Challenges of very high energy physics

In summary, the conversation revolves around the accuracy and strength of current experimental and theoretical tools at small distance scales, specifically those smaller than the proton's size. The idea of a quantum theory of gravity and the search for unified theories is also discussed, with the question of whether we are jumping the gun in our search. The conversation ends with a mention of the limitations and holes in current experimental support for the standard model.
  • #1
jfy4
649
3
Hi,

I'm not very "hip" with how accurate current experimental techniques are at distance scales less then that of the proton's size, but I am wondering about how strong our current theoretical tools are (and assumed to be) at smaller scales. I know we are searching for a quantum theory of gravity that is assumed to come into play at distance scales [itex]\approx 10^{-34}\text{m}[/itex], but looking at that number, it is outrageously small.

So small, that it seems to me there is as much "space" between the size of a proton and that length scale, as there is between our solar system and the proton size. Clearly physics as we know it changes dramatically between solar system dynamics, and atomic physics, are we possibly jumping the gun looking for unified theories etc... when we have so much "distance" still to cover? Another example, LQG displays that it can remain UV-finite even while coupling to a fermion field, yet, is there reason to believe that the fermion field physics remains the same in a domain nineteen orders of magnitude smaller then where it is found successful?

Thanks in advance,
 
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  • #2
We haven't reached energy scales where we can verify all aspects of standard model yet. So no, we are nowhere near probing nature at these scales, and I'm not sure we ever will be. But unified theory isn't guaranteed to give predictions that are verifiable only at these length/energy scales. There could be predictions we can actually test. Going back, again, to the fact that there are currently enough holes in experimental support for standard model. Whether any are there due to problems with model is impossible to tell, of course, because a lot of them are due to either experimental or numerical limitations.
 

FAQ: Challenges of very high energy physics

1. What is very high energy physics?

Very high energy physics is a branch of physics that focuses on the study of particles and interactions at extremely high energies, typically achieved through particle accelerators. This field is important for understanding the fundamental building blocks of the universe and the forces that govern them.

2. What are the main challenges in studying very high energy physics?

Some of the main challenges in studying very high energy physics include building and maintaining expensive and complex particle accelerators, analyzing and interpreting massive amounts of data, and understanding the fundamental theories and models that govern this field.

3. How do scientists deal with the challenges of very high energy physics?

Scientists use advanced technologies and techniques to build and operate particle accelerators, such as superconducting magnets and high-powered lasers. They also use computational tools and algorithms to analyze and interpret data, and collaborate with other researchers to develop and refine theories and models.

4. What are the potential benefits of studying very high energy physics?

Studying very high energy physics can lead to a deeper understanding of the fundamental laws of nature, which can have practical applications in fields such as energy production, medical imaging, and materials science. It can also provide insight into the origins and evolution of the universe.

5. What are some current areas of research in very high energy physics?

Some current areas of research in very high energy physics include the search for new particles and forces, such as the Higgs boson and dark matter, the study of the properties of known particles, and the exploration of the nature of space and time at the smallest scales.

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