has been cited by the following article(s):
[1]
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Quantum versus Classical nature of the early universe and its Consequences (Entanglement?)
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NULL |
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[2]
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How to determine a jump in energy prior to a causal barrier, with an attendant current, for an effective initial magnetic field. In the Pre Planckian to Planckian …
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2018 |
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[3]
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Does GW generation has semi classical features?
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Journal of High Energy Physics, Gravitation and Cosmology,
2017 |
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[4]
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Does GW Generation Have Semi-Classical Features?
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2017 |
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[5]
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Is the Cosmological Constant, a “Vacuum” Field? We Explore This by Squeezing Early Universe “Coherent-Semi Classical States”, and Compare This to Energy …
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2016 |
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[6]
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Is the Cosmological Constant, a “Vacuum” Field? We Explore This by Squeezing Early Universe “Coherent-Semi Classical States”, and Compare This to …
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2016 |
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[7]
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Is Nature fundamentally continuous or discrete, and what violations of the Null Energy Condition tell us about information exchange between prior to present universes ?
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2014 |
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[8]
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Entropy Production and a Toy Model as to Irregularities in the CMBR Spectrum
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dim,
2014 |
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[9]
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What violations of the Null Energy Condition tell us about information exchange between prior to present universes? How to obtain spectral index confirmation?
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dim,
2014 |
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[10]
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Is Nature fundamentally continuous or discrete, and what violations of the Null Energy Condition tell us about information exchange between prior to present universes?
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dim,
2014 |
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[1]
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Does GW Generation Have Semi-Classical Features?
Journal of High Energy Physics, Gravitation and Cosmology,
2017
DOI:10.4236/jhepgc.2017.31008
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[2]
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Is the Cosmological Constant, a “Vacuum” Field? We Explore This by Squeezing Early Universe “Coherent-Semi Classical States”, and Compare This to Energy from the Early Universe Heisenberg Uncertainty Principle
Journal of High Energy Physics, Gravitation and Cosmology,
2016
DOI:10.4236/jhepgc.2016.24047
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