Physics of the Dark Universe

Physics of the Dark Universe

  • Volume 4
  • Issue 4
  • ISSN 2212-6864
  • SCImago Journal Rank (SJR): 1.485
  • Source Normalized Impact per Paper (SNIP): 1.164
  • Impact Factor: 4.243
  • Five Year Impact Factor: 4.845
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Next planned ship date: Sep 22, 2021

Description

Physics of the Dark Universe is an innovative online-only journal that offers rapid publication of peer-reviewed, original research articles considered of high scientific impact.
The journal is focused on the understanding of Dark Matter, Dark Energy, Early Universe, gravitational waves and neutrinos, covering all theoretical, experimental and phenomenological aspects.

Physics of the Dark Universe encourages the submission of articles on the following subjects in this field:

Dark Matter:
  • Nature of particle Dark Matter
  • Direct searches
  • Indirect searches
  • Collider searches, including for example the Large Hadron Collider
  • New and existing models (e.g. SUSY, extra dimensions, axions, etc)
  • Low mass WIMP searches


  • Dark Energy:
  • Observations and experimental results
  • Forecast and design of new experiments
  • Models and theoretical properties of vacuum energy, quintessence, modified gravity, and in general of Dark Energy, cosmic acceleration and its alternative explanations


  • Early Universe:
  • Models and observational tests of Inflation


  • Dark Messengers:
  • Gravitational waves in cosmology
  • Cosmic neutrino background


  • In addition to submission of scientific papers in the usual formats, we encourage the submission of innovative articles, in the following forms:
  • Design Studies and Concept papers for new experiments or describing ideas for new experiments. In particular, experimental set up of the next generation of very large Dark Matter direct and indirect detectors, new underground laboratories for the study of Dark Matter, and new ground based or space based experiments on Dark Energy are particularly welcome. These articles can be longer than regular articles, describing the experiment while focusing on its scientific goals.
  • Software Description and Manuals can be published, if the software is proved to have scientific interest in the understanding of Dark Matter and Dark Energy. The paper can be enriched with (part of) the code itself, or the software and code can be separately published in the Open Access journal SoftwareX (https://www.journals.elsevier.com/softwarex/), which hosts software in a curated GitHub Repository.


  • Cover Images Credits: Photomultipliers, credits to XENON100 Collaboration; Cassiopea A, credits NASA/CXC/SAO/D.Patnaude et al; Millennium Simulation, credits Prof. Volker Springel; Bullet Cluster, credits: X-ray: NASA/CXC/CfA/M.Markevitch et al.; Optical: NASA/STScI; Magellan/U.Arizona/D. Clowe et al.; Lensing Map: NASA/STScI; ESO WFI; Magellan/U.Arizona/D.Clowe et al.

    Product details

    • SCImago Journal Rank (SJR): 1.485
    • Source Normalized Impact per Paper (SNIP): 1.164
    • Impact Factor: 4.243
    • Five Year Impact Factor: 4.845
    • ISSN: 2212-6864
    • Issues: 4
    • Volume: 4
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    Publication schedule

    Issue volumeIssue yearPlanned ship dateActual ship date
    31C2021Mar 19, 2021Mar 04, 2021
    32C2021Jun 24, 2021Jun 17, 2021
    33C2021Sep 22, 2021
    34C2021Dec 21, 2021
    35C2022Mar 28, 2022
    36C2022Jun 24, 2022
    37C2022Sep 23, 2022
    38C2022Dec 23, 2022