Can the hidden mass be negative?
Description
A consequence of modified nonrelativistic dynamics (MOND) which is incompatible with the hidden mass hypothesis (HMH) is discussed. If MOND is basically correct, there are mass configurations which, when probed dynamically using Newtonian dynamics will appear to contain negative hidden mass, so that the deduced mass density in such systems is, in some regions of space, smaller than the actual density. Generalities concerning the possible appearance of negative hidden mass are discussed, and a general procedure for determining gravitational masses and the conditions for the generation of negative phantom masses is described. Actual configurations where negative phantom mass is expected by MOND are presented, and prospects for detecting such negative densities are discussed. 16 references
Additional details
Additional titles
- Augmented title (English)
- In galactic clusters
Publishing Information
- Journal Title
- Astrophys. J.
- Journal Volume
- 306
- Series
- Astrophys. J.
- Journal Page Range
- 9-15
- ISSN
- 0004-637X
- CODEN
- ASJOA
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 18016757
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- COSMOLOGY; GALAXY CLUSTERS; MASS; MASS DISTRIBUTION; MECHANICS; MORPHOLOGICAL CHANGES; NEGATIVE MASS
- Descriptors DEC
- DISTRIBUTION; HYPOTHESIS; SPATIAL DISTRIBUTION