Paul W. Dixon
Registered Senior Member
Supernova From Experimentaton At Fermilab
SUPERNOVA FROM EXPERIMENTATION AT FERMILAB CERN, BROOKHAVEN AND HERA
The transition towards de Sitter Space, which is achieved through breaching the potential barrier between the continuum and the false de Sitter vacuum is accomplished via those energies which are now equivalent to those found at the point origin of this Universe under this postulation. The current unsupported hypothesis in the literature is that Type Ia Supernova have origin in white dwarf stars though the companion from whom mass is accreted has to be in all cases of having no hydrogen since Type Ia Supernova show no hydrogen at the time of maximum light. Also we now have evidence for a Type Ia Supernova which no longer conforms to the Chandrasekhar limit for the collapse of the 2.1 solar mass progenitor object. Having the companion object with no hydrogen for accretion, as well as being "The type Ia SNLA-03D3bb from a super-Chandrasekar-mass white dwarf star (D. Andrew Howell et al (2006) Nature,443, 7109, 308-311) are both unlikely events cosmologically. One can continue to invent post-hoc hypotheses to account for empirical observations up to a point when the entire structure of explanation collapses of it own weight.
Its time to wake up before we generate a Type Ia Supernova!!!
All the children will thank you for your kind actions on their behalf.
Yours sincerely,
Paul W. Dixon, Ph.D.
Supernova from Experimentation
SUPERNOVA FROM EXPERIMENTATION AT FERMILAB CERN, BROOKHAVEN AND HERA
The transition towards de Sitter Space, which is achieved through breaching the potential barrier between the continuum and the false de Sitter vacuum is accomplished via those energies which are now equivalent to those found at the point origin of this Universe under this postulation. The current unsupported hypothesis in the literature is that Type Ia Supernova have origin in white dwarf stars though the companion from whom mass is accreted has to be in all cases of having no hydrogen since Type Ia Supernova show no hydrogen at the time of maximum light. Also we now have evidence for a Type Ia Supernova which no longer conforms to the Chandrasekhar limit for the collapse of the 2.1 solar mass progenitor object. Having the companion object with no hydrogen for accretion, as well as being "The type Ia SNLA-03D3bb from a super-Chandrasekar-mass white dwarf star (D. Andrew Howell et al (2006) Nature,443, 7109, 308-311) are both unlikely events cosmologically. One can continue to invent post-hoc hypotheses to account for empirical observations up to a point when the entire structure of explanation collapses of it own weight.
Its time to wake up before we generate a Type Ia Supernova!!!
All the children will thank you for your kind actions on their behalf.
Yours sincerely,
Paul W. Dixon, Ph.D.
Supernova from Experimentation