5D World-Universe Model. Neutrinos. The World
Author(s)
Vladimir S. Netchitailo*
ABSTRACT
In this manuscript we discuss mass-varying neutrinos and propose their energy density to exceed that of baryonic and dark matter. We introduce cosmic Large Grains whose mass is about Planck mass, and their temperature is around 29 K. Large Grains are in fact Bose-Einstein condensates of proposed dineutrinos, and are responsible for the cosmic Far-Infrared Background (FIRB) radiation. The distribution of the energy density of all components of the World (protons, electrons, photons, neutrinos, and dark matter particles) is considered. We present an overview of the World- Universe Model (WUM) and pay particular attention to the self-consistent set of time-varying values of basic parameters of the World: the age and critical energy density; Newtonian parameter of gravitation and Hubble’s parameter; temperatures of the cosmic Microwave Background radiation and the peak of the cosmic FIRB radiation; Fermi coupling parameter and coupling parameters of the proposed Super-Weak and Extremely-Weak interactions. Additionally, WUM forecasts the masses of dark matter particles, axions, and neutrinos; proposes two fundamental parameters of the World: fine-structure constant α and the quantity Q which is the dimensionless value of the fifth coordinate, and three fundamental physical units: basic unit of momentum, energy density, and energy flux density. WUM suggests that all time-dependent parameters of the World are inter- connected and in fact dependent on Q. We recommend adding the quantity Q to the list of the CODATA-recommended values.
In this manuscript we discuss mass-varying neutrinos and propose their energy density to exceed that of baryonic and dark matter. We introduce cosmic Large Grains whose mass is about Planck mass, and their temperature is around 29 K. Large Grains are in fact Bose-Einstein condensates of proposed dineutrinos, and are responsible for the cosmic Far-Infrared Background (FIRB) radiation. The distribution of the energy density of all components of the World (protons, electrons, photons, neutrinos, and dark matter particles) is considered. We present an overview of the World- Universe Model (WUM) and pay particular attention to the self-consistent set of time-varying values of basic parameters of the World: the age and critical energy density; Newtonian parameter of gravitation and Hubble’s parameter; temperatures of the cosmic Microwave Background radiation and the peak of the cosmic FIRB radiation; Fermi coupling parameter and coupling parameters of the proposed Super-Weak and Extremely-Weak interactions. Additionally, WUM forecasts the masses of dark matter particles, axions, and neutrinos; proposes two fundamental parameters of the World: fine-structure constant α and the quantity Q which is the dimensionless value of the fifth coordinate, and three fundamental physical units: basic unit of momentum, energy density, and energy flux density. WUM suggests that all time-dependent parameters of the World are inter- connected and in fact dependent on Q. We recommend adding the quantity Q to the list of the CODATA-recommended values.
KEYWORDS
5D World-Universe Model, Medium of the World, Mass-Varying Neutrinos, Dineutrinos, Bose- Einstein Condensates, Far-Infrared Background Radiation, Time-Varying Parameters of the World
5D World-Universe Model, Medium of the World, Mass-Varying Neutrinos, Dineutrinos, Bose- Einstein Condensates, Far-Infrared Background Radiation, Time-Varying Parameters of the World
Cite this paper
Netchitailo, V. (2016) 5D World-Universe Model. Neutrinos. The World. Journal of High Energy Physics, Gravitation and Cosmology, 2, 1-18. doi: 10.4236/jhepgc.2016.21001.
Netchitailo, V. (2016) 5D World-Universe Model. Neutrinos. The World. Journal of High Energy Physics, Gravitation and Cosmology, 2, 1-18. doi: 10.4236/jhepgc.2016.21001.
References
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[1] Netchitailo, V.S. (2015) 5D World-Universe Model. Space-Time-Energy. Journal of High Energy Physics, Gravitation and Cosmology, 1, 25-34. http://dx.doi.org/10.4236/jhepgc.2015.11003 [2] Netchitailo, V.S. (2015) 5D World-Universe Model. Multicomponent Dark Matter. Journal of High Energy Physics, Gravitation and Cosmology, 1, 55-71. http://dx.doi.org/10.4236/jhepgc.2015.12006 [3] Pontecorvo B. and Smorodinsky, Y. (1962) The Neutrino and the Density of Matter in the Universe. Soviet Physics— JETP, 14, 173. [4] Kajita, T. (1998) Atmospheric neutrino results from Super-Kamiokande and Kamiokande—Evidence for νμ oscillations. arXiv: 9810001. [5] Sanchez, M. (2003) Oscillation Analysis of Atmospheric Neutrinos in Soudan 2. PhD Thesis, Tufts University, Medford/Somerville. http://nu.physics.iastate.edu/Site/Bio_files/thesis.pdf [6] Kaus, P. and Meshkov, S. (2003) Neutrino Mass Matrix and Hierarchy. AIP Conference Proceedings, 672, 117. http://dx.doi.org/10.1063/1.1594399 [7] Dermisek, R. (2004) Neutrino Masses and Mixing, Quark-Lepton Symmetry and Strong Right-Handed Neutrino Hierarchy. Physical Review D, 70, Article ID: 073016. [8] Gonzalez-Garcia, M.C. and Pena-Garay, C. (2003) Three-Neutrino Mixing after the First Results from K2K and KamLAND. Physical Review D, 68, Article ID: 093003. http://dx.doi.org/10.1103/PhysRevD.68.093003 [9] Maltoni, M., Schwetz, T., Tortola, M.A. and Valle, J.W.F. (2003) Status of Three-Neutrino Oscillations after the SNO- Salt Data. Physical Review D, 68, Article ID: 113010. http://dx.doi.org/10.1103/PhysRevD.68.113010 [10] Battye, R.A. and Moss, A. (2014) Evidence for Massive Neutrinos from CMB and Lensing Observations. arXiv: 1308.5870. [11] Landau, L.D. and Lifshitz, E.M. (1980) Statistical Physics. Third Edition, Part 1: Volume 5. Butterworth-Heinemann, Oxford. [12] NASA’s Planck Project Office (2013) Planck Mission Brings Universe into Sharp Focus. https://www.nasa.gov/mission_pages/planck/news/planck20130321.html#.VZ4k5_lViko [13] Hauser, M.G., Gillett, F.C., Low, F.J., Gautier, T.N., Beichman, C.A., Aumann, H.H., Neugebauer, G., Baud, B., Boggess, N. and Emerson, J.P. (1984) IRAS Observations of the Diffuse Infrared Background. The Astrophysical Journal, 278, L15-L18. http://dx.doi.org/10.1086/184212 [14] Low, F.J., Young, E., Beintema, D.A., Gautier, T.N., Beichman, C.A., Aumann, H.H., Gillett, F.C., Neugebauer, G., Boggess, N. and Emerson, J.P. (1984) Infrared Cirrus-New Components of the Extended Infrared Emission. The Astrophysical Journal, 278, L19-L22. http://dx.doi.org/10.1086/184213 [15] Wang, B. (1991) Integrated Far-Infrared Background from Galaxies. The Astrophysical Journal, 374, 465-474. http://dx.doi.org/10.1086/170136 [16] Wright, E.L. (2001) Cosmic InfraRed Background Radiation. http://www.astro.ucla.edu/~wright/CIBR/ [17] Fixsen, D.J., Cheng, E.S., Gales, J.M., Mather, J.C., ShaFer, R.A. and Wright, E.L. (1996) The Cosmic Microwave Background Spectrum from the Full COBE* FIRAS Data Set. The Astrophysical Journal, 473, 576-587. http://dx.doi.org/10.1086/178173 [18] Finkbeiner, D.P., Davis, M. and Schlegel, D.J. (1999) Extrapolation of Galactic Dust Emission at 100 Microns to CMBR Frequencies Using FIRAS. The Astrophysical Journal, 524, 867-886. [19] Draine, B.T. and Lazarian, A. (1998) Electric Dipole Radiation from Spinning Dust Grains. The Astrophysical Journal, 508, 157-179. http://dx.doi.org/10.1086/306387 [20] Finkbeiner, D.P. and Schlegel, D.J. (1999) Interstellar Dust Emission as a CMBR Foreground. The Astrophysical Journal, 524, 867-886. [21] Lagache, G., Abergel, A., Boulanger, F., Désert, F.X. and Puget, J.-L. (1999) First Detection of the Warm Ionized Medium Dust Emission. Implication for the Cosmic Far-Infrared Background. Astronomy and Astrophysics, 344, 322-332. [22] Finkbeiner, D.P., Davis, M. and Schlegel, D.J. (2000) Detection of a Far IR Excess with DIRBE at 60 and 100 Microns. The Astrophysical Journal, 544, 81-97. [23] Siegel, P.H. (2002) Terahertz Technology. IEEE Transactions on Microwave Theory and Techniques, 50, 910-928. http://dx.doi.org/10.1109/22.989974 [24] Phillips, T.G. and Keene, J. (1992) Submillimeter Astronomy [Heterodyne Spectroscopy]. Proceedings of the IEEE, 80, 1662-1678. http://dx.doi.org/10.1109/5.175248 [25] Dupac, X., et al. (2003) The Complete Submillimeter Spectrum of NGC 891. arXiv: 0305230. [26] Aguirre, J.E., Bezaire, J.J., Cheng, E.S., Cottingham, D.A., Cordone, S.S., Crawford, T.M., et al. (2003) The Spectrum of Integrated Millimeter Flux of the Magellanic Clouds and 30-Doradus from TopHat and DIRBE Data. 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