Search results for "Planck length"

showing 5 items of 5 documents

The role of the Planck scale in black hole radiance

2008

Lorentz invariance plays a pivotal role in the derivation of the Hawking effect, which crucially requires an integration in arbitrarily small distances or, equivalently, in unbounded energies. New physics at the Planck scale could, therefore, potentially modify the emission spectrum. We argue, however, that the kinematic invariance can be deformed in such a way that the thermal spectrum remains insensitive to trans-Planckian physics.

PhysicsPlanck energyPlanck particlePlanck massAstronomy and Astrophysicssymbols.namesakeMicro black holePlanck forceSpace and Planetary ScienceQuantum mechanicssymbolsVirtual black holeMathematical PhysicsHawking radiationPlanck length
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New constraints on coupled dark energy from the Planck satellite experiment

2013

We present new constraints on coupled dark energy from the recent measurements of the cosmic microwave background anisotropies from the Planck satellite mission. We found that a coupled dark energy model is fully compatible with the Planck measurements, deriving a weak bound on the dark matter-dark energy coupling parameter xi = -0.49(-0.31)(+0.19) at 68% C.L. Moreover if Planck data are fitted to a coupled dark energy scenario, the constraint on the Hubble constant is relaxed to H-0 = 72.1(-2.3)(+3.2) km/s/Mpc, solving the tension with the Hubble Space Telescope (HST) value. We show that a combined PLANCK + HST analysis provides significant evidence for coupled dark energy finding a nonzer…

PhysicsNuclear and High Energy PhysicsPlanck energyCosmologiaPlanck particlePlanck massHubble ConstantPlanck momentumPlanck temperatureAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysicssymbols.namesakePlanck timePlanck forcesymbolsAstronomiaBaryon acoustic-oscillationsphysicsAstrophysics::Galaxy AstrophysicsPlanck length
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Cosmology of the Planck Era from a Renormalization Group for Quantum Gravity

2001

Homogeneous and isotropic cosmologies of the Planck era before the classical Einstein equations become valid are studied taking quantum gravitational effects into account. The cosmological evolution equations are renormalization group improved by including the scale dependence of Newton's constant and of the cosmological constant as it is given by the flow equation of the effective average action for gravity. It is argued that the Planck regime can be treated reliably in this framework because gravity is found to become asymptotically free at short distances. The epoch immediately after the initial singularity of the Universe is described by an attractor solution of the improved equations w…

PhysicsInflation (cosmology)High Energy Physics - TheoryNuclear and High Energy PhysicsAstrophysics (astro-ph)FOS: Physical sciencesHierarchy problemGeneral Relativity and Quantum Cosmology (gr-qc)Cosmological constantAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsGeneral Relativity and Quantum CosmologyGeneral Relativity and Quantum CosmologyClassical mechanicsHigh Energy Physics - Theory (hep-th)Planck timeQuantum cosmologyFlatness problemMathematical physicsPlanck lengthLoop quantum cosmology
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The 2 + 1 Kepler problem and its quantization

2001

We study a system of two pointlike particles coupled to three dimensional Einstein gravity. The reduced phase space can be considered as a deformed version of the phase space of two special-relativistic point particles in the centre of mass frame. When the system is quantized, we find some possibly general effects of quantum gravity, such as a minimal distances and a foaminess of the spacetime at the order of the Planck length. We also obtain a quantization of geometry, which restricts the possible asymptotic geometries of the universe.

PhysicsPhysics and Astronomy (miscellaneous)SpacetimeFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)General Relativity and Quantum CosmologyGeneral Relativity and Quantum Cosmologysymbols.namesakeQuantization (physics)Classical mechanicsPhase spaceKepler problemsymbolsQuantum gravityPoint (geometry)EinsteinPlanck lengthClassical and Quantum Gravity
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Two-point functions with an invariant Planck scale and thermal effects

2008

Nonlinear deformations of relativistic symmetries at the Planck scale are usually addressed in terms of modified dispersion relations. We explore here an alternative route by directly deforming the two-point functions of an underlying field theory. The proposed deformations depend on a length parameter (Planck length) and preserve the basic symmetries of the corresponding theory. We also study the physical consequences implied by these modifications at the Planck scale by analyzing the response function of an accelerated detector in Minkowski space, an inertial one in de Sitter space, and also in a black hole spacetime.

PhysicsHigh Energy Physics - TheoryNuclear and High Energy PhysicsPlanck energy010308 nuclear & particles physicsDe Sitter spacePlanck massPlanck momentumFOS: Physical sciences01 natural sciencessymbols.namesakeGeneral Relativity and Quantum CosmologyClassical mechanicsPlanck forceHigh Energy Physics - Theory (hep-th)Relativitat general (Física)0103 physical sciencessymbolsEspai i temps010306 general physicsPlanck unitsVirtual black holePlanck length
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