Q&A on Gravitational Dynamics, Cosmic Structures, Magnetic Fields, and High-Energy Phenomena in Extended Classical Mechanics

Extended Classical Mechanics

This comprehensive Q&A session delves into the intricacies of extended classical mechanics, exploring its unique approach to gravitational dynamics, cosmic structures, magnetic fields, and high-energy phenomena. The discussion addresses critical questions on how this framework reinterprets the formation and evolution of galaxy clusters, cosmic magnetic fields, and the behaviour of quasars and blazars. It also examines the implications of effective mass, magneto-hydrodynamics, and gravitational interactions on the large-scale structure of the universe. By integrating principles of classical physics with modern insights, this analysis provides a fresh perspective on the fundamental processes shaping the cosmos.

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1. How does this extended classical mechanics framework address the cosmological constant's

2. Can this extended classical mechanics framework be applied to quantum systems?

3. What evidence supports the negative effective mass concept in extended classical mechanics?

4. How does extended classical mechanics accommodate the observed isotropy and homogeneity of the universe on large scales?

5. Can the negative effective mass concept be applied to explain specific astrophysical phenomena, such as galaxy rotation curves or gravitational lensing?

6. How does extended classical mechanics address the issue of singularity and black hole physics?

7. How does extended classical mechanics predict the behaviour of gravitational waves in the context of binary black hole mergers?

8. Can the framework explain the observed baryon acoustic oscillations (BAOs) in the large-scale structure of the universe?

9. How does extended classical mechanics address the cosmological horizon problem?

10. How does extended classical mechanics predict the behaviour of cosmological perturbations and their impact on structure formation?

11. Can the framework explain the observed properties of fast radio bursts (FRBs) and gamma-ray bursts (GRBs)?

12. How does extended classical mechanics address the issue of cosmic magnetic fields and their role in structure formation?

13. Can the framework explain the observed properties of blazars and active galactic nuclei (AGN)?

14. How does extended classical mechanics predict the behaviour of galaxy clusters and super clusters?

15. Can the framework explain the observed properties of quasars and their redshift distributions?

16. How does extended classical mechanics address the cosmic microwave background (CMB) radiation and its fluctuations?

Keywords: Gravitational Dynamics, Cosmic Structures, Magnetic Fields, High-Energy Phenomena, Mass-Energy Interactions

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