Galaxies Observation and Theoretical Features
A special issue of Galaxies (ISSN 2075-4434).
Deadline for manuscript submissions: closed (30 September 2021) | Viewed by 864
Special Issue Editors
2. ICRA-International Center for Relativistic Astrophysics C/O Physics Department, Sapienza University of Rome, Piazzale Aldo Moro, 5-00185 Rome, Italy
3. ICRANet- International Center for Relativistic Astrophysics Network, Piazza della Repubblica, 65122 Pescara, Italy
Interests: physics; mathematics
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Interests: general relativity theory; quantum gravity; astrophysics
2. Virtual Institute of Astroparticle Physics, 75018 Paris, France
3. Principal Researcher, Institute of Physics, Southern Federal University, Rostov on Don, Russia
Interests: cosmology; particle physics; beyond standard models; cosmoparticle physics; dark matter; primordial black holes; antimatter
Special Issues, Collections and Topics in MDPI journals
Special Issue Information
Dear Colleagues,
Galaxies observation has posed many new experimental challenges and produced new theoretical explanations that have not yet been completely confirmed. As far as the observation of galaxies is concerned, we have not yet established the nature of the central objects of galaxies, the galactic media, the nature of the galaxies rotation curves both for circular galaxies and for elliptical galaxies, and the constitution of the related intergalactic media. A consistent theoretical framework in which the observational evidence is captured has not been constructed. The elements obtained in the observational tests are characterized by parameters that are aimed at determining the structure of the celestial manifestations.
The search for pertinent consistent theoretical schemes has not yet reached modellization. Experimental observation has provided data that have not permitted the implementation of a clarified description of the galactic objects. The parameters requiring theoretical explanations have not been definitively verified. The techniques for the analysis of the observational data as well as for the estimation of the noise effects have not been refined. No definitive approach exists to the schematization of the theoretical and observed patterns, corresponding to a complete formulation of a consequential theoretical system. A consistent theoretical structure able to explain the formation galaxies, their composition, and evolution has not attained a complete formulation.
The structure and evolution of galaxies is strongly determined by the properties of dark matter and the exploration of galaxies can shed light on its physical nature involving methods of cosmoparticle physics of cross-disciplinary study of new physics in proper combination of its physical, astrophysical and cosmological signatures.
The papers of invited authors will be published, free of charge, with full open access after peer review to benefit both authors and readers.
Prof. Orchidea Maria Lecian
Prof. Alexander Al'bertovic Kirillov
Prof. Dr. Maxim Yu. Khlopov
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. Galaxies is an international peer-reviewed open access semimonthly journal published by MDPI.
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