An Extended Structure Model for Massive Galactic Cores

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An Extended Structure Model for Massive Galactic Cores T. Wilcox, UCLA Miami 2011

An Extended Structure Model for Massive Galactic Cores T. Wilcox, UCLA Miami 2011

Overview • Introduction • The Model • Computational Strategy • Results • Discussion •

Overview • Introduction • The Model • Computational Strategy • Results • Discussion • Summary • Conclusions

Introduction • Measurements of the size of the central radio source Sgr. A* and

Introduction • Measurements of the size of the central radio source Sgr. A* and motions of orbiting stars have been considered compelling evidence for the existence of a black hole of some 4. 4 million solar masses at the center of our galaxy. • An alternative that meets observational constraints is the possible existence of a gravitationally bound distribution of dark matter in the form of a fermion gas • The general relativistic model presented here includes an equation of state that predicts a fermion mass of 150 kev.

The Model The equations for the dark matter model are written as follows: ;

The Model The equations for the dark matter model are written as follows: ;

The Model (cont’d) Potential: Pressure: Density :

The Model (cont’d) Potential: Pressure: Density :

The Model (cont’d) The quantities appearing in the above equations are related to the

The Model (cont’d) The quantities appearing in the above equations are related to the standard metric of general relativity as follows: Boundary Conditions: ; ;

Computational Strategy Initially Set: • K(0), m(0) Metric functions at r=0 • Mass of

Computational Strategy Initially Set: • K(0), m(0) Metric functions at r=0 • Mass of dark fermion • Parameter (Required for correct boundary condition at large r) • Integrate outward from zero

Einstein Metric Functions 1. 20 E+00 1. 00 E+00 8. 00 E-01 6. 00

Einstein Metric Functions 1. 20 E+00 1. 00 E+00 8. 00 E-01 6. 00 E-01 H K 4. 00 E-01 2. 00 E-01 0. 00 E+00 1. 00 E+03 1. 00 E+06 1. 00 E+09 1. 00 E+12 1. 00 E+15 1. 00 E+18 1. 00 E+21 1. 00 E+24 Distance from Center (cm)

Density 3. 50 E+00 grams/cm^3 3. 00 E+00 2. 50 E+00 2. 00 E+00

Density 3. 50 E+00 grams/cm^3 3. 00 E+00 2. 50 E+00 2. 00 E+00 1. 50 E+00 1. 00 E+00 5. 00 E-01 0. 00 E+00 1. 00 E+03 1. 00 E+06 1. 00 E+09 1. 00 E+12 1. 00 E+15 1. 00 E+18 1. 00 E+21 1. 00 E+24 Distance from Center (cm)

grams Mass Function 1. 00 E+44 1. 00 E+40 1. 00 E+36 1. 00

grams Mass Function 1. 00 E+44 1. 00 E+40 1. 00 E+36 1. 00 E+32 1. 00 E+28 1. 00 E+24 1. 00 E+20 1. 00 E+16 1. 00 E+12 1. 00 E+08 1. 00 E+04 1. 00 E+00 1. 00 E+03 1. 00 E+06 1. 00 E+09 1. 00 E+12 1. 00 E+15 1. 00 E+18 1. 00 E+21 1. 00 E+24 Distance from Center (cm)

Stellar Velocity 1. 00 E+11 1. 00 E+10 cm/sec 1. 00 E+09 1. 00

Stellar Velocity 1. 00 E+11 1. 00 E+10 cm/sec 1. 00 E+09 1. 00 E+08 1. 00 E+07 1. 00 E+06 1. 00 E+05 1. 00 E+08 1. 00 E+10 1. 00 E+12 1. 00 E+14 1. 00 E+16 1. 00 E+18 1. 00 E+20 1. 00 E+22 1. 00 E+24 Distance from Center (cm)

Test Particle Geodesic Trajectories Breakup occurs if = 3 x 10^-7 (sun) =3 (white

Test Particle Geodesic Trajectories Breakup occurs if = 3 x 10^-7 (sun) =3 (white dwarf) = 3 x 10^5 (neutron star)

Tidal Forces cm Radial Position 1. 00 E+16 1. 00 E+15 1. 00 E+14

Tidal Forces cm Radial Position 1. 00 E+16 1. 00 E+15 1. 00 E+14 1. 00 E+13 1. 00 E+12 1. 00 E+11 0. 00 E+00 2. 00 E+07 4. 00 E+07 6. 00 E+07 Time (sec) 8. 00 E+07 1. 00 E+08

Discussion • Model Fits Data for most compact source candidate (1. 3 mm microwave;

Discussion • Model Fits Data for most compact source candidate (1. 3 mm microwave; site is colocated with Sgr. A*) • Core mass of 4. 4 x 10^6 solar masses • Distribution of matter is mechanically stable • Degenerate Fermi gas • Beyond the edge of degenerate region density falls abruptly (depends weakly on temperature) • Total mass (within volume of radius “r”) plateaus beyond radius of about 1. 4 AU out to about 1 kpc • Forms “atmosphere” mixed with visible matter • Drops off beyond 30 kpc (outer limit of ordinary matter) • If temperature sufficiently high total mass of dark matter increases without bound

Summary and Conclusions • Measured properties (mass and apparent size) of the stellar object

Summary and Conclusions • Measured properties (mass and apparent size) of the stellar object at the galactic center (Sgr. A*) can be fitted to a gravitationally bound fermi gas model that describes principle features of the massive core. • Stellar velocity curves fit observed forms in both the inner (100 -1000 AU) and outer (1 -30 kpc) galactic regions. • The two parameters of the model that generate the fit are the mass of the fermion and the density of dark matter at r=0. • The density of dark matter is virtually independent of temperature, provided the value does not exceed approximately degrees. • The model predicts the mass of the dark matter particle to be approximately. 2 electron masses.

The Debate: Modified Gravity or Dark Matter? • Is dark matter simply a fudge

The Debate: Modified Gravity or Dark Matter? • Is dark matter simply a fudge to “correct” the Newtonian law of gravity? - Co-evolution with normal matter; are they separable? * Must the distribution must be set in each instance? - Dissipative processes, what are they? * Can a concentration of dark matter “collapse” without them? * Gravitational scattering by large masses * If all else fails—dissipation via massless dark “photons” • Modified gravity: is it a truly “universal” i. e. , one (or perhaps a few) parameters to be set once and for all? -Gravitational lensing -Colliding galaxies