Possible research topics for high redshift galaxies and AGN

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Discussion Overview

The discussion revolves around potential research topics related to high redshift galaxies and active galactic nuclei (AGN). Participants explore various avenues for research, including specific areas of interest and broader theoretical implications.

Discussion Character

  • Exploratory
  • Technical explanation
  • Debate/contested

Main Points Raised

  • Simon expresses interest in researching the formation and evolution of high redshift galaxies and AGN, particularly in the optical and radio domains.
  • One participant suggests that Simon consult with a faculty advisor for guidance, emphasizing the importance of aligning research topics with the advisor's interests.
  • Another participant recommends reviewing recent conference materials to identify current trends and topics in the field.
  • A more speculative idea is presented regarding the implications of galaxies with greater redshift accelerating away from observers, proposing a question about the universe's half-life and its relationship to potential energy and dark energy.
  • A participant mentions an active AGN research group at Keele University, suggesting it as a resource for Simon's research endeavors.

Areas of Agreement / Disagreement

Participants generally agree on the importance of aligning research topics with faculty interests and exploring current trends in the field. However, there is no consensus on specific research topics, and the speculative idea presented introduces a contested theoretical perspective.

Contextual Notes

Some discussions involve assumptions about the relationship between redshift, acceleration, and energy concepts, which may not be universally accepted or resolved. The implications of these ideas remain open to interpretation and further exploration.

Who May Find This Useful

This discussion may be useful for students and researchers interested in high redshift galaxies, AGN, and the theoretical implications of cosmological observations.

Cptn.Shelly
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Hi all,

I am nearing the start of my final year at university and part of that year is a large research project on a subject of our choice. My main interests lie within the formation and evolution of high redshift (z ≥ 1) galaxies and AGN. At this stage I am only starting to think about what areas I could possibly research, but has anyone got any ideas of certain topics I could cover? I am particularly interested in the Optical and Radio side of things but I am definitely open to exploring more areas.

Thanks :)

Simon
 
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Aren't you working with a faculty member on this project? Usually there is some kind of guidance. That would be a good person to ask, because they will likely need to give you some background, so it should be something they are interested in and have a vested interest in a successful outcome.
 
I would suggest you find the homepage of some recent conference on the subject that interests you and brows the talk slides (if there are any) to see what is happening.

Also, realize that what you end up do is most strongly decided by what the good advisor is willing to do. And what they are willing to do is typically set independently of your interests.
 
I have an idea, as galaxies with a greater redshift are increasingly accelerating from the observer, the subtle understanding means that the space between the galaxies has no limit with respect to the speed of light and the overall speed of relative galaxies becomes additive and together can exceed the speed of light. You can use this info to ask the question;
"Does the universe have a half life?" And can a subtle change in understanding lead to measuring the half life as a function of space increasing (constant velocity) with respect to overall potential energy decreasing. This is not a reduction of total energy, just usable particle energy. If this is true, then potential energy decrease is a direct result of space increasing and dark energy just becomes Newton's second law of motion. A constant force of potential energy decrease = a decreasing mass with the resulting mass continuously increasing in acceleration until all the potential energy is used resulting in a universe becoming space itself. The key is to show no local control in between galaxies with respect to the speed of light.
How is that for making your statement?!
 
Cptn Shelley, there is a very active AGN research group at Keele University, UK. That's where I did my PhD (on stellar evolution and nucleosynthesis though). Have a poke!
 

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