MOdified Newtonian DynamicsMOdified Newtonian Dynamicsan introductory reviewan introductory review
Riccardo ScarpaRiccardo Scarpa
IACIAC
By
Justification for ModifyingJustification for Modifying Newtonian Dynamics Newtonian Dynamics
Increasing fine tuning required to explain observations Increasing fine tuning required to explain observations with non-baryonic dark matter.with non-baryonic dark matter.
Effects of non-baryonic dark matter appears Effects of non-baryonic dark matter appears when and when and only whenonly when the acceleration of gravity falls below a the acceleration of gravity falls below a certain value, baptized acertain value, baptized a00..
This acceleration, aThis acceleration, a00, is orders of magnitudes smaller , is orders of magnitudes smaller then the smallest probed in the solar system.then the smallest probed in the solar system.
Thus the idea is simple: Newtonian dynamics breaks down below a0
Proposed by M. Milgrom in 1983Proposed by M. Milgrom in 1983AA new constant of physics new constant of physics introduced: aintroduced: a
00~10~1088 cm s cm s22
Functional form derived fromrotation curves, where we know v = constant ⇒ a ∝1/r at large radii.Square root of Newtonian acceleration ∝ 1/r. Multiplied by an acceleration we get right dimensions.
An interpolation function derived empirically joins the two regimes
⇒
a≫a0a=GMr²
a≪a0 a=GMa0
r
f aa0=1
a0
a 2
a N=a f aa0
High Surface Brightness galaxies have in general flat rotation curves: Acceleration proportional to 1/r.Acceleration proportional to 1/r.
NGC 6503 – from Begeman, Broeils, and Sanders 1991
Comparing MOND to real dataComparing MOND to real data
DM
STARS
GAS MOND
Galaxies Rotation Curves with MONDGalaxies Rotation Curves with MOND
Velocity in km/sDistance in kpc
Sanders & Verheijen 1998. Rotation curves derived from stellar light and 21cm hydrogen line
a =GMa0
r
Fits to v(r) for LSB & HSB GalaxiesFits to v(r) for LSB & HSB GalaxiesSanders & McGaugh 02a0=1.2 x108 cm s2
Does MOND fit any rotation curve?
MOND DARK MATTER
This is a fake galaxy!Photometry from one object and velocity from another!
In this case, a failure is a good thing!
MOND fails to fit this one.
Counterexamples?!Counterexamples?!
Romanowsky et al 2003Claimed 3 elliptical galaxieswithout dark matter halo were discovered.
Dashed line: isothermal halo
Dotted line: constant masstolight ratio galaxy.
No! No! These galaxies are in Newtonian These galaxies are in Newtonian regimeregime
Milgrom & Sanders 03
Dotted line: Newtonian prediction for constant M/L. Solid line: MOND prediction for the same M/L.
The TullyFisher The TullyFisher RelationRelation
v ⇐
A relation between asymptotic velocity and luminosity of galaxies
L∝v4
Galaxies’ mean surface Galaxies’ mean surface brightnessbrightness s s = L/ = L/ππrr22
High surface Brightness Low surface brightness
Pega
sus
Newtonian dynamics and TFNewtonian dynamics and TF
The TF requires
τ2S= const.
M/L=τ depends on stellar population, basically the same in all galaxies
Surface brightness S varies significantly going from HSB to LSB galaxies and has nothing to do with M/L.
Link between two otherwise unrelated quantities implied.
v2=
GMr
L=S r2v4∝
M 2
LS= M2
L2 SL
TullyFisher relation and MONDTullyFisher relation and MOND
MOND requires M/L= constant
AND
The TF is universal
v2
r=GMa0
r v4
∝ML
L
The TullyFisher is universal as The TullyFisher is universal as MOND predictedMOND predicted
Sanders & Verheijen
LSB
HSB
Note that data for low surface brightness galaxies became available some 10 years after Milgrom made its prediction.
Baryonic TullyFisher McGaugh et al. 2000 ApJL, 533, 99
Left: “Luminous mass” vs. rotational Velocity. Galaxies with v<90 km/s fall below the relation.
Right: Including gas the relation is restored.
The solid line has slope 4
The TF is a relation between MASS and Velocity, as indeed predicted by MOND
Fundamental plane of Fundamental plane of ellipticals ellipticals
Edge on view of the fundamental planeHSB define a a relation M/L ∝ L 0.25
LSB define an opposite trend M/L ∝ L 0.40
LSBHSB
k1=log(2re)/√2∝ log(M)
MOND explanation of the tiltMOND explanation of the tiltTilt due to different trends of the strength of the gravitational field:
In HSB the acceleration decreases with size
In LSB the acceleration increases with size
This is demonstrated by their average surface brightness
MOND defines specific trendsMOND defines specific trends
The slopes predicted by MOND for LSB and HSB do agree with the known trends,0.4 and 0.25, respectively
Newtonian acceleration from velocity Newtonian acceleration from velocity and luminosityand luminosity
MOND agrees with real data over 6 orders of magnitude!
MOND prediction
Dense Clusters of GalaxiesDense Clusters of Galaxies(Sanders 1998)
This may be the only place where MOND fails (by a factor 2). MOND predicts some baryonic matter still to be discovered
Ultra Compact Dwarf Ultra Compact Dwarf GalaxiesGalaxies
Dwarf galaxies are usually FULL of dark matter with M/L~100, thus plenty of dark matter expected.
Drinkwater et al. 2000
DARK MATTER vs. MONDUCD luminosity and size imply internal acceleration > a0 everywhere, hence no dark matter should be found.
No Dark Matter in UCDsNo Dark Matter in UCDs
Accepted explanation: The dark matter was there but was lost together with the halo. Possible but NOT predicted and ad hoc
MOND explanation: simple, elegant, fully logic and exactly as predicted!
2<M/L<4(Drinkwater et al. 2003)
(Scarpa astroph 0504051)
2.1×108 cm s2
MOND and Globular clusters:MOND and Globular clusters:velocity dispersion constant at large radii.velocity dispersion constant at large radii.
Our UVES data (black diamonds) for 75 stars
Radial velocities from Meylan et al. 1995 and Meylan & Mayor 1986 (crosses)
Proper motion data from van Leeuwen et al. 2000
Scarpa, Marconi, & Gilmozzi 2003
All GCs behave the same wayAll GCs behave the same way
MOND or
Tidal Heating?
CarinaCarina
Wilkinson et al. 2006
LSB spheroidal galaxies have flat LSB spheroidal galaxies have flat velocity dispersion profilesvelocity dispersion profiles
Low surface brightness globular clustersLow surface brightness globular clustersNGC 288NGC 288
Internal acceleration below a0 everywhere. This is the equivalent of a LSB galaxy.
What should we expect?
NGC 288 behaves like a LSB galaxyNGC 288 behaves like a LSB galaxy
The velocity dispersion profile is flat!
Cosmological Difficulties with Modified Newtonian Dynamics (or: La Fin du MOND?) Astroph 0104435
In this paper it is argued that MOND had to be wrong because it failed to describe some fetures of modern cosmology.
Cosmology and MONDCosmology and MOND
Wrong approach: a law of physics DOESN'T have to agree with cosmology!!
It is cosmology that HAS TO AGREE with law of physics!!
MOND and WMAPMOND and WMAP
Dark matter NO dark matter
McGaugh 2004, ApJ 611, 26
Big Bang nuclesyntesisBig Bang nuclesyntesis
Values implied by WMAP fits systematically above prediction
McGaugh 2004, ApJ 611, 26
Virtually all theoretical predictions below 0.02
NoCDM models agree with BBN
Gravitational lensingGravitational lensing
Difficult to address because MOND lack(ed) a relativistic extension
The Usual assumption is that light is bent twice has much as predicted by Newton’s law. That is:
Compute field with MOND Double the effect⇒
Warning: Gravitational lensing NEVER occur in MOND regime.
We are left with We are left with MicrolensingMicrolensing
Mortlock & Turner 2001
AM =2p
c 2 GMa0
AM= 2” for M=1012 Msun
For a point sourcewe get an asymptoticdeviation:
The deflection is independent from the impact parameter as much as rotation velocity is independent from r.
Real data agree with MONDReal data agree with MOND
MOND is gaining consensusMOND is gaining consensus
The seminal paper by Milgrom in 1983 cited 450 times.
Conclusions for MONDConclusions for MOND Amazing ability to describe many properties of astronomical Amazing ability to describe many properties of astronomical
objects.objects.
Explains data taken after it was proposed. Agreement Explains data taken after it was proposed. Agreement generally improve as data quality improve.generally improve as data quality improve.
Keep focus on demonstrating whether Newtonian dynamics Keep focus on demonstrating whether Newtonian dynamics fails at low accelerations.fails at low accelerations.
At present, I would compare MOND to Borh’s atom, which At present, I would compare MOND to Borh’s atom, which was based on un-justified assumptions and worked only for was based on un-justified assumptions and worked only for Hydrogen. This model eventually became the basis for Hydrogen. This model eventually became the basis for quantum mechanics.quantum mechanics.
Similarly, MOND might be the way to the next great step in Similarly, MOND might be the way to the next great step in physics.physics.