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M

M.-L. Dubernet

Researcher at Janssen Pharmaceutica

Publications -  10
Citations -  617

M.-L. Dubernet is an academic researcher from Janssen Pharmaceutica. The author has contributed to research in topics: Potential energy surface & Hyperfine structure. The author has an hindex of 9, co-authored 10 publications receiving 608 citations. Previous affiliations of M.-L. Dubernet include Pierre-and-Marie-Curie University.

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Journal ArticleDOI

Rotational excitation of ortho-H$_{2}$O by para-H$_{2}$ (j$_{2}$ = 0, 2, 4, 6, 8) at high temperature

TL;DR: In this paper, the authors presented state-to-state rate coefficients among the 45 lowest levels of o-H2O with H2(j2 = 0) and Δj2= 0, +2, as well as with H 2(j 2 = 2) and δj2 ≥ 0, − 2a ndj2 = 2 with Δj 2 ≥ 2.
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Collisional excitation rate coefficients of N2H+ by He

TL;DR: Using a recoupling technique with close-coupling spin-free calculations de-excitation rate coefficients are obtained among hyperfine transitions for He colliding with N 2 H +, and a recently determined potential energy surface suitable for scattering calculations is used to investigate rate coefficients for temperatures between 5 and 50 K as mentioned in this paper.
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The Excitation of N2H+ in Interstellar Molecular Clouds. I. Models

TL;DR: In this article, a large velocity gradient and nonlocal radiative transfer calculations involving the rotational and hyperfine structure of the spectrum of N2H+ with collisional rate coefficients were presented.
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Influence of a new potential energy surface on the rotational (de)excitation of H2O by H2 at low temperature

TL;DR: In this article, a newly determined 5D potential energy surface for H2-H2O was used to provide an extended and revised set of rate coefficients for de-excitation of the lowest 10 para- and 10 ortho- rotational levels of H2O by collisions with para-(j=0) and orthoH2(j=1), for kinetic temperatures from 5 K to 20 K.
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The excitation of n2h + in interstellar molecular clouds. ii. observations

TL;DR: In this paper, the rotational transitions of N2H+ and N2D+ toward a sample of prototypical dark clouds have been interpreted using nonlocal radiative transfer models.