Big Bang soup; Hot, Cold, or Just Right
The Big Bang in Quantum Wave Cosmology (QWC) is more of a big event that causes the initial expansion; a big burst in QWC terms. And from the discussion of limits to energy density and the mass/gravity functioning threshold I have proposed a sequence of events that leads to the big burst.
One of those events in the sequence is the negation of particles and radiation into dense state energy. Negation occurs in a big crunch when the energy density of the particles exceeds the density range within which matter can function.
As a result, the matter that was formerly emitting gravity has ceased to exist as matter and has become dense state energy. There is no gravity emitted from dense state energy.
This post focuses on the temperature profile of the expansion scenario. Of course it is hot. Compression of mass due to gravity causes heat much like a gas when compressed heats up (not a perfect analogy). Accretion into the crunch heats particles and plasma to billions of degrees (not a scientific description of the process). Energy levels surrounding the crunch increase as the speed of the inflowing particles/matter/radiation/plasma approach the speed of light (not a scientific description).
Unless this process is interrupted the temperature continues to increase as the accretion proceeds. How hot can something get; this is the place where it happens whatever that temperature is whether or not there is even thought to be a maximum.
But in QWC there is a maximum temperature and it is associated with this process of building a big crunch from the galactic material caught up in the overlap of intersecting arenas. Because in QWC there is a point when the buildup stops, it follows that the engine that is causing the increase in temperature gets turned off gradually until the crunch fails and the burst occurs.
BBT starts 10^-30 (according to Alan Guth in 1996) seconds after the event and talks of a most extreme temperature. It follows the temperature profile of the universe through exponential expansion (Inflation) and through the cooling process. It says that the CMBR temperature that is ~2.7 degrees K everywhere is causally connected to the big bang event or at least to the 10^-30 point in time.
QWC has the big crunch surrounded by a CMBR already before the bang event occurs. If we did a temperature profile of a big bang event in existing space surrounded by background energy at a temperature down in those lowest ranges on the Kelvin scale there would be a different sequence of events and a different temperature profile associated with the different events. That is the case with QWC.
The energy background consisting of electromagnetic radiation resulting from a long history of arena action throughout the greater universe would have a signature temperature. I don’t know what it is but speculation (using the QWC methodology for speculation) suggests a temperature slightly lower than the 2.7 degrees that we observe today within the event horizon.
Whatever that temperature might be, since the dense dark energy of the initial expansion begins to equalize with the background energy from the first instant of expansion, the Inflation scenario would change. How would it change? Would we still be looking at ~14 billion years since the Big Bang? Would we still need superluminal inflation?
The Big Bang in Quantum Wave Cosmology (QWC) is more of a big event that causes the initial expansion; a big burst in QWC terms. And from the discussion of limits to energy density and the mass/gravity functioning threshold I have proposed a sequence of events that leads to the big burst.
One of those events in the sequence is the negation of particles and radiation into dense state energy. Negation occurs in a big crunch when the energy density of the particles exceeds the density range within which matter can function.
As a result, the matter that was formerly emitting gravity has ceased to exist as matter and has become dense state energy. There is no gravity emitted from dense state energy.
This post focuses on the temperature profile of the expansion scenario. Of course it is hot. Compression of mass due to gravity causes heat much like a gas when compressed heats up (not a perfect analogy). Accretion into the crunch heats particles and plasma to billions of degrees (not a scientific description of the process). Energy levels surrounding the crunch increase as the speed of the inflowing particles/matter/radiation/plasma approach the speed of light (not a scientific description).
Unless this process is interrupted the temperature continues to increase as the accretion proceeds. How hot can something get; this is the place where it happens whatever that temperature is whether or not there is even thought to be a maximum.
But in QWC there is a maximum temperature and it is associated with this process of building a big crunch from the galactic material caught up in the overlap of intersecting arenas. Because in QWC there is a point when the buildup stops, it follows that the engine that is causing the increase in temperature gets turned off gradually until the crunch fails and the burst occurs.
BBT starts 10^-30 (according to Alan Guth in 1996) seconds after the event and talks of a most extreme temperature. It follows the temperature profile of the universe through exponential expansion (Inflation) and through the cooling process. It says that the CMBR temperature that is ~2.7 degrees K everywhere is causally connected to the big bang event or at least to the 10^-30 point in time.
QWC has the big crunch surrounded by a CMBR already before the bang event occurs. If we did a temperature profile of a big bang event in existing space surrounded by background energy at a temperature down in those lowest ranges on the Kelvin scale there would be a different sequence of events and a different temperature profile associated with the different events. That is the case with QWC.
The energy background consisting of electromagnetic radiation resulting from a long history of arena action throughout the greater universe would have a signature temperature. I don’t know what it is but speculation (using the QWC methodology for speculation) suggests a temperature slightly lower than the 2.7 degrees that we observe today within the event horizon.
Whatever that temperature might be, since the dense dark energy of the initial expansion begins to equalize with the background energy from the first instant of expansion, the Inflation scenario would change. How would it change? Would we still be looking at ~14 billion years since the Big Bang? Would we still need superluminal inflation?