A theoretical case for negative mass-square for sub-eV particles
| dc.creator | Ahluwalia-Khalilova, D. V. | |
| dc.creator | Dymnikova, Irina | |
| dc.date | 2003-05-14 | |
| dc.date | 2003-11-03 | |
| dc.date.accessioned | 2026-07-07T11:31:25Z | |
| dc.date.available | 2026-07-07T11:31:25Z | |
| dc.description | Electroweak gauge bosons have masses of the order of 10^2 GeV, while masses of additional bosons involved in gravito-electroweak unification are expected to be still higher. These are at least eleven orders of magnitude higher than sub-eV range indications for neutrino masses. Under these circumstances we suspect that the sub-eV particles are created in a spacetime where gravitational effects of massive gauge bosons may become important. The question that we thus ask is: What is the spacetime group around a gravito-electroweak vertex? Modeling it as de-Sitter we find that sub-eV particles may carry a negative mass square of the order of - (3/8 π^3) (M_unif./M_Planck)^4 M_Planck^2. Neutrino oscillation data then hints at 30-75 TeV scale for M_unif., where M_unif. characterizes gravito-electroweak unification scale. | |
| dc.description | v3: Entirely re-written. An error (not a typo) corrected. Int. J. Mod. Phys. D (in press) v1: This essay received an "honorable mention" in the 2003 Essay Competition of the Gravity Research Foundation | |
| dc.identifier | https://arxiv.org/abs/hep-ph/0305158 | |
| dc.identifier | http://arxiv.org/abs/hep-ph/0305158 | |
| dc.identifier | Int.J.Mod.Phys.D12:1787-1794,2003 | |
| dc.identifier | doi:10.1142/S0218271803004328 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/197263 | |
| dc.subject | High Energy Physics - Phenomenology | |
| dc.subject | General Relativity and Quantum Cosmology | |
| dc.subject | High Energy Physics - Theory | |
| dc.subject | Nuclear Theory | |
| dc.title | A theoretical case for negative mass-square for sub-eV particles | |
| dc.type | text |