Big Bang: Unravelling the Temperature Mystery

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SUMMARY

The discussion centers on the concept of temperature in the context of the Big Bang, emphasizing that temperature is not solely a measure of kinetic energy of atomic particles. Instead, it is defined as the rate of energy change with respect to entropy, represented by the equation T=\frac{\partial E}{\partial S}. The conversation highlights that even in the absence of elementary particles, such as at the moment of the Big Bang, temperature can still be defined through electromagnetic radiation, as evidenced by cosmic microwave background (CMB) maps. Furthermore, it notes that classical models fail as one approaches time zero, necessitating the use of quantum cosmology models for accurate descriptions.

PREREQUISITES
  • Understanding of thermodynamics and the definition of temperature
  • Familiarity with cosmic microwave background (CMB) radiation
  • Basic knowledge of classical and quantum cosmology
  • Mathematical proficiency in calculus, particularly in understanding derivatives
NEXT STEPS
  • Research quantum cosmology models and their implications for early universe conditions
  • Study the properties and significance of cosmic microwave background radiation
  • Explore the mathematical foundations of temperature as defined by entropy
  • Investigate the breakdown of classical models in cosmology and the transition to quantum theories
USEFUL FOR

Astrophysicists, cosmologists, and students of physics interested in the fundamental concepts of temperature and energy in the early universe, as well as those exploring the implications of quantum mechanics in cosmological models.

Steven Harris
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If temperature is a measure of the kinetic energy of atomic particles in matter, and at the instant of the big bang no elementary particles existed, how can the early universe be said to have huge or nearly infinite temperature?
 
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Temperature isn't exclusively a measure of kinetic energy of atomic particles in matter; it's just what happens to be true for most simple systems. The proper definition of temperature is the rate at which energy changes with respect to entropy, i.e., [tex]T=\frac{\partial E}{\partial S}[/tex].
 
I didn't see Nick's reply! I was replying directly to the initial post.

Steven Harris said:
If temperature is a measure of the kinetic energy of atomic particles in matter, and at the instant ...
Well light has temperature.

You have seen those oval blue and red maps of the CMB sky (cosmic microwave background). Those maps show the temperature of electromagnetic radiation seen looking in different directions. Temperature of (black-body) radiation is well-defined, so you don't need conventional matter particles like electrons and quarks to have temperature. You can have an empty metal box with a vacuum inside and the space in the box will still have a well-defined temp.

A far more serious problem in talking about the very early (you mentioned the "instant") is that the classical model model breaks down---it stops being applicable as you approach time zero. "singularity" = breakdown of the old unquantized model. The math starts to give meaningless answers and can no longer be trusted.

Need quantum cosmology models then.
http://www.slac.stanford.edu/spires/find/hep/www?rawcmd=FIND+DK+QUANTUM+COSMOLOGY+AND+DATE+%3E+2005&FORMAT=www&SEQUENCE=citecount%28d%29
 
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