Alternative Interpretations of Observed Galactic Behaviors

A special issue of Galaxies (ISSN 2075-4434).

Deadline for manuscript submissions: 15 December 2024 | Viewed by 81

Special Issue Editors


E-Mail Website
Guest Editor
Department of Earth and Planetary Sciences, Washington University in Saint Louis, Louis, MO 63130, USA
Interests: heat transport; spectroscopy; classical physics; thermodynamics; inverse problems
Special Issues, Collections and Topics in MDPI journals

E-Mail Website
Guest Editor
Department of Earth and Planetary Sciences, Washington University in Saint Louis, Louis, MO 63130, USA
Interests: heat transport; spectroscopy; classical physics; thermodynamics; inverse problems
Special Issues, Collections and Topics in MDPI journals

Special Issue Information

Dear Colleagues,

The goal of this Special Issue is to stimulate discussion on a key issue in galactic astronomy. Namely, non-baryonic dark matter (NBDM) is now central to both modern cosmologic models and many models of galactic evolution. Yet, neither experimental confirmation nor direct observational evidence for NBDM exist, despite decades of concerted and expensive efforts (Acdermann et al., 2014; Giagu, 2019). Moreover, NBDM was invoked ~50 years ago to explain why galactic rotational velocities differ from the radial pattern of our solar system (Rubin and Foord, 1970) and became entrenched well before several authors proved both analytically and numerically that galactic rotation curves are wholly consistent with normal matter and ordinary gravitational forces, e.g., Feng and Gallo, 2014; Criss and Hofmeister, 2020; and Sipols and Pavlovich, 2020.

Consensus now describes the vast majority of publications in modern sciences (Park et al., 2023), and NBDM provides another example.  New ideas and alternative explanations of observations are now hidden in the immense and growing scientific literature. Conformity inherent in consensus impedes progress. Historic examples include widespread beliefs in geocentrism, caloric, indivisible atoms, and perpetual motion.  

Hence, we solicit exposés of new interpretations of galactic behaviors that are connected directly or indirectly with the postulated existence of NBDM. We also solicit alternative explanations of the redshift because popular cosmological models, which rest on the redshift being a Doppler effect, also require dark matter (Gupta, 2024), which is considered a reason for its existence.

We hope that this volume will feature papers that provide quantitative, parsimonious analyses of available data and observations on a specific galactic phenomenon. Transformative ideas should include testable hypotheses, avoid special pleading, invoke a minimum of free parameters, and explain a body of data.

Of particular interest are papers that address a long-standing question. Hallmarks of unresolved questions are protracted debates between a few entrenched “camps” and increasingly convoluted justifications of existing models, such as alternatively attributing dark matter to neutrinos, whimps, or imaginary axions (cf. Trimble (1987) to the subsequent literature). As exemplified by the poor advice tendered to Planck circa 1890 regarding the notion that everything in physics is already known, consensus can perpetuate inadequate concepts and discourage discovery. Thus, summaries of available hypotheses and historic perspectives are also welcome.

References

Ackermann, M.; Albert, A.; Anderson, B.; Baldini, L.; Ballet, J.; Barbiellini, G.; Bastieri, D.; Bechtol, K.; Bellazzini, R.; Bissaldi, E.; et al. (2014) Dark matter constraints from observations of 25 Milky Way satellite galaxies with the Fermi Large Area Telescope. Phys. Rev. D 2014, 89, 042001.
Criss, R.E.; Hofmeister, A.M. (2020) Density Profiles of 51 Galaxies from Parameter-Free Inverse Models of Their Measured Rotation Curves. Galaxies 2020, 8, 19.
Feng, J.Q.; Gallo, C.F. (2014) Mass distribution in rotating thin-disk galaxies according to Newtonian dynamics. Galaxies 2, 199–222.
Giagu, S. (2019) WIMP dark matter searches with the ATLAS detector at the Large Hadron Collider. Front. Phys. 7, 75.
Gupta, R.P. (2024) Testing CCC+TL Cosmology with Observed Baryon Acoustic Oscillation Features. The Astrophysical Journal 55, paper 964.
Park, M., Leahey, E. & Funk, R.J. (2023) Papers and patents are becoming less disruptive over time. Nature 613, 138–144.
Rubin, V.C.; Ford, W.K. (1970) Rotation of the Andromeda nebula from a spectroscopic survey of emission regions. Astrophys. J. 159, 379–403.
Sipols, A.; Pavlovich, A. (2020) Dark matter dogma: A study of 214 galaxies. Galaxies 2020, 8, 36.
Trimble, V. (1987). Existence and nature of dark matter in the universe. Annual Review of Astronomy and Astrophysics. 25, 425–472.

Prof. Dr. Anne M. Hofmeister
Prof. Robert E. Criss
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.

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Please visit the Instructions for Authors page before submitting a manuscript. The Article Processing Charge (APC) for publication in this open access journal is 1400 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

  • observations
  • theory
  • hypothesis
  • scientific method
  • debate
  • consensus

Published Papers

This special issue is now open for submission.
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