Solid matter with zero shear modulus in flat Universe
DOI10.1088/1361-6382/ac11aazbMath1482.83139arXiv2102.06051OpenAlexW3179174902MaRDI QIDQ5162925
Publication date: 8 November 2021
Published in: Classical and Quantum Gravity (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/2102.06051
Relativistic cosmology (83F05) Shear flows and turbulence (76F10) Gravitational energy and conservation laws; groups of motions (83C40) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Asymptotic procedures (radiation, news functions, (mathcal{H} )-spaces, etc.) in general relativity and gravitational theory (83C30) Dark matter and dark energy (83C56)
Cites Work
- Unnamed Item
- Unnamed Item
- Gauge-invariant second-order perturbations and non-Gaussianity from inflation
- ``CMB-slow or how to determine cosmological parameters by hand?
- Advanced General Relativity
- Perturbations of spacetime: gauge transformations and gauge invariance at second order and beyond
- Elastic stars in general relativity: I. Foundations and equilibrium models
- Bubble nucleation and inflationary perturbations
- Zoology of graviton non-Gaussianities
- Large scale anomalies in the CMB and non-Gaussianity in bouncing cosmologies
- The effect of a radiation-like solid on CMB anisotropies
- The cosmological constant problem
- Foundations of general relativistic high-pressure elasticity theory
This page was built for publication: Solid matter with zero shear modulus in flat Universe
