Inflation and GUTs: Energy Scales & Model Dependence

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In summary: This causal relation is also supported by the observation that the standard model GUTs are very sensitive to the energy scale.In summary, inflation and GUTs are independent, but there is a temporal sequence of events where inflation begins ~ 10^-37 sec after GUT symmetry breaking and the GUT energy corresponds to a time scale of about 10^-39 sec.
  • #1
Jim
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Can someone please clarify if the energy scales of Inflation & GUTs are identical,
or model-dependent ? One typically sees ~10^15 Gev to 2x10^16 Gev in the literature,
which is a small variance, but its not clear if there are `standard values'.

I am also curious if one can have inflation without GUTs ?
 
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  • #2
The scales of inflation and GUTs are independent, so yes, one can have inflation without GUTs. And on the flip side, GUTs don't automatically incorporate inflation. The usually quoted characteristic energy scale of inflation 10^15-10^16 Gev is based on observation. Unlike inflation, GUTs are hypothetical, and the energy scales associated with them are model-dependent. It just so happens that "standard" field theory GUTs require a scale of 10^16 Gev. But there are certainly GUTs, e.g. in theories with at least one extra dimension, in which the characteristic scale is of a different order of magnitude.
 
  • #3
Keep in mind, historically, inflation was partially invented to rescue GUT theories in cosmology. GUT theories are amongst the most widely held beliefs (that we can't prove) in the HEP community. They're almost taken for granted.

The problem is many typical models incorporate a preponderous of particles like magnetic monopoles and other various topological defects. Roughly, they should be everywhere, b/c the big bang would copiously produce them and that is flagrantly in violation of observation.

Enter an inflationary epoch somewhere around the GUT scale (typically a little bit higher energy), which dilutes the abundance to observational limits.
 
  • #4
Jim said:
I am also curious if one can have inflation without GUTs ?

Just a thought, particles are created near horizons, e.g. black holes. But acceleration also creates horizons, i.e. Unruh effect. So if space is expanding exponentially (inflation), then every point in space becomes an horizon due to acceleration. So perhaps it is that inflation is what is responsible for the original particles to begin with, and therefore connected in some way to GUT's
 
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  • #5
Thanx all for your quik responses !

Haelfix: Agree about the historical correlation. Running with the mSSM value of 2E16 Gev
for the GUT group to split into SU(3) and SU(2)xU(1), this occurs considerably prior to reheating at ~ 2E15 Gev, when FRW evolution kicks in again. The time scales are approx.,
Trh ~ 100Tgut. Clearly, there is a temporal sequence of events here.

In terms of chicken v. egg, accd'g to Guth, inflation began ~ 10^-37 sec. mSSM GUT energy corresponds to a time scale of about 10^-39 sec, which strongly suggests a causal relation, with the GUT symmetry breaking causing the phase transition driving inflation.
Indeed, it seems more aesthetic to have the GUT symmetry breaking initiate inflation, since GUTs correspond to ~ 100-1000 Planck lengths, whereas inflation ranges up into the macroscopic domain ~ centimeters.
 

Related to Inflation and GUTs: Energy Scales & Model Dependence

1. What is inflation and how does it relate to the Grand Unified Theory (GUT)?

Inflation is a period of rapid expansion of the universe that is believed to have occurred in the early stages of the universe's evolution. It is a key part of the Big Bang theory and helps to explain the large-scale structure of the universe. The Grand Unified Theory is a proposed theory that aims to unify the three fundamental forces of nature (strong nuclear force, weak nuclear force, and electromagnetism) into one single force. Inflation is thought to have occurred at energy scales close to those predicted by GUTs.

2. What is the energy scale of inflation and how is it measured?

The energy scale of inflation is estimated to be around 10^16 GeV (gigaelectronvolts), which is much higher than the energy scales currently accessible in particle accelerators. It is typically measured indirectly through observations of the cosmic microwave background radiation, which can provide information about the conditions of the early universe.

3. How does the energy scale of inflation affect the formation of the universe?

The high energy scale of inflation is believed to have driven the rapid expansion of the universe, allowing it to become smooth and homogeneous. This is important for the formation of large-scale structures, such as galaxies and clusters of galaxies, as well as the distribution of matter in the universe.

4. What is the role of GUTs in inflation models?

GUTs play a significant role in inflation models as they provide a framework for understanding the physics of the early universe at very high energies. Many inflation models are based on GUTs and use their predictions to make testable predictions about the universe.

5. How does the choice of inflation model affect our understanding of the universe?

The choice of inflation model can greatly impact our understanding of the universe, as different models make different predictions about the energy scale and duration of inflation, as well as the nature of the particles responsible for driving inflation. By studying the effects of different models, scientists can gain a better understanding of the fundamental laws of the universe and potentially rule out certain theories.

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