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  2. Borde–Guth–Vilenkin theorem - Wikipedia

    en.wikipedia.org/wiki/BordeGuthVilenkin...

    The BordeGuthVilenkin (BGV) theorem is a theorem in physical cosmology which deduces that any universe that has, on average, been expanding throughout its history cannot be infinite in the past but must have a past spacetime boundary. [1]

  3. Kalam cosmological argument - Wikipedia

    en.wikipedia.org/wiki/Kalam_cosmological_argument

    In publications, he would propose that the Borde–Guth–Vilenkin theorem is sufficient evidence for a beginning of the universe. [50] [51] [52] Craig has stated that, if anything existed before the past boundary described by the theorem, it would be a non-classical region described by an as-yet-undetermined theory of quantum gravity.

  4. Alexander Vilenkin - Wikipedia

    en.wikipedia.org/wiki/Alexander_Vilenkin

    In 1982, Paul Steinhardt presented the first model of eternal inflation, Vilenkin showed that eternal inflation is generic. [9] Furthermore, working with Arvind Borde and Alan Guth, he developed the Borde–Guth–Vilenkin theorem, showing that a period of inflation must have a beginning and that a period of time must precede it. [10]

  5. Category:Eponymous theorems of physics - Wikipedia

    en.wikipedia.org/wiki/Category:Eponymous...

    Borde–Guth–Vilenkin theorem; Buckingham π theorem; C. Carnot's theorem (thermodynamics) Castigliano's method; Chung–Fuchs theorem; Clairaut's theorem (gravity)

  6. Cosmological argument - Wikipedia

    en.wikipedia.org/wiki/Cosmological_argument

    For scientific evidence of the finitude of the past, Craig refers to the Borde-Guth-Vilenkin theorem, which posits a past boundary to cosmic inflation, and the general consensus on the standard model of cosmology, which refers to the origin of the universe in the Big Bang. [44] [45]

  7. Cosmic inflation - Wikipedia

    en.wikipedia.org/wiki/Cosmic_inflation

    The "no-hair" theorem works essentially because the cosmological horizon is no different from a black-hole horizon, except for not testable disagreements about what is on the other side. The interpretation of the no-hair theorem is that the Universe (observable and unobservable) expands by an enormous factor during inflation.

  8. Measure problem (cosmology) - Wikipedia

    en.wikipedia.org/wiki/Measure_problem_(cosmology)

    For such an observer, Bayes' theorem may appear to break down over this timescale due to anthropic selection effects; this hypothetical breakdown is sometimes called the "Guth–Vanchurin paradox". One proposed resolution to the paradox is to posit a physical "end of time" that has a fifty percent chance of occurring in the next few billion years.

  9. Timeline of gravitational physics and relativity - Wikipedia

    en.wikipedia.org/wiki/Timeline_of_gravitational...

    2003 – Arvind Borde, Alan Guth, and Alexander Vilenkin prove the Borde–Guth–Vilenkin theorem. [233] [234] 2002 – First data collection of the Laser Interferometer Gravitational-Wave Observatory (LIGO). 2002 – James Williams, Slava Turyshev, and Dale Boggs conduct stringent lunar test of violations of the principle of equivalence. [235]