Paul W. Dixon
Registered Senior Member
SUPERNOVA FROM EXPERIMENTATION AT FERMILAB
SUPERNOVA FROM EXPERIMENTATION AT FERMILAB
All friends and colleagues: please relay this information to all interested groups, websites, accelerator personnel, etc..
The values now given for Fermilab as seen on the Tevatron Status of the Acclerator Update posted on the homepage for FERMILAB are now set at about 2 TeV. This is a marked increase from the previous value of 1.8 TeV. The luminosity also increases after the initial value of about 7.6E30 to much higher values as the experiment proceeds. Please monitor the Accelerator Update live status to observe these effects.
The article in the Astronomical Journal (Leibgundgut, B., et al., (1993) SN 1991BG: A Type 1A Supernova with a difference (1) January 301-313) shows evidence for a supernova which has deflagrated below the Chandresekhar limit at .7 solar masses. This was also chronicled in the journal, Nature. Also from Peter M. Garnavich, "Early Spectra of Supernova 1993J in MB1, Astronomy Journal, 108 (3) (1994) on page 1006 it is stated: "The observed drop in H alpha flux inserted in this model implies a zero radius for the progenitor at March 29.5 regardless of expansion velocity assumed. This is clearly unphysical." Unless, it is as here postulated, a transition towards de Sitter space which provides for those vast energies of supernova deflagration: which is then clearly physical and of nearly zero dimensionality.
Every child on earth will thank you for your kind efforts on their behalf now and for all future time.
All Best Wishes for the New Year !!!
Yours sincerely,
Paul W. Dixon, Ph.D.
Supernova from Experimentation
SUPERNOVA FROM EXPERIMENTATION AT FERMILAB
All friends and colleagues: please relay this information to all interested groups, websites, accelerator personnel, etc..
The values now given for Fermilab as seen on the Tevatron Status of the Acclerator Update posted on the homepage for FERMILAB are now set at about 2 TeV. This is a marked increase from the previous value of 1.8 TeV. The luminosity also increases after the initial value of about 7.6E30 to much higher values as the experiment proceeds. Please monitor the Accelerator Update live status to observe these effects.
The article in the Astronomical Journal (Leibgundgut, B., et al., (1993) SN 1991BG: A Type 1A Supernova with a difference (1) January 301-313) shows evidence for a supernova which has deflagrated below the Chandresekhar limit at .7 solar masses. This was also chronicled in the journal, Nature. Also from Peter M. Garnavich, "Early Spectra of Supernova 1993J in MB1, Astronomy Journal, 108 (3) (1994) on page 1006 it is stated: "The observed drop in H alpha flux inserted in this model implies a zero radius for the progenitor at March 29.5 regardless of expansion velocity assumed. This is clearly unphysical." Unless, it is as here postulated, a transition towards de Sitter space which provides for those vast energies of supernova deflagration: which is then clearly physical and of nearly zero dimensionality.
Every child on earth will thank you for your kind efforts on their behalf now and for all future time.
All Best Wishes for the New Year !!!
Yours sincerely,
Paul W. Dixon, Ph.D.
Supernova from Experimentation
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