First Principles LCGO Calculation of the Magneto-optical Properties of Nickel and Iron

We report a first principles, self-consistent, all electron, linear combination of Gaussian orbitals (LCGO) calculation of a comprehensive collection of magneto-optical properties of nickel and iron based on density functional theory. Among the many magneto-optical effects, we have studied the equatorial Kerr effect for absorption in the optical as well as soft X-ray region, where it is called X-ray magnetic linear dichroism (X-MLD). In the optical region the effect is of the order of 2\% while in the X-ray region it is of the order of 1\% for the incident angles considered. In addition, the polar Kerr effect, X-ray magnetic circular dichroism (X-MCD) and total X-ray absorption at the L$_{2,3}$ edges, soft X-ray Faraday effect at the L$_{2,3}$ edges have also been calculated. Our results are in good agreement with experiments and other first principles methods that have been used to calculate some of these properties.Comment: 22 pages RevTex. 8 figures submitted separately as a uuencoded, compressed tar fil

HI gas in rejuvenated radio galaxies: GMRT observations of the DDRG J1247+6723

We report the detection of HI absorption towards the inner double of the double-double radio galaxy (DDRG) J1247+6723 with the Giant Metrewave Radio Telescope (GMRT). The inner double is a Giga-hertz peaked spectrum (GPS) source with a linear size of 14 pc while the overall size defined by the outer double is 1195 kpc, making it a giant radio source. The absorption profile is well resolved and consists of a number of components on either side of the optical systemic velocity. The neutral hydrogen column density is estimated to be N(HI)=6.73*10^{20}(T_s/100)(f_c/1.0) cm^{-2}, where T_s and f_c are the spin temperature and covering factor of the background source respectively. We explore any correlation between the occurrence of HI absorption and rejuvenation of radio activity and suggest that there could be a strong relationship between them.Comment: 5 pages, 2 figures, accepted for publication in MNRAS Letter

Detecting cold gas at intermediate redshifts: GMRT survey using Mg II systems

Intervening HI 21-cm absorption systems at z > 1.0 are very rare and only 4 confirmed detections have been reported in the literature. Despite their scarcity, they provide interesting and unique insights into the physical conditions in the interstellar medium of high-z galaxies. Moreover, they can provide independent constraints on the variation of fundamental constants. We report 3 new detections based on our ongoing Giant Metrewave Radio Telescope (GMRT) survey for 21-cm absorbers at 1.10< z_abs< 1.45 from candidate damped Lyman_alpha systems. The 21-cm lines are narrow for the z_abs = 1.3710 system towards SDSS J0108-0037 and z_abs = 1.1726 system toward SDSS J2358-1020. Based on line full-width at half maximum, the kinetic temperatures are <= 5200 K and <=800 K, respectively. The 21-cm absorption profile of the third system, z_abs =1.1908 system towards SDSS J0804+3012, is shallow, broad and complex, extending up to 100 km/s. The centroids of the 21-cm lines are found to be shifted with respect to the corresponding centroids of the metal lines derived from SDSS spectra. This may mean that the 21-cm absorption is not associated with the strongest metal line component.Comment: 13 pages with 5 figures. Accepted for publication in ApJ

A study to evaluate the immediate effect of proprioceptive neuromuscular facilitation versus active dynamic stretching during warm-up on 20-meter sprint in amateur soccer players

Background: Soccer is a highly popular sport and is played worldwide. It is an explosive sport and has a high incidence of injuries. In soccer, sprinting dominates the majority of the game, and it imposes a demand on players to have strong, flexible, and dynamic lower limbs. Amateur soccer players don’t usually practice warm-ups before their matches; hence, an appropriate warm-up protocol is required that can be incorporated into the training routine of players to avoid injuries and improve performance. The current study aims to evaluate and compare the immediate effect of PNF stretching versus active dynamic stretching during warm-up on 20-meter sprint performance in amateur soccer players. Methods: According to the inclusion criteria, 80 amateur soccer players participated in this cross-sectional study design. They were randomly distributed into 2 groups: A) PNF stretching (N = 40) and B) active dynamic stretching (N = 40). Participants in both groups performed the 20-meter sprint test initially, followed by their respective warm-up intervention, after which the 20-meter sprint test was repeated and new readings were recorded. Results: Both Group A and Group B showed improved performance; however, Group B was significantly better. (p value&lt;0.05). Conclusions: This study therefore concludes that both PNF and active dynamic stretching can be used as a warm-up protocol. However, according to the inter-group comparison, active dynamic stretching shows a noteworthy improvement in 20-m sprint performance in amateur soccer players

Unification scheme and the distribution of neutral gas in compact radio sources

We examine the consistency of HI properties with the unification scheme for radio galaxies and quasars, and any correlation with the symmetry parameters for a sample of CSS and GPS sources. In our sample, 15 out of 23 galaxies exhibit 21-cm absorption as against 1 out of 9 quasars, which is broadly consistent with the unification scheme. Also there is a tendency for the detection rate as well as the column density for galaxies to increase with core prominence, f_c, a statistical indicator of the orientation of the jet axis to the line of sight. This can be understood in a scenario where radio sources are larger than the scale of the circumnuclear HI disk so that the lines of sight to the lobes at very large inclinations do not intersect the disk. The sources in our sample also exhibit the known anti-correlation between HI column density and source size. This suggests that small linear size, along with intermediate values of core prominence, is a good recipe for detecting 21-cm absorption in CSS and GPS objects. Some of the absorption could also be arising from clouds which may have interacted with the radio jet. The HI column density and velocity shift of the primary absorption component, however, show no dependence on the degree of misalignment and the separation ratio of the radio sources.Comment: 6 pages, 4 figures, accepted for publication in MNRA