (WT) littermates were fed a 10% white button mushroom (WBM) feed ad libitum three times per week, in addition to their normal diet. Morris water maze (MWM) was conducted at 14 and 32 weeks of age to assess spatial memory and Aβ plaque pathology in the hippocampus was analyzed. Our results showed that hAPP mice on the WBM diet were faster in reaching the platform in the MWM compared to hAPP mice on the control diet at 32 weeks (p < 0.05). Significantly fewer plaque deposits were found in the hippocampi of hAPP mice on the WBM diet compared to those on the control diet at 32 weeks (p < 0.05). Overall, hAPP mice on the WBM diet had improved spatial memory at 32 weeks of age compared to those on the control diet and exhibited fewer amyloid plaques.
On the sbottom resonance in dark matter scattering

A resonance in the neutralino-nucleus elastic scattering cross section is usually purported when the neutralino-sbottom mass difference m{sub b-tilde}−m{sub χ} is equal to the bottom quark mass m{sub b} ∼ 4 GeV. Such a scenario has been discussed as a viable model for light ( ∼ 10 GeV) neutralino dark matter as explanation of possible DAMA and CoGeNT direct detection signals. Here we give physical and analytical arguments showing that the sbottom resonance may actually not be there. In particular, we show analytically that the one-loop gluon-neutralino scattering amplitude has no pole at m{sub b-tilde} = m{sub χ}+m{sub b}, while by analytic continuation to the regime m{sub b-tilde} < m{sub χ}, it develops a pole at m{sub b-tilde} = m{sub χ}−m{sub b}. In the limit of vanishing gluon momenta, this pole corresponds to the only cut of the neutralino self-energy diagram with a quark and a squark running in the loop, when the decay process χ→ Q-tilde +Q becomes kinematically allowed. The pole can be interpreted as the formation of a b-tilde b-bar qqq or b-tilde *bqqq resonant state (where qqq are the nucleon valence quarks), which is however kinematically not accessible if the neutralino is the LSP. Our analysismore » shows that the common practice of estimating the neutralino-nucleon cross section by introducing an ad-hoc pole at m{sub b-tilde} = m{sub χ}+m{sub b} into the effective four-fermion interaction (also including higher-twist effects) should be discouraged, since it corresponds to adding a spurious pole to the scattering process at the center-of-mass energy (s){sup 1/2} ≅ m{sub χ} ≅ m{sub b-tilde}−m{sub b}. Our considerations can be extended from the specific case of supersymmetry to other similar cases in which the dark matter particle scatters off nucleons through the exchange of a b-flavored state almost degenerate in mass with the dark matter particle, such as for instance in theories with extra dimensions and in other mass-degenerate dark matter scenarios recently discussed in the literature. « less
FURTHER EVIDENCE FOR A SUPERMASSIVE BLACK HOLE MASS–PITCH ANGLE RELATION

We present new and stronger evidence for a previously reported relationship between galactic spiral arm pitch angle P (a measure of the tightness of spiral structure) and the mass MBH of a disk galaxy's nuclear supermassive black hole (SMBH). We use an improved method to accurately measure the spiral arm pitch angle in disk galaxies to generate quantitative data on this morphological feature for 34 galaxies with directly measured black hole masses. We find a relation of log (M/M☉) = (8.21 ± 0.16) − (0.062 ± 0.009)P. This method is compared with other means of estimating black hole mass to determine its effectiveness and usefulness relative to other existing relations. We argue that such a relationship is predicted by leading theories of spiral structure in disk galaxies, including the density wave theory. We propose this relationship as a tool for estimating SMBH masses in disk galaxies. This tool is potentially superior when compared to other methods for this class of galaxy and has the advantage of being unambiguously measurable from imaging data alone.
Analysis of Turbulence Reports and ERA5 Turbulence Diagnostics in a Tropopause‐Based Vertical Framework

In the tropopause region turbulence exhibits a common feature with posing a threat for aviation as well as presenting a pathway for cross tropopause exchange. However, current numerical weather prediction and in particular climate models still struggle to resolve a large part of the dynamics responsible for turbulence generation. This renders high resolution observations of turbulence to be very valuable to identify the spatio‐temporal distribution of turbulence. In this study we use aircraft observations along with reanalysis data over the North Atlantic during winter season to analyze turbulence occurrence. Using a tropopause‐based coordinate system, we found that turbulence occurs within a sharp unimodal distribution which maximizes just below the tropopause. Turbulence also significantly affects the first 2 km above the tropopause which highlights its potential impact on the formation of the so called extratropical mixing layer around the tropopause.
The linear rms—flux relation in an ultraluminous X-ray source

We report the first detection of a linear correlation between rms variability amplitude and flux in the ultraluminous X-ray source (ULX) NGC 5408 X-1. The rms–flux relation has previously been observed in several galactic black hole X-ray binaries (BHBs), several active galactic nuclei (AGN) and at least one neutron star X-ray binary. This result supports the hypothesis that a linear rms–flux relation is common to all luminous black hole accretion and perhaps even a fundamental property of accretion flows about compact objects. We also show for the first time the cross-spectral properties of the variability of this ULX, comparing variations below and above 1 keV. The coherence and time delays are poorly constrained but consistent with high coherence between the two bands, over most of the observable frequency range and a significant time delay (with hard leading soft variations). The magnitude and frequency dependence of the lags are broadly consistent with those commonly observed in BHBs, but the direction of the lag is reversed. These results indicate that ULX variability studies, using long X-ray observations, hold great promise for constraining the processes driving ULXs behaviour, and the position of ULXs in the scheme of black hole accretion from BHBs to AGN.
An Observational Study of Serum Vitamin D Status in Critically Ill Children Admitted to the Pediatric Intensive Care Unit

Vitamin D is a pleiotropic hormone involved in the functioning of organ systems including those central to critical illness pathophysiology. We evaluated the longitudinal vitamin D status in the pediatric intensive care unit (PICU) and its relevance to patient outcomes.Thirty-six PICU-admitted patients, and 40 age- and sex-matched healthy children were enrolled. Serum total 25-hydroxyvitamin D [25(OH)D] levels were analyzed on PICU days 1, 5, and 10 in the patient group, and once in the control group. Patients were divided into sufficient (>30 ng/mL), insufficient (20–30 ng/mL), and deficient (<20 ng/mL) subgroups. Outcome measures between the subgroups and alterations in 25(OH)D levels were examined.The mean 25(OH)D levels of PICU patients initially and control cases were not different (25.4±6.0 and 25.9±5.8 ng/mL, respectively). Although all patients with vitamin D deficiency were hospitalized for infectious diseases, the mean 25(OH)D level of patients hospitalized for infections was not different from other patients. There was no difference between vitamin D subgroups in demographic variables, admission season, illness severity, respiratory/inotropic support, duration of stay, and mortality. Vitamin D deficient patients had lower albumin concentrations (p˂0.05). On days 5 and 10, the mean 25(OH)D levels of the patients were 24.5±5.7 and 23.6±5.8 ng/mL, respectively, both different from the admission level (p˂0.001). Hypovitaminosis D, which is common in healthy children, is also common in PICU admission and tends to be more profound during the stay. Further studies are required to evaluate the bioavailability of vitamin D in critical illness.
THE CORRELATION BETWEEN Hα EMISSION AND VISUAL MAGNITUDE DURING LONG-TERM VARIATIONS IN CLASSICAL Be STARS

Hα equivalent widths and UBV magnitudes are calculated for Be star disk models that grow in size and/or density with time. We show that these simple models are consistent with the known Be star classes of positive and inverse correlations between long-term variations in Hα and V magnitude as identified by Harmanec. We support the conclusion of Harmanec that the distinction is controlled by the inclination of the disk to the line of sight. We demonstrate that the strength of these correlations, particularly those of an inverse correlation where the system becomes fainter as the Hα emission strength grows, is strongly influenced by the scale height of the inner Be star disk and the extent of the gravitational darkening of the central B star due to rapid rotation. This dependence may allow coordinated spectroscopic and photometric observations to better constrain these poorly known Be star parameters.
Histomorphological and carbohydrate histochemical study of the pancreas in native ducks (Anas Platyrhynchos)

In the current study, the histomorphological and histochemical characteristics of the pancreas in native ducks are examined with a particular emphasis on the structure of pancreatic acini and Langerhans islets (LI). Five adult male native ducks ( Anas Platyrhynchos ) are examined from the local market of Mosul. All samples are processed routinely for histological and histochemical analyses. Hematoxylin & Eosin, PAS-AB (pH 2.5), Toluidine blue, and Masson's Trichrome stains are used. The morphological examination reveals that male ducks’ pancreas is made up of three major lobes (dorsal, ventral, and third lobes). The pancreas is a small, semi-wide structure with a pale to white pinkish tone located between the duodenum branches. The findings show that the pancreas is enveloped in a thin layer of loose connective tissue capsule and mesothelial; septa extend from the capsule into parenchyma dividing it into many lobules. The study concludes that the pancreatic lobules are composed of a large area of exocrine acini and a small amount of LI, with an exocrine component consisting of round or oval acini with zymogen granules. The endocrine component is represented by three distinct LI types and lacks defined boundaries. Alpha islets are formed of alpha cells (ACs) and a few delta cells (DCs); beta islets are composed of peripherally located beta cells (BCs) and a few (DCs); and mixed islets are composed of alpha, beta, and delta cells. The present study sheds light on the morphological, histological, and histochemical characteristics of the indigenous duck pancreas. However, future research should focus on the pancreas of other bird species as well.
Mathematical Proceedings of the Cambridge Philosophical Society

Let (cid:2) be an elliptic curve deﬁned over Q , all of whose 2-division points are rational, and let (cid:2) b be its quadratic twist by b . Subject to a mild additional condition on (cid:2) , we ﬁnd the limit of the probability distribution of the dimension of the 2-Selmer group of (cid:2) b as the number of prime factors of b increases; and we show that this distribution depends only on whether the 2-Selmer group of (cid:2) has odd or even dimension.
Protein, fatty acid, mineral profiles and antioxidant potential of Kupres cheese at different stage of ripening

Kupres cheese is a traditional Bosnian full-fat hard cheese. This paper deals with the change of protein and fatty acid profiles, mineral content and antioxidant potential during the period of three months of its ripening. Proteolysis was monitored by the electrophoresis of total extracts and water-soluble fractions under reducing conditions, whereas fatty acid profiles were determined by gas chromatography. The mineral content in the ripened cheeses was determined by using methods of Inductively coupled plasma - optical emission spectrometry (ICP-OES) for microelements and Inductively coupled plasma mass spectrometry (ICP-MS) for microelements, respectively. Ripening of Kupres cheese during three months is characterised by a relatively slow proteolysis, especially during the first month and by the increase in desirable fatty acid content. After 30 days of ripening, the WSN/TN and TCA/TN contents increased from 8.23% and 2.25% to 10.15% and 3.59%, respectively. Further, ripening induced higher increase of these parameters and more intensive degradation of the major caseins, especially αs-CN. After three months of ripening, residual level of αs-CN and β-CN was 12.02% and 80.96%, respectively. Three month-old cheese had improved indexes of lipid quality as well as improved reducing power and ability to scavenge free radicals. Ripening affected the content of Ca, P and Na whereas no significant changes of the other macro- and microelements of Kupres cheese were observed.
Stellar Superfluids

Neutron stars provide a fertile environment for exploring superfluidity under extreme conditions. It is not surprising that Cooper pairing occurs in dense matter since nucleon pairing is observed in nuclei as energy differences between even-even and odd-even nuclei. Since superfluids and superconductors in neutron stars profoundly affect neutrino emissivities and specific heats, their presence can be observed in the thermal evolution of neutron stars. An evergrowing number of cooling neutron stars, now amounting to 13 thermal sources, and several additional objects from which upper limits to temperatures can be ascertained, can now be used to discriminate among theoretical scenarios and even to dramatically restrict properties of nucleon pairing at high densities. In addition, observations of pulsars, including their spin-downs and glitch histories, additionally support the conjecture that superfluidity and superconductivity are ubiquitous within, and important to our understanding of, neutron stars.
Callus Production and Analysis of Isoflavonoids and Some Terpenes from Bituminaria bituminosa

Background: Bituminaria bituminosa is a long-day plant. The plant has a high pastoral value and palatability. It is grazed by cattle, goats and sheep. Leaves and stems contain four furanocoumarins’ psoralen, angelicin, xanthotoxin and bergapten. The seed is covered by the fruit. Germination was not observed in beaked fruits. A cut with a scalpel can increase the germination rate. According to the literature there are not enough studies about the culture media and convenient conditions. Methods: In our study, we tried six medium for callus production with different hormone concentrations including 2,4-D, BAP and kinetin. In this study, a protocol for callus induction and analysis of isoflavonoids and terpenes of Bituminaria bituminosa has been developed. Result: Maximum callus induction frequency was observed on Murashige and Skoog (MS) medium supplemented with 0.75 mg/L 2,4-D + 2.5 mg/L kinetin in young primary leaves. 0.75 mg/L 2,4-D+2.5 mg/L kinetin medium is more successful in the production ofses of flavonoids that can be produced in vitro and is more successful in producing phenols. In terpene production, it is seen that 1.25 mg/L 2,4-D+3.5 mg/L BAP, which is the best callus producing medium containing BAP, is the most successful medium among all tested mediums.
THE CIRCULAR VELOCITY FUNCTION OF GROUP GALAXIES

A robust prediction of ΛCDM cosmology is the halo circular velocity function (CVF), a dynamical cousin of the halo mass function. The correspondence between theoretical and observed CVFs is uncertain, however: cluster galaxies are reported to exhibit a power-law CVF consistent with N-body simulations, but that of the field is distinctly Schechter-like, flattened compared to ΛCDM expectations at circular velocities vc ≲ 200 km s−1. Groups offer a powerful probe of the role environment plays in this discrepancy as they bridge the field and clusters. Here, we construct the CVF for a large, mass- and multiplicity-complete sample of group galaxies from the Sloan Digital Sky Survey. Using independent photometric vc estimators, we find no transition from field to ΛCDM-shaped CVF above vc = 50 km s−1 as a function of group halo mass. All groups with 12.4 ≲ log Mhalo/M☉ ≲ 15.1 (Local Group analogs to rich clusters) display similar Schechter-like CVFs marginally suppressed at low vc compared to that of the field. Conversely, some agreement with N-body results emerges for samples saturated with late-type galaxies, with isolated late-types displaying a CVF similar in shape to ΛCDM predictions. We conclude that the flattening of the low-vc slope in groups is due to their depressed late-type fractions—environment affecting the CVF only to the extent that it correlates with this quantity—and that previous cluster analyses may suffer from interloper contamination. These results serve as useful benchmarks for cosmological simulations of galaxy formation.
Broad‐band timing properties of the accreting white dwarf MV Lyrae

We present a broad-band timing analysis of the accreting white dwarf system MV Lyrae based on data obtained with the Kepler satellite. The observations span 633 d at a cadence of 58.8 s and allow us to probe four orders of magnitude in temporal frequency. The modelling of the observed broad-band noise components is based on the superposition of multiple Lorentzian components, similar to the empirical modelling adopted for X-ray binary systems. We also present the detection of a frequency varying Lorentzian component in the light curve of MV Lyrae, where the Lorentzian characteristic frequency is inversely correlated with the mean source flux. Because in the literature similar broad-band noise components have been associated with either the viscous or dynamical time-scale for different source types (accreting black holes or neutron stars), we here systematically explore both scenarios and place constraints on the accretion disc structure. In the viscous case we employ the fluctuating accretion disc model to infer parameters for the viscosity and disc scale height, and infer uncomfortably high parameters to be accommodated by the standard thin disc, whilst in the dynamical case we infer a large accretion disc truncation radius of ≈10RWD. More importantly however, the phenomenological properties between the broad-band variability observed here and in X-ray binaries and active galactic nuclei are very similar, potentially suggesting a common origin for the broad-band variability.
Conventional superconductivity at 190 K at high pressures

The highest critical temperature of superconductivity Tc has been achieved in cuprates: 133 K at ambient pressure and 164 K at high pressures. As the nature of superconductivity in these materials is still not disclosed, the prospects for a higher Tc are not clear. In contrast the Bardeen-Cooper-Schrieffer (BCS) theory gives a clear guide for achieving high Tc: it should be a favorable combination of high frequency phonons, strong coupling between electrons and phonons, and high density of states. These conditions can be fulfilled for metallic hydrogen and covalent hydrogen dominant compounds. Numerous followed calculations supported this idea and predicted Tc=100-235 K for many hydrides but only moderate Tc~17 K has been observed experimentally. Here we found that sulfur hydride transforms at P~90 GPa to metal and superconductor with Tc increasing with pressure to 150 K at ~200 GPa. This is in general agreement with recent calculations of Tc~80 K for H2S. Moreover we found superconductivity with Tc~190 K in a H2S sample pressurized to P>150 GPa at T>220 K. This superconductivity likely associates with the dissociation of H2S, and formation of SHn (n>2) hydrides. We proved occurrence of superconductivity by the drop of the resistivity at least 50 times lower than the copper resistivity, the decrease of Tc with magnetic field, and the strong isotope shift of Tc in D2S which evidences a major role of phonons in the superconductivity. H2S is a substance with a moderate content of hydrogen therefore high Tc can be expected in a wide range of hydrogen-contain materials. Hydrogen atoms seem to be essential to provide the high frequency modes in the phonon spectrum and the strong electron-phonon coupling.