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Gary Ng Research review 2013 (Astrophysical neutrinos) |
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Report so far, as of 21/10/2013: NeutrinoReportLatex.tex
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- Why study v & what is special about them?
- To 'map' the sky / universe with methods other than visible light range.
- Tiny mass, very rarely interact, travels through medium.
- How & when did the concept of v come about?
- What were the initial theories? Are they still valid?
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- Is there only 1 type of v?
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- Is there only 1 source of v?
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- Solar v, Atmospheric v, SN v
- What are the similarities and/or differences between each type of v?
- Do they travel at different velocities?
- Do they have the same energies?
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- Were they all detected initially?
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- What equipment was used?
- What detection medium used?
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- No.
- Because they changed types, due to v oscillation.
- Neutrino Oscillaion
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- Have all types of v been detected now? How?
- Are all types of v detected together every time? Why not?
- Why are we studying SN v?
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- Production mechanism of SN v
- Why SN1987A ?
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- It was close enough to be observed
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- What is speical about SN v?
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- What is special about SN v?
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- Are they the same as when they were just produced, inside the SN?
- How do we detect SN v?
- With the experiments, do we just detect SN v?
- How do we distinguish which v are from what source?
- What is special / different about each detection method?
- Are there any differences in detection methods x years ago?
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- What are the results for the differnt methods?
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- What are the results for the different methods?
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- Does the results correspond to theory / prediction?
- Can we tell the direction of the SN v? If so, how?
- Can we tell the origin (location) of the SN v? If so, how?
- Can we tell the origin (time) of the SN v? If so, how?
- Can we tell the original type of the SN v? If so, how?
- ... (more questions) ...
- What will future SN v detection lead to?
Research Papers Topics:
- Supernovae SN1978A (see attachment)
- Core-collapse massive star to Supernovae theory proved.
- Solar neutrinos
- Solar neutrino problem
- Source of neutrino measurements
- Other high energy neutrino sources
Ideas:
- Investigate different types of neutrino detectors ('today')
- A timeline about neutrinos
- From theory to proof, to now-a-days research, to possible future developments
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| META FILEATTACHMENT |
attachment="Supernova_1987A.pdf" attr="" comment="" date="1381098823" name="Supernova_1987A.pdf" path="Supernova 1987A.pdf" size="6828394" user="zvah093" version="1" |
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| META FILEATTACHMENT |
attachment="Neutrinos_A_Different_Way_To_Look_At_The_Sky.pdf" attr="" comment="" date="1382361690" name="Neutrinos_A_Different_Way_To_Look_At_The_Sky.pdf" path="E:\RHUL\PH 4110 - Reserach Review (Astrophysical Neutrinos)\Neutrinos Papers\Neutrinos A Different Way To Look At The Sky.pdf" size="177485" user="zvah093" version="1" |
| META FILEATTACHMENT |
attachment="Supernova_neutrino_detection_-_Scholberg.pdf" attr="" comment="" date="1382361718" name="Supernova_neutrino_detection_-_Scholberg.pdf" path="Supernova_neutrino_detection_-_Scholberg.pdf" size="963464" user="zvah093" version="1" |
| META FILEATTACHMENT |
attachment="NeutrinoReportLatex.tex" attr="" comment="21/10/2013" date="1382367536" name="NeutrinoReportLatex.tex" path="NeutrinoReportLatex.tex" size="9996" user="zvah093" version="2" |
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