Rationale of α-Ketoanalogue Supplemented with Low Protein Diet for the Treatment of Chronic Kidney Disease

Background: Chronic kidney disease (CKD) has challenged the healthcare system for years. Use of α-ketoanalogue (KA) supplemented with a low protein diet (LPD) may improve renal function. In this study, we aim to find out the effectiveness of KA supplemented with LPD for the therapy of CKD. Methods: A descriptive cross-sectional study was conducted at Shree Birendra Hospital with 25 control and 25 treatment group. The control group was treated with LPD (0.8 g/kg/day), while the test group was treated with KA (3 tablets/day for 4 weeks followed by 6 tablets/day for the next 16 weeks) along with LPD. The baseline parameters were measured on day 0, then subsequently at week 4, week 12, and lastly at the end of week 16. Results were then compared with the control group for analysis. Results: Serum level of creatinine showed a progressive decline in the treatment group in comparison to the control group. However, there was a progressive decline in the level of blood urea in the first 4 weeks (84.33) and 12 weeks (72.11) of treatment, a slight increment was observed in week 16 (86.06) but the level was below the baseline value. Similarly, the blood level of sodium and potassium was slightly affected by the increase in sodium and decrease in potassium level from the baseline in the treatment group.  The level of serum albumin was increased in the treatment group as compared to the control group.  The systolic blood pressure was increased in both treatment and control group whereas diastolic blood pressure was decreased in the treatment group rather than the control group. Conclusion: KA supplemented with LPD shows a significant improvement in renal function of CKD III patients that delay the time for dialysis or transplant. However, further substantial multi-institutional randomized studies are necessary to generalize the findings

microRNA-146a modulates behavioural activity, neuroinflammation, and oxidative stress in adult mice

Small non-coding miRNA act as key regulators of several physiological processes due to their ability to interact with numerous target mRNA within a network. Whilst several miRNA can act in concert to regulate target mRNA expression, miR-146a has emerged as a critical modulator of inflammation by targeting key upstream signalling proteins of the nuclear factor kappa-light-chain-enhancer of activated B cells (NF-κB) pathway and reductions in this miRNA have been observed in several neurological and neurodegenerative disorders. However, a targeted assessment of behaviour and neural tissues following the loss of miR-146a has not been documented. In this study, we examined the behavioural and neuroinflammatory phenotype of mice lacking miR-146a to determine the role of this miRNA in neurological function. Adult miR-146a−/− mice displayed no overt developmental phenotype with the exception of enlarged spleens. Behavioural testing revealed a mild but significant reduction in exploratory locomotor activity and increase in anxiety-like behaviour, with no changes in short-term spatial memory, fear conditioning, or sensorimotor gating. In the brain, the lack of miR-146a resulted in a significant compensatory miR-155 expression with no significant changes in expression of the target Interleukin 1 Receptor Associated Kinase (Irak) gene family. Despite these effects on upstream NF-κB mediators, downstream expression of cytokine and chemokine messengers was significantly elevated in miR-146a−/− mice compared to wild-type controls. Moreover, this increase in inflammatory cytokines was observed alongside an induction of oxidative stress, driven in part by nicotinamide adenine dinucleotide phosphate (NADPH)-oxidase, and included reduced thiol antioxidant concentrations and increased oxidised protein carbonyl concentrations. In female miR-146a mice, this increase in oxidative stress resulted in an increased expression of superoxide dismutase 1 (SOD1). Together, this suggests miR-146a plays a key role in regulating inflammation even in the absence of inflammatory stimuli and reduced levels of this miRNA have the capacity to induce limited behavioural effects whilst exacerbating both inflammation and oxidative stress in the brain

Spin correlated electronic state on the surface of a spin-orbit Mott system (Layered Iridates)

Novel phases of two dimensional electron systems resulting from new surface or interface modified electronic structures have generated significant interest in material science. We utilize photoemission spectroscopy to show that the near-surface electronic structure of a bulk insulating iridate Sr$_3$Ir$_2$O$_7$ lying near metal-Mott insulator transition exhibit weak metallicity signified by finite electronic spectral weight at the Fermi level. The surface electrons exhibit a unique spin structure resulting from an interplay of spin-orbit, Coulomb interaction and surface quantum magnetism, distinct from a topological insulator state. Our results suggest the experimental realization of a novel quasi two dimensional interacting electron surface ground state, opening the door for exotic quantum entanglement and transport phenomena in iridate-based oxide devices.Comment: 17 pages, 4 Figure

System of crop intensification for more productive, resource-conserving, climate-resilient, and sustainable agriculture: experience with diverse crops in varying agroecologies

With continually increasing demand for food accompanied by the constraints of climate change and the availability and quality of soil and water, the world’s farmers are challenged to produce more food per hectare with less water, and with fewer agrochemical inputs if possible. The ideas and methods of the system of rice intensification which is improving irrigated rice production are now being extended/adapted to many other crops: wheat, maize, finger millet, sugarcane, tef, mustard, legumes, vegetables, and even spices. Promoting better root growth and enhancing the soil’s fertility with organic materials are being found effective means for raising the yields of many crop plants with less water, less fertilizer, reduced seeds, fewer agrochemicals, and greater climate resilience. In this article, we review what is becoming known about various farmer-centred innovations for agroecological crop management that can contribute to agricultural sustainability. These changes represent the emerging system of crop intensification, which is being increasingly applied in Asian, African, and Latin American countries. More research will be needed to verify the efficacy and impact of these innovations and to clarify their conditions and limits. But as no negative effects for human or environmental health have been identified, making these agronomic options more widely known should prompt more investigation and, to the extent justified by results, utilization of these methodologies

GW190412: Observation of a Binary-Black-Hole Coalescence with Asymmetric Masses

We report the observation of gravitational waves from a binary-black-hole coalescence during the first two weeks of LIGO’s and Virgo’s third observing run. The signal was recorded on April 12, 2019 at 05∶30∶44 UTC with a network signal-to-noise ratio of 19. The binary is different from observations during the first two observing runs most notably due to its asymmetric masses: a ∼30 M_⊙ black hole merged with a ∼8 M_⊙ black hole companion. The more massive black hole rotated with a dimensionless spin magnitude between 0.22 and 0.60 (90% probability). Asymmetric systems are predicted to emit gravitational waves with stronger contributions from higher multipoles, and indeed we find strong evidence for gravitational radiation beyond the leading quadrupolar order in the observed signal. A suite of tests performed on GW190412 indicates consistency with Einstein’s general theory of relativity. While the mass ratio of this system differs from all previous detections, we show that it is consistent with the population model of stellar binary black holes inferred from the first two observing runs

Properties and Astrophysical Implications of the 150 M_⊙ Binary Black Hole Merger GW190521

The gravitational-wave signal GW190521 is consistent with a binary black hole (BBH) merger source at redshift 0.8 with unusually high component masses, 85⁺²¹₋₁₄ M_⊙ and 66⁺¹⁷₋₁₈ M_⊙, compared to previously reported events, and shows mild evidence for spin-induced orbital precession. The primary falls in the mass gap predicted by (pulsational) pair-instability supernova theory, in the approximate range 65–120 M_⊙. The probability that at least one of the black holes in GW190521 is in that range is 99.0%. The final mass of the merger 142⁺²⁸₋₁₆ M_⊙) classifies it as an intermediate-mass black hole. Under the assumption of a quasi-circular BBH coalescence, we detail the physical properties of GW190521's source binary and its post-merger remnant, including component masses and spin vectors. Three different waveform models, as well as direct comparison to numerical solutions of general relativity, yield consistent estimates of these properties. Tests of strong-field general relativity targeting the merger-ringdown stages of the coalescence indicate consistency of the observed signal with theoretical predictions. We estimate the merger rate of similar systems to be 0.13_(-0.11)^(+0.30) Gpc⁻³ yr⁻¹. We discuss the astrophysical implications of GW190521 for stellar collapse and for the possible formation of black holes in the pair-instability mass gap through various channels: via (multiple) stellar coalescences, or via hierarchical mergers of lower-mass black holes in star clusters or in active galactic nuclei. We find it to be unlikely that GW190521 is a strongly lensed signal of a lower-mass black hole binary merger. We also discuss more exotic possible sources for GW190521, including a highly eccentric black hole binary, or a primordial black hole binary

Diving below the spin-down limit:constraints on gravitational waves from the energetic young pulsar PSR J0537-6910

We present a search for continuous gravitational-wave signals from the young, energetic X-ray pulsar PSR J0537-6910 using data from the second and third observing runs of LIGO and Virgo. The search is enabled by a contemporaneous timing ephemeris obtained using NICER data. The NICER ephemeris has also been extended through 2020 October and includes three new glitches. PSR J0537-6910 has the largest spin-down luminosity of any pulsar and is highly active with regards to glitches. Analyses of its long-term and inter-glitch braking indices provided intriguing evidence that its spin-down energy budget may include gravitational-wave emission from a time-varying mass quadrupole moment. Its 62 Hz rotation frequency also puts its possible gravitational-wave emission in the most sensitive band of LIGO/Virgo detectors. Motivated by these considerations, we search for gravitational-wave emission at both once and twice the rotation frequency. We find no signal, however, and report our upper limits. Assuming a rigidly rotating triaxial star, our constraints reach below the gravitational-wave spin-down limit for this star for the first time by more than a factor of two and limit gravitational waves from the l = m = 2 mode to account for less than 14% of the spin-down energy budget. The fiducial equatorial ellipticity is limited to less than about 3 x 10⁻⁵, which is the third best constraint for any young pulsar

Constraints on the cosmic expansion history from GWTC-3

We use 47 gravitational-wave sources from the Third LIGO-Virgo-KAGRA Gravitational-Wave Transient Catalog (GWTC-3) to estimate the Hubble parameter $H(z)$, including its current value, the Hubble constant $H_0$. 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 $34\, {\rm M_\odot}$, followed by a drop-off. Assuming this mass scale does not evolve with redshift results in a $H(z)$ measurement, yielding $H_0=68^{+12}_{-7} {\rm km\,s^{-1}\,Mpc^{-1}}$ ($68\%$ credible interval) when combined with the $H_0$ measurement from GW170817 and its electromagnetic counterpart. This represents an improvement of 17% with respect to the $H_0$ 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 $H_0=68^{+8}_{-6} {\rm km\,s^{-1}\,Mpc^{-1}}$ with the galaxy catalog method, an improvement of 42% with respect to our GWTC-1 result and 20% with respect to recent $H_0$ 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 $H_0$) is the well-localized event GW190814