SlideShare une entreprise Scribd logo
1  sur  21
Télécharger pour lire hors ligne
Explorations in Higher
Dimensional Gravity Theory
PhD- thesis proposal
Prepared by: Safinaz Ramadan
March 2019
Al-Azhar University
Faculty of Science
Physics Department
1
Highlights
Introduction: ( the way for higher dimensions )
- 1915: General Theory of Relativity.
- 1970: Standard Model of Elementary particles.
- 1973: Supersymmetry ( SUSY).
- 1976: Supergravity (SUGRA).
- 1984: Manifestation of SUGRA as an effective theory of
string theory.
D = 5 N = 2 supergravity
- Dimensional reduction from D=11 supergravity.
- Model the universe as a 3-brane embedded in 5-D
spacetime N=2 supergravity.
- Studying the time evolution of the universe.
- Studying the cosmological constant problem.
2
Unification to Higher
Dimensions
3
From Special Relativity (1905) to General
Relativity
The line interval between A and
B can be defined by the metric
ds2
= − c2
dt2
+ dx2
+ dy2
+ dz2
( Minkowski flat space- time)
The speed of light in a vacuum is
constant and nothing can exceed
light’s speed.
But what if
the sun
disappeared
??
4
Einstein Field equations
Riemann curvature tensor
Rμν −
1
2
gμνR = κ Tμν
Rμν = Rρ
μρν
Minkowski s-t
Rρ
μνσ = 0 →
Tμν = (ρ + p)uμ
uν
− pδμν
.
The Energy-Momentum tensor
In IRF for perfect
fluid
Ricci scalar
R = gμνRμν
Curvature in s-t
Matter
Ricci tensor
Rμν −
1
2
gμνR = κ Tμν
5
By demanding we get EFE in the absence of matter.
The Einstein–Hilbert action
F(R) gravity
SEH =
∫R
R −g d4
x
δSEH = 0
S =
∫
d4
x −g(R + R2
+ 3R3
+ . . . . ),
Modified Gravity Theories
S =
∫
d4
x −g F(R) .
6
dF
dR
= FR, and make conformal transformation ̂
gμν =
1
FR
gμν ,
S =
∫
d4
x −g[ ̂
R −
1
2
(∂α
ϕ)(∂αϕ) − V(ϕ)] .
The ordinary E.H.A term plus extra scalar field terms
( the inflaton).
7
The Standard Model
Internal symmetry group
SU(3)C × SU(2)L × U(1)Y
ψ′

(x) = eiϵa(x) ta ψ(x),
a = 1,2,3, SU(2), 1,..,8, SU(3) .
Drawbacks 🙁
- it is not a truly unified theory because the
gluons and the photons governed by totally
different rules.
- Too many unanswered questions ( masses,
and charges of particles) , and too many
constants ( with brute force values).
- Dark matter 23% and dark energy 73% of
our universe !! Couldn’t been explained.
- Unification? No gravity !!
8
Supersymmetry
- Space-time
4D QFT.
-Poincaré
symmetry
δψ = − iσμ
ζ̄∂ϕ
δϕ = ζ . ψ
Lfree WZ = ∂μϕ*∂μ
ϕ + ψ̄γμ
∂μψ .
9
10
Supergravity
Introduce vector spinor field with spin 3/2 ( the
gravitino) with Noether coupling
LWZ is not invarinat under ϵ → ϵ(x)
δL = ∂μϵα
Kμ
α + h . c .
Kα
μ = − ∂μϕ*ψα
−
i
2
ψβ
(σμσ̄ν
)α
β∂μϕ*,
Ψμ
α → Ψμ
α +
1
k
∂μ
ϵα,
LN = kKα
μΨμ
α, Transforming as
However δ(L + LN) = kψ̄μγνϵTμν
11
Lg = − gμνTμν
This contribution can only be canceled adding a new term
δgμν = kΨ̄μγνϵ
In the presence of local supersymmetry we must
include also the gravity supermultiplet the
graviton and gravitino respectively (N=1) SUGRA.
(gμν, Ψα
μ)
12
SUGRA as an effective theory of superstring
13
D=5 N=2
Supergravity
14
Dimensional reduction over Calabi-Yau
Manifold
S11 =
1
2κ2
11
∫
d11
x −G (R −
1
48
F2
) −
1
12κ2
11
∫
A ∧ F ∧ F,
S5 =
1
2κ2
5
∫
d5
x −g [R −
1
2
(∂μσ)(∂μ
σ) − Gi¯
j (∂μzi
)(∂μ
z
¯
j
)
−
1
48
e−2σ
FμνρσFμνρσ
−
1
24
ϵ̄μνρσαFμνρσ
Kα
(ζ, ζ̄) + eσ
Lμ
μ(ζ, ζ̄)],
Calabi-Yau
Manifold
15
Where the z's are the CY's complex structure (M) moduli,
h2,1 is the dimension of M.
Two gravitini and a set of hyperini; the superpartenrs
of the hypermultiples bosons.
The particle content at 5 D N=2
(a, σ, ζ0
, ¯
ζ0
) the universal hypermultiplet
(zi
, z̄i
, ζi
, ζ̄i
: i = 1,...,h2,1)
16
The universe as a 3-brane embedded
in 5 D
5 D space-time.
The Bulk:
The moduli
Live here
We live
here
4 spatial D.
3 spatial D.
17
Time evolution of the universe
More understanding for the inflation epoch where the early
universe expanded exponential rate for 10^-36 seconds after the
Big Bang , then the universe continued to expand in less rapid
rates until nowadays
18
The cosmological constant
Einstein’s Greatest Blunder
In 1916 Rμν −
1
2
gμνR = κTμν − Λgμν .
1929 Edwin Hubble : the expansion of the universe
It gives negative pressure, and thus acts as a repulsive
force counteracting the attractive gravitational effect ->
static universe
In 1998 : from observing type IA supernova indicated that
the universe is also accelerating in its expansion
19
So the cosmological constant term should be considered
to explain the vacuum energy or “ Dark Energy” that
produces repulsion of the universe
However when measuring the quantum vacuum energy
On the other hand the observed value of the darkenergy
density required for the current rate of acceleration of
the universe is roughly
The cosmological constant problem !!
ρ ∼ 10112
erg/cm3
ρ ∼ 10−8
erg/cm3
catastrophy !!
20
21

Contenu connexe

Similaire à Explorations in Higher-Dimensional Gravity Theory.pdf

Faltenbacher - Simulating the Universe
Faltenbacher - Simulating the UniverseFaltenbacher - Simulating the Universe
Faltenbacher - Simulating the Universe
CosmoAIMS Bassett
 
Day 6 cosmo_inflation_ss09
Day 6 cosmo_inflation_ss09Day 6 cosmo_inflation_ss09
Day 6 cosmo_inflation_ss09
Atner Yegorov
 
Manifolds and Catastrophes for Physical Systems
Manifolds and Catastrophes for Physical SystemsManifolds and Catastrophes for Physical Systems
Manifolds and Catastrophes for Physical Systems
BRNSSPublicationHubI
 
THE MASS OF ASYMPTOTICALLY HYPERBOLIC MANIFOLDS
THE MASS OF ASYMPTOTICALLY HYPERBOLIC MANIFOLDSTHE MASS OF ASYMPTOTICALLY HYPERBOLIC MANIFOLDS
THE MASS OF ASYMPTOTICALLY HYPERBOLIC MANIFOLDS
MichaelRabinovich
 
Gravity origin & evolution
Gravity origin & evolutionGravity origin & evolution
Gravity origin & evolution
dsvthampi
 
chapter5-gravitationppt-copy-211229151431 (2).pdf
chapter5-gravitationppt-copy-211229151431 (2).pdfchapter5-gravitationppt-copy-211229151431 (2).pdf
chapter5-gravitationppt-copy-211229151431 (2).pdf
RavindraWaykole
 
Gravity as entanglement, and entanglement as gravity
Gravity as entanglement, and entanglement as gravityGravity as entanglement, and entanglement as gravity
Gravity as entanglement, and entanglement as gravity
Vasil Penchev
 

Similaire à Explorations in Higher-Dimensional Gravity Theory.pdf (20)

Gravitomagnetism successes (3)
Gravitomagnetism successes (3)Gravitomagnetism successes (3)
Gravitomagnetism successes (3)
 
Quantization of the Orbital Motion of a Mass In The Presence Of Einstein’s Gr...
Quantization of the Orbital Motion of a Mass In The Presence Of Einstein’s Gr...Quantization of the Orbital Motion of a Mass In The Presence Of Einstein’s Gr...
Quantization of the Orbital Motion of a Mass In The Presence Of Einstein’s Gr...
 
Miao
MiaoMiao
Miao
 
Topological Strings Invariants
Topological Strings InvariantsTopological Strings Invariants
Topological Strings Invariants
 
GR.ppt
GR.pptGR.ppt
GR.ppt
 
lecture5
lecture5lecture5
lecture5
 
Faltenbacher - Simulating the Universe
Faltenbacher - Simulating the UniverseFaltenbacher - Simulating the Universe
Faltenbacher - Simulating the Universe
 
Day 6 cosmo_inflation_ss09
Day 6 cosmo_inflation_ss09Day 6 cosmo_inflation_ss09
Day 6 cosmo_inflation_ss09
 
Neven Bilic, "Dark Matter, Dark Energy, and Unification Models"
Neven Bilic, "Dark Matter, Dark Energy, and Unification Models"Neven Bilic, "Dark Matter, Dark Energy, and Unification Models"
Neven Bilic, "Dark Matter, Dark Energy, and Unification Models"
 
space blackhole
space blackholespace blackhole
space blackhole
 
Manifolds and Catastrophes for Physical Systems
Manifolds and Catastrophes for Physical SystemsManifolds and Catastrophes for Physical Systems
Manifolds and Catastrophes for Physical Systems
 
Schrödinger wave equation
Schrödinger wave equationSchrödinger wave equation
Schrödinger wave equation
 
Planetary Motion- The simple Physics Behind the heavenly bodies
Planetary Motion- The simple Physics Behind the heavenly bodiesPlanetary Motion- The simple Physics Behind the heavenly bodies
Planetary Motion- The simple Physics Behind the heavenly bodies
 
Enric Verdaguer-Simposio Internacional sobre Solitón
Enric Verdaguer-Simposio Internacional sobre SolitónEnric Verdaguer-Simposio Internacional sobre Solitón
Enric Verdaguer-Simposio Internacional sobre Solitón
 
THE MASS OF ASYMPTOTICALLY HYPERBOLIC MANIFOLDS
THE MASS OF ASYMPTOTICALLY HYPERBOLIC MANIFOLDSTHE MASS OF ASYMPTOTICALLY HYPERBOLIC MANIFOLDS
THE MASS OF ASYMPTOTICALLY HYPERBOLIC MANIFOLDS
 
Presentation.pptx
Presentation.pptxPresentation.pptx
Presentation.pptx
 
Gravity origin & evolution
Gravity origin & evolutionGravity origin & evolution
Gravity origin & evolution
 
PHYSICS CLASS XI Chapter 5 - gravitation
PHYSICS CLASS XI Chapter 5 - gravitationPHYSICS CLASS XI Chapter 5 - gravitation
PHYSICS CLASS XI Chapter 5 - gravitation
 
chapter5-gravitationppt-copy-211229151431 (2).pdf
chapter5-gravitationppt-copy-211229151431 (2).pdfchapter5-gravitationppt-copy-211229151431 (2).pdf
chapter5-gravitationppt-copy-211229151431 (2).pdf
 
Gravity as entanglement, and entanglement as gravity
Gravity as entanglement, and entanglement as gravityGravity as entanglement, and entanglement as gravity
Gravity as entanglement, and entanglement as gravity
 

Dernier

Porella : features, morphology, anatomy, reproduction etc.
Porella : features, morphology, anatomy, reproduction etc.Porella : features, morphology, anatomy, reproduction etc.
Porella : features, morphology, anatomy, reproduction etc.
Silpa
 
The Mariana Trench remarkable geological features on Earth.pptx
The Mariana Trench remarkable geological features on Earth.pptxThe Mariana Trench remarkable geological features on Earth.pptx
The Mariana Trench remarkable geological features on Earth.pptx
seri bangash
 
LUNULARIA -features, morphology, anatomy ,reproduction etc.
LUNULARIA -features, morphology, anatomy ,reproduction etc.LUNULARIA -features, morphology, anatomy ,reproduction etc.
LUNULARIA -features, morphology, anatomy ,reproduction etc.
Silpa
 
Phenolics: types, biosynthesis and functions.
Phenolics: types, biosynthesis and functions.Phenolics: types, biosynthesis and functions.
Phenolics: types, biosynthesis and functions.
Silpa
 
CYTOGENETIC MAP................ ppt.pptx
CYTOGENETIC MAP................ ppt.pptxCYTOGENETIC MAP................ ppt.pptx
CYTOGENETIC MAP................ ppt.pptx
Silpa
 
biology HL practice questions IB BIOLOGY
biology HL practice questions IB BIOLOGYbiology HL practice questions IB BIOLOGY
biology HL practice questions IB BIOLOGY
1301aanya
 

Dernier (20)

Porella : features, morphology, anatomy, reproduction etc.
Porella : features, morphology, anatomy, reproduction etc.Porella : features, morphology, anatomy, reproduction etc.
Porella : features, morphology, anatomy, reproduction etc.
 
Zoology 5th semester notes( Sumit_yadav).pdf
Zoology 5th semester notes( Sumit_yadav).pdfZoology 5th semester notes( Sumit_yadav).pdf
Zoology 5th semester notes( Sumit_yadav).pdf
 
The Mariana Trench remarkable geological features on Earth.pptx
The Mariana Trench remarkable geological features on Earth.pptxThe Mariana Trench remarkable geological features on Earth.pptx
The Mariana Trench remarkable geological features on Earth.pptx
 
Genetics and epigenetics of ADHD and comorbid conditions
Genetics and epigenetics of ADHD and comorbid conditionsGenetics and epigenetics of ADHD and comorbid conditions
Genetics and epigenetics of ADHD and comorbid conditions
 
LUNULARIA -features, morphology, anatomy ,reproduction etc.
LUNULARIA -features, morphology, anatomy ,reproduction etc.LUNULARIA -features, morphology, anatomy ,reproduction etc.
LUNULARIA -features, morphology, anatomy ,reproduction etc.
 
Phenolics: types, biosynthesis and functions.
Phenolics: types, biosynthesis and functions.Phenolics: types, biosynthesis and functions.
Phenolics: types, biosynthesis and functions.
 
Call Girls Ahmedabad +917728919243 call me Independent Escort Service
Call Girls Ahmedabad +917728919243 call me Independent Escort ServiceCall Girls Ahmedabad +917728919243 call me Independent Escort Service
Call Girls Ahmedabad +917728919243 call me Independent Escort Service
 
CYTOGENETIC MAP................ ppt.pptx
CYTOGENETIC MAP................ ppt.pptxCYTOGENETIC MAP................ ppt.pptx
CYTOGENETIC MAP................ ppt.pptx
 
biology HL practice questions IB BIOLOGY
biology HL practice questions IB BIOLOGYbiology HL practice questions IB BIOLOGY
biology HL practice questions IB BIOLOGY
 
Gwalior ❤CALL GIRL 84099*07087 ❤CALL GIRLS IN Gwalior ESCORT SERVICE❤CALL GIRL
Gwalior ❤CALL GIRL 84099*07087 ❤CALL GIRLS IN Gwalior ESCORT SERVICE❤CALL GIRLGwalior ❤CALL GIRL 84099*07087 ❤CALL GIRLS IN Gwalior ESCORT SERVICE❤CALL GIRL
Gwalior ❤CALL GIRL 84099*07087 ❤CALL GIRLS IN Gwalior ESCORT SERVICE❤CALL GIRL
 
Chemistry 5th semester paper 1st Notes.pdf
Chemistry 5th semester paper 1st Notes.pdfChemistry 5th semester paper 1st Notes.pdf
Chemistry 5th semester paper 1st Notes.pdf
 
Thyroid Physiology_Dr.E. Muralinath_ Associate Professor
Thyroid Physiology_Dr.E. Muralinath_ Associate ProfessorThyroid Physiology_Dr.E. Muralinath_ Associate Professor
Thyroid Physiology_Dr.E. Muralinath_ Associate Professor
 
Dr. E. Muralinath_ Blood indices_clinical aspects
Dr. E. Muralinath_ Blood indices_clinical  aspectsDr. E. Muralinath_ Blood indices_clinical  aspects
Dr. E. Muralinath_ Blood indices_clinical aspects
 
Role of AI in seed science Predictive modelling and Beyond.pptx
Role of AI in seed science  Predictive modelling and  Beyond.pptxRole of AI in seed science  Predictive modelling and  Beyond.pptx
Role of AI in seed science Predictive modelling and Beyond.pptx
 
Climate Change Impacts on Terrestrial and Aquatic Ecosystems.pptx
Climate Change Impacts on Terrestrial and Aquatic Ecosystems.pptxClimate Change Impacts on Terrestrial and Aquatic Ecosystems.pptx
Climate Change Impacts on Terrestrial and Aquatic Ecosystems.pptx
 
Site Acceptance Test .
Site Acceptance Test                    .Site Acceptance Test                    .
Site Acceptance Test .
 
Atp synthase , Atp synthase complex 1 to 4.
Atp synthase , Atp synthase complex 1 to 4.Atp synthase , Atp synthase complex 1 to 4.
Atp synthase , Atp synthase complex 1 to 4.
 
Molecular markers- RFLP, RAPD, AFLP, SNP etc.
Molecular markers- RFLP, RAPD, AFLP, SNP etc.Molecular markers- RFLP, RAPD, AFLP, SNP etc.
Molecular markers- RFLP, RAPD, AFLP, SNP etc.
 
Cyanide resistant respiration pathway.pptx
Cyanide resistant respiration pathway.pptxCyanide resistant respiration pathway.pptx
Cyanide resistant respiration pathway.pptx
 
PATNA CALL GIRLS 8617370543 LOW PRICE ESCORT SERVICE
PATNA CALL GIRLS 8617370543 LOW PRICE ESCORT SERVICEPATNA CALL GIRLS 8617370543 LOW PRICE ESCORT SERVICE
PATNA CALL GIRLS 8617370543 LOW PRICE ESCORT SERVICE
 

Explorations in Higher-Dimensional Gravity Theory.pdf

  • 1. Explorations in Higher Dimensional Gravity Theory PhD- thesis proposal Prepared by: Safinaz Ramadan March 2019 Al-Azhar University Faculty of Science Physics Department 1
  • 2. Highlights Introduction: ( the way for higher dimensions ) - 1915: General Theory of Relativity. - 1970: Standard Model of Elementary particles. - 1973: Supersymmetry ( SUSY). - 1976: Supergravity (SUGRA). - 1984: Manifestation of SUGRA as an effective theory of string theory. D = 5 N = 2 supergravity - Dimensional reduction from D=11 supergravity. - Model the universe as a 3-brane embedded in 5-D spacetime N=2 supergravity. - Studying the time evolution of the universe. - Studying the cosmological constant problem. 2
  • 4. From Special Relativity (1905) to General Relativity The line interval between A and B can be defined by the metric ds2 = − c2 dt2 + dx2 + dy2 + dz2 ( Minkowski flat space- time) The speed of light in a vacuum is constant and nothing can exceed light’s speed. But what if the sun disappeared ?? 4
  • 5. Einstein Field equations Riemann curvature tensor Rμν − 1 2 gμνR = κ Tμν Rμν = Rρ μρν Minkowski s-t Rρ μνσ = 0 → Tμν = (ρ + p)uμ uν − pδμν . The Energy-Momentum tensor In IRF for perfect fluid Ricci scalar R = gμνRμν Curvature in s-t Matter Ricci tensor Rμν − 1 2 gμνR = κ Tμν 5
  • 6. By demanding we get EFE in the absence of matter. The Einstein–Hilbert action F(R) gravity SEH = ∫R R −g d4 x δSEH = 0 S = ∫ d4 x −g(R + R2 + 3R3 + . . . . ), Modified Gravity Theories S = ∫ d4 x −g F(R) . 6
  • 7. dF dR = FR, and make conformal transformation ̂ gμν = 1 FR gμν , S = ∫ d4 x −g[ ̂ R − 1 2 (∂α ϕ)(∂αϕ) − V(ϕ)] . The ordinary E.H.A term plus extra scalar field terms ( the inflaton). 7
  • 8. The Standard Model Internal symmetry group SU(3)C × SU(2)L × U(1)Y ψ′  (x) = eiϵa(x) ta ψ(x), a = 1,2,3, SU(2), 1,..,8, SU(3) . Drawbacks 🙁 - it is not a truly unified theory because the gluons and the photons governed by totally different rules. - Too many unanswered questions ( masses, and charges of particles) , and too many constants ( with brute force values). - Dark matter 23% and dark energy 73% of our universe !! Couldn’t been explained. - Unification? No gravity !! 8
  • 9. Supersymmetry - Space-time 4D QFT. -Poincaré symmetry δψ = − iσμ ζ̄∂ϕ δϕ = ζ . ψ Lfree WZ = ∂μϕ*∂μ ϕ + ψ̄γμ ∂μψ . 9
  • 10. 10
  • 11. Supergravity Introduce vector spinor field with spin 3/2 ( the gravitino) with Noether coupling LWZ is not invarinat under ϵ → ϵ(x) δL = ∂μϵα Kμ α + h . c . Kα μ = − ∂μϕ*ψα − i 2 ψβ (σμσ̄ν )α β∂μϕ*, Ψμ α → Ψμ α + 1 k ∂μ ϵα, LN = kKα μΨμ α, Transforming as However δ(L + LN) = kψ̄μγνϵTμν 11
  • 12. Lg = − gμνTμν This contribution can only be canceled adding a new term δgμν = kΨ̄μγνϵ In the presence of local supersymmetry we must include also the gravity supermultiplet the graviton and gravitino respectively (N=1) SUGRA. (gμν, Ψα μ) 12
  • 13. SUGRA as an effective theory of superstring 13
  • 15. Dimensional reduction over Calabi-Yau Manifold S11 = 1 2κ2 11 ∫ d11 x −G (R − 1 48 F2 ) − 1 12κ2 11 ∫ A ∧ F ∧ F, S5 = 1 2κ2 5 ∫ d5 x −g [R − 1 2 (∂μσ)(∂μ σ) − Gi¯ j (∂μzi )(∂μ z ¯ j ) − 1 48 e−2σ FμνρσFμνρσ − 1 24 ϵ̄μνρσαFμνρσ Kα (ζ, ζ̄) + eσ Lμ μ(ζ, ζ̄)], Calabi-Yau Manifold 15
  • 16. Where the z's are the CY's complex structure (M) moduli, h2,1 is the dimension of M. Two gravitini and a set of hyperini; the superpartenrs of the hypermultiples bosons. The particle content at 5 D N=2 (a, σ, ζ0 , ¯ ζ0 ) the universal hypermultiplet (zi , z̄i , ζi , ζ̄i : i = 1,...,h2,1) 16
  • 17. The universe as a 3-brane embedded in 5 D 5 D space-time. The Bulk: The moduli Live here We live here 4 spatial D. 3 spatial D. 17
  • 18. Time evolution of the universe More understanding for the inflation epoch where the early universe expanded exponential rate for 10^-36 seconds after the Big Bang , then the universe continued to expand in less rapid rates until nowadays 18
  • 19. The cosmological constant Einstein’s Greatest Blunder In 1916 Rμν − 1 2 gμνR = κTμν − Λgμν . 1929 Edwin Hubble : the expansion of the universe It gives negative pressure, and thus acts as a repulsive force counteracting the attractive gravitational effect -> static universe In 1998 : from observing type IA supernova indicated that the universe is also accelerating in its expansion 19
  • 20. So the cosmological constant term should be considered to explain the vacuum energy or “ Dark Energy” that produces repulsion of the universe However when measuring the quantum vacuum energy On the other hand the observed value of the darkenergy density required for the current rate of acceleration of the universe is roughly The cosmological constant problem !! ρ ∼ 10112 erg/cm3 ρ ∼ 10−8 erg/cm3 catastrophy !! 20
  • 21. 21