The role of the neutrino electromagnetic moments in the stellar energy loss rate

Kerimov, B.K.; Zeinalov, S.M.; Alizade, V.N.; Mourão, A.

doi:10.1016/0370-2693(92)92019-d

Cited by 19 publications

(14 citation statements)

References 21 publications

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“…In this regard, the stellar energy loss rates data have been used to put constraints on the properties and interaction of light particles [118][119][120][121]. In addition, one of the most interesting possibilities to use stars as particle physics laboratories [122,123] is to study the backreaction of the novel energy loss rates implied by the existence of new low-mass particles such as axions [124,125], or by non-standard neutrino properties such as magnetic moment and electric dipole moment [10,11,[126][127][128].…”

Section: Results and Conclusionmentioning

confidence: 99%

Probing the electromagnetic dipole moments of the tau-neutrino in theU(1)B−Lmodel at the ILC and CLIC energies

2017

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Section: Results and Conclusionmentioning

confidence: 99%

Probing the electromagnetic dipole moments of the tau-neutrino in theU(1)B−Lmodel at the ILC and CLIC energies

2017

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“…The expression for the stellar ELRs for pair-annihilation process in ( 17) is determined by [4,19,20,43]:…”

Section: B Stellar Energy Loss Ratesmentioning

confidence: 99%

“…Consequently, there exist dipole moments. The interaction of neutrino with photon via dipole moment can affect the ELR [19][20][21].…”

Section: Introductionmentioning

confidence: 99%

Neutrino Energy Loss Rates in 3-3-1 Models

Binh,

Hue,

Binh

et al. 2021

Preprint

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The stellar energy-loss rates Q due to the production of neutrino pair in the framework of 3-3-1 models are presented. The energy loss rate Q is evaluated for different values of3 in which β is a parameter used to define the charge operator in the 3-3-1 models. The correction to the rate which is compared with that of the Standard Model (δQ) is also evaluated. We show that the correction does not exceed 14% and gets the highest withThe contribution of dipole moment to the energy loss rate is small compared to the contribution of new natural gauge boson Z and this sets constraints for the mass of Z' m Z ≤ 4000GeV. This mass range is within the searching range for Z boson at LHC.

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“…These interactions are expected to generate observable effects in astrophysical environments [24][25][26][27][28]. Furthermore, they will be of relevance in cosmology [14], and terrestrial neutrino experiments [29].…”

Section: Introductionmentioning

confidence: 99%

Stellar energy loss rates beyond the standard model

Llamas-Bugarin¹,

Gutiérrez‐Rodríguez²,

González-Sánchez³

et al. 2020

Preprint

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It is known that the dipole moments of the neutrino lead to important astrophysical and cosmological effects. In this regard, within the context of a U (1) B−L model, we develop and present novel analytical formulas to assess the effects of the anomalous magnetic moment and electric dipole moment of the neutrino on the stellar energy loss rates through some common physical process of pair-annihilation e + e − → (γ, Z, Z ′ ) → ν ν. Our results show that the stellar energy loss rates strongly depends on the effective magnetic moment of the neutrino, but also on the parameters which characterize the adopted U (1) B−L model.

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The role of the neutrino electromagnetic moments in the stellar energy loss rate

Cited by 19 publications

References 21 publications

Probing the electromagnetic dipole moments of the tau-neutrino in theU(1)B−Lmodel at the ILC and CLIC energies

Probing the electromagnetic dipole moments of the tau-neutrino in theU(1)B−Lmodel at the ILC and CLIC energies

Neutrino Energy Loss Rates in 3-3-1 Models

Stellar energy loss rates beyond the standard model

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