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How generalized Minkowski four-force
leads to scalar-tensor gravity
György SzondyLogic, Relativity and Beyond
2nd International ConferenceAugust 9-13 2015, Budapest
LRB15 - Szondy: Scalar-Tensor Gravity 2
Theories of Gravitation
http://en.wikipedia.org/wiki/History_of_gravitational_theory
~50 alternatives and
extensions
A lot of results in addition to GR2015.08.09.
LRB15 - Szondy: Scalar-Tensor Gravity 3
• Special Relativity and Minkowski four-force
• Scalar-Tensor Gravity
• Quantum effects (causing this Scalar field)
Topics
2015.08.09.
LRB15 - Szondy: Scalar-Tensor Gravity 4
Minkowski (four)-force
P2
𝑭⊥𝒑↔𝐹 𝑖𝑝𝑖=0
𝑚0=√𝐸2−𝑝2
Special case
proper time m0
𝑐=1
REST MASS is INVARIANT
t
x
𝑭=𝑚𝒂=𝑚𝑑𝒖𝑑𝜏
=𝑑𝒑𝑑𝜏
FF
F
2015.08.09.
orthogonal
𝑎𝑖𝑢𝑖=0↔𝒂⊥𝒖𝒂=
𝑑𝒖𝑑𝜏
LRB15 - Szondy: Scalar-Tensor Gravity 5
Generalized minkowski-force
m1
m2
F
Károly Novobátzky in the ´50s
General 4-force might change rest mass
t
x
𝐹 𝑖𝑝𝑖≠0
𝑭=𝑑𝒑𝑑𝜏
=𝑑 (𝑚𝒖)𝑑𝜏
=𝑚 𝑑𝒖𝑑𝜏
+𝒖 𝑑𝑚𝑑𝜏
𝑭=𝐹⊥+𝐹∥
𝑚 (𝑥 )=𝑚0+𝜙 (𝒙 )
𝑭 ∥
𝑭⊥
Similar to Higgs-field
𝜙𝑝 (𝒙 )≠𝜙𝑒 (𝒙 )
2015.08.09.
6
𝐸=𝑚0𝑐
2
√1− 𝑣2𝑐2
Static gravitational field
m1m2
FE = const
(Brans & Dicke 1961)
𝐸=𝑚0𝑐
2√𝑔00
√1− 𝑣2𝑐2
𝑚 (𝑥 )=𝑚0√𝑔00
Scalar-tensor gravity
t
x
0=𝛿∫𝑚 √(𝑔𝑖𝑗𝑢𝑖𝑢 𝑗 )𝑑𝑠𝑑 (𝑚𝑢𝑖)𝑑𝑠
−12𝑚𝑔 𝑗𝑘 ,𝑖𝑢
𝑗𝑢𝑘−𝑚,𝑖=0
LRB15 - Szondy: Scalar-Tensor Gravity
𝐸=𝑚 (𝑥 )𝑐2
√1− 𝑣2𝑐2
𝑚(𝑥)=𝑚0 𝑓 (𝑥)
2015.08.09.
7
𝐸=𝑚0𝑐
2
√1− 𝑣2𝑐2
Static gravitational field - remarks
(Brans & Dicke 1961)
𝐸=𝑚0𝑐
2√𝑔00
√1− 𝑣2𝑐2
𝑚 (𝑥 )=𝑚0√𝑔00
Exact transformation between STG & GR
0=𝛿∫𝑚 √(𝑔𝑖𝑗𝑢𝑖𝑢 𝑗 )𝑑𝑠𝑑 (𝑚𝑢𝑖)𝑑𝑠
−12𝑚𝑔 𝑗𝑘 ,𝑖𝑢
𝑗𝑢𝑘−𝑚,𝑖=0
LRB15 - Szondy: Scalar-Tensor Gravity
𝐸=𝑚 (𝑥 )𝑐2
√1− 𝑣2𝑐2
2015.08.09.
1. Light has no rest- mass same as GR
2. represents the Newtonian gravitational force.
3. Mercury perihelion advance can be calculated from the curvature effects
4. B&D in they original paper insisted on the constancy of rest mass, and used conform transformation to transform their result back to GR and tried to vary the gravitational constant
LRB15 - Szondy: Scalar-Tensor Gravity 8
Conformal transformation applied by Brans & Dicke
Scalar-Tensor theory:
Conformal transformation : 𝑔𝑖𝑗= 𝑓2g𝑖𝑗
𝑑𝑠2= 𝑓 2d 𝑠2 , 𝑢𝑖= 𝑓 − 1𝑢𝑖
Getting back General Relativistic equation of motion:
𝑚 (𝑥 )= 𝑓 (𝑥 )𝑚0
𝑚=𝑐𝑜𝑛𝑠𝑡
2015.08.09.
𝑑 (𝑚𝑢𝑖)𝑑𝑠
−12𝑚𝑔 𝑗𝑘 ,𝑖𝑢
𝑗𝑢𝑘−𝑚,𝑖=0
We use the results of GR in STG
LRB15 - Szondy: Scalar-Tensor Gravity 9
How to transform Schwarzscild solution to Scalar-Tensor gravity
Schwarschild solution uses standard coordinates
Isotropic coordinates
)sin()()( 2222222 ddrdrrBdtrAds
)sin)((')(' 22222222 dddBdtAds
2)4
1(
srr
2015.08.09.
𝑔𝑖𝑗= 𝑓2g𝑖𝑗
Coordinatetransformation
)sin(4
1
41
41
222222
4
2
2
2
ddd
rdt
r
r
ds g
g
g
Schwarzschild metric:
LRB15 - Szondy: Scalar-Tensor Gravity 10
Understanding Schwarzscild metric
0.5 1 1.5 2rg1
2
3
4
5
rrg𝑟 /𝑟 𝑠
𝜌 /𝑟 𝑠Event horizon
stan
dard
isotropic
2)4
1(
srr
… in isotropic coordinates
-5-2.5
0
2.5
5
-5
-2.5
0
2.55
-4
-2
0
2
4
-5-2.5
0
2.5
5
-5
-2.5
0
2.55
Einstein-Rosen bridge
2015.08.09.
LRB15 - Szondy: Scalar-Tensor Gravity 11
Scalar field - Coordinate independent?g00 in isotropic coordinates
(gravitational potential)
0.5 1 1.5 2rg0.2
0.4
0.6
0.8
1
g00
0.5 1 1.5 2
0.2
0.4
0.6
0.8
1
1.2
R
Rest mass depends on Ricci scalar
𝒈𝟎𝟎=𝟏−𝟒√ 𝟐𝟑 (−𝑹)
𝒎 (𝒙 )=𝒎𝟎√𝒈𝟎𝟎
𝒎 (𝒙 )=𝒎𝟎√𝟏−𝟒√ 𝟐𝟑 (−𝑹 (𝒙))
√−𝑅𝑔00
𝑟 /𝑟 𝑠𝑟 /𝑟 𝑠
Ricci scalar in isotropic coords (after conformal transformation)
2015.08.09.
LRB15 - Szondy: Scalar-Tensor Gravity 12
How can curvature effect Rest-Mass?Particle model from caracteristic lengths
Different possible particles
0.5 1 1.5 2m
2
4
6
r
2
2
c
Gmrs
mc
hkkr ComptonQ
22
Schwarzschild-radius
Quantum-radius
Rest-mass and size depends on ‚k’ quantum number
2015.08.09.
LRB15 - Szondy: Scalar-Tensor Gravity 13
How can background-curvature effect Rest-Mass?
Particle model from caracteristic lengths
is different for p+ and e– 𝑚=𝑚0𝑠 (𝑟𝑝 ,𝑅𝑈)
𝑚(𝑞) /𝑚0
𝑞=𝑟𝑝𝑎𝑟𝑡𝑖𝑐𝑙𝑒 /𝑅𝑈𝑛𝑖𝑣𝑒𝑟𝑠𝑒
𝑞=𝑟𝑝𝑎𝑟𝑡𝑖𝑐𝑙𝑒 /𝑅𝑈𝑛𝑖𝑣𝑒𝑟𝑠𝑒
Background curvature
Modified Schwarzschild-radius
𝑟 𝑠 (𝑞 )=1−√1−16𝐺𝑚𝑞𝑐2
4𝑞
G might be different for different particles?2015.08.09.
LRB15 - Szondy: Scalar-Tensor Gravity 14
Conclusion
• General force field can change rest mass• In scalar-tensor gravity Newtonian gravity and
curvature-effects are seperated• Background curvature changes rest mass• Rest mass change are due to quantum effects• Gravitational constant is different for different
elementary particles
There is a lot to do2015.08.09.
LRB15 - Szondy: Scalar-Tensor Gravity 15
References1. Gy. Szondy, A Pure Geometric Approach to Derive Quantum Gravity from
General Relativity; viXra:1312.0222 (2013)2. Gy. David, Lecture 2011.04.27, https://www.youtube.com (Novobatzky)3. C. Brans and R. H. Dicke, Mach's Principle and a Relativistic Theory of
Gravitation, Phys. Rev. D 124 925-935 1961 4. Gy. Szondy, Linear Relativity as a Result of Unit Transformation,
arXiv:physics/0109038 (2001) 5. Gy. Szondy, Mathematical Equivalency of the Ether Based Gavitation
Theory of Janossy and General Relativity, arXiv:gr-qc/0310108
2015.08.09.