Gueorguiev & Maeder 2
The 14th Interna6onal Conference on Gravita6on, Astrophysics and Cosmology (ICGAC14),
Na6onal Central University, Jhongli, Taiwan, 17 – 21 August 2020
in collabora*on with
André Maeder, Geneva Observatory, Switzerland
Vesselin G. Gueorguiev
Institute for Advanced Physical Studies, Sofia, Bulgaria
& Ronin Institute for Independent Scholarship, NJ, USA
Fotosearch Royalty Free Stock Photography (h/ps://www.fotosearch.com)
Scale-Invariant Vacuum Theory (SIVT)– Applica:ons:
The Growth of the Density Fluctua:ons in the SIVT
Physics of the Dark Universe 25 (2019) 100315 [arXiv:1811.03495]
Scale-invariant dynamics of galaxies,
MOND, dark ma,er, and the dwarf spheroidals
Monthly No6ces of the Royal Astronomical Society 492, 2698 (2020) [arXiv:2001.04978]
The 14th Interna:onal Conference on Gravita:on, Astrophysics and Cosmology (ICGAC14),
Na:onal Central University, Jhongli, Taiwan, 17 – 21 August 2020
Gueorguiev & Maeder VGG talk at ICGAC14 via zoom on 18 August 2020 3
Key Results!
 Equa6ons for Cosmology within the Scale-Invariant Vacuum Theory (SIVT)
 The Growth of the Density Perturba6on within the SIVT
 SIVT Descrip6on of the Dwarf Spheroidals - failure of ΛCDM and MOND!
’Integrable Weyl Geometry
Gueorguiev & Maeder VGG talk at ICGAC14 via zoom on 18 August 2020 4
Canuto et al 1977
Alike in GR, vacuum proper6es do not depend on the material content
Within SIVT:
The empty space!
If l =const.=1
 usual equa6ons.
The cosmological
equa:ons :
If dR/dt > 0, addi6onal accelera6on
opposed to gravity.
No need of unknown Dark Stu9!
COSMOLOGY
Maeder (2017)
λ∝1/t
-
L
3
The Ield equa6on with the R-W metric
√3
Λ
Gueorguiev & Maeder VGG talk at ICGAC14 via zoom on 18 August 2020 5
SIVT vs. ΛCDM (k=0)
Maeder, 2017aThe Astrophysical Journal, 834:194 (16pp), 2017
Gueorguiev & Maeder ICGAC14 via Zoom on 18 August 2020 6
Equa6ons of con6nuity, of Euler, and Poisson within the SIVT:
Applied to a density perturba6on d they give:
The 6me deriva6ve
of the Irst one and
the divergence of
the second eqs.,
with p=0, lead to:
n
Euler h-order of δ.
Maeder &
Gueorguiev, 2018
The Growth of the Density Perturba6on
Physics of the Dark Universe 25 (2019) 100315; arXiv:1811.03495 [astro-ph.CO]
(t)= 1/t
n-dependence of the growth
-1
-2
-3
-4
-5
logd
3.0 2.5 2.0 1.5 1.0 0.5
log (1+z)
EdS model
Different values of n
n = 5, 3, 2, 1
Dotted lines:
initial z=3000 and
z=500 for n=2.
Ωm=0.10, ini6al value δ = 10−5
at z = 1376
Gueorguiev & Maeder ICGAC14 via Zoom on 18 August 2020 7
FAST GROWTH OF THE DENSITY FLUCTUATIONS
(short free-fall 6me, addi6onal infall velocity)
DARK MATTER NEEDS NOT TO BE PRESENT!
Gueorguiev & Maeder ICGAC14 via Zoom on 18 August 2020 8
Gueorguiev & Maeder VGG talk at ICGAC14 via zoom on 18 August 2020 9
k2
= 10-10.85
Lelli et al. (2017)
Gueorguiev & Maeder VGG talk at ICGAC14 via zoom on 18 August 2020 10
The geodesics: curve whose tangent vector um
=dxm
/ds is transported by
parallel displacement along the curve. Dirac, 1973
From an ac:on: Bouvier & Maeder, 1978
k(t) = 1/tPoten6al F=GM/r
is scale invariant
The ra6o of the 2 terms is
GM
THE WEAK FIELD APPROXIMATION for SIVT
x = k v r2
Gueorguiev & Maeder VGG talk at ICGAC14 via zoom on 18 August 2020 11
x = k v r2
GM
k= 1/t= H
x
At any 6me,
Using v = (r gobs)1/2
 x =
Consider 2 gravit. systems 1 and 2 at the same t and r,
gobs - gbar__________
gbar
2nd
degree equa6on
Calling gobs,2  g and gbar,2  gN
for system 2, system 1 is a reference
gbarx
H (r gobs)1/2
~
k2
is the lower limit of g for gN  0, this limit is the same everywhere
If gN >> k2
, then g  gN
If gN  0 , then g  k2
thus k2
≥ min [gN]
for any r
TOWARDS the RAR
Explicit scale invariance!
Gueorguiev & Maeder VGG talk at ICGAC14 via zoom on 18 August 2020 12
For gN >> 10-10
, g  gN+ (gN k2
)1/2
k2
= 10-10.85
 SIV paradigm is a minimal generalization of the Einstein GR,
 Provides New framework for Cosmology & Gravity,
 Density perturbations can grow fast enough!
 No need of Dark Matter!
 Explains the Dwarf Spheroidal, unlike MOND!
 Scale invariance might explain dark matter effects!
 New perspective on dark energy and the CC problem?
 Universe 2020, 6(8), 108; https://doi.org/10.3390/universe6080108
Thank You!
Conclusion:
Revisiting the Cosmological Constant Problem within Quantum Cosmology in Universe 2020, 6(8), 108;
https://doi.org/10.3390/universe6080108
The Growth of the Density Fluctuations in the SIV theory
Physics of the Dark Universe 25 (2019) 100315, https://arxiv.org/abs/1811.03495
Scale-invariant dynamics of galaxies, MOND, dark matter, and the dwarf spheroidals,
Monthly Notices of the Royal Astronomical Society
NNRAS 492, 2698 (2020), https://arxiv.org/abs/2001.04978
The Scale-Invariant Vacuum (SIV) Theory: A Possible Origin of Dark Matter and Dark
Energy, Universe 2020, 6, 46; https://doi.org/10.3390/universe6030046
Revisiting the Cosmological Constant Problem within Quantum Cosmology,
Universe 2020, 6, 108; https://doi.org/10.3390/universe6080108
Special Issue "Nature and Origin of Dark Matter and Dark Energy"
https://www.mdpi.com/si/41677
References:

The Scale Invariant Vacuum Theory as viable Cosmology Model

  • 1.
    Gueorguiev & Maeder2 The 14th Interna6onal Conference on Gravita6on, Astrophysics and Cosmology (ICGAC14), Na6onal Central University, Jhongli, Taiwan, 17 – 21 August 2020 in collabora*on with André Maeder, Geneva Observatory, Switzerland Vesselin G. Gueorguiev Institute for Advanced Physical Studies, Sofia, Bulgaria & Ronin Institute for Independent Scholarship, NJ, USA Fotosearch Royalty Free Stock Photography (h/ps://www.fotosearch.com) Scale-Invariant Vacuum Theory (SIVT)– Applica:ons: The Growth of the Density Fluctua:ons in the SIVT Physics of the Dark Universe 25 (2019) 100315 [arXiv:1811.03495] Scale-invariant dynamics of galaxies, MOND, dark ma,er, and the dwarf spheroidals Monthly No6ces of the Royal Astronomical Society 492, 2698 (2020) [arXiv:2001.04978] The 14th Interna:onal Conference on Gravita:on, Astrophysics and Cosmology (ICGAC14), Na:onal Central University, Jhongli, Taiwan, 17 – 21 August 2020
  • 2.
    Gueorguiev & MaederVGG talk at ICGAC14 via zoom on 18 August 2020 3 Key Results!  Equa6ons for Cosmology within the Scale-Invariant Vacuum Theory (SIVT)  The Growth of the Density Perturba6on within the SIVT  SIVT Descrip6on of the Dwarf Spheroidals - failure of ΛCDM and MOND! ’Integrable Weyl Geometry
  • 3.
    Gueorguiev & MaederVGG talk at ICGAC14 via zoom on 18 August 2020 4 Canuto et al 1977 Alike in GR, vacuum proper6es do not depend on the material content Within SIVT: The empty space! If l =const.=1  usual equa6ons. The cosmological equa:ons : If dR/dt > 0, addi6onal accelera6on opposed to gravity. No need of unknown Dark Stu9! COSMOLOGY Maeder (2017) λ∝1/t - L 3 The Ield equa6on with the R-W metric √3 Λ
  • 4.
    Gueorguiev & MaederVGG talk at ICGAC14 via zoom on 18 August 2020 5 SIVT vs. ΛCDM (k=0) Maeder, 2017aThe Astrophysical Journal, 834:194 (16pp), 2017
  • 5.
    Gueorguiev & MaederICGAC14 via Zoom on 18 August 2020 6 Equa6ons of con6nuity, of Euler, and Poisson within the SIVT: Applied to a density perturba6on d they give: The 6me deriva6ve of the Irst one and the divergence of the second eqs., with p=0, lead to: n Euler h-order of δ. Maeder & Gueorguiev, 2018 The Growth of the Density Perturba6on Physics of the Dark Universe 25 (2019) 100315; arXiv:1811.03495 [astro-ph.CO] (t)= 1/t
  • 6.
    n-dependence of thegrowth -1 -2 -3 -4 -5 logd 3.0 2.5 2.0 1.5 1.0 0.5 log (1+z) EdS model Different values of n n = 5, 3, 2, 1 Dotted lines: initial z=3000 and z=500 for n=2. Ωm=0.10, ini6al value δ = 10−5 at z = 1376 Gueorguiev & Maeder ICGAC14 via Zoom on 18 August 2020 7
  • 7.
    FAST GROWTH OFTHE DENSITY FLUCTUATIONS (short free-fall 6me, addi6onal infall velocity) DARK MATTER NEEDS NOT TO BE PRESENT! Gueorguiev & Maeder ICGAC14 via Zoom on 18 August 2020 8
  • 8.
    Gueorguiev & MaederVGG talk at ICGAC14 via zoom on 18 August 2020 9 k2 = 10-10.85 Lelli et al. (2017)
  • 9.
    Gueorguiev & MaederVGG talk at ICGAC14 via zoom on 18 August 2020 10 The geodesics: curve whose tangent vector um =dxm /ds is transported by parallel displacement along the curve. Dirac, 1973 From an ac:on: Bouvier & Maeder, 1978 k(t) = 1/tPoten6al F=GM/r is scale invariant The ra6o of the 2 terms is GM THE WEAK FIELD APPROXIMATION for SIVT x = k v r2
  • 10.
    Gueorguiev & MaederVGG talk at ICGAC14 via zoom on 18 August 2020 11 x = k v r2 GM k= 1/t= H x At any 6me, Using v = (r gobs)1/2  x = Consider 2 gravit. systems 1 and 2 at the same t and r, gobs - gbar__________ gbar 2nd degree equa6on Calling gobs,2  g and gbar,2  gN for system 2, system 1 is a reference gbarx H (r gobs)1/2 ~ k2 is the lower limit of g for gN  0, this limit is the same everywhere If gN >> k2 , then g  gN If gN  0 , then g  k2 thus k2 ≥ min [gN] for any r TOWARDS the RAR Explicit scale invariance!
  • 11.
    Gueorguiev & MaederVGG talk at ICGAC14 via zoom on 18 August 2020 12 For gN >> 10-10 , g  gN+ (gN k2 )1/2 k2 = 10-10.85
  • 12.
     SIV paradigmis a minimal generalization of the Einstein GR,  Provides New framework for Cosmology & Gravity,  Density perturbations can grow fast enough!  No need of Dark Matter!  Explains the Dwarf Spheroidal, unlike MOND!  Scale invariance might explain dark matter effects!  New perspective on dark energy and the CC problem?  Universe 2020, 6(8), 108; https://doi.org/10.3390/universe6080108 Thank You! Conclusion: Revisiting the Cosmological Constant Problem within Quantum Cosmology in Universe 2020, 6(8), 108; https://doi.org/10.3390/universe6080108
  • 13.
    The Growth ofthe Density Fluctuations in the SIV theory Physics of the Dark Universe 25 (2019) 100315, https://arxiv.org/abs/1811.03495 Scale-invariant dynamics of galaxies, MOND, dark matter, and the dwarf spheroidals, Monthly Notices of the Royal Astronomical Society NNRAS 492, 2698 (2020), https://arxiv.org/abs/2001.04978 The Scale-Invariant Vacuum (SIV) Theory: A Possible Origin of Dark Matter and Dark Energy, Universe 2020, 6, 46; https://doi.org/10.3390/universe6030046 Revisiting the Cosmological Constant Problem within Quantum Cosmology, Universe 2020, 6, 108; https://doi.org/10.3390/universe6080108 Special Issue "Nature and Origin of Dark Matter and Dark Energy" https://www.mdpi.com/si/41677 References: