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09 (2012) 026 and 04 (2013) 010
astro-ph/1205.2384 and 1211.4045
Maxim Eingorn
Gravitational potentials anddynamics of galaxies againstthe cosmological background
North Carolina Central UniversityCREST and NASA Research Centers
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Outline
– the Universe deep inside of the cell of uniformity
– inhomogeneously distributed discrete structures(galaxies and their groups / clusters)
– hyperbolic, flat and spherical spaces
– gravitational potentials
– motion of test bodies (for example, dwarf galaxies)
– gravitational attraction vs. cosmological expansion
– the Hubble flow at a few Mpc for our Local Group
– Milky Way and Andromeda destiny
0=K1−=K
1+=K
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gravitational attractioncosmological expansion
(0;0)
Milky Way
Andromeda
An arbitrary dwarf galaxy
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Introduction
less than 150 Mpc
?
inhomogeneous and anisotropic Universe
?
Hubble’s law
more than 150 Mpc
the “ΛCDM” model
homogeneous and isotropic Universe
hydrodynamical / continuous approach
Hubble’s law
[Labini, CQG, 2011]
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Typical values of peculiar velocities~ 200-400 km/sec
The present value of the Hubble parameter~ 70 km/sec/Mpc
Distances at which the Hubble flow velocityis of the same order as peculiar velocities~ 3-6 Mpc
Hence, the Hubble flow can be observed at distances greater than this rough estimate.
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It looks reasonable that EdwinHubble discovered his law in1929 after observing galaxieson scales less than~ 20 Mpc.
However, recent observations indicate thepresence of the Hubble flows at distanceseven less than3 Mpc!
[Sandage, Karachentsev, 1999-2012]
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Theoretical substantiation?
At which distances from gravitating masses does cosmological expansion (the Hubble flow) overcome gravitational attraction?
What is the size of the region of local gravity where attraction prevails over expansion?
At which points does a free falling cosmic body have the zero acceleration?
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Hydrodynamical approach = myopiaL.D. Landau & E.M. Lifshitz “Fluid Mechanics”
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COSMOLOGICAL IDEAL FLUIDS
Any small volume element in thecosmologicalfluidis always supposed so large that it still contains avery great number of moleculesgalaxies.
“physically” infinitely small = very small comparedwith the volume of the body Universe, but largecompared with the distances between the moleculesgalaxies
“a cosmologicalfluid particle” ,“a point in a cosmologicalfluid”
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Hydrodynamics Mechanics
( )2
1/2=
( ) [ ]
i kjik
jj
m c dx dx dsT
g t ds ds cdtδ −
−∑ r r
Energy-momentumtensor components:
Rest mass density:
( )jjj
m rr −∑ δγ
ρ21
1=
Final and irrevocable conclusion
Hydrodynamical / continuous approach isinapplicable at distances less than the cellof uniformity size ~ 150 Mpc.
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The energy-momentum tensor choice
– The energy-momentum tensor of a system ofpoint-like particles is acceptable if the distancesbetween the bodies, modeled by them, are muchgreater than their sizes. This condition is satisfiedvery well in cosmology: cosmic bodies = galaxies.
– Exactly the same energy-momentum tensorchoice in astrophysics underlies the prevalentweak gravitational field approximation and givessure-fire results for the planets in the Solar systemincluding prediction of relativistic effects.
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Mechanical / discrete approach
Background: the “ΛCDM” model(the homogeneous and isotropic Universe)
hyperbolicflatsphericalspaces
0=K
1−=K
1+=K
( )( )
+++
−−2
222
22222
41
1
==
zyxK
dxdxdadxdxdads
βααββα
αβδ
ηγη
openflatclosedUniverses
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( ) Λ++Η 002
2
=3
Ta
K κ
Λ+Η+Η′=
22
2
a
K
The Friedmann equations
ηd
da
aa
a 1=′
=Η
4
8
c
GNπκ =
ikT are the average energy-momentum tensor
components of dust (pressureless matter).
3200 /= acT ρThe average energy density
is the only non-zero mixed component.
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quantity symbol dimension
scale factor a L (length)
rest mass density
in comoving frame
ρ M (mass)
average
rest mass density
in comoving frame
ρ M (mass)
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and are the values of the scale factor and the Hubble parameter at present time
Ω+Ω+Ω−Λ+
Λ 2
20
3
302
02
22
3
422 =
33==
a
a
a
aH
a
Kcc
a
c
a
aH KM
ρκɺ
Ω+Ω−Λ+− Λ3
302
0
2
3
4
2
1=
36=
a
aH
c
a
c
a
aM
ρκɺɺ
0a 0H a
dt
da
aa
aH
1==ɺ
0=t
20
20
2
20
2
30
20
4
=,3
=,3 Ha
Kc
H
c
aH
cKM −ΩΛΩ=Ω Λ
ρκ1=KM Ω+Ω+Ω Λ
Contributionof radiation is
neglected.
H
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11
= ≪cdt
dxa
d
dx αα
η0
00 || TT δδ β ≪
The slightly perturbed “ΛCDM” model(the weakly inhomogeneous and
anisotropic Universe)
The nonrelativistic limitin the comoving frame:
Indeed, the typical present value~ 300 km/secof peculiar velocities is only1/1000(0.1 %) ofthe speed of light.
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00
2
2
1=3)(3 TaK δκΨ+ΗΦ+Ψ′Η−Ψ∆
0=2
1=)( 02
ββ δκ Tax
ΗΦ+Ψ′∂
∂
( )
( )
2
2
; ;
1(2 ) 2 ( )
2
1 1=
2 2
K
a T
αβ
ασ αβσ β
δ
γ κ δ
′′ ′ ′Ψ + Η Ψ + Φ + Η + Η Φ + ∆ Φ − Ψ − Ψ −
− Φ − Ψ −
LaplaceoperatorΨΦ = [Mukhanov, Rubakov]
βααβγη dxdxdads )2(1)2(1 222 Ψ−−Φ+≈
Scalar perturbations
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0=)( ΗΦ+Φ′∂
∂βx )(
)(=),(
2 ηϕη
ac
rrΦ
00
2
2
1=3)(3 TaK δκΦ+ΗΦ+Φ′Η−Φ∆
2 2 20
0 rad rad3 3 3 4
3 3= =
c c cT
a a a a
δρ ρ δρ ρϕδ δε δεΦ+ + + +
)(4=3 ρρπϕϕ −+∆ NGK
( )2 2 2rad rad
1 13 2 =
2 6K a p aκ δ κ δε′′ ′ ′Φ + ΗΦ + Η + Η Φ − Φ =
ρρδρ −= (the difference between real andaverage rest mass densities)
rad 4
3
a
ρϕδε = −
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The nonrelativistic gravitational potential isdefined by the positions of the galaxies, butnot by their velocities!
[Landau]
)(4= ρρπϕ −∆ NG
I. Flat space / Universe 0=K
ρ−The role of the term : the gravitational(Neumann-Seeliger) paradox is absent butspatial distribution of inhomogeneities isnot arbitrary! It is an essential drawback!
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22
222 )(== ΩΣ+ dddxdxdl χχγ βααβ
−+∞∈+∞∈
+∈Σ
1=,)[0,,sinh
0=,)[0,,
1=,][0,,sin
=)(
K
K
K
χχχχ
πχχχ
The nonzero spatial curvature case
K
GN
3
4=
ρπϕφ +
0≠K
ρπφφ NGK 4=3+∆
The Helmholtz equation:
Spatial distribution of inhomogeneitiesis absolutely arbitrary!
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0=3)()(
1 22
φχφχ
χχK
d
d
d
d +
Σ
Σ
One gravitating mass in the origin of coordinates:
the Newtonianlimit at
II. The spherical space= the closed Universe 1= +K
χχ sin=)(Σ
01 0
0
1= 2 cos 2sin
sinN
N
G mC G m
χφ χ χ
χ χ→
− − → −
0→χdivergent at
πχ →
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denotes the geodesic distance between the i-th mass and the point of observation
III. The hyperbolic space= the open Universe 1= −K
χχ sinh=)(Σ
0
exp( 2 )= 0
sinhNG mχ
χφχ →+∞
−− →No gravitationalparadox!
An arbitrary number of gravitating masses:
3
4
sinh
)2(exp= 0
ρπϕ N
i
ii
iN
G
l
lmG +
−− ∑
il
im0
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χaR =The physical distance
1≪≪ χ⇒aR
320
20
2
1= 108.4<= −− ×Ω
Ha
cK [Komatsu, 2011]
Mpca 50
41= 10410 ×≈⇒≈Ω −
−K
1105≪≪ χ⇒MpcR
χφ 0mGN−≈
1180 102.3// 70 −−×≈≈ secMpcseckmH
0.27≈ΩM0.73≈ΩΛ
Experimental data:
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2=
22vma
a
mL +− ϕ
The Lagrange function:
The Lagrange equation:
The physical distance
The physical velocity
Motion of a nonrelativistic test bodywith the mass m
( )r
v∂∂− ϕ
aa
dt
d 1=2
a=R r
( )vR
rRV a
a
a
dt
ad
dt
d +===ɺ
the physical peculiar velocity
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The reason for the Hubble flow is the global cosmological expansion of the Universe.
22
0
11 1
=,= ccRc
RV adta
t
aaa
a
t
++ ∫ɺ
22
0
121 1
=,= ccrc
v +∫ dta
t
at
physical peculiarvelocity
Hubblevelocity
The case of the negligible gravitational potential
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The Lagrange function in spherical coordinates :ψπθ /2,=,r
Lagrange equations:
( )2222
2= ψϕ
ɺɺ rrma
a
mL ++−
( )2 22 2
= 0 =d M
ma rdt ma r
ψ ψ⇒ɺ ɺ
( )322
22 1
=ram
M
rara
dt
d +∂∂− ϕ
ɺ
The case of spherical symmetry of the problem
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32
2
20
3
302
032
2
20
2
1==
Rm
M
R
mGR
a
aH
Rm
M
R
mGR
a
aR N
MN +−
Ω+Ω−+− Λ
ɺɺɺɺ
|/2|=
|/| 20
0
0=
03
0=
32
0
M
N
aa
NH
aa
N
H
mG
aa
mGRR
R
mGR
a
a
Ω−Ω==⇒=
Λɺɺ
ɺɺ
cosmological expansion,responsible for the Hubble flow
gravitationalattraction
?=
1.4HR Mpc≈
The zero-acceleration sphere
This value is close to theobserved one ~ 1 Mpc!
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2/3
1/21/2
1/21/21/3
~2
3cosh~
2
3sinh1=~
Ω
ΩΩ+
Ω
ΩΩ+
ΩΩ
ΛΛ
ΛΛ
Λtta
MM
M
gMm Sun4512
0 103.8101.9 ×≈×≈
[Karachentsev, 2012]
Dimensionless units:
4220
22
00
=~
,=~
,=~,=~
HH RmH
MM
R
RRtHt
a
aa
3
2
232
2
~
~
~/2~
~2=~
~
R
M
RR
atd
Rd MM +Ω−Ω−
Ω+Ω− ΛΛ
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0=~
M
(1;1)
Solid and dashed lines correspond to presence and absence of the gravitational
attraction respectively.
sec100~
kmVV ×≈MpcRR 1.4
~ ×≈
VHRtd
RdV
H 0
1=~
~=
~
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1=~
M
2=~
M
3=~
M
0~ ≠M
0=~
M
(1;0)
the dashed black line = the pure Hubble flow
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The average gravitational potential is zero, as it should be!
The average gravitational potential
3
4
sinh
)2(exp= 0
ρπϕ N
i
ii
iN
G
l
lmG +
−− ∑
this constant term does not affect motion ofnonrelativistic bodies, but it contributes to themetrics, and at present time this contribution is
32
20
20
20
102=3
8×
Ω∼
c
aH
ca
G MN ρπ
There is no any contradiction,because
3
4=total
ρπφ NG−
0=ϕ
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For the sake of revolution
less than 150 Mpc
the slightly perturbed “ΛCDM” model
weaklyinhomogeneous and anisotropic Universe
mechanical /discrete approach
Hubble’s law
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, ,i i i i i iX ax Y ay Z az= = =
( )( ) ( ) ( )
( )
( )( ) ( ) ( )
( )
( )( ) ( ) ( )
( )
3 22 2 2
3 22 2 2
3 22 2 2
1
1
1
j i j
N i ij i
i j i j i j
j i j
N i ij i
i j i j i j
j i j
N i ij i
i j i j i j
m X XG X a aX
aX X Y Y Z Z
m Y YG Y a aY
aX X Y Y Z Z
m Z ZG Z a aZ
aX X Y Y Z Z
≠
≠
≠
−− = −
− + − + −
−− = −
− + − + −
−− = −
− + − + −
∑
∑
∑
ɺɺ ɺɺ
ɺɺ ɺɺ
ɺɺ ɺɺ
Physical coordinates:
The Lagrange equations for the i-th mass:
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( )( ) ( )
( )( ) ( )
2 2
3 22 22 2
2 2
3 22 22 2
1 1, , 1,...,
1 1, , 1,...,
j i jii
j ii j i j
j i jii
j ii j i j
m X Xd X d aX i j N
dt m a dtX X Y Y
m Y Yd Y d aY i j N
dt m a dtX X Y Y
≠
≠
−= − + =
− + −
−= − + =
− + −
∑
∑
ɶ ɶɶ ɶɶ
ɶ ɶɶɶ ɶ ɶ ɶ
ɶ ɶɶ ɶɶ
ɶ ɶɶɶ ɶ ɶ ɶ
Motion on the plane 0Z =1
1 N
ii
m mN =
= ∑
1 31 3 1220
1 31 3 1220
10
0.95 Mpc
10
0.95 Mpc
ii i
N
ii i
N
MH XX X
G m m
MH YY Y
G m m
= =
= =
⊙
⊙
ɶ
ɶ
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Dynamics of three gravitating masseswith zero initial velocities
0t =ɶ 1t =ɶ 2t =ɶ
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Four masses, nonzero initial velocities
0; 1; 2t =ɶ 0; 0.3; 0.6t =ɶ
both attraction and expansionexpansion only
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The collision betweenMilky Way and Andromeda
Separation distance ~ 0.78 Mpc
Longitudinal velocity ~ 120 km/s
Transversal velocity ~ 100 km/s
Merger distance ~ 100 Kpc
Mass of MW ~ 1012 M
Mass of M31 ~ 1.6 × 1012 M
[Cox and Loeb, 2008]
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The separation distance as a functionof time in the free fall approximation
without dynamical friction
both attraction and expansionattraction only
zero transversalvelocity
nonzerotransversalvelocity
no collisioncollisionin 3.68 Gyr
290 Kpc4.44 Gyr
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Chandrasekhar’s dynamical friction
( ) ( )2
ph, 23
4 2erf expN mM
MM
QG Md
dt V
π ρ χχ χπ
= − − −
VV
MV Mis the physical velocity of the mass
ph,mρ is the physical rest mass density of the intragroup media
2MVχσ
= ( )21ln 1
2Q λ= +
is the Coulomb logarithm defined by the largest impact parameter , the initial relative velocity and the masses andMm
maxb0V
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pec,
2i
i
vχ
σ=ɶ
ɶɶ
1 320
0 N
H
H G m
σσ
=
ɶ
20
ph, cr
3, 10
8mN
H
Gρ αρ α α
π= = ∼
The physical rest mass density begins todecrease at scales where cosmological expansiondominates over gravitational attraction, that isapproximately at 1 Mpc. Here . Therefore,1 .
~ 1Q
ph,mρ
kT
mσ =
m is the mass of the intragroup media particle
5α ∼
510 KT ∼
max ~ 1 Mpcb
( )2 2
max 0 max 0
N N
b V b V
G M m G Mλ = ≈
+
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( )( ) ( )
( ) ( )
( )( ) ( )
2 2
3 22 22 2
23pec,
2 2
3 22 2 2
1 1
3 2 1erf exp , , , ;
2
1 1
j i jii
i j i j
i i ii i i
i
j i ji
i j i j
m X Xd X d aX
dt m a dtX X Y Y
Qm dX daX i j A B i j
mv dt a dt
m Y Yd Y d a
dt m a dtX X Y Y
α χχ χπ
−= − +
− + −
− − − − = ≠
−= − +
− + −
ɶ ɶɶ ɶɶ
ɶ ɶɶɶ ɶ ɶ ɶ
ɶɶ ɶɶɶ ɶ
ɶ ɶɶ ɶ
ɶ ɶɶ ɶ
ɶ ɶɶɶ ɶ ɶ ɶ
( ) ( )
2
23pec,
3 2 1erf exp , , , ;
2
i
i i ii i i
i
Y
Qm dY daY i j A B i j
mv dt a dt
α χχ χπ
− − − − = ≠
ɶ
ɶɶ ɶɶɶ ɶ
ɶ ɶɶ ɶ
pec,
1 22 2
pec,
1 1, , ,
1 1
i ii i i
i ii i
dX dYda daX Y i A B
dt a dt dt a dt
dX dYda dav X Y
dt a dt dt a dt
= − − =
= − + −
vɶ ɶɶ ɶ
ɶ ɶɶɶ ɶ ɶ ɶɶ ɶ
ɶ ɶɶ ɶɶ ɶɶ
ɶ ɶ ɶ ɶɶ ɶ
( ) ( )2
0
2erf exp
x
x dξ ξπ
= −∫
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The separation distance
67 MeVIGMm >
The touch of the galaxies will take place during the first passage for the intragroup media particle masses
100 Kpc
1.17σ =ɶ
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The corresponding trajectoriesof MW (blue) and M31 (green)
collision in 6 Gyr
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The merger willtake place for
17 MeVIGMm >
The separation distance
1 Mpc
2.31σ =ɶ
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The corresponding trajectories of MW
(blue) and M31 (green)
collision in 37 Gyr
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The dwarf galaxy acceleration
2
2
1 1d d a
dt a dt a
ϕ∂= = −∂
VW R
R
ɶ ɶɶɶ ɶ
ɶɶ ɶɶ ɶ
( )2 3
0 0
1
Na H G mϕ ϕ=ɶ
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Right =Milky Way
Left = Andromeda
Vector field
0yW =ɶ0xW =ɶ
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The contour plot of the acceleration absolute value,if the cosmological expansion is disregarded
0x yW W= =ɶ ɶ
0=Wɶ
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The real contour plot
The exact zero acceleration surface is absent.
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The mechanical approach in modern cosmologyis consistently developed and substantiated.
The late Universe inside the cell of uniformity(less than 150 Mpc) is described by the slightlyperturbed “ ΛCDM” model:
– the metrics
– the gravitational potential
Results and conclusions
βααβγη dxdxdads )2(1)2(1 222 Φ−−Φ+≈
)(
)(=),(
2 ηϕη
ac
rrΦ
)(4=3 ρρπϕϕ −+∆ NGK
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In the case (the hyperbolic space = theopen Universe):
– inhomogeneities may be distributed completely randomly;
– the gravitational potential is finite at any vacuum point and its average value is zero;
– at present time the distance from our LocalGroup of galaxies, at which the cosmologicalexpansion ‘=’ the gravitational attraction, or thezero acceleration sphere radius, ~ 1.4 Mpc, andthis theoretical value is close to the observedone, namely 1 Mpc.
1−=K
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The observations of the Hubbleflows even at a few Mpc mayreveal presence of dark energyin the Universe.
The mechanical approach gives a possibility tosimulate the dynamical behavior of an arbitrarynumber of randomly distributed inhomogeneitiesinside the cell of uniformity, including the MilkyWay and Andromeda galaxies together with thedwarf galaxies, taking into account gravitationalinteraction between them as well as cosmologicalexpansion of the Universe.
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THANK YOU FOR ATTENTION !