The MOND Fundamental Plane
arXiv:1011.5741 · doi:10.1111/j.1365-2966.2010.18081.x
Abstract
Modified Newtonian Dynamics (MOND) has been shown to be able to fit spiral galaxy rotation curves as well as giving a theoretical foundation for empirically determined scaling relations, such as the Tully - Fisher law, without the need for a dark matter halo. As a complementary analysis, one should investigate whether MOND can also reproduce the dynamics of early - type galaxies (ETGs) without dark matter. As a first step, we here show that MOND can indeed fit the observed central velocity dispersion of a large sample of ETGs assuming a simple MOND interpolating functions and constant anisotropy. We also show that, under some assumptions on the luminosity dependence of the Sersic n parameter and the stellar M/L ratio, MOND predicts a fundamental plane for ETGs : a log - linear relation among the effective radius , and the mean effective intensity . However, we predict a tilt between the observed and the MOND fundamental planes.
16 pages, 2 figures, 2 tables, accepted for publication on MNRAS
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- Testing Yukawa-like potentials from f(R)-gravity in elliptical galaxies
- Systematic variations of central mass density slopes in early-type galaxies
- SPIDER - VI. The Central Dark Matter Content of Luminous Early-Type Galaxies: Benchmark Correlations with Mass, Structural Parameters and Environment
- The Faber-Jackson relation and Fundamental Plane from halo abundance matching
- Observational constraints on Yukawa cosmology and connection with black hole shadows
- Remarks on the properties of elliptical galaxies in modified Newtonian dynamics
- MOND and IMF variations in early-type galaxies from
- Probing the dark matter issue in f(R)-gravity via gravitational lensing
- Dark matter signatures of black holes with Yukawa potential
- Testing Verlinde's emergent gravity in early-type galaxies
- Dark Universe Phenomenology from Yukawa Potential?
- Unraveling the interplay between SIDM and baryons in MW halos: defining where baryons dictate heat transfer
- Elliptical galaxies kinematics within general relativity with renormalization group effects
- Charged Black Holes with Yukawa Potential
- An updated analysis of two classes of f(R) theories of gravity
- Testing the tensor-vector-scalar Theory with the latest cosmological observations
- Origin of the fundamental plane of elliptical galaxies in the Coma Cluster without fine-tuning
- Apparent Dark Matter Inspired by Einstein Equation of State
- Dark matter and alternative recipes for the missing mass
- The Virial Relation and Intrinsic Shape of Early-Type Galaxies
- Towards a new generalized space expansion dynamics applied to the rotation of galaxies and Tully Fisher law
- Pattern dark matter and galaxy scaling relations
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- Milgrom's Law and Lambda's Shadow: How Massive Gravity Connects Galactic and Cosmic Dynamics