Streamer evolution arrest governed amplified AC breakdown strength of graphene and CNT colloids

The present article experimentally explores the concept of large improving the AC dielectric breakdown strength of insulating mineral oils by the addition of trace amounts of graphene or CNTs to form stable dispersions. The nano-oils infused with these nanostructures of high electronic conductance indicate superior AC dielectric behaviour in terms of augmented breakdown strength compared to the base oils. Experimental observations of two grades of synthesized graphene and CNT nano-oils show that the nanomaterials not only improve the average breakdown voltage but also significantly improve the reliability and survival probabilities of the oils under AC high voltage stressing. Improvement of the tune of ~ 70-80 % in the AC breakdown voltage of the oils has been obtained via the present concept. The present study examines the reliability of such nano-colloids with the help of two parameter Weibull distribution and the oils show greatly augmented electric field bearing capacity at both standard survival probability values of 5 % and 63.3 %. The fundamental mechanism responsible for such observed outcomes is reasoned to be delayed streamer development and reduced streamer growth rates due to effective electron scavenging by the nanostructures from the ionized liquid insulator. A mathematical model based on the principles of electron scavenging is proposed to quantify the amount of electrons scavenged by the nanostructures. The same is then employed to predict the enhanced AC breakdown voltage and the experimental values are found to match well with the model predictions. The present study can have strong implications in efficient, reliable and safer operation of real life AC power systems

Structural domain and spin ordering induced glassy magnetic phase in single layered manganite Pr0.22_{0.22}Sr1.78_{1.78}MnO4_4

The single layered manganite Pr$_{0.22}$Sr$_{1.78}$MnO$_4$ undergoes structural transition from high temperature tetragonal phase to low temperature orthorhombic phase below room temperature. The orthorhombic phase was reported to have two structural variants with slightly different lattice parameters and Mn-3$d$ levels show orbital ordering within both the variants, albeit having mutually perpendicular ordering axis. In addition to orbital ordering, the orthorhombic variants also order antiferromagnetically with different N\'eel temperatures. Our magnetic investigation on the polycrystalline sample of Pr$_{0.22}$Sr$_{1.78}$MnO$_4$ shows large thermal hysteresis indicating the first order nature of the tetragonal to orthorhombic transition. We observe magnetic memory, large relaxation, frequency dependent ac susceptbility and aging effects at low temperature, which indicate spin glass like magnetic ground state in the sample. The glassy magnetic state presumably arises from the interfacial frustration of orthorhombic domains with orbital and spin orderings playing crucial role toward the competing magnetic interactions.Comment: 6 pages, 4 figures, Accepted in Europhysics Letter

Incidence of Chirodiscoides caviae in Laboratory Rats-Screening, Identification and Treatment

This is a report on the incidence and treatment of the guinea pig fur mite Chirodiscoides caviae, which  was so far considered as host specific, in a conventional colony of laboratory rats. Chirodiscoides caviae  infestation in laboratory rats was accidentally observed during the screening of Syphacia obvelata by the  peri-anal cellophane tape test (CTT). The organism was identified by comparing the morphology described  by various researchers and was differentially diagnosed from other common mites of rat, Radfordia ensifera  and Notoedres muris. The adult male mites (n=15) were of 330.2±13.3 μm long and the females (n=15)  495.5±25.2 μm. Later on, the entire rat colony consisting of Wistar, Sprague Dawley and Spontaneously  Hypertensive Rats (SHR) and the mice colony of Balb/c and Swiss Albino were randomly sampled and  screened for the presence of the mite by the cellophane tape technique. All the rat strains were found positive  for C. caviae infestation, which was more concentrated towards the posterior region of the body and,  collectively, the screening results of C. caviae revealed that the posterio-dorsal and peri-anal regions are  most suitable for sampling-suggesting that, the infestation pattern of C. caviae in rats has similarities to that  of guinea pigs. Interestingly the mice colony was found free from the infestation. The Cellophane tape test was found to be an easier method than fur examination by hair plucking and equally  accurate for screening of fur mite in a colony of laboratory rats. No clinical symptoms were observed in  any of the animals in the colony, which possessed infestation. The facility strictly practised physical separation  of animals by species, which pointed to the only possibility of cross infestation being through indirect  contact between guinea pigs and laboratory rats and thereby questioning previous reports on the mode of  transmission of C. caviae. The entire colony was effectively treated with 0.2% Ivermectin spray followed by  1% spray in an interval of 2 weeks. This report is the first one, which demonstrates the guinea pig fur mite  in laboratory rats. It also questions the so far documented “host specificity” and “direct contact” mode of  transmission and demonstrates indirect contact as a possible mode of transmission.

The non-linear behavior of the black hole system GRS 1915+105

Using non-linear time series analysis, along with surrogate data analysis, it is shown that the various types of long term variability exhibited by the black hole system GRS 1915+105, can be explained in terms of a deterministic non-linear system with some inherent stochastic noise. Evidence is provided for a non-linear limit cycle origin of one of the low frequency QPO detected in the source, while some other types of variability could be due to an underlying low dimensional chaotic system. These results imply that the partial differential equations which govern the magneto-hydrodynamic flow of the inner accretion disk, can be approximated by a small number ($\approx 3 -5$) of non-linear but {\it ordinary} differential equations. While this analysis does not reveal the exact nature of these approximate equations, they may be obtained in the future, after results of magneto-hydrodynamic simulation of realistic accretion disks become available.Comment: Accepted for publication in ApJ. Numerical code that is used in the analysis is available at http://www.iucaa.ernet.in/~rmisra/NL