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Problematic appearance of quantities beyond the Planck scale
In black hole physics and inflationary cosmology, the trans-Planckian problem is the problem of the appearance of quantities beyond the Planck scale, which
Trans-Planckian_problem
Hypothetical astrophysical effect
radiation in which the trans-Planckian problem is addressed.[citation needed] The key point is that similar trans-Planckian problems occur when the modes
Hawking_radiation
Theory of rapid universe expansion
entropic considerations. Another problem that has occasionally been mentioned is the trans-Planckian problem or trans-Planckian effects. Since the energy scale
Cosmic_inflation
temperature Planck epoch Planck postulate Planck scale Planck star Trans-Planckian problem 1069 Planckia, asteroid Max Planck Society Planck's principle Planck
List of things named after Max Planck
List_of_things_named_after_Max_Planck
Units defined only by physical constants
2πABH. cGh physics Dimensional analysis Doubly special relativity Trans-Planckian problem Zero-point energy For example, both Frank Wilczek and Barton Zwiebach
Planck_units
Scientific theory
[citation needed] Black hole information paradox Quantum gravity Trans-Planckian problem Positive energy theorem Kallosh, Renata; Linde, Andrei; Ortín,
Extremal_black_hole
Hall Trailing edge Train noise Trajectory Trajectory optimization Trans-Planckian problem Transactional interpretation Transduction (biophysics) Transfer-matrix
Index_of_physics_articles_(T)
Hypothetical black hole formed soon after the Big Bang
Carneiro, S.; de Holanda, P. C.; Saa, A. (2021). "Neutrino primordial Planckian black holes". Physics Letters. B822 136670. Bibcode:2021PhLB..82236670C
Primordial_black_hole
Argentinian & French physicist and astronomer
doi:10.1103/PhysRevD.16.937. Sanchez, Norma G. (20 June 2023). "Quantum trans-Planckian physics inside black holes and its spectrum". Physical Review D. 107
Norma_Sanchez
Fluctuations in the energy spectrum of the microwave background
Bremsstrahlung. This allows the photon field to quickly relax back to a Planckian distribution, even if for a very short phase a spectral distortion appears
Cosmic microwave background spectral distortions
Cosmic_microwave_background_spectral_distortions
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