Prediction and Derivation of the Hubble Constant from Subatomic Data Utilizing the Harmonic Neutron Hypothesis

DOI: 10.4236/jmp.2015.63033   PDF   HTML   XML   3,635 Downloads   4,075 Views   Citations

Abstract

Purpose: To accurately derive H0 from subatomic constants in abscence of any standard astronomy data. Methods: Recent astronomical data have determined a value of Hubble’s constant to range from 76.9+3.9-3.4+10.0-8.0 to 67.80 ± 0.77 (km/s)/Mpc. An innovative prediction of H0 is obtained from harmonic properties of the frequency equivalents of neutron, n0, in conjunction with the electron, e; the Bohr radius, α0; and the Rydberg constant, R. These represent integer natural unit sets. The neutron is converted from its frequency equivalent to a dimensionless constant,, where “h” = Planck’s constant, and “s” is measured in seconds. The fundamental frequency, Vf, is the first integer series set . All other atomic data are scaled to Vf as elements in a large, but a countable point set. The present value of H0 is derived and ΩM assumed to be 0. An accurate derivation of H0 is made using a unified power law. The integer set of the first twelve integers N12 {1,2,,11,12}, and their harmonic fractions exponents of Vf represent the first generation of bosons and particles. Thepartial harmonic fraction, -3/4, is exponent of Vf which represents H0. The partial fraction 3/4 is associated with a component of neutron beta decay kinetic energy. Results: H0 is predicted utilizing a previously published line used to derive Planck time, tp. The power law line of the experimental H0 and tp conforms to the predicted line. Conclusions: H0 can be predicted from subatomic data related to the neutron and hydrogen.

Share and Cite:

Chakeres, D. and Vento, R. (2015) Prediction and Derivation of the Hubble Constant from Subatomic Data Utilizing the Harmonic Neutron Hypothesis. Journal of Modern Physics, 6, 283-302. doi: 10.4236/jmp.2015.63033.

Conflicts of Interest

The authors declare no conflicts of interest.

References

[1] Ade, P.A.R., Aghanim, N., Alves, M.I.R., et al. (2014) Astronomy & Astrophysics, 571, Article ID: A1.
[2] Bonamente, M., Joy, M.K., Laroque, S.J., Carlstrom, J.E., Reese, E.D. and Dawson, K.S. (2006) The Astrophysical Journal, 647, 25-54.
http://dx.doi.org/10.1086/505291
[3] Freedman, W.L. and Madore, B.F. (2010) Annual Review of Astronomy and Astrophysics, 48, 673-710.
http://dx.doi.org/10.1146/annurev-astro-082708-101829
[4] Bennett, C.L., Larson, D., Weiland, J.L., Jarosik, N., Hinshaw, G., Odegard, N., Smith, R.S., Hill, K.M., Gold, B., et al. (2013) The Astrophysical Journal Supplement Series, 208, 19.
[5] Freedman, W.L., Madore, B.F., Scowcroft, V., Burns, C., Monson, A., Persson, S.E., Seibert, M. and Rigby, J. (2012) The Astrophysical Journal, 758, 24.
[6] Ade, P.A.R., Aghanim, N., Armitage-Caplan, C., Arnaud, M., Ashdown, M., Atrio-Barandela, F., et al. (2014) Astronomy & Astrophysics, 571, Article ID: A16.
[7] Chakeres, D.W. (2009) Particle Physics Insights, 2, 1-20.
[8] Chakeres, D.W. (2011) Particle Physics Insights, 4, 19-23.
http://dx.doi.org/10.4137/PPI.S7961
[9] Chakeres, D.W. (2011) Particle Physics Insights, 4, 25-31.
http://dx.doi.org/10.4137/PPI.S8241
[10] Chakeres, D.W. (2013) Particle Physics Insights, 6, 1-7.
http://dx.doi.org/10.4137/PPI.S12390
[11] Chakeres, D.W. (2011) Particle Physics Insights, 4, 33-38.
http://dx.doi.org/10.4137/PPI.S8269
[12] Chakeres, D.W. (2012) Bulletin of the American Physical Society, 57.
[13] Chakeres, D.W. (2006) The Imaginary Number Neutron Symphony. US Copyright, TXu1-295-777/2006-09-15.
[14] Chakeres, D.W. (2014) Journal of Modern Physics, 5, 1670-1683.
http://dx.doi.org/10.4236/jmp.2014.516167
[15] Lauterbur, P.C. (1973) Nature, 242, 190-191.
http://dx.doi.org/10.1038/242190a0
[16] Ljunggren, S. (1983) Journal of Magnetic Resonance, 54, 338-343.
http://dx.doi.org/10.1016/0022-2364(83)90060-4
[17] Cajori, F. (1909) A History of the Logarithmic Slide Rule and Allied Instruments. The Engineering News Publishing Company, New York.
[18] Ng, Y.J., Christiansen, W.A. and van Dam, H. (2003) The Astrophysical Journal, 591, L87-L89.
http://dx.doi.org/10.1086/377121
[19] Lykken, J. and Spiropulu, M. (2014) Scientific American, 310, 34-39.
http://dx.doi.org/10.1038/scientificamerican0514-34

  
comments powered by Disqus

Copyright © 2020 by authors and Scientific Research Publishing Inc.

Creative Commons License

This work and the related PDF file are licensed under a Creative Commons Attribution 4.0 International License.