Confusing dark matter particle properties with modifications to General Relativity
arXiv:1912.09222 · doi:10.1103/PhysRevD.102.104010
Abstract
Cold Dark Stars made of self-gravitating fermions in the degenerate limit are constructed in General Relativity and in R-square gravity, . The properties of the resulting Cold Dark Stars in both theories of gravity are studied. It is found that the same gravitational potential is generated for different election of the parameters of the model, such as the mass of the fermion, the self-interacting strength or the value of , thus, a possible confusion in the determination of the dark matter properties and the favored theory of gravity might arise.
arXiv commentAccepted for publication in Physical Review D
References in corpus (45)
- Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant
- Nine-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Parameter Results
- Detection of the Baryon Acoustic Peak in the Large-Scale Correlation Function of SDSS Luminous Red Galaxies
- Extended Theories of Gravity
- The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological analysis of the DR12 galaxy sample
- The Complete Light-curve Sample of Spectroscopically Confirmed Type Ia Supernovae from Pan-STARRS1 and Cosmological Constraints from The Combined Pantheon Sample
- Observational evidence for self-interacting cold dark matter
- The 2dF Galaxy Redshift Survey: Power-spectrum analysis of the final dataset and cosmological implications
- Large Magellanic Cloud Cepheid Standards Provide a 1% Foundation for the Determination of the Hubble Constant and Stronger Evidence for Physics Beyond LambdaCDM
- Models of f(R) Cosmic Acceleration that Evade Solar-System Tests
- Planck 2018 results. I. Overview and the cosmological legacy of Planck
- Disappearing cosmological constant in f(R) gravity
- H0LiCOW XIII. A 2.4% measurement of from lensed quasars: tension between early and late-Universe probes
- The Carnegie-Chicago Hubble Program. VIII. An Independent Determination of the Hubble Constant Based on the Tip of the Red Giant Branch
- Gravitational Vacuum Condensate Stars
- Implications of the Neutron Star Merger GW170817 for Cosmological Scalar-Tensor Theories
- Tests of General Relativity with GW170817
- The non-gravitational interactions of dark matter in colliding galaxy clusters
- Constraints on Perturbative f(R) Gravity via Neutron Stars
- Exponential Gravity
- Dark Matter from R^2-gravity
- The BAO+BBN take on the Hubble tension
- The realistic models of relativistic stars in f(R) = R + alpha R^2 gravity
- Compact stars made of fermionic dark matter
- Gravitational Wave Signatures of Highly Compact Boson Star Binaries
- A supermassive boson star at the galactic center?
- Strange quark stars within the Nambu-Jona-Lasinio model
- Self-gravitating system made of axions
- Gravitational-Wave Signature of an Inspiral into a Supermassive Horizonless Object
- On the 1/c Expansion of f(R) Gravity
- Fermionic warm dark matter produces galaxy cores in the observed scales because of quantum mechanics
- Is exponential gravity a viable description for the whole cosmological history?
- Dark Matter Densities during the Formation of the First Stars and in Dark Stars
- Small-scale clumps of dark matter
- Spherical Boson Stars as Black Hole mimickers
- Constraining scalar fields with stellar kinematics and collisional dark matter
- Dark Stars: A Review
- Gravitational Waves from Dark Boson Star binary mergers
- Axion Stars in the Infrared Limit
- Dwarf spheroidal galaxies as degenerate gas of free fermions
- Quantum WDM fermions and gravitation determine the observed galaxy structures
- Cores in Dwarf Galaxies from Fermi Repulsion
- New mass bound on fermionic dark matter from a combined analysis of classical dSphs
- Constraining ultra light fermionic dark matter with Milky-Way observations
- Constraining light fermionic dark matter with binary pulsars