Comment on “Spin light of neutrino in matter: a new type of electromagnetic radiation”

نویسندگان

  • A. V. Kuznetsov
  • N. V. Mikheev
چکیده

We show that a criticism made in hep-ph/0610294 against our paper Mod. Phys. Lett. A21, 1769 (2006) has no ground. We confirm that all results of investigations of the socalled “spin light of neutrino (SLν)” are incorrect because of the medium influence on photon dispersion. With taking account of this influence, both the SLν radiation rate and the total power are zero for neutrinos in all real astrophysical conditions. In an extended series of papers [1–11], there was proposed and investigated in detail the socalled “spin light of neutrino” (SLν), the process of the radiative neutrino transition νL → νRγ, caused by the additional energy W acquired in medium by the ultra-relativistic left-handed neutrino [12]. In their analysis the authors neglected the medium influence on the photon dispersion. It looked unnatural, because the neutrino dispersion was defined by the weak interaction while the photon dispersion was defined by the electromagnetic interaction. In the paper [13] we evaluated the effective mass acquired by a photon in the astrophysical conditions used by those authors, and we have shown qualitatively that consideration of the radiative neutrino transition νL → νRγ without taking account of the photon dispersion in medium should be incorrect. In a short reply [14], the authors wrote that our analysis was wrong because “the momentum conservation law has not been accounted for”. It was declared instead of performing an accurate application of this conservation law to the process. As we have shown further in the papers [15, 16], just the energy-momentum conservation law with the photon effective mass taken into account, has led to the threshold value for the initial neutrino energy: E > E0 ≃ mγ 2W , (1) wheremγ is the effective mass of the photon (plasmon) in medium. Evaluation of these threshold energies for different astrophysical situations shows that the value E0 is always greater in orders of magnitude than the typical neutrino energy. Thus, the photon dispersion leaves no room for “spin light of neutrino”, except for a pure theoretical possibility when an ultra-high energy ∗ e-mail: [email protected] † e-mail: [email protected]

برای دانلود متن کامل این مقاله و بیش از 32 میلیون مقاله دیگر ابتدا ثبت نام کنید

ثبت نام

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

منابع مشابه

ar X iv : h ep - p h / 05 06 00 7 v 1 1 J un 2 00 5 High energy neutrino spin light

The quantum theory of spin light (electromagnetic radiation emitted by a Dirac massive neutrino propagating in dense matter due to the weak interaction of a neutrino with background fermions) is developed. In contrast to the Cherenkov radiation, this effect does not disappear even if the medium refractive index is assumed to be equal to unity. The formulas for the transition rate and the total ...

متن کامل

Radiative transitions of high energy neutrino in dense matter

The quantum theory of the “spin light” (electromagnetic radiation emitted by a massive neutrino propagating in dense matter due to the weak interaction of a neutrino with background fermions) is developed. In contrast to the Cherenkov radiation, this effect does not disappear even if the medium refractive index is assumed to be equal to unity. The formulas for the transition rate and the total ...

متن کامل

Neutrino energy quantization in rotating medium

Exact solution of the modified Dirac equation in rotating medium is found in polar coordinates in the limit of vanishing neutrino mass. The solution for the active lefthanded particle exhibit properties similar to those peculiar for the charged particle moving in the presence of a constant magnetic field. Accordingly, the particle in the rotating matter has circle orbits with energy levels, ana...

متن کامل

Neutrinos, Electrons and Muons in Electromagnetic Fields and Matter: the Method of Exact Solutions

We present a powerful method for exploring various processes in the presence of strong external fields and matter. The method implies utilization of the exact solutions of the modified Dirac equations which contain the effective potentials accounting for the influences of external electromagnetic fields and matter on particles. We briefly discuss the basics of the method and its applications to...

متن کامل

Decay-Produced Neutrino Hot Dark Matter

We investigate different types of neutrino hot dark matter with respect to structure formation and anisotropies in the cosmic microwave background radiation (CMBR). The possibility of neutrino hot dark matter produced through the decay of a heavier neutrino by the process νH → νL+φ, where φ is a scalar particle, is discussed in detail. This type of dark matter can possibly be distinguished obse...

متن کامل

ذخیره در منابع من


  با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید

برای دانلود متن کامل این مقاله و بیش از 32 میلیون مقاله دیگر ابتدا ثبت نام کنید

ثبت نام

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

عنوان ژورنال:

دوره   شماره 

صفحات  -

تاریخ انتشار 2006