Aims. This paper presents an ab initio characterization of linear isomers of C3Si, which are suitable species for astrophysical detection in carbon-rich sources. Methods. By the help of multiconfigurational calculations, two linear minima are characterized, namely l-SiCCC and l-CSiCC, whose relative energy is 3.3 eV, and their electronic ground states have X3Σ − symmetry, and their electronic spectra present a high density of electronic states at low energy. Anharmonic spectroscopic parameters are predicted for both isomers and for different isotopomers using second order perturbation theory and force fields derived form 6D-potential energy surfaces. Results. The fundamental frequencies of the IR active bendings are predicted to lie around ...
2382-2391The exploration of the potential energy surface of C3Si2H4, which is derived from the wel...
Small silicon-carbon clusters are important gas-phase constituents of stellar atmospheres, and are t...
The molecular equilibrium structures of two conformers (cis and gauche) of C<sub>3</sub>H<sub>5</sub...
Aims. This paper presents an ab initio characterization of linear isomers of C3Si, which are suitabl...
Aims. This paper presents an ab initio characterization of linear isomers of C3Si, which are suitabl...
Aims. This paper presents an ab initio characterization of linear isomers of C3Si, which are suita...
Author Institution: Departamento de Astrofisica Molecular e Infrarroja; Instituto de Estructura de l...
International audienceFor the most stable linear isomer of C3S in its X-1 Sigma(+) state a six- dime...
Silacyclopropynylidene, SiC2, is a known and highly abundant circumstellar molecule. Its spectrum ha...
The equilibrium geometries, excitation energies, force constants and vibrational frequencies for the...
International audienceUsing coupled-cluster approach full six-dimensional analytic potential energy ...
Small silicon carbides are of particular interest to the astrochemical community given the appearanc...
Molecular species of group 14 elements e.g. carbon, silicon, and germanium are well suited to study ...
Author Institution: Harvard-Smithsonian Center for Astrophysics; Harvard University; Division of Eng...
$^{1}$ J. Fulara, P. Freivogel, M. Grutter, and J. P. Maier, J. Phys. Chem. 100, 18042 (1996).Author...
2382-2391The exploration of the potential energy surface of C3Si2H4, which is derived from the wel...
Small silicon-carbon clusters are important gas-phase constituents of stellar atmospheres, and are t...
The molecular equilibrium structures of two conformers (cis and gauche) of C<sub>3</sub>H<sub>5</sub...
Aims. This paper presents an ab initio characterization of linear isomers of C3Si, which are suitabl...
Aims. This paper presents an ab initio characterization of linear isomers of C3Si, which are suitabl...
Aims. This paper presents an ab initio characterization of linear isomers of C3Si, which are suita...
Author Institution: Departamento de Astrofisica Molecular e Infrarroja; Instituto de Estructura de l...
International audienceFor the most stable linear isomer of C3S in its X-1 Sigma(+) state a six- dime...
Silacyclopropynylidene, SiC2, is a known and highly abundant circumstellar molecule. Its spectrum ha...
The equilibrium geometries, excitation energies, force constants and vibrational frequencies for the...
International audienceUsing coupled-cluster approach full six-dimensional analytic potential energy ...
Small silicon carbides are of particular interest to the astrochemical community given the appearanc...
Molecular species of group 14 elements e.g. carbon, silicon, and germanium are well suited to study ...
Author Institution: Harvard-Smithsonian Center for Astrophysics; Harvard University; Division of Eng...
$^{1}$ J. Fulara, P. Freivogel, M. Grutter, and J. P. Maier, J. Phys. Chem. 100, 18042 (1996).Author...
2382-2391The exploration of the potential energy surface of C3Si2H4, which is derived from the wel...
Small silicon-carbon clusters are important gas-phase constituents of stellar atmospheres, and are t...
The molecular equilibrium structures of two conformers (cis and gauche) of C<sub>3</sub>H<sub>5</sub...