Re: Doing the Bose Nova

Posted by sol on September 21, 2003 at 22:09:37:

In Reply to: Re: Doing the Bose Nova posted by lanecove on September 21, 2003 at 10:08:28:

Lanecove,

   Unsymmetrical-cooling-gravity weaker
              Expanding
            \            /
             \          /
              \        /
              _\      /___
             /  \    /    /
            /    \  /    /
           /      \/    /<--------300,000 years
          /            /          Gravity strong
          -------------           Symmetrical
                ^
                I
            seedlike
 
                    
   Q-------------Quark measure
            \        /
             \      /
              \    /
               \  /
               Q--Q
                                     

Now in the Quark measure in the CMB Cobe Map, we understand the energy involved in the early universe and in a expansive mode the field measure weak because unsymmetrical values in discreteness apply?

I feel there are corrections that need to take place here, and one is in the understanding of the expansive mode and what we might have see of a triangle as it stretches?

Star light, gives us distant measure, but the blackness of the distance between those two stars say something else? IN the one sense one can think of a big blackhole we are in(?), and with the expansive mode and cooling nature, distance between these two stars would become greater?

If the blackhole was to expand, and what is represented here, in the space between those two stars, that we could not have seen the beginning of the universe?

I could use your help here:)

Sol

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Follow Ups: (Reload page to see most recent)

• Re: Doing the Bose Nova -- Ramanujan12 9/22/03 (1)
  • Supergravity -- sol 9/22/03 (0)
• The Quark Gluon Event -- sol 9/22/03 (0)

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