Published December 1988
| Version v1
Journal article
Inhomogeneous cosmology with spinning fluid
Description
The energy-momentum tensor of a spinning fluid written in a form structurally similar to that of an imperfect fluid is used to investigate the evolution of an inhomogeneous and anisotropic cosmological model. It is observed that the model evolves into the Friedmann model due to the effect of spin
Additional details
Publishing Information
- Journal Title
- Nuovo Cimento, B
- Journal Volume
- 102
- Journal Issue
- 6
- Series
- Nuovo Cim., B.
- Journal Page Range
- 573-581
- ISSN
- 0369-3554
- CODEN
- NCIBA
INIS
- Country of Publication
- Italy
- Country of Input or Organization
- Italy
- INIS RN
- 21004575
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- COSMOLOGICAL MODELS; COSMOLOGY; ENERGY-MOMENTUM TENSOR; FLUIDS; SPIN
- Descriptors DEC
- ANGULAR MOMENTUM; MATHEMATICAL MODELS; PARTICLE PROPERTIES; TENSORS