SlideShare a Scribd company logo
Galadriel’s Mirror
Presentation by Reece Boston
April 23, 2014
Introduction to Galadriel’s Mirror
The proposed device is predicted to allow light to travel from the
future and into the past
What you will see, if you leave the Mirror free to work, I
cannot tell. For it shows things that were, and things that
are, and things that may yet be. But which it is that he sees,
even the wisest cannot always tell. Do you wish to look?
— Lady Galadriel, The Lord of the Rings
Begin with General Relativity, which allows for spacetimes that result
in time travel.
Transformation Optics: curved spacetimes −→ bi-anisotropic media
Bi-anistropy: D = E + γ1H, B = µH + γ2E.
We take a spacetime from GR that allows for time travel, and mimic it
using TO
Resultant material is Galadriel’s Mirror. Causes light to time travel.
Review of Transformation Optics in 3D
Maxwell’s Equations in a linear medium:
∂
∂xi
( ij
Ej ) = 0
∂
∂xi
(µij
Hj ) = 0
[ijk]
∂
∂xj
Ek = −
∂
∂t
(µij
Hj ) [ijk]
∂
∂xj
Hk =
1
c2
∂
∂t
( ij
Ej )
Maxwell’s Equations in curved space:
∂
∂xi
(
√
ggij
Ej ) = 0
∂
∂xi
(
√
ggij
Hj ) = 0
[ijk]
∂
∂xj
Ek = −
∂
∂t
(
√
ggij
Hj ) [ijk]
∂
∂xj
Hk =
1
c2
∂
∂t
(
√
ggij
Ej )
By comparing the two sets of equations, we find ij = µij =
√
ggij .
Light does not care. Curved space ⇔ linear medium.
Illustration: Cloak of Invisibility
In cylindrical coordinates, make transformation r → r = r−R1
R2
.
This will take origin, r = 0, and expand it into a cylinder of radius R1.
From Leonhardt’s paper
Illustration: Cloak of Invisibility
In cylindrical coordinates, make transformation r → r = r−R1
R2
.
This will take origin, r = 0, and expand it into a cylinder of radius R1.
The transformed space, r , θ , z , is a “curved” space, with spatial
metric tensor
gij =


a cos2 φ + b sin2
φ (a − b) cos φ sin φ 0
(a − b) cos φ sin φ a sin2
φ + b cos2 φ 0
0 0 1


for a = R2
R2−R1
3
and b = a r
r−R1
2
Light moving in the transformed space will not be able to reach the
area r < R1: that region is invisible.
More on Cloak of Invisibility
We take the curved space with metric tensor gij from previous slide.
We reinterpret the curved space, and insist that space is flat.
To make space flat and have same effect on light, we must also have a
linear material
ij
= µij
=
√
ggij
=


er cos2 φ + eφ sin2
φ (er − eφ) cos φ sin φ 0
(er − eφ) cos φ sin φ er sin2
φ + eφ cos2 φ 0
0 0 ez


for er = r−R1
r , eφ = r
r−R1
, and ez = R2
R2−R1
2
er .
Light will not care if we have medium , µ or curved space g
Both spaces will cause all objects in r < R1 to be invisible.
In summary...
We take a curved space describable by a metric tensor gij .
We may construct such a curved space through a transformation, but it
is gij that is important and not the transformation of space.
Using two sets of Maxwell Equations, we find a corresponding , µ.
Now we have a material that bends light in some desired way.
For the Cloak, the curvature is purely spatial; there is no need to
consider spacetime or magnetoelectric effect.
For the Mirror, exactly the same fundamental situation and
process...but in spacetime!
Invisibility cloak uses curved space with hidden region: the Mirror
uses curved spacetime with time-travel regions.
Time travel in General Relativity
This has long disturbed physicists by its refusal to be impossible.
Most succumb to “Garbage In/Garbage Out.”
The fundamental equation for General Relativity is the Einstein
Equation:
Rµν −
1
2
gµνR + Λgµν =
8πG
c4
Tµν
Relates the stress-energy density Tµν to the curvature of space in
Rα
µβν and gµν.
A particular gµν satisfying the above for a given Tµν is called a
solution.
Time travel in General Relativity
There exist solutions gµν and Tµν to the Einstein Equation that allow
for time-travel.
However: most of them require T that violate other rules of physics:
Wormholes require negative energy density
Tipler cylinders require infinitely-long cylinders
Godel space requires a slowly rotating universe, which is
empirically false
Kerr blackholes allow time travel, but only inside the event
horizon
The tools of GR very easily lend themselves to time-travel, so long as
we do not care about the physicality of Tµν or solving the Einstein
Equation...
...And we don’t!
We are not General Relativists. We are Transformation Opticians!
Therefore we propose a physically absurd spacetime that will not
solve the Einstein Equation
. .. and will not arise from a physically realistic stress-energy T
. .. but it will allow for time travel. ...on paper and in our imagination.
Transformation Optics does not care about Tµν or the Einstein
Equation, only about gµν, therefore we can turn our imagination in to
reality.
Once I’ve shown that time-travel is possible with a given gµν, we use
TO to make it real in a material
Time-Like Curves
We start with the line element,
ds2
= dx2
+ dy2
+ dz2
− c2
dt2
which is a scalar invariant quantity. Also called metric function,
metric form.
The above equation gives infinitesimal spacetime distances along a
given worldline.
In the rest frame of any massive object, dx2 + dy2 + dz2 = 0, i.e. it is
not moving.
Therefore, for a massive object, in its rest-frame, ds2 = −c2dt2 < 0.
Such a spacetime distance is called “time-like.”
A “time-like curve” is a curve on which every spacetime distance is
time-like. It is also a curve that can be followed by a massive object.
Massive objects on time-like curves perceive themselves as moving
forward in time, i.e. experience positive proper time dτ = −ds/c.
Null or Light-Like Curves
For light, dx2 + dy2 + dz2 = c2dt2.
Therefore ds2 = dx2 + dy2 + dz2 − c2dt2 = 0.
Light experiences zero spacetime displacement and zero proper time.
Any displacement ds satisfying ds = 0 is called “null” or “light-like.”
A curve is null if all displacements along it are null displacements.
All massless objects must move on null curves.
Time-like curves and null curves are both classified together as
“causal curves,” because objects traveling on them can have causal
effect on events further down the world line.
The set of all null curves originating from an event in spacetime is
called the “light cone”, defines barrier of causal region
Space-like Curves
If two events have positive spacetime displacement, ds > 0, then they
are “space-like separated”.
This designation means that there does not exist any path in spacetime
that can bring a massive object from one event to the other.
Space-like separations are non-causal. Spatial distance is too great for
even light to traverse in given time.
If massive objets could be made to travel along space-like curves
(FTL), then time travel to the past would be very simple.
The difference between causal and non-causal is often illustrated with
the light cone.
The Light Cone and Causal Structure of Spacetime
(Presenter is not professional artist.)
The Light Cone and Causal Structure of Spacetime
The Light Cone and Causal Structure of Spacetime
The Light Cone and Causal Structure of Spacetime
Making the Unphysical Physical by Curving Spacetime
The pink trajectory on the last slide is unphysical in Minkowski space
Problem is orientation of light cones — up/down.
Think of spacetime curvature as tipping over light cones.
If we curve spacetime just right, we can make the pink trajectory to be
time-like by tipping over light cones so that the path is always inside a
light cone — i.e. is always time-like
If a time-like curve crosses itself, it is a Closed Time-like Curve
(CTC); such curves allow for time-travel in to the past.
Curved Spacetime Allowing Closed Time-Like Curves
Describing Curved Spacetime
It is useful to set c = 1.
Line element ds2 = −dt2 + dx2 + dy2 + dz2 = ηαβdxαdxβ.
ηαβ =




−1 0 0 0
0 1 0 0
0 0 1 0
0 0 0 1



 −→ gαβ =




g00 g01 g02 g03
g10 g11 g12 g13
g20 g21 g22 g23
g30 g31 g32 g33




Line element ds2 = gαβdxαdxβ.
The g0i elements are what cause the light cones to tip along xi
direction.
Example of Tipped Light Cones: Alcubierre Warp-Drive
Metric function ds2 = −dt2 + (dx − v(r)dt)2 + dy2 + dz2
Almost flat. Function v(r) → 0 for r → ∞ and v(0) = vo.
Along r = 0, metric function ds2 = ds2
flat − 2vodxdt + v2
o dt2.
Last two terms are what tip light cone.
A massive object at r = 0 will have speed dx
dt = 1 + vo, which is
(globally) faster than light.
Locally, however, object moves with speed dx
dτ < 1 (i.e. is inside local
light cones).
Illustration of Alcubierre Warp-Drive
Light cones in warp-drive spacetime. Here D/T > 1 (Global FTL),
yet locally an observer that stays on thick black line (r=0) always
moves slower than light.
Closed Time-Like Curves
Here, as above, we tip the light cones, but along the angular direction.
We introduce metric form
ds2
= −dt2
+ dr2
+ dz2
+ 2f (r, φ)dφdt + r2
(1 − a/r)dφ2
.
Note simple case for dz = dt = dr = 0 and r < a: then
ds2
= r2
(1 − a/r)dφ2
< 0
This is a time-like curve: a massive object in this spacetime could
move along a curve of constant radius, height, and time.
Not useful for time travel though as curve does not traverse coordinate
time at all (dt = 0)
Illustration of Closed Time-Like Curves
(Presenter is not professional artist)
Making Closed Null Geodesics
In our case, we only care about behavior of light
Light moves on null geodesics, ds2 = 0
Note that if r = a and dr = dz = dt = 0, then
ds2
= r2
(1 − a/a)dφ2
= 0.
Not all null curves are null geodesics, seemingly in contrast to reason.
This point actually throws a slight wrench in the Mirror design...
A null geodesic satisfies
ds2
= 0 = gαβdxα
dxβ
(Null)
0 = d2
xα
+ Γα
βγdxβ
dxγ
(Geodesic)
We will need a special form of g0φ = gφ0 = f (r, φ)
...a Fly in the Ointment
The Mirror was made under the assumption that all null curves are
geodesics.
Pretend this is the case, until recalculations are made.
The primary differences will be form of trajectory, t(φ) and the
metric element gφφ = r2(1 − a/r).
Besides not being a geodesic, everything else is correct in what
follows.
This is a closed null curve that light could follow in spacetime,
resulting in time travel. Just pretend that it is also a geodesic.
Using Closed Null Curves for Time Travel
Consider the curve r = a, z = 0, t(φ) = ∆t sin2 φ
2 + to. May as well
set to = 0.
Over 0 < φ < 2π, we now have 0 < t(φ) < ∆t, and
t(0) = t(2π) = 0.
For this to be null curve, 0 = −dt2 + 2f (r, φ)dφdt.
Function f (r, φ) unspecified; set to make equation work.
Rearranging
dt
dφ
= 2f (r, φ) = ∆t sin
φ
2
cos
φ
2
.
Therefore set f (r, φ) = A(r)∆t
4 sin φ, where A(r) is the radial part.
Now the curve t(φ) = ∆t sin2 φ
2 is a null curve by definition,
traversing total time ∆t
The Null Curve
t(φ) = ∆t sin2 φ
2
Let’s Stop Here
So Far:
How Transformation Optics works in 3D, taking curved space
gab and returning material ab, µab
Illustration of 3D Transformation Optics with Invisibility Cloak
Illustration of “tipped” light cones allowing for FTL in
Alcubierre warp-drive
Illustration of null and time-like curves in spacetime
ds2 = −dt2 + dr2 + dz2 + r2(1 − a/r)dφ2 + 2fdφdt
Next Time:
How Transformation Optics works in 3+1D, using Plebanski
equations
Derivation of ab, µab, γab
1 , γab
1 from gαβ
Discussion of physical feasibility of such a medium.
And eventually everything re-worked in terms of a Closed Null
Geodesic instead of a Closed Null Curve.

More Related Content

What's hot

Kgeppt spvm 0_try1
Kgeppt spvm 0_try1Kgeppt spvm 0_try1
Kgeppt spvm 0_try1
foxtrot jp R
 
Causal Dynamical Triangulations
Causal Dynamical TriangulationsCausal Dynamical Triangulations
Causal Dynamical Triangulations
Rene García
 
Introduction to Diffusion Monte Carlo
Introduction to Diffusion Monte CarloIntroduction to Diffusion Monte Carlo
Introduction to Diffusion Monte Carlo
Claudio Attaccalite
 
Large scale coherent structures and turbulence in quasi-2D hydrodynamic models
Large scale coherent structures and turbulence in quasi-2D hydrodynamic modelsLarge scale coherent structures and turbulence in quasi-2D hydrodynamic models
Large scale coherent structures and turbulence in quasi-2D hydrodynamic modelsColm Connaughton
 
Feedback of zonal flows on Rossby-wave turbulence driven by small scale inst...
Feedback of zonal flows on  Rossby-wave turbulence driven by small scale inst...Feedback of zonal flows on  Rossby-wave turbulence driven by small scale inst...
Feedback of zonal flows on Rossby-wave turbulence driven by small scale inst...Colm Connaughton
 
Weak Isotropic three-wave turbulence, Fondation des Treilles, July 16 2010
Weak Isotropic three-wave turbulence, Fondation des Treilles, July 16 2010Weak Isotropic three-wave turbulence, Fondation des Treilles, July 16 2010
Weak Isotropic three-wave turbulence, Fondation des Treilles, July 16 2010
Colm Connaughton
 
Origin of Universe (Twin)
Origin of Universe (Twin)Origin of Universe (Twin)
Origin of Universe (Twin)
omsai_999
 
Cluster aggregation with complete collisional fragmentation
Cluster aggregation with complete collisional fragmentationCluster aggregation with complete collisional fragmentation
Cluster aggregation with complete collisional fragmentationColm Connaughton
 
Nonequilibrium statistical mechanics of cluster-cluster aggregation, School o...
Nonequilibrium statistical mechanics of cluster-cluster aggregation, School o...Nonequilibrium statistical mechanics of cluster-cluster aggregation, School o...
Nonequilibrium statistical mechanics of cluster-cluster aggregation, School o...Colm Connaughton
 
Introduction to Quantum Monte Carlo
Introduction to Quantum Monte CarloIntroduction to Quantum Monte Carlo
Introduction to Quantum Monte Carlo
Claudio Attaccalite
 
Universe (Twin)
Universe (Twin)Universe (Twin)
Universe (Twin)
omsai_999
 
Fluctuations and rare events in stochastic aggregation
Fluctuations and rare events in stochastic aggregationFluctuations and rare events in stochastic aggregation
Fluctuations and rare events in stochastic aggregation
Colm Connaughton
 
Causality in special relativity
Causality in special relativityCausality in special relativity
Causality in special relativity
Muhammad Ishaq
 
Rich Mathematical Problems in Astronomy
Rich Mathematical Problems in AstronomyRich Mathematical Problems in Astronomy
Rich Mathematical Problems in Astronomy
smiller5
 
Backreaction of hawking_radiation_on_a_gravitationally_collapsing_star_1_blac...
Backreaction of hawking_radiation_on_a_gravitationally_collapsing_star_1_blac...Backreaction of hawking_radiation_on_a_gravitationally_collapsing_star_1_blac...
Backreaction of hawking_radiation_on_a_gravitationally_collapsing_star_1_blac...
Sérgio Sacani
 
PART X.2 - Superstring Theory
PART X.2 - Superstring TheoryPART X.2 - Superstring Theory
PART X.2 - Superstring Theory
Maurice R. TREMBLAY
 
Circular and gavitational force
Circular and gavitational forceCircular and gavitational force
Circular and gavitational force
eshwar360
 
The inverse droplet coagulation problem
The inverse droplet coagulation problemThe inverse droplet coagulation problem
The inverse droplet coagulation problem
Colm Connaughton
 

What's hot (20)

Kgeppt spvm 0_try1
Kgeppt spvm 0_try1Kgeppt spvm 0_try1
Kgeppt spvm 0_try1
 
Causal Dynamical Triangulations
Causal Dynamical TriangulationsCausal Dynamical Triangulations
Causal Dynamical Triangulations
 
Introduction to Diffusion Monte Carlo
Introduction to Diffusion Monte CarloIntroduction to Diffusion Monte Carlo
Introduction to Diffusion Monte Carlo
 
Large scale coherent structures and turbulence in quasi-2D hydrodynamic models
Large scale coherent structures and turbulence in quasi-2D hydrodynamic modelsLarge scale coherent structures and turbulence in quasi-2D hydrodynamic models
Large scale coherent structures and turbulence in quasi-2D hydrodynamic models
 
Feedback of zonal flows on Rossby-wave turbulence driven by small scale inst...
Feedback of zonal flows on  Rossby-wave turbulence driven by small scale inst...Feedback of zonal flows on  Rossby-wave turbulence driven by small scale inst...
Feedback of zonal flows on Rossby-wave turbulence driven by small scale inst...
 
Weak Isotropic three-wave turbulence, Fondation des Treilles, July 16 2010
Weak Isotropic three-wave turbulence, Fondation des Treilles, July 16 2010Weak Isotropic three-wave turbulence, Fondation des Treilles, July 16 2010
Weak Isotropic three-wave turbulence, Fondation des Treilles, July 16 2010
 
Origin of Universe (Twin)
Origin of Universe (Twin)Origin of Universe (Twin)
Origin of Universe (Twin)
 
Cluster aggregation with complete collisional fragmentation
Cluster aggregation with complete collisional fragmentationCluster aggregation with complete collisional fragmentation
Cluster aggregation with complete collisional fragmentation
 
Nonequilibrium statistical mechanics of cluster-cluster aggregation, School o...
Nonequilibrium statistical mechanics of cluster-cluster aggregation, School o...Nonequilibrium statistical mechanics of cluster-cluster aggregation, School o...
Nonequilibrium statistical mechanics of cluster-cluster aggregation, School o...
 
Lec04
Lec04Lec04
Lec04
 
Introduction to Quantum Monte Carlo
Introduction to Quantum Monte CarloIntroduction to Quantum Monte Carlo
Introduction to Quantum Monte Carlo
 
Universe (Twin)
Universe (Twin)Universe (Twin)
Universe (Twin)
 
Fluctuations and rare events in stochastic aggregation
Fluctuations and rare events in stochastic aggregationFluctuations and rare events in stochastic aggregation
Fluctuations and rare events in stochastic aggregation
 
Causality in special relativity
Causality in special relativityCausality in special relativity
Causality in special relativity
 
Rich Mathematical Problems in Astronomy
Rich Mathematical Problems in AstronomyRich Mathematical Problems in Astronomy
Rich Mathematical Problems in Astronomy
 
Backreaction of hawking_radiation_on_a_gravitationally_collapsing_star_1_blac...
Backreaction of hawking_radiation_on_a_gravitationally_collapsing_star_1_blac...Backreaction of hawking_radiation_on_a_gravitationally_collapsing_star_1_blac...
Backreaction of hawking_radiation_on_a_gravitationally_collapsing_star_1_blac...
 
Wave functions
Wave functionsWave functions
Wave functions
 
PART X.2 - Superstring Theory
PART X.2 - Superstring TheoryPART X.2 - Superstring Theory
PART X.2 - Superstring Theory
 
Circular and gavitational force
Circular and gavitational forceCircular and gavitational force
Circular and gavitational force
 
The inverse droplet coagulation problem
The inverse droplet coagulation problemThe inverse droplet coagulation problem
The inverse droplet coagulation problem
 

Viewers also liked

ข่าวการศึกษา (สพฐ.) วันที่ 6 ธ.ค. 59
ข่าวการศึกษา (สพฐ.) วันที่ 6 ธ.ค. 59ข่าวการศึกษา (สพฐ.) วันที่ 6 ธ.ค. 59
ข่าวการศึกษา (สพฐ.) วันที่ 6 ธ.ค. 59
Sitthikorn Chaiwut
 
Aporte personal(r esumenes expos)
Aporte personal(r esumenes expos)Aporte personal(r esumenes expos)
Aporte personal(r esumenes expos)
Franziss Maloik
 
Giáo án sinh học 12 cơ bản
Giáo án sinh học 12 cơ bảnGiáo án sinh học 12 cơ bản
Giáo án sinh học 12 cơ bản
Con Nhok Tự Kỉ
 
ข่าวการศึกษา (สพฐ.) วันที่ 13 ธ.ค. 59
ข่าวการศึกษา (สพฐ.) วันที่ 13 ธ.ค. 59ข่าวการศึกษา (สพฐ.) วันที่ 13 ธ.ค. 59
ข่าวการศึกษา (สพฐ.) วันที่ 13 ธ.ค. 59
Sitthikorn Chaiwut
 
V2n2a02
V2n2a02V2n2a02
Ada adicional
Ada adicionalAda adicional
Ada adicional
Nishu Diaz
 
Building Ventilation
Building VentilationBuilding Ventilation
Building Ventilation
Christopher Solomon Raj G.F.S.
 
CLASE DE LITIASIS VESICULAR
CLASE DE LITIASIS VESICULARCLASE DE LITIASIS VESICULAR
CLASE DE LITIASIS VESICULAR
LUIS del Rio Diez
 
La Novela Española posterior a la Guerra Civil
La Novela Española posterior a la Guerra CivilLa Novela Española posterior a la Guerra Civil
La Novela Española posterior a la Guerra CivilRaul Espasandin
 
TRAUMA CARDÍACO PENETRANTE. EXPERIENCIA DE 4 AÑOS EN UN CENTRO DE TRAUMA DE R...
TRAUMA CARDÍACO PENETRANTE. EXPERIENCIA DE 4 AÑOS EN UN CENTRO DE TRAUMA DE R...TRAUMA CARDÍACO PENETRANTE. EXPERIENCIA DE 4 AÑOS EN UN CENTRO DE TRAUMA DE R...
TRAUMA CARDÍACO PENETRANTE. EXPERIENCIA DE 4 AÑOS EN UN CENTRO DE TRAUMA DE R...
LUIS del Rio Diez
 

Viewers also liked (11)

ข่าวการศึกษา (สพฐ.) วันที่ 6 ธ.ค. 59
ข่าวการศึกษา (สพฐ.) วันที่ 6 ธ.ค. 59ข่าวการศึกษา (สพฐ.) วันที่ 6 ธ.ค. 59
ข่าวการศึกษา (สพฐ.) วันที่ 6 ธ.ค. 59
 
Aporte personal(r esumenes expos)
Aporte personal(r esumenes expos)Aporte personal(r esumenes expos)
Aporte personal(r esumenes expos)
 
Giáo án sinh học 12 cơ bản
Giáo án sinh học 12 cơ bảnGiáo án sinh học 12 cơ bản
Giáo án sinh học 12 cơ bản
 
ข่าวการศึกษา (สพฐ.) วันที่ 13 ธ.ค. 59
ข่าวการศึกษา (สพฐ.) วันที่ 13 ธ.ค. 59ข่าวการศึกษา (สพฐ.) วันที่ 13 ธ.ค. 59
ข่าวการศึกษา (สพฐ.) วันที่ 13 ธ.ค. 59
 
V2n2a02
V2n2a02V2n2a02
V2n2a02
 
ฟอร์มหนังสือภายใน
ฟอร์มหนังสือภายในฟอร์มหนังสือภายใน
ฟอร์มหนังสือภายใน
 
Ada adicional
Ada adicionalAda adicional
Ada adicional
 
Building Ventilation
Building VentilationBuilding Ventilation
Building Ventilation
 
CLASE DE LITIASIS VESICULAR
CLASE DE LITIASIS VESICULARCLASE DE LITIASIS VESICULAR
CLASE DE LITIASIS VESICULAR
 
La Novela Española posterior a la Guerra Civil
La Novela Española posterior a la Guerra CivilLa Novela Española posterior a la Guerra Civil
La Novela Española posterior a la Guerra Civil
 
TRAUMA CARDÍACO PENETRANTE. EXPERIENCIA DE 4 AÑOS EN UN CENTRO DE TRAUMA DE R...
TRAUMA CARDÍACO PENETRANTE. EXPERIENCIA DE 4 AÑOS EN UN CENTRO DE TRAUMA DE R...TRAUMA CARDÍACO PENETRANTE. EXPERIENCIA DE 4 AÑOS EN UN CENTRO DE TRAUMA DE R...
TRAUMA CARDÍACO PENETRANTE. EXPERIENCIA DE 4 AÑOS EN UN CENTRO DE TRAUMA DE R...
 

Similar to GM

PRINCE 305FINAL113.pptx
PRINCE 305FINAL113.pptxPRINCE 305FINAL113.pptx
PRINCE 305FINAL113.pptx
SayedulHassan1
 
The klein gordon field in two-dimensional rindler space-time 2psqrd
The klein gordon field in two-dimensional rindler space-time 2psqrdThe klein gordon field in two-dimensional rindler space-time 2psqrd
The klein gordon field in two-dimensional rindler space-time 2psqrd
foxtrot jp R
 
Classical String Calculations in curved space
Classical String Calculations in curved spaceClassical String Calculations in curved space
Classical String Calculations in curved space
Ismail Abdulaziz
 
Seminar yefak 2019
Seminar yefak 2019Seminar yefak 2019
General Relativity and Cosmology
General Relativity and CosmologyGeneral Relativity and Cosmology
General Relativity and CosmologyPratik Tarafdar
 
GR.ppt
GR.pptGR.ppt
The klein gordon field in two-dimensional rindler space-time 200920ver-display
The klein gordon field in two-dimensional rindler space-time 200920ver-displayThe klein gordon field in two-dimensional rindler space-time 200920ver-display
The klein gordon field in two-dimensional rindler space-time 200920ver-display
foxtrot jp R
 
The klein gordon field in two-dimensional rindler space-time 28072020ver-drft...
The klein gordon field in two-dimensional rindler space-time 28072020ver-drft...The klein gordon field in two-dimensional rindler space-time 28072020ver-drft...
The klein gordon field in two-dimensional rindler space-time 28072020ver-drft...
foxtrot jp R
 
The klein gordon field in two-dimensional rindler space-time 14072020
The klein gordon field in two-dimensional rindler space-time  14072020The klein gordon field in two-dimensional rindler space-time  14072020
The klein gordon field in two-dimensional rindler space-time 14072020
foxtrot jp R
 
Bernard schutz gr
Bernard schutz grBernard schutz gr
Bernard schutz gr
jcklp1
 
Dr. Arpan Bhattacharyya (Indian Institute Of Science, Bangalore)
Dr. Arpan Bhattacharyya (Indian Institute Of Science, Bangalore)Dr. Arpan Bhattacharyya (Indian Institute Of Science, Bangalore)
Dr. Arpan Bhattacharyya (Indian Institute Of Science, Bangalore)
Rene Kotze
 
The klein gordon field in two-dimensional rindler space-time 23052020-sqrd
The klein gordon field in two-dimensional rindler space-time  23052020-sqrdThe klein gordon field in two-dimensional rindler space-time  23052020-sqrd
The klein gordon field in two-dimensional rindler space-time 23052020-sqrd
foxtrot jp R
 
The klein gordon field in two-dimensional rindler space-time 04232020updts
The klein gordon field in two-dimensional rindler space-time  04232020updtsThe klein gordon field in two-dimensional rindler space-time  04232020updts
The klein gordon field in two-dimensional rindler space-time 04232020updts
foxtrot jp R
 
The klein gordon field in two-dimensional rindler space-time -sqrdupdt41220
The klein gordon field in two-dimensional rindler space-time -sqrdupdt41220The klein gordon field in two-dimensional rindler space-time -sqrdupdt41220
The klein gordon field in two-dimensional rindler space-time -sqrdupdt41220
foxtrot jp R
 
The klein gordon field in two-dimensional rindler space-time 16052020
The klein gordon field in two-dimensional rindler space-time 16052020The klein gordon field in two-dimensional rindler space-time 16052020
The klein gordon field in two-dimensional rindler space-time 16052020
foxtrot jp R
 
The klein gordon field in two-dimensional rindler space-time - smcprt
The klein gordon field in two-dimensional rindler space-time - smcprtThe klein gordon field in two-dimensional rindler space-time - smcprt
The klein gordon field in two-dimensional rindler space-time - smcprt
foxtrot jp R
 
Presentation.pptx
Presentation.pptxPresentation.pptx
Presentation.pptx
GOURABSAHOO11
 

Similar to GM (20)

PRINCE 305FINAL113.pptx
PRINCE 305FINAL113.pptxPRINCE 305FINAL113.pptx
PRINCE 305FINAL113.pptx
 
FDTD Presentation
FDTD PresentationFDTD Presentation
FDTD Presentation
 
The klein gordon field in two-dimensional rindler space-time 2psqrd
The klein gordon field in two-dimensional rindler space-time 2psqrdThe klein gordon field in two-dimensional rindler space-time 2psqrd
The klein gordon field in two-dimensional rindler space-time 2psqrd
 
Classical String Calculations in curved space
Classical String Calculations in curved spaceClassical String Calculations in curved space
Classical String Calculations in curved space
 
Dark Matter
Dark MatterDark Matter
Dark Matter
 
Seminar yefak 2019
Seminar yefak 2019Seminar yefak 2019
Seminar yefak 2019
 
General Relativity and Cosmology
General Relativity and CosmologyGeneral Relativity and Cosmology
General Relativity and Cosmology
 
GR.ppt
GR.pptGR.ppt
GR.ppt
 
The klein gordon field in two-dimensional rindler space-time 200920ver-display
The klein gordon field in two-dimensional rindler space-time 200920ver-displayThe klein gordon field in two-dimensional rindler space-time 200920ver-display
The klein gordon field in two-dimensional rindler space-time 200920ver-display
 
The klein gordon field in two-dimensional rindler space-time 28072020ver-drft...
The klein gordon field in two-dimensional rindler space-time 28072020ver-drft...The klein gordon field in two-dimensional rindler space-time 28072020ver-drft...
The klein gordon field in two-dimensional rindler space-time 28072020ver-drft...
 
The klein gordon field in two-dimensional rindler space-time 14072020
The klein gordon field in two-dimensional rindler space-time  14072020The klein gordon field in two-dimensional rindler space-time  14072020
The klein gordon field in two-dimensional rindler space-time 14072020
 
Bernard schutz gr
Bernard schutz grBernard schutz gr
Bernard schutz gr
 
Dr. Arpan Bhattacharyya (Indian Institute Of Science, Bangalore)
Dr. Arpan Bhattacharyya (Indian Institute Of Science, Bangalore)Dr. Arpan Bhattacharyya (Indian Institute Of Science, Bangalore)
Dr. Arpan Bhattacharyya (Indian Institute Of Science, Bangalore)
 
Kk graviton redo.july5,2012
Kk graviton redo.july5,2012Kk graviton redo.july5,2012
Kk graviton redo.july5,2012
 
The klein gordon field in two-dimensional rindler space-time 23052020-sqrd
The klein gordon field in two-dimensional rindler space-time  23052020-sqrdThe klein gordon field in two-dimensional rindler space-time  23052020-sqrd
The klein gordon field in two-dimensional rindler space-time 23052020-sqrd
 
The klein gordon field in two-dimensional rindler space-time 04232020updts
The klein gordon field in two-dimensional rindler space-time  04232020updtsThe klein gordon field in two-dimensional rindler space-time  04232020updts
The klein gordon field in two-dimensional rindler space-time 04232020updts
 
The klein gordon field in two-dimensional rindler space-time -sqrdupdt41220
The klein gordon field in two-dimensional rindler space-time -sqrdupdt41220The klein gordon field in two-dimensional rindler space-time -sqrdupdt41220
The klein gordon field in two-dimensional rindler space-time -sqrdupdt41220
 
The klein gordon field in two-dimensional rindler space-time 16052020
The klein gordon field in two-dimensional rindler space-time 16052020The klein gordon field in two-dimensional rindler space-time 16052020
The klein gordon field in two-dimensional rindler space-time 16052020
 
The klein gordon field in two-dimensional rindler space-time - smcprt
The klein gordon field in two-dimensional rindler space-time - smcprtThe klein gordon field in two-dimensional rindler space-time - smcprt
The klein gordon field in two-dimensional rindler space-time - smcprt
 
Presentation.pptx
Presentation.pptxPresentation.pptx
Presentation.pptx
 

GM

  • 1. Galadriel’s Mirror Presentation by Reece Boston April 23, 2014
  • 2. Introduction to Galadriel’s Mirror The proposed device is predicted to allow light to travel from the future and into the past What you will see, if you leave the Mirror free to work, I cannot tell. For it shows things that were, and things that are, and things that may yet be. But which it is that he sees, even the wisest cannot always tell. Do you wish to look? — Lady Galadriel, The Lord of the Rings Begin with General Relativity, which allows for spacetimes that result in time travel. Transformation Optics: curved spacetimes −→ bi-anisotropic media Bi-anistropy: D = E + γ1H, B = µH + γ2E. We take a spacetime from GR that allows for time travel, and mimic it using TO Resultant material is Galadriel’s Mirror. Causes light to time travel.
  • 3. Review of Transformation Optics in 3D Maxwell’s Equations in a linear medium: ∂ ∂xi ( ij Ej ) = 0 ∂ ∂xi (µij Hj ) = 0 [ijk] ∂ ∂xj Ek = − ∂ ∂t (µij Hj ) [ijk] ∂ ∂xj Hk = 1 c2 ∂ ∂t ( ij Ej ) Maxwell’s Equations in curved space: ∂ ∂xi ( √ ggij Ej ) = 0 ∂ ∂xi ( √ ggij Hj ) = 0 [ijk] ∂ ∂xj Ek = − ∂ ∂t ( √ ggij Hj ) [ijk] ∂ ∂xj Hk = 1 c2 ∂ ∂t ( √ ggij Ej ) By comparing the two sets of equations, we find ij = µij = √ ggij . Light does not care. Curved space ⇔ linear medium.
  • 4. Illustration: Cloak of Invisibility In cylindrical coordinates, make transformation r → r = r−R1 R2 . This will take origin, r = 0, and expand it into a cylinder of radius R1. From Leonhardt’s paper
  • 5. Illustration: Cloak of Invisibility In cylindrical coordinates, make transformation r → r = r−R1 R2 . This will take origin, r = 0, and expand it into a cylinder of radius R1. The transformed space, r , θ , z , is a “curved” space, with spatial metric tensor gij =   a cos2 φ + b sin2 φ (a − b) cos φ sin φ 0 (a − b) cos φ sin φ a sin2 φ + b cos2 φ 0 0 0 1   for a = R2 R2−R1 3 and b = a r r−R1 2 Light moving in the transformed space will not be able to reach the area r < R1: that region is invisible.
  • 6. More on Cloak of Invisibility We take the curved space with metric tensor gij from previous slide. We reinterpret the curved space, and insist that space is flat. To make space flat and have same effect on light, we must also have a linear material ij = µij = √ ggij =   er cos2 φ + eφ sin2 φ (er − eφ) cos φ sin φ 0 (er − eφ) cos φ sin φ er sin2 φ + eφ cos2 φ 0 0 0 ez   for er = r−R1 r , eφ = r r−R1 , and ez = R2 R2−R1 2 er . Light will not care if we have medium , µ or curved space g Both spaces will cause all objects in r < R1 to be invisible.
  • 7. In summary... We take a curved space describable by a metric tensor gij . We may construct such a curved space through a transformation, but it is gij that is important and not the transformation of space. Using two sets of Maxwell Equations, we find a corresponding , µ. Now we have a material that bends light in some desired way. For the Cloak, the curvature is purely spatial; there is no need to consider spacetime or magnetoelectric effect. For the Mirror, exactly the same fundamental situation and process...but in spacetime! Invisibility cloak uses curved space with hidden region: the Mirror uses curved spacetime with time-travel regions.
  • 8. Time travel in General Relativity This has long disturbed physicists by its refusal to be impossible. Most succumb to “Garbage In/Garbage Out.” The fundamental equation for General Relativity is the Einstein Equation: Rµν − 1 2 gµνR + Λgµν = 8πG c4 Tµν Relates the stress-energy density Tµν to the curvature of space in Rα µβν and gµν. A particular gµν satisfying the above for a given Tµν is called a solution.
  • 9. Time travel in General Relativity There exist solutions gµν and Tµν to the Einstein Equation that allow for time-travel. However: most of them require T that violate other rules of physics: Wormholes require negative energy density Tipler cylinders require infinitely-long cylinders Godel space requires a slowly rotating universe, which is empirically false Kerr blackholes allow time travel, but only inside the event horizon The tools of GR very easily lend themselves to time-travel, so long as we do not care about the physicality of Tµν or solving the Einstein Equation...
  • 10. ...And we don’t! We are not General Relativists. We are Transformation Opticians! Therefore we propose a physically absurd spacetime that will not solve the Einstein Equation . .. and will not arise from a physically realistic stress-energy T . .. but it will allow for time travel. ...on paper and in our imagination. Transformation Optics does not care about Tµν or the Einstein Equation, only about gµν, therefore we can turn our imagination in to reality. Once I’ve shown that time-travel is possible with a given gµν, we use TO to make it real in a material
  • 11. Time-Like Curves We start with the line element, ds2 = dx2 + dy2 + dz2 − c2 dt2 which is a scalar invariant quantity. Also called metric function, metric form. The above equation gives infinitesimal spacetime distances along a given worldline. In the rest frame of any massive object, dx2 + dy2 + dz2 = 0, i.e. it is not moving. Therefore, for a massive object, in its rest-frame, ds2 = −c2dt2 < 0. Such a spacetime distance is called “time-like.” A “time-like curve” is a curve on which every spacetime distance is time-like. It is also a curve that can be followed by a massive object. Massive objects on time-like curves perceive themselves as moving forward in time, i.e. experience positive proper time dτ = −ds/c.
  • 12. Null or Light-Like Curves For light, dx2 + dy2 + dz2 = c2dt2. Therefore ds2 = dx2 + dy2 + dz2 − c2dt2 = 0. Light experiences zero spacetime displacement and zero proper time. Any displacement ds satisfying ds = 0 is called “null” or “light-like.” A curve is null if all displacements along it are null displacements. All massless objects must move on null curves. Time-like curves and null curves are both classified together as “causal curves,” because objects traveling on them can have causal effect on events further down the world line. The set of all null curves originating from an event in spacetime is called the “light cone”, defines barrier of causal region
  • 13. Space-like Curves If two events have positive spacetime displacement, ds > 0, then they are “space-like separated”. This designation means that there does not exist any path in spacetime that can bring a massive object from one event to the other. Space-like separations are non-causal. Spatial distance is too great for even light to traverse in given time. If massive objets could be made to travel along space-like curves (FTL), then time travel to the past would be very simple. The difference between causal and non-causal is often illustrated with the light cone.
  • 14. The Light Cone and Causal Structure of Spacetime (Presenter is not professional artist.)
  • 15. The Light Cone and Causal Structure of Spacetime
  • 16. The Light Cone and Causal Structure of Spacetime
  • 17. The Light Cone and Causal Structure of Spacetime
  • 18. Making the Unphysical Physical by Curving Spacetime The pink trajectory on the last slide is unphysical in Minkowski space Problem is orientation of light cones — up/down. Think of spacetime curvature as tipping over light cones. If we curve spacetime just right, we can make the pink trajectory to be time-like by tipping over light cones so that the path is always inside a light cone — i.e. is always time-like If a time-like curve crosses itself, it is a Closed Time-like Curve (CTC); such curves allow for time-travel in to the past.
  • 19. Curved Spacetime Allowing Closed Time-Like Curves
  • 20. Describing Curved Spacetime It is useful to set c = 1. Line element ds2 = −dt2 + dx2 + dy2 + dz2 = ηαβdxαdxβ. ηαβ =     −1 0 0 0 0 1 0 0 0 0 1 0 0 0 0 1     −→ gαβ =     g00 g01 g02 g03 g10 g11 g12 g13 g20 g21 g22 g23 g30 g31 g32 g33     Line element ds2 = gαβdxαdxβ. The g0i elements are what cause the light cones to tip along xi direction.
  • 21. Example of Tipped Light Cones: Alcubierre Warp-Drive Metric function ds2 = −dt2 + (dx − v(r)dt)2 + dy2 + dz2 Almost flat. Function v(r) → 0 for r → ∞ and v(0) = vo. Along r = 0, metric function ds2 = ds2 flat − 2vodxdt + v2 o dt2. Last two terms are what tip light cone. A massive object at r = 0 will have speed dx dt = 1 + vo, which is (globally) faster than light. Locally, however, object moves with speed dx dτ < 1 (i.e. is inside local light cones).
  • 22. Illustration of Alcubierre Warp-Drive Light cones in warp-drive spacetime. Here D/T > 1 (Global FTL), yet locally an observer that stays on thick black line (r=0) always moves slower than light.
  • 23. Closed Time-Like Curves Here, as above, we tip the light cones, but along the angular direction. We introduce metric form ds2 = −dt2 + dr2 + dz2 + 2f (r, φ)dφdt + r2 (1 − a/r)dφ2 . Note simple case for dz = dt = dr = 0 and r < a: then ds2 = r2 (1 − a/r)dφ2 < 0 This is a time-like curve: a massive object in this spacetime could move along a curve of constant radius, height, and time. Not useful for time travel though as curve does not traverse coordinate time at all (dt = 0)
  • 24. Illustration of Closed Time-Like Curves (Presenter is not professional artist)
  • 25. Making Closed Null Geodesics In our case, we only care about behavior of light Light moves on null geodesics, ds2 = 0 Note that if r = a and dr = dz = dt = 0, then ds2 = r2 (1 − a/a)dφ2 = 0. Not all null curves are null geodesics, seemingly in contrast to reason. This point actually throws a slight wrench in the Mirror design... A null geodesic satisfies ds2 = 0 = gαβdxα dxβ (Null) 0 = d2 xα + Γα βγdxβ dxγ (Geodesic) We will need a special form of g0φ = gφ0 = f (r, φ)
  • 26. ...a Fly in the Ointment The Mirror was made under the assumption that all null curves are geodesics. Pretend this is the case, until recalculations are made. The primary differences will be form of trajectory, t(φ) and the metric element gφφ = r2(1 − a/r). Besides not being a geodesic, everything else is correct in what follows. This is a closed null curve that light could follow in spacetime, resulting in time travel. Just pretend that it is also a geodesic.
  • 27. Using Closed Null Curves for Time Travel Consider the curve r = a, z = 0, t(φ) = ∆t sin2 φ 2 + to. May as well set to = 0. Over 0 < φ < 2π, we now have 0 < t(φ) < ∆t, and t(0) = t(2π) = 0. For this to be null curve, 0 = −dt2 + 2f (r, φ)dφdt. Function f (r, φ) unspecified; set to make equation work. Rearranging dt dφ = 2f (r, φ) = ∆t sin φ 2 cos φ 2 . Therefore set f (r, φ) = A(r)∆t 4 sin φ, where A(r) is the radial part. Now the curve t(φ) = ∆t sin2 φ 2 is a null curve by definition, traversing total time ∆t
  • 28. The Null Curve t(φ) = ∆t sin2 φ 2
  • 29. Let’s Stop Here So Far: How Transformation Optics works in 3D, taking curved space gab and returning material ab, µab Illustration of 3D Transformation Optics with Invisibility Cloak Illustration of “tipped” light cones allowing for FTL in Alcubierre warp-drive Illustration of null and time-like curves in spacetime ds2 = −dt2 + dr2 + dz2 + r2(1 − a/r)dφ2 + 2fdφdt Next Time: How Transformation Optics works in 3+1D, using Plebanski equations Derivation of ab, µab, γab 1 , γab 1 from gαβ Discussion of physical feasibility of such a medium. And eventually everything re-worked in terms of a Closed Null Geodesic instead of a Closed Null Curve.