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Exploring Gauge-Higgs Inflation with Extra Dimensions: Abstract and Introduction
This story was originally published on HackerNoon at: https://hackernoon.com/exploring-gauge-higgs-inflation-with-extra-dimensions-abstract-and-introduction.
Delve into the mysteries of inflation with 5D U(1) gauge theory in a warped spacetime, exploring its implications for early universe dynamics.
Check more stories related to tech-stories at: https://hackernoon.com/c/tech-stories.
You can also check exclusive content about #cosmology, #inflation, #5d-gauge-theory, #warped-spacetime, #randall-sundrum-model, #early-universe-dynamics, #quantum-corrections, #gauge-higgs-inflation, and more.
This story was written by: @phenomenology. Learn more about this writer by checking @phenomenology's about page,
and for more stories, please visit hackernoon.com.
Inflation can solve both the flatness problem and the horizon problem at the same time and also explain temperature fluctuations of the cosmic microwave background (CMB) It is almost certain that inflation occurred in the early universe. In our model, fields involved in inflation obey a different type of boundary condition from that of the visible particles. A surviving Wilson line phase can play a specific role for physics beyond the standard model.
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By HackerNoonThis story was originally published on HackerNoon at: https://hackernoon.com/exploring-gauge-higgs-inflation-with-extra-dimensions-abstract-and-introduction.
Delve into the mysteries of inflation with 5D U(1) gauge theory in a warped spacetime, exploring its implications for early universe dynamics.
Check more stories related to tech-stories at: https://hackernoon.com/c/tech-stories.
You can also check exclusive content about #cosmology, #inflation, #5d-gauge-theory, #warped-spacetime, #randall-sundrum-model, #early-universe-dynamics, #quantum-corrections, #gauge-higgs-inflation, and more.
This story was written by: @phenomenology. Learn more about this writer by checking @phenomenology's about page,
and for more stories, please visit hackernoon.com.
Inflation can solve both the flatness problem and the horizon problem at the same time and also explain temperature fluctuations of the cosmic microwave background (CMB) It is almost certain that inflation occurred in the early universe. In our model, fields involved in inflation obey a different type of boundary condition from that of the visible particles. A surviving Wilson line phase can play a specific role for physics beyond the standard model.