555 results on '"VOLKAS, RAYMOND R."'
Search Results
202. SU(5)grand unification on a domain-wall brane from anE6-invariant action
203. Solution to the hierarchy problem from an almost decoupled hidden sector within a classically scale invariant theory
204. Electroweak Higgs as a pseudo-Goldstone boson of broken scale invariance
205. Neutrino mass in radiatively broken scale-invariant models
206. SCALAR KINK BRANEWORLDS AND COSMOLOGY
207. Kink modes and effective four dimensional fermion and Higgs brane models
208. Cosmology and fermion confinement in a scalar-field-generated domain wall brane in five dimensions
209. Leptogenesis implications in models with Abelian family symmetry and one extra real Higgs singlet
210. A domain-wall-brane-localized standard model
211. The brane as a Higgs domain wall: ideas and issues
212. Searching for radiative neutrino mass generation at the LHC.
213. MIRROR DARK MATTER
214. Neutrino masses in quartification schemes
215. A4flavour symmetry breaking scheme for understanding quark and neutrino mixing angles
216. Stability of domain walls coupled to Abelian gauge fields
217. Unification via intermediate symmetry breaking scales with the quartification gauge group
218. Clash of symmetries in a Randall-Sundrum-like spacetime
219. Kink-induced symmetry breaking patterns in brane-worldSU(3)3trinification models
220. The AGASA and SUGAR Anisotropies and TeV Gamma Rays from the Galactic Center: A Possible Signature of Extremely High Energy Neutrons
221. Neutrinos from the Galactic Center in the Light of Its Gamma-Ray Detection at TeV Energy
222. O(10)kinks: Clash of symmetries on the brane and the gauge hierarchy problem
223. State permutations from manipulation of near-level-crossings
224. Tribimaximal mixing, discrete family symmetries, and a conjecture connecting the quark and lepton mixing matrices
225. Searching for Long‐Wavelength Neutrino Oscillations in the Distorted Neutrino Spectrum of Galactic Supernova Remnants
226. Entanglement and quantal coherence: Study of two limiting cases of rapid system-bath interactions
227. Generation of entangled states and error protection from adiabatic avoided level crossings
228. Neutrinos in cosmology, with some significant digressions.
229. NEUTRINOPROPAGATION INDENSEASTROPHYSICALSYSTEMS
230. Synchronisation and MSW sharpening of neutrinos propagating in a flavour blind medium
231. Relic neutrino asymmetries.
232. MIRROR NEUTRINOS AND THE EARLY UNIVERSE.
233. Bottom-up model for maximalνμ−ντmixing
234. Further studies on relic neutrino asymmetry generation. I. The adiabatic Boltzmann limit, nonadiabatic evolution, and the classical harmonic oscillator analogue of the quantum kinetic equations
235. Further studies on relic neutrino asymmetry generation. II. A rigorous treatment of repopulation in the adiabatic limit
236. Oscillating Neutrinos from the Galactic Center
237. Linking the geometric mass hierarchy with threefold family replication
238. Relic neutrino asymmetry evolution from first principles
239. Energy-dependent solar neutrino flux depletion in the exact parity model and implications for SNO, SuperKamiokande, and BOREXINO
240. Radiative generation of quark and lepton mass hierarchies from a top-quark mass seed
241. NEUTRINO PROPAGATION IN DENSE ASTROPHYSICAL SYSTEMS.
242. Solutions for intersecting domain walls with internal structure in six dimensions from a Z2 X Z2-invariant action.
243. Large lepton mixing angles from a 4 + 1-dimensional SU (5) × A4 domain-wall braneworld model.
244. Reflecting on chirality: CP-violating extensions of the single scalar-leptoquark solutions for the (g-2)e,μ puzzles and their implications for lepton EDMs.
245. Getting chirality right: Single scalar leptoquark solutions to the (g-2)e,μ puzzle.
246. g-2of the muon from compositeness in the model of Abbott and Farhi
247. PREFACE.
248. Classification of three-family flavoured DFSZ axion models that have no domain wall problem.
249. Phenomenological analysis of an E6-inspired seesaw model.
250. Origin of neutrino masses at the LHC: ΔL=2 effective operators and their ultraviolet completions.
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