Weyl conformal symmetry for gravitation and cosmology
Article Sidebar
Main Article Content
Downloads
Article Details
Copyright (c) 2022 Nesbet RK.
This work is licensed under a Creative Commons Attribution 4.0 International License.
Licensing and protecting the author rights is the central aim and core of the publishing business. Peertechz dedicates itself in making it easier for people to share and build upon the work of others while maintaining consistency with the rules of copyright. Peertechz licensing terms are formulated to facilitate reuse of the manuscripts published in journals to take maximum advantage of Open Access publication and for the purpose of disseminating knowledge.
We support 'libre' open access, which defines Open Access in true terms as free of charge online access along with usage rights. The usage rights are granted through the use of specific Creative Commons license.
Peertechz accomplice with- [CC BY 4.0]
Explanation
'CC' stands for Creative Commons license. 'BY' symbolizes that users have provided attribution to the creator that the published manuscripts can be used or shared. This license allows for redistribution, commercial and non-commercial, as long as it is passed along unchanged and in whole, with credit to the author.
Please take in notification that Creative Commons user licenses are non-revocable. We recommend authors to check if their funding body requires a specific license.
With this license, the authors are allowed that after publishing with Peertechz, they can share their research by posting a free draft copy of their article to any repository or website.
'CC BY' license observance:
|
License Name |
Permission to read and download |
Permission to display in a repository |
Permission to translate |
Commercial uses of manuscript |
|
CC BY 4.0 |
Yes |
Yes |
Yes |
Yes |
The authors please note that Creative Commons license is focused on making creative works available for discovery and reuse. Creative Commons licenses provide an alternative to standard copyrights, allowing authors to specify ways that their works can be used without having to grant permission for each individual request. Others who want to reserve all of their rights under copyright law should not use CC licenses.
Weyl H. Reine Infinitesimalgeometrie. Math.Zeit.1918; 2: 384.
Weyl H. Gravitation und Elektrizit[Math Processing Error]t. Sitzungber.Preuss.Akad.Wiss. 1918; 465.
Mannheim PD, Kazanas D. Exact vacuum solution to conformal Weyl gravity and galactic rotation curves. ApJ 1989; 342: 635.
Mannheim PD. Some exact solutions to conformal Weyl gravity. Annals N.Y.Acad.Sci. 1991; 631: 194.
Mannheim PD, Kazanas D. Newtonian limit of conformal gravity and the lack of necessity of the second order Poisson equation. Gen.Rel.Grav. 1994; 26: 337.
Mannheim PD. Alternatives to dark matter and dark energy, Prog.Part.Nucl.Phys. 2006; 56: 340.
Mannheim PD. Schwarzschild limit of conformal gravity in the presence of macroscopic scalar fields. Phys.Rev.D 2007; 75: 124006.
Nesbet RK. Cosmological implications of conformal field theory. Mod.Phys.Lett.A 2011; 26: 893.
Nesbet RK. Dark energy density predicted and explained. Europhys.Lett. 2019; 125: 19001.
Nesbet RK. Dark galactic halos without dark matter. Europhys.Lett. 2015; 109: 59001.
Nesbet RK. Conformal theory of gravitation and cosmology. Europhys.Lett. 2020; 131: 10002.
Friedmann A. On the possibility of the world with constant negative curvature. Z.Phys. 1922; 10: 377.
Mannheim PD. Are galactic rotation curves really flat? ApJ 1997; 479: 659.
O’Brien JG, Chiarelli TL, Mannheim PD. Universal properties of centripetal accelerations of spiral galaxies. Phys.Lett.B 2018; 782: 433.
Mannheim PD, O'Brien JG. Impact of a global quadratic potential on galactic rotation curves. Phys Rev Lett. 2011 Mar 25;106(12):121101. doi: 10.1103/PhysRevLett.106.121101. Epub 2011 Mar 23. PMID: 21517292.
Mannheim PD, O’Brien JG, Fitting galactic rotation curves with conformal gravity and a global quadratic potential. Phys.Rev.D 2012; 85: 124020.
O’Brien JG, Mannheim PD. Fitting dwarf galaxy rotation curves with conformal gravity. MNRAS 2012; 421: 1273.
O’Brien JG, Moss RJ. Rotation curve for the Milky Way galaxy in conformal gravity. J.Phys.Conf. 2015; 615: 012002.
Higgs PW. Broken symmetries and the masses of gauge bosons. Phys.Rev.Lett. 1964; 13: 508.
Cottingham WN, Greenwood DA. An Introduction to the Standard Model of Particle Physics (Cambridge Univ. Press, New York, 1998).
Nesbet RK. Conformal Higgs model: gauge fields can produce a 125GeV resonance. Mod.Phys.Lett.A 2021; 36: 2150161.
Milgrom M. A modification of the Newtonian dynamics: implications for galaxies. ApJ 1983; 270: 371.
Sanders RH. The Dark Matter Proble. (Cambridge Univ. Press, New York, 2010).
Famaey B, McGaugh SS. Modified Newtonian Dynamics (MOND): Observational Phenomenology and Relativistic Extensions. Living Rev Relativ. 2012;15(1):10. doi: 10.12942/lrr-2012-10. Epub 2012 Sep 7. PMID: 28163623; PMCID: PMC5255531.
Tully RB, Fisher JR. A new method of determining distances to galaxies. Astron.Astrophys. 1977; 54: 661.
McGaugh SS. The baryonic Tully-Fisher relation of galaxies with extended rotation curves and the stellar mass of rotating galaxies. ApJ 2005; 632: 859.
McGaugh SS. Novel test of modified Newtonian dynamics with gas rich galaxies. Phys Rev Lett. 2011 Mar 25;106(12):121303. doi: 10.1103/PhysRevLett.106.121303. Epub 2011 Mar 21. Erratum in: Phys Rev Lett. 2011 Nov 25;107(22):229901. PMID: 21517295.
McGaugh SS, Lelli F, Schombert JM. Radial Acceleration Relation in Rotationally Supported Galaxies. Phys Rev Lett. 2016 Nov 11;117(20):201101. doi: 10.1103/PhysRevLett.117.201101. Epub 2016 Nov 9. PMID: 27886485.
Nesbet RK. Theoretical implications of the galactic radial acceleration relation of McGaugh, Lelli, and Schombert. MNRAS 2018; 476: L69.