Foundation for the Mass Scaling Upgrade and Ramanujan Inspired p series Deformation
Authors/Creators
Description
This paper is the first of two protocols that collectively build a complete theory of modified gravity based on Ramanujan's p-series. Protocol 1 focuses exclusively on the field-theoretic foundation of the deformation kernel.
Key Results:
1. 5D Warped Geometry: The theory is formulated in a 5D anti-de Sitter (AdS_5) bulk with a warped extra dimension, bounded by a UV brane at z=0 and an IR brane at z=R_0.
2. Action Principle: A bulk scalar field Psi(x,z) is coupled to a 4D gravitational potential phi(x) on the UV brane. The action is explicitly written and varied.
3. KK Decomposition: Separation of variables leads to a Bessel equation for the extra-dimensional wavefunctions. Boundary conditions (Neumann at UV, Dirichlet at IR) quantize the KK spectrum to mu_n = n divided by R_0.
4. Effective Potential: The static gravitational potential is proportional to (1/R) times the sum over n of (n/R_0) to the power (p-2) times e to the power (-nR/R_0).
5. Poisson Resummation: The discrete sum is exactly evaluated to obtain the normalized deformation kernel: K_p(R) = zeta(p, 1 + R/R_0) divided by zeta(p).
6. UV Regularization: The R=0 singularity is resolved by introducing a UV cutoff r_0. The regularized potential is Phi_reg(R) = -GM divided by the square root of (R squared plus r_0 squared) times K_p of (square root of (R squared plus r_0 squared) divided by R_0). The potential becomes finite at the origin.
7. Regge-Wheeler Perturbations: Axial gravitational perturbations with angular momentum l=2 are analyzed. The effective potential is derived, and the shift in the quasinormal mode frequency is computed using third-order WKB: delta omega over omega is approximately equal to negative one-ninth times (r_0 divided by R_s) squared.
8. LIGO-Virgo Constraint: From GW150914, the bound |delta omega / omega| is less than or equal to 0.015 gives: r_0 is less than or equal to 0.367 times R_s.
9. Dynamical Scaling of r_0: To avoid low-mass black hole conflicts (such as GW230529), r_0 scales with the Planck length: r_0(M) = (Planck length squared times R_s) to the one-third power, which is proportional to M to the one-third power. This yields r_0 approximately 10 to the power -21 meters for stellar-mass black holes, satisfying all experimental bounds.
Included Material:
· Full derivations of all equations (no steps skipped)
· Python code for WKB frequency shift calculation
· Complete bibliography with 7 references
· Summary tables of boundary conditions, quantization, and resolved critiques
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Ramanujan p series Deformation foundation.pdf
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Additional details
References
- S. Ramanujan, Collected Papers of Srinivasa Ramanujan, Cambridge University Press, Cambridge (1927).
- G. H. Hardy, Ramanujan: Twelve Lectures on Subjects Suggested by His Life and Work, Cambridge University Press, Cambridge (1940).
- E. T. Whittaker and G. N. Watson, A Course of Modern Analysis, 4th ed., Cambridge University Press, Cambridge (1927)
- N. N. Lebedev, Special Functions and Their Applications, Dover Publications, New York (1972)
- E. C. Titchmarsh, The Theory of the Riemann Zeta-Function, 2nd ed., Oxford University Press, Oxford (1986)
- M. Abramowitz and I. A. Stegun (eds.), Handbook of Mathematical Functions, National Bureau of Standards, Washington DC (1964)
- S. Chandrasekhar, An Introduction to the Study of Stellar Structure, Dover Publications, New York (1957)
- Vallado, D. A. (2013). Fundamentals of Astrodynamics and Applications (4th ed.). Microcosm Press and Springer.
- Battin, R. H. (1999). An Introduction to the Mathematics and Methods of Astrodynamics. American Institute of Aeronautics and Astronautics.
- Montenbruck, O., & Gill, E. (2000). Satellite Orbits: Models, Methods, and Applications. Springer.
- Curtis, H. D. (2014). Orbital Mechanics for Engineering Students (3rd ed.). Elsevier Butterworth-Heinemann.
- Prussing, J. E., & Conway, B. A. (2012). Orbital Mechanics (2nd ed.). Oxford University Press.
- Schaub, H., & Junkins, J. L. (2018). Analytical Mechanics of Space Systems (4th ed.). American Institute of Aeronautics and Astronautics.
- Hairer, E., Nørsett, S. P., & Wanner, G. (1993). Solving Ordinary Differential Equations I: Nonstiff Problems. Springer.
- Tapley, B. D., Schutz, B. E., & Born, G. H. (2004). Statistical Orbit Determination. Elsevier Academic Press.
- Montgomery, R., Marsden, J., & Ratiu, T. (2006). Mathematical Methods of Classical Mechanics. Springer.
- Virtanen, P. et al. (2020). SciPy 1.0: Fundamental Algorithms for Scientific Computing in Python. Nature Methods, 17, 261–272.
- Harris, C. R. et al. (2020). Array Programming with NumPy. Nature, 585, 357–362.