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Eiichi Takasugi

Publications and source records attributed to Eiichi Takasugi.

40 records · Page 3Linked to original sources

Analytic Solutions of the Regge-Wheeler Equation and the Post-Minkowskian Expansion

Analytic solutions of the Regge-Wheeler equation are presented in the form of series of hypergeometric functions and Coulomb wave functions which have different regions of convergence. Relations between these solutions are established. The series solutions are given as the Post-Minkowskian expansion with respect to a parameter $ε\equiv 2Mω$, $M$ being the mass of black hole. This expansion corresponds to the post-Newtonian expansion when they are applied to the gravitational radiation from a particle in circular orbit around a black hole. These solutions can also be useful for numerical computations.

gr-qc↗

Analytic Solutions of the Teukolsky Equation and their Low Frequency Expansions

Analytic solutions of the Teukolsky equation in Kerr geometries are presented in the form of series of hypergeometric functions and Coulomb wave functions. Relations between these solutions are established. The solutions provide a very powerful method not only for examining the general properties of solutions and physical quantities when they are applied to, but also for numerical computations. The solutions are given in the expansion of a small parameter $ε\equiv 2Mω$, $M$ being the mass of black hole, which corresponds to Post-Minkowski expansion by $G$ and to post-Newtonian expansion when they are applied to the gravitational radiation from a particle in circular orbit around a black hole. It is expected that these solutions will become a powerful weapon to construct the theoretical template towards LIGO and VIRGO projects.

gr-qc↗

Composite Neutrinos and Double Beta Decay

Neutrinoless double beta decay $(\b\b)_{0ν}$ occurs through the magnetic coupling of dimension five, $λ_W^{(ν*)}/m_{ν*}$, among the excited electron neutrino $ν^*$, electron and $W$ boson if $ν^*$ is a massive Majorana neutrino. If the coupling is not small, i.e., $λ_W^{(ν*)}>1$ the mass of the excited neutrino must not be gless than the $Z$ boson mass, $m_Z$. Since $ν^*$ contributes in the $(\b\b)_{0ν}$ decay as a vertual state, this decay will give an oppotunity to explore the much heavier mass region of $ν^*$. In this paper, we present the decay formula of $(\b\b)_{0ν}$ decay through the $ν^*$ exchange and discuss the constraint on the coupling constant and the mass of the excited neutrino. By comparing the recent data for ${}^{76}$Ge, we find $λ_W^{(ν*)}({1\rm TeV}/m_{ν*})) (m_N/{1\rm TeV})^{\frac 12}< 4.1\cdot 10^{-3}$ where $m_N$ is the Majorana mass of the excited electron neutrino. If $m_N=m_{ν*}$ and $λ_W^{(ν*)}>1$, we find the mass bound for the excited Majorana neutrino as $m_{ν^*} > 5.9\cdot 10^4$TeV. In order to obtain the constraint on the composite scale $Λ$, we have to specify the model. For the mirror type and the homodoublet type models, $λ_W^{(ν*)}/m_{ν*}=f/(\sqrt 2 Λ)$ where $f$ is the relative strength of gauge couplings. Then, we obtain $Λ> 170 f (m_N/{1\rm TeV})^{\frac 12}$TeV. For the sequential type model, $λ/m_{ν*}=fv/(\sqrt 2 Λ^2)$ where $v$ is the vacuum expectation value of the dopublet Higgs boson, i.e., $v=$250GeV. In this model, we find $Λ> 6.6 f^{\frac 12} (m_N/{1\rm TeV})^{\frac 14}$TeV.

hep-ph↗

Twisting Toroidal Magnetic Fields and the Seasonal Oscillation of the Solar Neutrino Flux II

An intriguing possibility is explored that the solar neutrino data could be used as a probe to the magnetic field structure in the sun. Various cyclic phenomena occurring on the surface of the sun have been accounted for by the so-called dynamo-mechanism. According to this, a self-generating mechanism of solar cyclic activities gives rise to twisting toroidal magnetic fields in the convective zone. Although its magnitude is not known, the orientation of the twist is certainly opposite in northern and southern hemispheres of the sun. We show by numerical calculation that the solar neutrino flux, being sensitive to the twist, could exhibit observable seasonal oscillation, provided that the twist is sizable in magnitude and the neutrinos have reasonably large magnetic moments. This oscillation is ascribed to the fact that the earth's orbit is slightly inclined to the sun's equator, and that solar neutrinos pass through the northern (southern) hemisphere of the sun around September (March). We also argue that similar seasonal oscillation could be exhibited in the azimuthal asymmetry of recoiling electrons scattered by the solar neutrinos which are expected to be observed in the super-Kamiokande detector.

hep-ph↗