Results 61 to 70 of about 38,508 (240)

Phenomenology of loop quantum cosmology [PDF]

open access: yesJournal of Physics: Conference Series, 2010
After introducing the basic ingredients of Loop Quantum Cosmology, I will briefly discuss some of its phenomenological aspects. Those can give some useful insight about the full Loop Quantum Gravity theory and provide an answer to some long-standing questions in early universe cosmology.
openaire   +2 more sources

“Lock and Key”: Binding Behavior of Malachite Green and Functional Nucleic Acids and Their Multidimensional Applications

open access: yesSmall Structures, EarlyView.
The review comprehensively summarizes the binding behaviors and multidimensional applications of malachite green with diverse functional nucleic acids. By integrating structural mechanisms, comparative analysis, and application strategies across eight domains, it provides theoretical guidance and future perspectives for developing intelligent nucleic ...
Keren Chen   +4 more
wiley   +1 more source

Inflation and Loop Quantum Cosmology [PDF]

open access: yesProceedings of 35th International Conference of High Energy Physics — PoS(ICHEP 2010), 2011
5 pages, Proceedings of the 35th International Conference on High Energy Physics, Paris, 2010 (ICHEP 2010)
openaire   +3 more sources

Spaceborne and spaceborn: Physiological aspects of pregnancy and birth during interplanetary flight

open access: yesExperimental Physiology, EarlyView.
Abstract Crewed interplanetary return missions that are on the planning horizon will take years, more than enough time for initiation and completion of a pregnancy. Pregnancy is viewed as a sequence of processes – fertilization, blastocyst formation, implantation, gastrulation, placentation, organogenesis, gross morphogenesis, birth and neonatal ...
Arun V. Holden
wiley   +1 more source

Tachyonic inflation in loop quantum cosmology

open access: yesEuropean Physical Journal C: Particles and Fields, 2019
A tachyon field might be responsible for cosmological inflation at an early time and contribute to cosmological dark matter at a later time. We investigate tachyonic inflation by analyzing a tachyon field with different potentials in the framework of ...
Kui Xiao
doaj   +1 more source

Universal features of quantum bounce in loop quantum cosmology

open access: yesPhysics Letters B, 2017
In this Letter, we study analytically the evolutions of the flat Friedmann–Lemaitre–Robertson–Walker (FLRW) universe and its linear perturbations in the framework of the dressed metric approach in loop quantum cosmology (LQC). Assuming that the evolution
Tao Zhu   +4 more
doaj   +1 more source

Thermodynamics in new model of loop quantum cosmology

open access: yesEuropean Physical Journal C: Particles and Fields, 2021
The thermodynamic properties of loop quantum cosmology (LQC) without considering the Lorentz term were established in Li and Zhu (Adv High Energy Phys 2009:905705, 2009).
Xiangdong Zhang
doaj   +1 more source

Observational Exclusion of a Consistent Quantum Cosmology Scenario

open access: yes, 2015
It is often argued that inflation erases all the information about what took place before it started. Quantum gravity, relevant in the Planck era, seems therefore mostly impossible to probe with cosmological observations.
Barrau, Aurelien   +3 more
core   +3 more sources

Loop Quantum Cosmology: A cosmological theory with a view [PDF]

open access: yesJournal of Physics: Conference Series, 2011
Loop Quantum Gravity is a background independent, nonperturbative approach to the quantization of General Relativity. Its application to models of interest in cosmology and astrophysics, known as Loop Quantum Cosmology, has led to new and exciting views of the gravitational phenomena that took place in the early universe, or that occur in spacetime ...
openaire   +4 more sources

Positive cosmological constant in loop quantum cosmology [PDF]

open access: yesPhysical Review D, 2012
The k=0 Friedmann Lemaitre Robertson Walker model with a positive cosmological constant and a massless scalar field is analyzed in detail. If one uses the scalar field as relational time, new features arise already in the Hamiltonian framework of classical general relativity: In a finite interval of relational time, the universe expands out to infinite
Abhay Ashtekar   +3 more
openaire   +3 more sources

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