Asymptotically safe cosmology with non-canonical scalar field
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Publication:6561095
DOI10.1088/1361-6382/AD4AE3zbMATH Open1545.83033MaRDI QIDQ6561095
Publication date: 24 June 2024
Published in: Classical and Quantum Gravity (Search for Journal in Brave)
Relativistic cosmology (83F05) Quantization of the gravitational field (83C45) Dark matter and dark energy (83C56)
Cites Work
- Title not available (Why is that?)
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- \(f(R)\) theories
- The asymptotic safety scenario in quantum gravity
- Dark energy cosmology: the equivalent description via different theoretical models and cosmography tests
- A new type of isotropic cosmological models without singularity
- Fixed points of quantum gravity
- Inflation
- <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mi>f</mml:mi><mml:mrow><mml:mo>(</mml:mo><mml:mi>R</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:mrow></mml:math>theories of gravity
- Inflationary solutions in asymptotically safe f ( R ) theories
- Renormalization Group and Critical Phenomena. I. Renormalization Group and the Kadanoff Scaling Picture
- DYNAMICS OF DARK ENERGY
- Renormalization group flow in scalar-tensor theories: I
- Renormalization group flow in scalar-tensor theories: II
- Cosmology of Bianchi type-I metric using renormalization group approach for quantum gravity
- FIELD THEORY OF TACHYON MATTER
- Cosmological Imprint of an Energy Component with General Equation of State
- Exact renormalization group with optimal scale and its application to cosmology
- Cosmologies with a general non-canonical scalar field
- \(k\)-inflation
- Perturbations in \(k\)-inflation
- An alternative to quintessence
- Cosmology with self-adjusting vacuum energy density from a renormalization group fixed point
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