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Pandey, S. K.

Publications and source records attributed to Pandey, S. K..

Ultrafast optical message encryption–decryption system using semiconductor optical amplifier based XOR logic gate

Encryption of information is required to secure data transmitted in optical networks. In this communication, authors propose simple and novel scheme for all-optical encryption–decryption at 120 Gb/s. Encryption–decryption system is based on XOR logic designed using semiconductor optical amplifier (SOA) based Mach–Zehnder interferometers. SOA model is presented theoretically from the stand point of high-speed application and implemented in encryption decryption setups for simulation. Extinction ratio for encrypted and decrypted signal is obtained as 10.5 dB and 8.30 dB respectively with satisfactory quality factor. The system has simple, compact architecture and easily integrable with other photonic devices.

71 CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSIC↗

Modeling and design of tin doped group IV alloy based QWEAM

This work investigates vital characteristics of tin doped group IV based quantum well for its potential as an electroabsorption modulator (EAM). Absorption coefficient and refractive index variation in proposed EAM structure are evaluated and studied under variation of electric field. Performance parameters like extinction ratio, chirp factor, etc. are calculated for different electric fields and Sn content of GeSn quantum well. A significant negative chirp and high extinction ratio has been obtained at midinfrared range of wavelength. The result reveals that appropriate selection of external field and Sn content plays a decisive role in the performance of QWEAM. Moreover, there is a tradeoff between extinction ratio and insertion loss on increasing length of the modulator.

71 CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSIC↗

Isophotal shapes of early-type galaxies to very faint levels

We report on a study of the isophotal shapes of early-type galaxies to very faint levels, reaching ∼0.1% of the sky brightness. The galaxies are from the Large Format Camera (LFC) fields obtained using the Palomar 5 m Hale Telescope, with integrated exposures ranging from 1 to 4 hr in the Sloan Digital Sky Survey r, i, and z bands. The shapes of isophotes of early-type galaxies are important, as they are correlated with the physical properties of the galaxies and are influenced by galaxy formation processes. In this paper, we report on a sample of 132 E and SO galaxies in one LFC field. We have redshifts for 53 of these, obtained using AAOmega on the Anglo-Australian Telescope. The shapes of early-type galaxies often vary with radius. We derive average values of isophotal shape parameters in four different radial bins along the semi-major axis in each galaxy. We obtain empirical fitting formulae for the probability distribution of the isophotal parameters in each bin and investigate for possible correlations with other global properties of the galaxies. Our main finding is that the isophotal shapes of the inner regions are statistically different from those in the outer regions. This suggests that the outer and inner parts of early-type galaxies have evolved somewhat independently.

79 ASTRONOMY AND ASTROPHYSICS↗