Effect of Electromagnetic Induction and Heat Treatment on the Mechanical and Wear Properties of LM25 Alloy

AbstractMainly for aluminum castings the properties depend on the grain structure, it is desirable to achieve a fine equiaxed grain structure. The formation of fine equiaxed grain structure depends on the rate of solidification, addition of grain refiners. Al-Ti-B master alloys are used in Al-Si alloys casting industries as a grain refiner to improve the casting properties. This research work investigates the combined effect of the addition of 2% Al-5Ti-1B and electromagnetic induction with T6 heat treatment on the mechanical properties and wear properties of LM25 alloy casting. The mechanical properties assessed are hardness and ultimate tensile strength (UTS), microstructure examination, fracture analysis of the castings are studied. It is found that mechanical properties and wear properties of LM25 alloy have been considerably improved by subjecting the alloy to combined effect of the addition of 2% Al-5Ti-1B and electromagnetic induction with T6 heat treatment

The burden of unintentional drowning: Global, regional and national estimates of mortality from the Global Burden of Disease 2017 Study

__Background:__ Drowning is a leading cause of injury-related mortality globally. Unintentional drowning (International Classification of Diseases (ICD) 10 codes W65-74 and ICD9 E910) is one of the 30 mutually exclusive and collectively exhaustive causes of injury-related mortality in the Global Burden of Disease (GBD) study. This study's objective is to describe unintentional drowning using GBD estimates from 1990 to 2017. __Methods:__ Unintentional drowning from GBD 2017 was estimated for cause-specific mortality and years of life lost (YLLs), age, sex, country, region, Socio-demographic Index (SDI) quintile, and trends from 1990 to 2017. GBD 2017 used standard GBD methods for estimating mortality from drowning. __Results:__ Globally, unintentional drowning mortality decreased by 44.5% between 1990 and 2017, from 531 956 (uncertainty interval (UI): 484 107 to 572 854) to 295 210 (284 493 to 306 187) deaths. Global age-standardised mortality rates decreased 57.4%, from 9.3 (8.5 to 10.0) in 1990 to 4.0 (3.8 to 4.1) per 100 000 per annum in 2017. Unintentional drowning-associated mortality was generally higher in children, males and in low-SDI to middle-SDI countries. China, India, Pakistan and Bangladesh accounted for 51.2% of all drowning deaths in 2017. Oceania was the region with the highest rate of age-standardised YLLs in 2017, with 45 434 (40 850 to 50 539) YLLs per 100 000 across both sexes. __Conclusions:__ There has been a decline in global drowning rates. This study shows that the decline was not consistent across countries. The results reinforce the need for continued and improved policy, prevention and research efforts, with a focus on low-and middle-income countries

Search for gravitational waves from Scorpius X-1 in the second Advanced LIGO observing run with an improved hidden Markov model

We present results from a semicoherent search for continuous gravitational waves from the low-mass x-ray binary Scorpius X-1, using a hidden Markov model (HMM) to track spin wandering. This search improves on previous HMM-based searches of LIGO data by using an improved frequency domain matched filter, the J-statistic, and by analyzing data from Advanced LIGO's second observing run. In the frequency range searched, from 60 to 650 Hz, we find no evidence of gravitational radiation. At 194.6 Hz, the most sensitive search frequency, we report an upper limit on gravitational wave strain (at 95% confidence) of h095%=3.47×10-25 when marginalizing over source inclination angle. This is the most sensitive search for Scorpius X-1, to date, that is specifically designed to be robust in the presence of spin wandering. © 2019 American Physical Society

Search for gravitational-wave transients associated with magnetar bursts in advanced LIGO and advanced Virgo data from the third observing run

Gravitational waves are expected to be produced from neutron star oscillations associated with magnetar giant f lares and short bursts. We present the results of a search for short-duration (milliseconds to seconds) and longduration (∼100 s) transient gravitational waves from 13 magnetar short bursts observed during Advanced LIGO, Advanced Virgo, and KAGRA’s third observation run. These 13 bursts come from two magnetars, SGR1935 +2154 and SwiftJ1818.0−1607. We also include three other electromagnetic burst events detected by FermiGBM which were identified as likely coming from one or more magnetars, but they have no association with a known magnetar. No magnetar giant flares were detected during the analysis period. We find no evidence of gravitational waves associated with any of these 16 bursts. We place upper limits on the rms of the integrated incident gravitational-wave strain that reach 3.6 × 10−²³ Hz at 100 Hz for the short-duration search and 1.1 ×10−²² Hz at 450 Hz for the long-duration search. For a ringdown signal at 1590 Hz targeted by the short-duration search the limit is set to 2.3 × 10−²² Hz. Using the estimated distance to each magnetar, we derive upper limits upper limits on the emitted gravitational-wave energy of 1.5 × 1044 erg (1.0 × 1044 erg) for SGR 1935+2154 and 9.4 × 10^43 erg (1.3 × 1044 erg) for Swift J1818.0−1607, for the short-duration (long-duration) search. Assuming isotropic emission of electromagnetic radiation of the burst fluences, we constrain the ratio of gravitational-wave energy to electromagnetic energy for bursts from SGR 1935+2154 with the available fluence information. The lowest of these ratios is 4.5 × 103

Open data from the third observing run of LIGO, Virgo, KAGRA, and GEO

The global network of gravitational-wave observatories now includes five detectors, namely LIGO Hanford, LIGO Livingston, Virgo, KAGRA, and GEO 600. These detectors collected data during their third observing run, O3, composed of three phases: O3a starting in 2019 April and lasting six months, O3b starting in 2019 November and lasting five months, and O3GK starting in 2020 April and lasting two weeks. In this paper we describe these data and various other science products that can be freely accessed through the Gravitational Wave Open Science Center at https://gwosc.org. The main data set, consisting of the gravitational-wave strain time series that contains the astrophysical signals, is released together with supporting data useful for their analysis and documentation, tutorials, as well as analysis software packages

A joint Fermi-GBM and Swift-BAT analysis of gravitational-wave candidates from the third gravitational-wave observing run

We present Fermi Gamma-ray Burst Monitor (Fermi-GBM) and Swift Burst Alert Telescope (Swift-BAT) searches for gamma-ray/X-ray counterparts to gravitational-wave (GW) candidate events identified during the third observing run of the Advanced LIGO and Advanced Virgo detectors. Using Fermi-GBM onboard triggers and subthreshold gamma-ray burst (GRB) candidates found in the Fermi-GBM ground analyses, the Targeted Search and the Untargeted Search, we investigate whether there are any coincident GRBs associated with the GWs. We also search the Swift-BAT rate data around the GW times to determine whether a GRB counterpart is present. No counterparts are found. Using both the Fermi-GBM Targeted Search and the Swift-BAT search, we calculate flux upper limits and present joint upper limits on the gamma-ray luminosity of each GW. Given these limits, we constrain theoretical models for the emission of gamma rays from binary black hole mergers

Constraints on the cosmic expansion history from GWTC–3

We use 47 gravitational wave sources from the Third LIGO–Virgo–Kamioka Gravitational Wave Detector Gravitational Wave Transient Catalog (GWTC–3) to estimate the Hubble parameter H(z), including its current value, the Hubble constant H0. Each gravitational wave (GW) signal provides the luminosity distance to the source, and we estimate the corresponding redshift using two methods: the redshifted masses and a galaxy catalog. Using the binary black hole (BBH) redshifted masses, we simultaneously infer the source mass distribution and H(z). The source mass distribution displays a peak around 34 M⊙, followed by a drop-off. Assuming this mass scale does not evolve with the redshift results in a H(z) measurement, yielding ${H}_{0}={68}_{-8}^{+12}\,\mathrm{km}\ \,\ {{\rm{s}}}^{-1}\,{\mathrm{Mpc}}^{-1}$ (68% credible interval) when combined with the H0 measurement from GW170817 and its electromagnetic counterpart. This represents an improvement of 17% with respect to the H0 estimate from GWTC–1. The second method associates each GW event with its probable host galaxy in the catalog GLADE+, statistically marginalizing over the redshifts of each event's potential hosts. Assuming a fixed BBH population, we estimate a value of ${H}_{0}={68}_{-6}^{+8}\,\mathrm{km}\ \,\ {{\rm{s}}}^{-1}\,{\mathrm{Mpc}}^{-1}$ with the galaxy catalog method, an improvement of 42% with respect to our GWTC–1 result and 20% with respect to recent H0 studies using GWTC–2 events. However, we show that this result is strongly impacted by assumptions about the BBH source mass distribution; the only event which is not strongly impacted by such assumptions (and is thus informative about H0) is the well-localized event GW190814

Comparative regulatory network of transcripts behind radicle emergence and seedling stage of maize (Zea mays L.)

The transition from radicle emergence to seedling growth in maize is a crucial phase in the plant's life cycle, where rapid physiological and biochemical changes occur to facilitate successful development. In this study, we conducted a comparative transcriptomic analysis to gain a deeper understanding of the molecular processes driving this critical transition. The early divergence in gene expression patterns highlighted the upregulation of a substantial number of genes during radicle emergence. During radicle emergence, gene ontology (GO) term enrichment analysis unveiled active participation in biological processes such as chromatin assembly, cellular response to abiotic stress, and hormone signaling. This indicates that the initial stages of growth are marked by cellular expansion and adaptation to environmental stimuli. Conversely, in the seedling growth stage, GO analysis demonstrated a shift toward processes such as photosynthesis, nitrogen metabolism, and secondary metabolite biosynthesis, reflecting a transition to energy production and enhanced growth. In contrast, seedling growth was characterized by pathways related to photosynthesis and the production of gibberellins, crucial for robust seedling development. Hormonal regulation and starch metabolism were also prominent during radicle emergence, with various hormones, including auxins, diterpenoids, and brassinosteroids, driving processes like cell enlargement and stem growth. Moreover, starch and sucrose metabolism genes were expressed to mobilize stored reserves for energy during this stage. These findings offer valuable insights into the dynamic regulation of genes and pathways during this critical phase of maize development

Awareness of medical students in a medical college in Mangalore, Karnataka, India concerning infection prevention practices

Background: Healthcare-associated infections (HCAIs) are an important public health problem. It is estimated that approximately 1 out of every 20 hospitalized patients will contract an HCAI. The risk is substantial not only to patients but also to healthcare workers, who may contract deadly blood-borne infectious diseases. Hence, it is essential for healthcare professionals to have adequate knowledge regarding infection prevention practices (IPPs) to reduce the burden of these illnesses among patients seeking care. Methods: This cross-sectional study was conducted among 268 medical students at Kasturba Medical College, Mangalore. Information regarding important IPPs such as hand hygiene (HH), needle-stick injuries (NSIs), and standard precautions (SPs) was collected using a semi-structured questionnaire. The collected information was analyzed using SPSS v.11. Fisher's exact test was used to test the association between variables of interest. Results: Overall, knowledge levels regarding HH were low in aspects such as healthcare workers’ hands as sources of infection (40%) and the minimum time needed to apply hand rubs (45.7%), whereas knowledge levels were high in aspects such as indications for using HH. Regarding NSI prevention, knowledge levels were low in aspects such as activities with the highest NSI risk (56%). However, knowledge levels were high in relation to SPs. Conclusion: The knowledge levels regarding infection practices were not adequate among the participants, particularly in the case of hand hygiene methods. Other important aspects, such as needle-stick injuries and use of standard precautions, were better understood, although many aspects still require improvement. These findings suggest the need to consider strengthening the training related to IPPs as a separate entity in the existing curriculum. Keywords: Awareness, Infection prevention, Medical students, Indi