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Neutrinos interact with matter through the weak interaction. For the neutrino flux to have a measurable effect on decay rates, an enormous flux of neutrinos would be needed, not available from the sun. Consider that it takes years to gather some thousands of events from neutrinos of the sun in the neutrino experiments.

A mole of matter, radioactive or not, consists of $\sim10^{23}$ particles and it is evident that the neutrino-matter interactions are too weak to present a field that might affect decay rates, the way that in this link electric and magnetic fields do affect slightly decay rates.

The difference is that electromagnetism couples contributing with a strength of ($1/137$) to the cross section by each vertex, but weak interactions by $(10^{-6})^2$$(10^{-6})$ as seen in this table:

fundamental forces

The existing neutrino experiments, together with the decay rates and interactions of weak interactions, are an experimental proof that neutrinos from the sun can be ignored as far as nuclear decays go.

Neutrinos interact with matter through the weak interaction. For the neutrino flux to have a measurable effect on decay rates, an enormous flux of neutrinos would be needed, not available from the sun. Consider that it takes years to gather some thousands of events from neutrinos of the sun in the neutrino experiments.

A mole of matter, radioactive or not, consists of $\sim10^{23}$ particles and it is evident that the neutrino-matter interactions are too weak to present a field that might affect decay rates, the way that in this link electric and magnetic fields do affect slightly decay rates.

The difference is that electromagnetism couples contributing with a strength of ($1/137$) to the cross section by each vertex, but weak interactions by $(10^{-6})^2$ as seen in this table:

fundamental forces

The existing neutrino experiments, together with the decay rates and interactions of weak interactions, are an experimental proof that neutrinos from the sun can be ignored as far as nuclear decays go.

Neutrinos interact with matter through the weak interaction. For the neutrino flux to have a measurable effect on decay rates, an enormous flux of neutrinos would be needed, not available from the sun. Consider that it takes years to gather some thousands of events from neutrinos of the sun in the neutrino experiments.

A mole of matter, radioactive or not, consists of $\sim10^{23}$ particles and it is evident that the neutrino-matter interactions are too weak to present a field that might affect decay rates, the way that in this link electric and magnetic fields do affect slightly decay rates.

The difference is that electromagnetism couples contributing with a strength of ($1/137$) to the cross section by each vertex, but weak interactions by $(10^{-6})$ as seen in this table:

fundamental forces

The existing neutrino experiments, together with the decay rates and interactions of weak interactions, are an experimental proof that neutrinos from the sun can be ignored as far as nuclear decays go.

3 Minor improvements in typography and punctuation
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Neutrinos interact with matter through the weak interaction. ForFor the neutrino flux to have a measurable effect on decay rates  , an enormous flux of neutrinos would be needed, not available from the sun. Consider that it takes years toto gather some thousands of events from neutrinos of the sun in the neutrino experiments  .A mole

A mole of matter, radioactive or not, consists of ~10^23$\sim10^{23}$ particles and it is evident that the neutrino-matter interactions are too weak to present a field that might affect decay rates, the way that in this link electric and magnetic fields do affect slightly decay rates.

The difference is that electromagnetism couples contributing with a strength of (1/137$1/137$) to the crossectioncross section by each vertex, butbut weak interactions by (10^-6)^2$(10^{-6})^2$ as seen in this table:

fundamental forces

The existing neutrino experiments, together with the decay rates and interactions of weak interactions, are an experimental proof that neutrinos from the sun can be ignored as far as nuclear decays go.

Neutrinos interact with matter through the weak interaction. For the neutrino flux to have a measurable effect on decay rates  , an enormous flux of neutrinos would be needed, not available from the sun. Consider that it takes years to gather some thousands of events from neutrinos of the sun in the neutrino experiments  .A mole of matter, radioactive or not, consists of ~10^23 particles and it is evident that the neutrino-matter interactions are too weak to present a field that might affect decay rates, the way that in this link electric and magnetic fields do affect slightly decay rates

The difference is that electromagnetism couples contributing with a strength of (1/137) to the crossection by each vertex, but weak interactions by (10^-6)^2 as seen in this table:

fundamental forces

The existing neutrino experiments, together with the decay rates and interactions of weak interactions, are an experimental proof that neutrinos from the sun can be ignored as far as nuclear decays go.

Neutrinos interact with matter through the weak interaction. For the neutrino flux to have a measurable effect on decay rates, an enormous flux of neutrinos would be needed, not available from the sun. Consider that it takes years to gather some thousands of events from neutrinos of the sun in the neutrino experiments.

A mole of matter, radioactive or not, consists of $\sim10^{23}$ particles and it is evident that the neutrino-matter interactions are too weak to present a field that might affect decay rates, the way that in this link electric and magnetic fields do affect slightly decay rates.

The difference is that electromagnetism couples contributing with a strength of ($1/137$) to the cross section by each vertex, but weak interactions by $(10^{-6})^2$ as seen in this table:

fundamental forces

The existing neutrino experiments, together with the decay rates and interactions of weak interactions, are an experimental proof that neutrinos from the sun can be ignored as far as nuclear decays go.

2 added 49 characters in body
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Neutrinos interact with matter through the weak interaction. For the neutrino flux to have a measurable effect on decay rates , an enormous flux of neutrinos would be needed, not available from the sun. Consider that it takes years to gather some thousands of events from neutrinos of the sun in the neutrino experiments .A mole of matter, radioactive or not, consists of ~10^23 particles and it is evident that the neutrino-matter interactions are too weak to present a field that might affect decay rates, the way that in this link electric and magnetic fields do affect slightly decay rates

The difference is that electromagnetism couples contributing with a strength of (1/137)^2 but to the crossection by each vertex, but weak interactions by (10^-6)^2 as seen in this table:

fundamental forces

The existing neutrino experiments, together with the decay rates and interactions of weak interactions, are an experimental proof that neutrinos from the sun can be ignored as far as nuclear decays go.

Neutrinos interact with matter through the weak interaction. For the neutrino flux to have a measurable effect on decay rates , an enormous flux of neutrinos would be needed, not available from the sun. Consider that it takes years to gather some thousands of events from neutrinos of the sun in the neutrino experiments .A mole of matter, radioactive or not, consists of ~10^23 particles and it is evident that the neutrino-matter interactions are too weak to present a field that might affect decay rates, the way that in this link electric and magnetic fields do affect slightly decay rates

The difference is that electromagnetism couples with a strength of (1/137)^2 but weak interactions by (10^-6)^2 as seen in this table:

fundamental forces

The existing neutrino experiments, together with the decay rates and interactions of weak interactions, are an experimental proof that neutrinos from the sun can be ignored as far as nuclear decays go.

Neutrinos interact with matter through the weak interaction. For the neutrino flux to have a measurable effect on decay rates , an enormous flux of neutrinos would be needed, not available from the sun. Consider that it takes years to gather some thousands of events from neutrinos of the sun in the neutrino experiments .A mole of matter, radioactive or not, consists of ~10^23 particles and it is evident that the neutrino-matter interactions are too weak to present a field that might affect decay rates, the way that in this link electric and magnetic fields do affect slightly decay rates

The difference is that electromagnetism couples contributing with a strength of (1/137) to the crossection by each vertex, but weak interactions by (10^-6)^2 as seen in this table:

fundamental forces

The existing neutrino experiments, together with the decay rates and interactions of weak interactions, are an experimental proof that neutrinos from the sun can be ignored as far as nuclear decays go.

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