Friday, August 24, 2012

Congratulations to Dr. Lekh Nath Adhikari

We would like to congratulate Dr. Lekh Nath Adhikari for successfully defending his PhD dissertation from department of chemistry at University of Nevada, Reno. He has started working on the same department. We would also like to wish him a successful future ahead. Below is the abstract of his research work.


Reactions of simple amines, alcohols, ethers, and bi-functional molecules on the Si(100) -(2x1) surface were studied theoretically and experimentally. Additionally, theoretical calculations were performed for the interaction of several of these types of molecules on the 3C-SiC(100), 4H-SiC(1000), and 6H-SiC(1000) surfaces. The adsorption and desorption experiments on the Si(100)-(2x1) surface were performed in an ultra-high vacuum (UHV) chamber using Auger electron spectroscopy (AES), low-energy electron diffraction (LEED), and thermal desorption spectroscopy (TDS). Theoretical studies were performed for the adsorption of these molecules onto clusters that are representative of the Si(100)-(2x1), 3C-SiC(100)-(3x2), 4H-SiC(1000)-(2x2), and 6H-SiC(1000)-(3x3) surfaces using the Gaussian suite of programs.

AES studies showed a rapid increase in surface carbon and nitrogen signals for all amines studied and a similar increase in carbon and oxygen signals for all alcohols studied. The signals appear to level off with increasing dose in all cases, indicating surface saturation after room temperature adsorption of these molecules onto the Si(100)-(2x1) surface. Primary amines and alcohols give a saturation coverage of roughly one half of a monolayer, indicating one molecule reacting per silicon surface dimer, while mixed alcohol/amines (3-amino-propanol) and ethers, such as diethyl ether, dihydrofuran, and tetrahydrofuran, appear to have lower saturation coverages that depend on the identity of the adsorbing species.

All saturated primary amines (methylamine, ethylamine, and propylamine) studied showed a parent ion desorption peak in TDS, along with an imine formation channel. These are interpreted as arising from surface-bound alkyl amidogen radicals resulting from N-H bond cleavage upon adsorption on the Si(100)-(2x1) surface. Hydrogen elimination from a surface bound alkyl containing radical appears to be a common decomposition reaction, yielding imines in the case of adsorbed saturated primary amines, aldehydes in the case of adsorbed saturated alcohols, and alkenes in the case of adsorbed saturated ethers. Unsaturated amines and alcohols, however, appear to react with the surface to produce alkene products upon TDS, which must involve hydrogen addition instead of elimination. The energetics for these reactions, as revealed through TDS, are sensitive to the exact nature of the adsorbing radical species.

Theoretical studies of the interaction of amines and alcohols on the cubic SiC(100)-(3x2) surface showed similar results to those observed for these molecules on the Si(100)-(2x1) surface. However, the adsorbed products on the cubic SiC(100) surface were predicted to be slightly more stable than those on the Si(100) surface in all cases. Hexagonal SiC surfaces (4H- and 6H-) appear to be less reactive with water and ammonia than that of cubic surface based on these computational results.

Friday, August 10, 2012

Chemistry experiments on Mars by "Curiosity rover"

NASA's new Mars rover Curiosity has landed on Mars surface after a ~year journey (354 million miles) and already started sending photographs of the red planet. This $2.5 billion rover will stay in the red planet for 2 years and will explore and help us understand whether this planet has ever been able to support any kind of life. To answer this BIG question, Curiosity will collect rock/soil/dust samples and will perform whole bunch of analytical chemistry to analyse them.

Curiosity is basically an entire chemistry lab containing variety of 10 analytical equipments, which can test the chemical composition of soil, packed in one mobile unit. Lets see what analytical equipment it has and 
  1. The Chemistry and Mineralogy (CheMin) Instrument: It is a powder x-ray diffraction with x-ray fluorescence capabilities and will tell something about mineral composition of Mars.
  2. Chemistry and Camera (ChemCam) Instrument:  ChemCam fires invisible laser pulses at a target. It then views the resulting spark with a telescope and spectrometers to identify chemical elements. 
  3. The Sample Analysis at Mars (SAM) instrument:  It has three laboratory tools for analyzing chemistry. The tools will examine gases from the Martian atmosphere, as well as gases that ovens and solvents pull from powdered rock and soil samples. SAM focuses on the detection of organics and the characterization of compounds in the Martian soil that could be used as nutrients for life, in particular nitrates and perchlorates. 
  4. The Rover Environmental MonitoringStation (REMS) instrument: REMS will provide daily weather reports from the Red Planet. It consists of a suite of meteorological instruments that will record hourly measurements of wind, pressure, temperature, humidity, and ultra violet (UV) radiation. 

Watch these videos.


Test results from these instruments will pave the way for future Mars missions, and may provide insight in the search for life on other planets.


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