Nature and Origin of Dark Matter and Dark Energy II

A special issue of Symmetry (ISSN 2073-8994). This special issue belongs to the section "Physics".

Deadline for manuscript submissions: 31 March 2025 | Viewed by 93

Special Issue Editors


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Guest Editor
1. Ronin Institute for Independent Scholarship, 127 Haddon Pl., Montclair, NJ 07043, USA
2. Institute for Advanced Physical Studies, Boulevard “Tsarigradsko Shose” 111, Sofia 1784, Bulgaria
Interests: nuclear and particle physics; theoretical and mathematical physics; gravity and general relativity; cosmology and astrophysics
Special Issues, Collections and Topics in MDPI journals

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Guest Editor
1. Insitute of Cosmology and Gravitation, University of Portsmouth, Portsmouth PO1 3FX, UK
2. Institute of Space Sciences (ICE, CSIC), 08193 Barcelona, Spain
3. Institut d Estudis Espacials de Catalunya (IEEC), 08034 Barcelona, Spain
Interests: cosmology; dark cosmos; large scale structure of the universe

Special Issue Information

Dear Colleagues,

Dark matter (DM) and dark energy (DE) are the two most challenging problems in contemporary physics and astrophysics. DM and DE constitute about 95% of the Universe's energy content, but their nature remains unknown. Supporting evidence for DM has been obtained from astronomical observations of the rotation curve of galaxies, the growth of the density fluctuations in the Universe, gravitational lenses, Cosmic Microwave Background (CMB) fluctuations, etc. DE evidence originates from the observed acceleration of the expansion of the Universe. For over three decades, studies in large particle physics labs like CERN have failed to identify the nature of DM and DE. On the theoretical side, physicists have explored two main avenues: the existence of unknown particles and modifications to fundamental symmetry properties in gravitational theory and cosmology.

This Special Issue of Symmetry is devoted to presenting both new results on the observational constraints of dark matter and dark energy and new theoretical interpretations regarding their nature and origin.

Dr. Vesselin Gueorguiev
Prof. Dr. Enrique Gaztanaga
Guest Editors

Manuscript Submission Information

Manuscripts should be submitted online at www.mdpi.com by registering and logging in to this website. Once you are registered, click here to go to the submission form. Manuscripts can be submitted until the deadline. All submissions that pass pre-check are peer-reviewed. Accepted papers will be published continuously in the journal (as soon as accepted) and will be listed together on the special issue website. Research articles, review articles as well as short communications are invited. For planned papers, a title and short abstract (about 100 words) can be sent to the Editorial Office for announcement on this website.

Submitted manuscripts should not have been published previously, nor be under consideration for publication elsewhere (except conference proceedings papers). All manuscripts are thoroughly refereed through a single-blind peer-review process. A guide for authors and other relevant information for submission of manuscripts is available on the Instructions for Authors page. Symmetry is an international peer-reviewed open access monthly journal published by MDPI.

Please visit the Instructions for Authors page before submitting a manuscript. The Article Processing Charge (APC) for publication in this open access journal is 2400 CHF (Swiss Francs). Submitted papers should be well formatted and use good English. Authors may use MDPI's English editing service prior to publication or during author revisions.

Keywords

  • dark matter
  • dark energy
  • cosmology
  • galaxies
  • CMB
  • universe
  • expansion
  • cosmological constant

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Published Papers

This special issue is now open for submission.
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