Consequences of a fourth neutrino type

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Homework Help Overview

The discussion revolves around the implications of a hypothetical fourth type of neutrino on the development of the universe, particularly in relation to the production of photons and helium-4. Participants explore how this additional neutrino might influence baryonic matter and the temperature evolution of the early universe.

Discussion Character

  • Exploratory, Conceptual clarification, Assumption checking

Approaches and Questions Raised

  • Participants discuss various potential outcomes of introducing a fourth neutrino type, including its effects on photon and helium-4 production. Questions arise regarding the relationship between neutrinos and the temperature evolution of the universe, as well as the implications for baryonic matter and neutron-to-proton ratios.

Discussion Status

The discussion is ongoing, with participants sharing their thoughts and reasoning. Some guidance has been provided regarding the influence of neutrinos on the early universe, and there is an acknowledgment of the need to consider conservation principles. Multiple interpretations are being explored, particularly regarding the effects on neutron and proton ratios.

Contextual Notes

Participants note the absence of specific equations or relations that could clarify the problem, and there is a recognition of the complexities involved in understanding neutrino interactions and their consequences in cosmology.

szcsongor
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Homework Statement
If there was a fourth neutrino type it would have affected Universe's development the following way...
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Hi,

I got this question on a recent astronomy course but can't really find the right answer (rough translation from Swedish):

If there was a fourth neutrino type it would have affected Universe's development the following way:
a. more photons and more He-4 generated
b. less photons and less He-4
c. more neutrons and more He-4
d. more protons and more He-4

My guess would be answer (a) but I'm not sure.
 
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Relevant Equations
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Are you sure you don't have equations describing the evolution of the early universe? How does its temperature change over time? How does that depend on neutrinos?
szcsongor said:
My guess would be answer (a) but I'm not sure.
Why do you guess (a)?
 
Hi,

Thanks for the quick reply. I was on holiday, so couldn't answer sooner.
I was thinking about this question but unfortunately I don't know how to start solving it. I guess there are some relations (equations?) to use here but I'm unable to see it :(

The temperature of the universe is decreasing constantly, but I don't see the relation with neutrinos.
My guess was a) because I was thinking that neutrinos are produced in the process of H-1 -> He-4 alongside with photons, so another type of neutrinos could be a consequence of more He-4 and photons produced. But it might be true only in stars... Or might be that I'm wrong completely :)
 
Think earlier. How did neutrinos influence the temperature evolution?
Electron neutrinos were important for the neutron to proton ratio, but a fourth generation neutrino shouldn't affect that directly as it doesn't couple to electrons.

If you prefer you can also look up how Planck measured the number of neutrino generations in the early universe. Their result was 3...
 
Thanks for trying to help.
I think I see now how I should proceed with this. I also found clues in the course material now when I read through it:

If we "put in" an other type of neutrino into the universe there should be less baryonic matter to comply with the principle of conservation of mass. But since neutrinos do not interact with matter (and also almost massless), the universe would have expanded faster. The consequence would have been more neutrons (higher neutron / proton ratio) because there would have been less time for the n -> p + e + v reaction. And more neutrons mean more He-4 generated. Therefore answer (c) seem to be the right one.
Am I right? :)
 
Sounds plausible.
 

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