Radical-radical and radical-neutral interaction schemes are very important for the formation of comparatively complex molecules in low-temperature chemistry. The formation of amino acids, such as serine, in the interstellar medium is quite difficult. We explored the possibility of serine formation in the interstellar medium through detected interstellar molecules such as CH, CO, and OH by radical-radical and radical-neutral interactions in the gaseous phase using rigorous quantum-chemical calculations. The reaction energies, the low potential barrier and the structures of all the geometries involved in the reaction path show that serine formation is possible in interstellar space via the reaction paths
Context. Cytosine, thymine, and uracil are three of the five primary nucleobases that function as th...
Ph.D. (Chemistry)Abstract: “How the most essential life elements, i.e., amino-acids, were formed in ...
It is proposed that the glycine precursor NH2CH2CN may be synthesised in interstellar dust clouds by...
Radical-radical and radical-neutral interaction schemes are very important for the formation of comp...
The interstellar medium, the vast space between the stars, is a rich reservoir of molecular material...
Gas phase chemistry in the cold interstellar clouds is dominated by ion-molecule and radical-radical...
International audienceContext. Many organic molecules have been observed in the interstellar medium ...
Interstellar space is a notoriously harsh environment, where temperatures are known to be as low as ...
This work aims to understand the formation routes of a variety of interstellar molecules. The format...
For many years, scientists suspected that the interstellar medium was too hostile for organic specie...
Context. Many organic molecules have been observed in the interstellar medium thanks to advances in ...
Amino acids have been identified in carbonaceous chondrites, but their origin is yet unknown. Previo...
For many years, scientists suspected that the interstellar medium was too hostile for organic specie...
International audienceWork on the chemical evolution of pre-biotic molecules remains incomplete sinc...
none3noFor many years, scientists suspected that the interstellar medium was too hostile for organic...
Context. Cytosine, thymine, and uracil are three of the five primary nucleobases that function as th...
Ph.D. (Chemistry)Abstract: “How the most essential life elements, i.e., amino-acids, were formed in ...
It is proposed that the glycine precursor NH2CH2CN may be synthesised in interstellar dust clouds by...
Radical-radical and radical-neutral interaction schemes are very important for the formation of comp...
The interstellar medium, the vast space between the stars, is a rich reservoir of molecular material...
Gas phase chemistry in the cold interstellar clouds is dominated by ion-molecule and radical-radical...
International audienceContext. Many organic molecules have been observed in the interstellar medium ...
Interstellar space is a notoriously harsh environment, where temperatures are known to be as low as ...
This work aims to understand the formation routes of a variety of interstellar molecules. The format...
For many years, scientists suspected that the interstellar medium was too hostile for organic specie...
Context. Many organic molecules have been observed in the interstellar medium thanks to advances in ...
Amino acids have been identified in carbonaceous chondrites, but their origin is yet unknown. Previo...
For many years, scientists suspected that the interstellar medium was too hostile for organic specie...
International audienceWork on the chemical evolution of pre-biotic molecules remains incomplete sinc...
none3noFor many years, scientists suspected that the interstellar medium was too hostile for organic...
Context. Cytosine, thymine, and uracil are three of the five primary nucleobases that function as th...
Ph.D. (Chemistry)Abstract: “How the most essential life elements, i.e., amino-acids, were formed in ...
It is proposed that the glycine precursor NH2CH2CN may be synthesised in interstellar dust clouds by...