Carla Maria Coppola
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View article: Electron impact ro-vibrational transitions and dissociative recombination of H <sub>2</sub> <sup>+</sup> and HD <sup>+</sup>
Electron impact ro-vibrational transitions and dissociative recombination of H <sub>2</sub> <sup>+</sup> and HD <sup>+</sup> Open
Context . Molecular hydrogen and its cation H 2 + are among the first species formed in the early Universe, and play a key role in the thermal and chemical evolution of the primordial gas. In molecular clouds, H 2 + ions formed through ion…
View article: High‐Resolution On‐Chip Digitally Tunable Spectrometer Based on Double‐Cascaded Ring Resonators
High‐Resolution On‐Chip Digitally Tunable Spectrometer Based on Double‐Cascaded Ring Resonators Open
Fast and accurate detection and analysis of light spectrum emerge as an important tool in several scientific fields and applications, hence demanding the design of precise, reliable, and fast instruments. In this article, an integrated spe…
View article: Electron impact ro-vibrational transitions and dissociative recombination of H2+ and HD+: Rate coefficients and astrophysical implications
Electron impact ro-vibrational transitions and dissociative recombination of H2+ and HD+: Rate coefficients and astrophysical implications Open
Context. Molecular hydrogen and its cation H+2 are among the first species formed in the early Universe, and play a key role in the thermal and chemical evolution of the primordial gas. In molecular clouds, H+2 ions formed through ionizati…
View article: i-PHAOS: An Overview with an Open-Source Collaborative Database on Miniaturized Integrated Spectrometers
i-PHAOS: An Overview with an Open-Source Collaborative Database on Miniaturized Integrated Spectrometers Open
On-chip spectrometers are increasingly becoming tools that might help in everyday life needs. The possibility offered by several available integration technologies and materials to be used to miniaturize spectrometers has led to a plethora…
View article: i-PHAOS: An Overview with an Open-Source Collaborative Database on Miniaturized Integrated Spectrometers
i-PHAOS: An Overview with an Open-Source Collaborative Database on Miniaturized Integrated Spectrometers Open
On-chip spectrometers are increasingly becoming tools that might help in everyday life needs. The possibility offered by the several available integration technologies and materials to be used to miniaturize spectrometers has led to a plet…
View article: Collisional excitation of HD by H
Collisional excitation of HD by H Open
The HD molecule plays an important role in many astrophysical environments. Accurate modelling of the gas cooling induced by HD and its abundance in such media requires a proper modelling of its excitation by both radiative and collisional…
View article: The unbiased diffusion Monte Carlo: a versatile tool for two-electron systems confined in different geometries
The unbiased diffusion Monte Carlo: a versatile tool for two-electron systems confined in different geometries Open
View article: The unbiased Diffusion Monte Carlo: a versatile tool for two-electron\n systems confined in different geometries
The unbiased Diffusion Monte Carlo: a versatile tool for two-electron\n systems confined in different geometries Open
Computational codes based on the Diffusion Monte Carlo method can be used to\ndetermine the quantum state of two-electron systems confined by external\npotentials of various nature and geometry. In this work, we show how the\napplication o…
View article: Matrix formulation of the energy exchange problem of multi-level systems and the code FRIGUS
Matrix formulation of the energy exchange problem of multi-level systems and the code FRIGUS Open
View article: A database approach for materials selection for hydrogen storage in aerospace technology
A database approach for materials selection for hydrogen storage in aerospace technology Open
View article: Temperature and density dependent cooling function for H2 with updated H2/H collisional rates
Temperature and density dependent cooling function for H2 with updated H2/H collisional rates Open
The energy transfer among the components in a gas determines its fate. Especially at low temperatures, inelastic collisions drive the cooling and the heating mechanisms. In the early Universe as well as in zero- or low-metallicity environm…
View article: Non-thermal photons and direct photodissociation of H2, HD and HeH+ in the chemistry of the primordial Universe
Non-thermal photons and direct photodissociation of H2, HD and HeH+ in the chemistry of the primordial Universe Open
Non-thermal photons deriving from radiative transitions among the internal\nladder of atoms and molecules are an important source of photons in addition to\nthermal and stellar sources in many astrophysical environments. In the present\nwo…
View article: The CLT dataset for 7Li1H
The CLT dataset for 7Li1H Open
The dataset is an archive of ExoMol page, https://exomol.com/data/molecules/LiH/7Li-1H/CLT. Please check the reference details according to the following description or directly from the website.Definitions file:7Li-1H__CLT.defRoot referen…
View article: The CLT dataset for 7Li1H
The CLT dataset for 7Li1H Open
The dataset is an archive of ExoMol page, https://exomol.com/data/molecules/LiH/7Li-1H/CLT. Please check the reference details according to the following description or directly from the website.Definitions file:7Li-1H__CLT.defRoot referen…
View article: The CLT dataset for 7Li1H+
The CLT dataset for 7Li1H+ Open
The dataset is an archive of ExoMol page, https://exomol.com/data/molecules/LiH_p/7Li-1H_p/CLT.Please check the reference details according to the following description or directly from the website. NB: The html description skips d…
View article: The CLT dataset for 7Li1H+
The CLT dataset for 7Li1H+ Open
The dataset is an archive of ExoMol page, https://exomol.com/data/molecules/LiH_p/7Li-1H_p/CLT.Please check the reference details according to the following description or directly from the website. NB: The html description skips d…
View article: Constraining cloud parameters using high density gas tracers in galaxies
Constraining cloud parameters using high density gas tracers in galaxies Open
\n Far-infrared molecular emission is an important tool used to understand the excitation mechanisms of the gas in the interstellar medium (ISM) of star-forming galaxies. In the present work, we model the emission from rotational transitio…
View article: State-to-state vibrational kinetics of H<sub>2</sub>and H$_2^+$ in a post-shock cooling gas with primordial composition
State-to-state vibrational kinetics of H<sub>2</sub>and H$_2^+$ in a post-shock cooling gas with primordial composition Open
The radiative cooling of shocked gas with primordial chemical composition is an important process relevant to the formation of the first stars and structures, as well as taking place also in high-velocity cloud collisions and supernovae ex…
View article: Role of the $\mathrm{H}_2^+$ channel in the primordial star formation under strong radiation field and the critical intensity for the supermassive star formation
Role of the $\mathrm{H}_2^+$ channel in the primordial star formation under strong radiation field and the critical intensity for the supermassive star formation Open
We investigate the role of the $\\mathrm{H}_2^+$ channel on H2 molecule formation during the collapse of primordial gas clouds immersed in strong radiation fields which are assumed to have the shape of a diluted blackbody spectra with temp…
View article: Complementarity between Quantum and Classical Mechanics in Chemical Modeling. The H + HeH<sup>+</sup> → H<sub>2</sub><sup>+</sup> + He Reaction: A Rigourous Test for Reaction Dynamics Methods
Complementarity between Quantum and Classical Mechanics in Chemical Modeling. The H + HeH<sup>+</sup> → H<sub>2</sub><sup>+</sup> + He Reaction: A Rigourous Test for Reaction Dynamics Methods Open
In this work we present a dynamical study of the H + HeH+ → H2+ + He reaction in a collision energy range from 0.1 meV to 10 eV, suitable to be used in applicative models. The paper extends and complements a recent work [ Phys. Chem. Chem.…