Induced electric charge of the neutrino in a dispersive medium

Oraevsky, V. N.; Semikoz, V. B.

doi:10.1016/0378-4371(87)90021-5

Cited by 56 publications

(31 citation statements)

References 6 publications

Supporting

Mentioning

Contrasting

Order By: Relevance

“…20). Also, the latest data do not confirm the anticorrelation: large number of the sunspots in 1991-1992 was accompanied by high counting rate [38].…”

Section: Neutrinos and This Is Exactly What Is Needed To Qualitativementioning

confidence: 99%

See 1 more Smart Citation

The Charged Neutrino: A New Approach to the Solar Neutrino Problem

Ignatiev

Joshi

1994

Mod. Phys. Lett. A

View full text Add to dashboard Cite

show abstract

“…20). Also, the latest data do not confirm the anticorrelation: large number of the sunspots in 1991-1992 was accompanied by high counting rate [38].…”

Section: Neutrinos and This Is Exactly What Is Needed To Qualitativementioning

confidence: 99%

“…The point is that the neutrino electromagnetic properties get modified by plasma effects and under certain conditions these modifications result in an induced electric charge of the neutrino [20]. We stress that it happens in the Minimal Standard Model where the neutrino has zero intrinsic electric charge.…”

mentioning

confidence: 99%

The Charged Neutrino: A New Approach to the Solar Neutrino Problem

Ignatiev

Joshi

1994

Mod. Phys. Lett. A

View full text Add to dashboard Cite

show abstract

“…The electromagnetic wave passing throuth the plasma, is modified because of the mobile charged particle in the medium and it consists of coherent vibration of the electromagnetic field as well as the density of the charged particles [1]. Photons no longer propagate at the speed of light and satisfy the dispersion relations for transverse and longitudinal modes.…”

Section: Introductionmentioning

confidence: 99%

Cherenkov radiation of longitudinal photons by neutrinos

Sahu

1997

Phys. Rev. D

View full text Add to dashboard Cite

In a relativistic plasma neutrino can emit plasmons by the Cerenkov process which is kinematically allowed for a range of frequencies for which refractive index is greater than one. We have calculated the rate of energy emission by this process. We compute the energy deposited in a stalled supernova shock wave by the Cerenkov process and find that it is much smaller than the Bethe-Wilson mechanism.

show abstract

“…Besides the dispersion relation, another quantity of interest is the effective electromagnetic coupling of the neutrino in the background medium [2,3,4,5,6,7,8]. That coupling is the basis of some of the neutrino processes that can occur in a medium but not in the vacuum, such as the plasmon decay and the Cherenkov radiation process [1].…”

Section: Introductionmentioning

confidence: 99%

Nucleon contribution to the induced charge of neutrinos in a matter background and a magnetic field

Nieves

2004

Phys. Rev. D

View full text Add to dashboard Cite

We study the nucleon contribution to the electromagnetic vertex function of neutrinos that propagate in a matter background in the presence of a magnetic field. Starting from the one-loop expression for the corresponding terms of the vertex function, and taking into account the anomalous magnetic coupling of the nucleons, we calculate the B-dependent part of the form factors that determine the induced charge of the neutrino. A formula for the neutrino induced charge is obtained, and it is evaluated for various illustrative situations. The terms due to the nucleons can be important in some cases, depending on the physical conditions of the environment.

show abstract

Induced electric charge of the neutrino in a dispersive medium

Cited by 56 publications

References 6 publications

The Charged Neutrino: A New Approach to the Solar Neutrino Problem

The Charged Neutrino: A New Approach to the Solar Neutrino Problem

Cherenkov radiation of longitudinal photons by neutrinos

Nucleon contribution to the induced charge of neutrinos in a matter background and a magnetic field

Contact Info

Product

Resources

About