Evidence map›Paper›PMID 34318825›Full record

ArticlePhysical chemistry chemical physics : PCCP2021

A method for calculating temperature-dependent photodissociation cross sections and rates.

Marco Pezzella, Sergei N Yurchenko, Jonathan Tennyson

Abstract read
In one paragraph

Article in Physical chemistry chemical physics : PCCP, 2021. The graph could read no effect estimate from its abstract, so it casts no vote on the map. Cited by 6 papers.

0numbers the graph read from it
0cells of the map it votes in
6citing papers in PubMed
–field-weighted citation impact
1 · What the graph read from it

What it found

Each row is one number read from the abstract, on the scale the paper reported it, with its interval. Left of the dashed line favours the treatment, right favours the comparator. Under each row is the sentence it came from. New to these charts? A ten-minute tutorial.

The abstract states no effect estimate the extractor could read, or names no intervention and outcome on the map, so this paper lights no cell and moves no belief. It is still indexed, cited and linked below.

2 · The registry

The trial behind it

Trials whose registry record cites this paper, or whose number appears in the abstract. A trial that started after this paper was published is citing it as background, not reporting it.

Neither the registry nor the abstract names a trial number. If this is a trial report, that itself is worth knowing.

3 · Its place in the literature

Who cites it

6 citing papers in PubMed.

  1. Non-adiabatic effects in the photodissociation of HPhysical chemistry chemical physics : PCCP · 2026
    Article
  2. First Principles Rovibronic Absorption Spectra of HF Molecule.Journal of computational chemistry · 2026
    Article
  3. Theoretical investigation of the APhysical chemistry chemical physics : PCCP · 2025
    Article
  4. Article
  5. AnPhysical chemistry chemical physics : PCCP · 2022
    Article
  6. Article
4 · The record

Corrections and comments

PubMed lists nothing against this paper. Absence here is not a guarantee, only a check that was made.

5 · Who and what money

Authors and funding

3 authors.

Marco PezzellaDepartment of Physics & Astronomy, University College London, London WC1E 6BT, UK. j.tennyson@ucl.ac.uk.ORCID http://orcid.org/0000-0003-2902-309X
Sergei N YurchenkoDepartment of Physics & Astronomy, University College London, London WC1E 6BT, UK. j.tennyson@ucl.ac.uk.ORCID http://orcid.org/0000-0001-9286-9501
Jonathan TennysonDepartment of Physics & Astronomy, University College London, London WC1E 6BT, UK. j.tennyson@ucl.ac.uk.ORCID http://orcid.org/0000-0002-4994-5238

Funding

No grant is acknowledged in the PubMed record.

6 · The paper itself

Abstract

The destruction of molecules by photodissociation plays a major role in many radiation-rich environments, including the evolution of the atmospheres of exoplanets, which often exist close to UV-rich stars. Most current photodissociation calculations and databases assume T = 0 K, which is inadequate for hot exoplanets and stars. A method is developed for computing photodissociation spectra of diatomic molecules as a function of temperature exploiting bound state variational nuclear motion program Duo and post-processing program ExoCross. Discrete transition intensities are spread out to represent a continuous photodissociation spectrum either by Gaussian smoothing or by averaging calculations over a range of different grid sizes. Our approach is tested on four different chemical species (HCl, HF, NaCl and BeH+), showing its ability to reproduce photodissociation cross sections and rates computed with other approaches and experiment. The temperature dependence of photodissociation cross sections and rates is studies showing strong temperature variation of the photodissociation cross sections.

Identifiers

PMID34318825
PMCPMC8972202

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Read under generation 80e0d062 · epoch 390. Bibliography from PubMed, PubMed Central and OpenAlex; grants from NIH RePORTER; trial links from ClinicalTrials.gov; estimates, votes and beliefs from the OpenQuestion graph.