Chromatographic Separation of Te(IV) & Te(VI)

443-44

Separation of Chromium(III) & Chromium(VI) from Their Binary Mixture by Paper & Thin Layer Chromatographic Techniques

282-28

Effect of calcium channel blocker as anticonvulsant and its potentiating effect when used along with sodium valproate in pentylenetetrazole induced seizures in Albino rats

Background: Many antiepileptic drugs were introduced for the treatment of epilepsy. Ideal antiepileptic drug should not only prevent but also correct the underlying pathophysiology without altering the normal neurotransmission. Calcium channel blockers may form such group because initiation of seizure is associated intrinsic burst firing which is triggered by large inward calcium current, so this study was done to evaluate the anticonvulsant effect of amlodipine in albino rats.Methods: A total of 42 adult albino rats were included in the study and divided into 7 groups, each containing 6 rats. Group 1 received distilled water, group 2,3 received sodium valproate 50mg/kg and 100mg/kg, group 4-6 received amlodipine 1, 2, 4mg/kg and group 7 received combination of Amlodipine 1 mg/kg and sodium valproate 50mg/kg. Pentylenetetrazole induced seizures model was done and onset of myoclonic jerks, onset of clonic convulsions and duration of clonic convulsions was studied.Results: There was a significant anticonvulsant effect in Amlodipine doses 2, 4mg/kg (p <0.001). The combination of Amlodipine (1mg/kg) and Sodium valproate (50mg/kg) also had significant anticonvulsant effect.Conclusions: Amlodipine, a calcium channel blocker has anticonvulsant effect and also potentiated the anticonvulsant effect of low dose sodium valproate

Anterior Segmental Distraction Osteogenesis in the Hypoplastic Cleft Maxilla : Report of five cases

Orthognathic surgery and distraction osteogenesis play a prime role in the correction of maxillary hypoplasia in patients with cleft lip and palate (CLP). Advancement of the anterior maxilla alone without interfering with the velopharyngeal sphincter may be advantageous in cleft patients, who more commonly have speech deficits and dental crowding. We present a case series of anterior maxillary segmental distraction for maxillary hypoplasia in 5 CLP patients with a one-year follow-up. A custom-made tooth-borne distraction device with a hyrax screw positioned anteroposteriorly was used. The evaluation comprised of hard and soft tissue analysis and speech assessment. A stable occlusion with positive overjet and correction of dental-crowding without extraction was achieved at one year post-distraction. Facial profile and lip support improved. There was no deterioration in speech

Infrared attenuation due to phase change from amorphous to crystalline observed in astrochemical propargyl ether ices

Astrochemical ices are known to undergo morphological changes, from amorphous to crystalline, upon warming the ice from lower (10 K) to higher temperatures. Phase changes are mostly identified by the observation of significant changes in the InfraRed (IR) spectrum, where the IR bands that are broad in the amorphous phase are narrower and split when the ice turns crystalline. To-date all the molecules that are studied under astrochemical conditions are observed to follow such a behaviour without significant attenuation in the IR wavelength. However, in this paper we report a new observation when propargyl ether ($C_3H_3OC_3H_3$) is warmed from the amorphous phase, at 10 K, through the phase transition temperature of 170 K, the crystalline ice being found to strongly attenuate IR photons at the mid-IR wavelengths

Residue from vacuum ultraviolet irradiation of benzene ices: Insights into the physical structure of astrophysical dust

We have irradiated benzene ices deposited at 4 K on a cold, interstellar dust analog with vacuum ultraviolet (9 eV) irradiation for periods lasting from several hours to nearly a day, after which the irradiated ice was warmed to room temperature. Vacuum ultraviolet photoabsorption spectra of the aromatic residue left at room temperature were recorded and showed the synthesis of benzene derivatives. The residue was also imaged using an electron microscope and revealed crystals of various sizes and shapes. The result of our experiments suggests such geometrically shaped dust particles may be a key component of interstellar dust

Experimental and Computational Study of Ethanolamine Ices under Astrochemical Conditions

Ethanolamine (NH2CH2CH2OH) has recently been identified in the molecular cloud G+0.693-0.027, situated in the SgrB2 complex in the Galactic center. However, its presence in other regions, and in particular in star-forming sites, is still elusive. Given its likely role as a precursor to simple amino acids, understanding its presence in the star-forming region is required. Here, we present the experimentally obtained temperature-dependent spectral features and morphological behavior of pure ethanolamine ices under astrochemical conditions in the 2–12 μm (MIR) and 120–230 nm (VUV) regions for the first time. These features would help in understanding its photochemical behavior. In addition, we present the first chemical models specifically dedicated to ethanolamine. These models include all the discussed chemical routes from the literature, along with the estimated binding energies and activation energies from quantum chemical calculations reported in this work. We have found that surface reactions CH2OH + NH2CH2 → NH2CH2CH2OH and NH2 + C2H4OH → NH2CH2CH2OH in warmer regions (60–90 K) could play a significant role in the formation of ethanolamine. Our modeled abundance of ethanolamine complements the upper limit of ethanolamine column density estimated in earlier observations in hot core/corino regions. Furthermore, we provide a theoretical estimation of the rotational and distortional constants for various species (such as HNCCO, NH2CHCO, and NH2CH2CO) related to ethanolamine that have not been studied in existing literature. This study could be valuable for identifying these species in the future