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Homework Statement
Just basically want to see if my algebra is ok.
Homework Equations
All are relevent.
The Attempt at a Solution
Calculating Rates in Magnetic Moments to Predict Period Interaction Between a Fermion and the Zero-Point Field
First we must identify the net magnetization \vec{M} as the sum of individual magnetic moments [1],
1. \vec{M}= \sum^{N}_{i=1} \vec{\mu}_i
The magnetic moment \vec{\mu}_i is a magnitude of the constant expression of \frac{e \hbar}{2Mc}. If these equations where pertaining to a spinor field \psi (or simply an electron) then the electron in a certain magnitude of magnetic moments act like a clock to potentially absorb a photon at an energy of \frac{e^2 h}{4Mc} [2] from the ZPF (zero-point field) which would imply an interaction term. Using the algebra of a limiting vector on the classical vector component \vec{\mu}_i then we would find the upper bound at the squared value of 15MeV.
Taking the dot product between the magnetic moment (the sum of the magnetization field \vec{M} which should not be mistaken for a mass, or the magnetic moment identity in the equation F= \nabla(M \cdot B) where here M is the magnetic moment) and the magnetic field B of Equation 1. we have:
2. F= \nabla(\vec{M} \cdot B)= \nabla(\sum^{N}_{i=1} \vec{\mu}_i \cdot B)
which implies also that
3. \nabla(\sum^{N}_{i=1} \vec{\mu}_i \cdot B)= \nabla(MBcos \theta)
The force here can now be viewed in terms of a Lorentz force where the charge is seen in terms of magnetism. This can be seen in a simple substitution:
4. \nabla(\sum^{N}_{i=1} (\vec{\mu}_i \cdot B)= (\oint (B -\mu_0M) \cdot \partial \mathbf{A})v \times B
where \mu_0 is the permeability.
= q_Mv \times B
Which would imply a force due to magnetism F_M, where q_M is the magnetic charge. Since the sum of magnetic moments calculate the exact absorption rate of photons when electrons have an energy of \frac{e^2h}{4Mc} then the magnetization can be seen as giving rise to the interaction between the electron and the zero point field - remember, the magnetization is the sum of the magnetic moments, and the magnetic moment is a magnitude of one half less than that required for zero-point energy absorption. The rate in which an electron may obtain an upper bound of energy at hf=15MeV and their respective Magnetizations should be investigated as possible co-roles.
The magnetization field has an energy, as do all quantum fields in a vacuum, and small perturbations as would be expected from a model of an electron with an absorption rate for photon in the ZPF-connection can be seen in terms of the work of the field and the H-Field as \delta W= H \cdot \delta B, so trivially substituting this into our equations we can have:
\delta W = H \cdot \delta B = \nabla(\sum^{N}_{i=1} \vec{\mu}_i \cdot B)vt
Where we have multiplied the quantity of vt on both sides to give the appropriate dimensions.
Ref.
http://www.pma.caltech.edu/~ph77/labs/nmr.pdf
http://books.google.co.uk/books?id=...t energy contribute to a hamiltonian?&f=false
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