The Case for a Fourth Spatial Dimension and the Hyperspherical Force

• Authors: Marco Pereira
• Languages of publication: EN

Abstracts

EN

Here we present evidence of an extra spatial dimension and that our 3D Universe is embedded as a lightspeed expanding hyperspherical hypersurface. Support for this hypothesis comes from (a) SDSS BOSS dataset analysis showing the seeding of Galaxies on the largest scale by spherical acoustic oscillations, (b) the discovery of an Hyperspherical Force, a constraint force that exists only because of the lightspeed hyperspherical expansion. That solves the Spiral Galaxy Rotation Conundrum, (c) the parameterless predictions of all type 1a Supernovae (SN1a) distances from their redshifts z. Lightspeed hyperspherical expansion permits simple short-distance compliance with the Hubble Law.

Keywords

EN

4D; L-CDM; cosmology; extra dimension; general relativity; topology

Discipline

• ASTRONOMY: ASTRONOMY

• Publisher: Scientific Publishing House „DARWIN”
• Journal: World Scientific News
• Year: 2018
• Volume: 98
• Pages: 127-139

Contributors

author

Marco Pereira

• Rutgers University, Department of Mathematics, The Rutgers University of the State of New Jersey, New Brunswick, NJ, USA

References

• [1] G. Lemaitre, Nn. Soc. Sc. Bruxelles A 53, 51 (1933).
• [2] A. Friedman, Z. Phys. (in Ger. 10 377--386. (1922).
• [3] S. Dodelson, Modern Cosmology, 4. [print.]. (Academic Press, San Diego, CA [Etc.], 2008).
• [4] X.-F. Deng, Y.-Q. Chen, Q. Zhang, and J.-Z. He, Chin. J. Astron. Astrophys 6, 35 (2006).
• [5] S. Alam, F. D. Albareti, C. A. Prieto, F. Anders, S. F. Anderson, T. Anderton, B. H. Andrews, E. Armengaud, É. Aubourg, S. Bailey, S. Basu, J. E. Bautista, R. L. Beaton, T. C. Beers, C. F. Bender, A. A. Berlind, F. Beutler, V. Bhardwaj, J. C. Bird, D. Bizyaev, C. H. Blake, M. R. Blanton, M. Blomqvist, J. J. Bochanski, A. S. Bolton, J. Bovy, A. S. Bradley, W. N. Brandt, D. E. Brauer, J. Brinkmann, P. J. Brown, J. R. Brownstein, A. Burden, E. Burtin, N. G. Busca, Z. Cai, D. Capozzi, A. C. Rosell, M. A. Carr, R. Carrera, K. C. Chambers, W. J. Chaplin, Y.-C. Chen, C. Chiappini, S. D. Chojnowski, C.-H. Chuang, N. Clerc, J. Comparat, K. Covey, R. A. C. Croft, A. J. Cuesta, K. Cunha, L. N. da Costa, N. Da Rio, J. R. A. Davenport, K. S. Dawson, N. De Lee, T. Delubac, R. Deshpande, S. Dhital, L. Dutra-Ferreira, T. Dwelly, A. Ealet, G. L. Ebelke, E. M. Edmondson, D. J. Eisenstein, T. Ellsworth, Y. Elsworth, C. R. Epstein, M. Eracleous, S. Escoffier, M. Esposito, M. L. Evans, and X. Fan, ApJS 219, 12 (2015).
• [6] M. Pereira, World Scientific News 82, 1 (2017).
• [7] E. Corbelli and P. Salucci, Mon. Not. R. Astron. Soc. 311, 441 (2000).
• [8] W. J. G. de Blok and A. Bosma, Astron. Astrophys. 385, 816 (2002).
• [9] V. C. Rubin, N. Thonnard, and W. K. . J. Ford, Astrophys. J. 225, L107 (1978).
• [10] M. Milgrom, Cent. Astrophys. Weizmann Inst. 1 (2008).
• [11] K. Dewhurst, Br. J. Hist. Sci. 1, 365 (1963).

• Document Type: article