by Peter Hickman
Email: peter.hickman1@ntlworld.com
ABSTRACT
In this paper, the extension of Riemann geometry to include an asymmetric metric tensor is presented. A new co-variant derivative is derived, and used in the commutator of two co-variant derivatives of a vector. This leads to two equations which describe spin 1 bosons. The energy-stress tensor arises as a contraction of the curvature tensor, its divergence enables the number of dimensions of Space-Time to be determined. A weak field approximation gives potential equations for both massless and massive bosons of at least 206.6GeV/c^2.
Affine Connection
| The invariant interval between two points on a Riemann manifold is | |
|
| 1.1 |
| Let | |
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| 1.2 |
| For the affine connection to be determined by a metric tensor only, two cases arise: | |
| Case I: The metric and affine connection are both symmetric | |
|
| 1.3 |
| With the conditions given by equation 1.2, and 1.3, the symmetric affine connection are the Christoffel Symbols, see reference [1] | |
|
| 1.4 |
| Case 2: The metric and affine connection are both asymmetric: | |
|
| 1.5 |
| With the conditions given by equation 1.2, and 1.5, the asymmetric affine connection is | |
|
| 1.6 |
| A general affine connection can be formed from equations 1.4 and 1.6 | |
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| 1.7 |
| where the imaginary part of the connection is asymmetric in m and n | |
| It can be shown that using condition 1.2 with the connection 1.7, that the affine connection is | |
| 1.8 | |
| where | |
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| 1.9 |
| the asymmetric affine connection is completely asymmetric. |
The Field Equations
| The commutator of 2 co-variant derivatives of a complex vector using 1.8 (http://homepage.ntlworld.com/peter.hickman1/page1.htm) for the affine connection gives | |
|
| 2.1 |
| where | |
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| |
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| |
| By adding | |
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| 2.2 |
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| 2.3 |
| Contracting equation 2.3 by setting n =b gives | |
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| 2.4 |
| In a geodesic frame, this reduces to | |
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| |
| and since | |
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| 2.5 |
| The vector | |
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| |
| where | |
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| 2.6 |
|
| 2.7 |
| For | |
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| |
| where I is the
6x6 unit matrix. A solution for the | |
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| |
| where the matrices
| |
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| |
| These are the
matrices for Spin 1 particles, thus the vector |
Calculation of N, dimensions of Space-Time
| The symmetric connection in equations 2.6 (http://homepage.ntlworld.com/peter.hickman1/page2.htm)and 2.7 (http://homepage.ntlworld.com/peter.hickman1/page2.htm) can be eliminated to yield | |
|
| 3.1 |
| Multiply the expression in parenthesis by hc gives the total energy E, | |
|
| 3.2 |
| where N is the number of dimensions. Contracting equation 3.2 gives G=NS, so equation 3.2 can be written as | |
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| 3.3 |
| which can be written as | |
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| 3.4 |
| compare with Einsteins field equations of gravitation with a cosmological term, see reference [1] | |
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| |
| gives | |
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| 3.5 |
| With the aid of the following identities | |
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| |
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| |
| with f=3 to N, the following expression arises when calculating the divergence of | |
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| which vanishes if (1-3/N)=3/N, gives N=6, Space-Time is 6d | |
| The divergence of equation 3.4 becomes | |
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The Weak Field Approximation
| From equation 3.6 (http://homepage.ntlworld.com/peter.hickman1/page3.htm), the equation for the current densities is | |
|
| 4.1 |
| where | |
| The weak field approximation for the asymmetric metric tensor is | |
|
| 4.2 |
| where w
is scalar field and | |
| To an approximation, equation 4.1 is | |
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| 4.3 |
| Using equation
4.2 for the asymmetric metric, applying the gauge condition
| |
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| 4.4 |
|
| |
| With w =constant, equation 4.4 reduces to the classical wave-equation. In general equations 4.4 is for interactions mediated by massive bosons. For w constant, equation 4.3 can be written in a more familiar form: | |
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| 4.5 |
| If | |
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| 4.6 |
| Maxwells equations of Electro-magnetism are obtained. see reference [3] | |
| For the special case of w =constant, equation 3.2 (http://homepage.ntlworld.com/peter.hickman1/page3.htm) is found to be, to an approximation: | |
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| |
| Compare with Einsteins field equations: see reference [1] | |
| Gives | |
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| |
| Is the energy-stress tensor of the Electro-magnetic field. see reference [3] | |
| Equations 4.3 consist of 4 sets of equations, for the index f=3 to 6. | |
| It can be shown that there are 4 'Electric' fields, given by the following equations | |
|
| 4.7a |
|
| 4.7b |
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| 4.7c |
| There are 4 'Magnetic' fields given by | |
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| Where i=1,2,3 | |
| The following identification can be made : | |
| |
Rest Mass Of Bosons
| The rest-mass of bosons depends on the scalar field w , which is determined by the following equation | |
|
| 5.1 |
| A general solution in spherical co-ordinates is | |
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| 5.2 |
| where | |
| Applying the following conditions | |
|
| |
| with l,m,n integers, gives the particular solution for w | |
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| 5.3 |
| A general time-independent solution for the potentials is | |
|
| 5.4 |
| where | |
| The integral of the 44-component of the energy-stress tensor for a Boson at rest is to an approximation with 2p r=l is | |
|
| 5.5 |
| Using Plancks
relation for the energy | |
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| 5.6 |
| Equate the gravitational
field strength | |
| Substituting for w and let l=m=n, and finally solve for E gives | |
|
| 5.7 |
| Evaluating E for n=0,1,2 gives | |
| E(0) = 4.87x10^27 eV | |
| E(1) = 3.17x10^19 eV | |
| E(2) = 206.6GeV | |
| Thus, the existence of a massive boson, of 206.6GeV is predicted. | |
The Cosmological Term
| With N=6, equation 3.5 (http://homepage.ntlworld.com/peter.hickman1/page3.htm) for the cosmological term is | |
|
| 6.1 |
| Using the Robertson-Walker metric see reference [1], the current value for the cosmological term is | |
|
| 6.2 |
| where | |
![]() | |
| For k=0, and | |
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| |
| which agrees well with observations |
Modified De Broglie Momentum Equation
| It can be shown that | |
|
| 7.1 |
|
| 7.2 |
| For | |
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| 7.3 |
| For | |
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| 7.4 |
| For r/t=c and
| |
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| 7.5 |
| Since the LHS of equation 7.5 is positive,
then | |
| Planck Length which implies particles have a maximum size of 1.6x10^-35m |