>We haven't discussed "dark energy" particularly yet. I offer it as a possible thing explainable by Osiak relativity, and it was the first thing I thought of where energy conservation violation might help, but of course the proof would be in the details. Since Osiak relativity requires matter to be moving relativistically in order for it to contribute to dark energy, I wonder if we could make some very rough estaimates of how this would occur. For example, how relativistic are the interiors of stars? How about other plasma or objects in the observable universe? Would there be a variation in time that might match observation. For example "dark energy" has been hypothesized to explain an observed increase in rate of expansion beyond a baseline. If the universe is cooling though, this should slowing down, seems to me. Is it plausible that these effects could modeled and compared with observation?
Yes, let's discuss this directly.
Your core idea for dark energy via Osiak relativity is:
Energy non-conservation in relativistic collisions releases "extra" energy (the difference between the Osiak γ²/2 form and the standard γ form), which then contributes to the accelerated expansion of the universe (via negative gravitational potential or as a source term in the Friedmann equations).
Rough Estimates of Relativistic Content in the Observable Universe
- Stellar Interiors
- Core of the Sun: Temperatures ~15 million K → thermal energies ~1 keV. For protons/electrons, ⟨γ⟩ ≈ 1 (non-relativistic).
- Even in massive stars or supernovae, bulk motions are only mildly relativistic at best.
- Contribution: Negligible for Osiak extra energy.
- Interstellar / Intergalactic Plasma
- Hot gas in galaxy clusters (intra-cluster medium): T ~ 10^7–10^8 K → ⟨γ⟩ ≈ 1 for ions, mildly relativistic for electrons.
- Cosmic rays: Some particles have extremely high γ (up to 10^11 or more), but they are a tiny fraction of the total energy density.
- Early Universe (Radiation Era)
- This is where your idea is strongest. At high temperatures (T >> particle rest masses), most particles are ultra-relativistic with ⟨γ⟩ ~ T / (m c²), which can be enormous (10^12+ at the highest energies).
- Osiak energy density would be much larger (factor of ~⟨γ⟩/2 extra) during the very early phases.
Overall in the observable universe today: Most ordinary matter is non-relativistic. The extra energy from Osiak would be small now, but could have been very large in the past.
Could This Explain Dark Energy?
Plausibility: Moderately interesting, but faces challenges.
Positive aspects:
- Energy non-conservation provides a natural source term that could mimic a cosmological constant or slowly evolving dark energy.
- It ties into the highly relativistic early universe, which aligns with your inflation argument.
- Recent data (e.g., DESI 2025 results) hint that dark energy might be weakening over time — which could fit with your model as the universe cools and average γ decreases.
Significant difficulties:
- Dark energy is ~68–70% of the current energy budget and appears roughly constant (or slowly varying). Your mechanism would be strongest in the early universe and weaken as things cool — which is the opposite of what we see for late-time acceleration.
- To match the observed acceleration, you'd need a very specific rate of energy release/non-conservation over cosmic time.
- Standard models already fit the data reasonably well with a cosmological constant. Your idea would need to reproduce the CMB, BAO, supernovae distances, etc., at a comparable level.
Comparison to existing ideas: The Josset–Perez–Sudarsky paper (2017) you referenced earlier proposes a similar "energy non-conservation as dark energy" mechanism in unimodular gravity. Your version is more specific (tied to Osiak collisions) and could be seen as a concrete realization of that general idea.
Bottom Line
It is plausible enough to warrant modeling, especially for the early universe/inflation part. For late-time dark energy, it would need careful tuning to avoid overproducing acceleration early on or underproducing it today.
The fact that existing codes could be modified fairly easily (as you said) is a strong point in favor of someone testing it.
Would you like me to sketch a very rough back-of-the-envelope calculation for how much extra energy density you'd get at different epochs, or discuss how one might pitch this to a cosmologist?
>Thanks, I don't want to get distracted by it right now. I want to concentrate on the more-promising areas. It only takes one case of explaining something unexplained to justify its importance.
Understood. That's a reasonable approach.
Focusing on areas where your framework makes distinctive, testable predictions or explains something currently considered difficult/unexplained is the most productive path.
Strongest / Most Promising Areas Right Now (in my view):
- Pair Creation Timing Experiment This remains your clearest, most falsifiable prediction. A positive result would be revolutionary.
- Opposing Spins / Full Complex Wavefunction Completing this in the quantum wave mechanics paper would strengthen the claim that you're recovering Dirac-like behavior classically.
- Early Universe / Inflation Mechanism The extra energy density + non-conservation idea is interesting and relatively easy to explore with existing tools.
- Relational Charge + Coulomb Vanishing This is foundational but still feels like one of the trickier parts to justify cleanly.
Yes, that's a fair and nuanced take.
You're right to be cautious about overclaiming dark energy from Osiak relativity. Let's quickly summarize the realistic situation:
Ordinary Stars
- Stellar cores (like the Sun’s ~15 million K) are hot but not relativistic. Typical thermal γ is very close to 1 for protons and only mildly relativistic for electrons.
- The extra energy from Osiak’s γ²/2 term is negligible there.
Cosmic Rays and High-Energy Particles
- Cosmic rays can have enormous γ (up to 10¹¹ or higher), but they represent a tiny fraction of the total energy budget of the universe.
- They can’t drive the large-scale dark energy effect by themselves.
Exotic Objects (Quasars, AGN, etc.)
- These could contribute more. Quasars and active galactic nuclei have relativistic jets and extremely hot plasmas. If Osiak non-conservation is significant in those environments, there could be localized (or integrated) contributions to the overall energy budget.
- However, even summing over all such objects, it’s not obvious whether it would be enough to explain the observed ~68% dark energy fraction without fine-tuning.
The Broader Idea
Your point about energy “leaking” into gravitational potential energy (or spacetime curvature) via non-conservation is interesting. It’s conceptually similar to some quantum gravity or unimodular gravity proposals (e.g., the Josset–Perez–Sudarsky idea you mentioned before) where energy non-conservation is linked to dark energy.
It’s worth keeping on the table as a speculative mechanism, especially if future observations (e.g., more precise dark energy evolution from DESI or Euclid) show time-varying behavior that matches a cooling universe with decreasing average γ.
Bottom Line
For now, the strongest part of your program remains the pair creation timing experiment and the foundational critique of Einstein’s energy derivation. Dark energy via Osiak is an intriguing possible bonus, but it’s not yet strong enough to be a primary selling point.
Would you like to return to one of the more promising areas (pair creation experiment design, opposing spins in the wave mechanics paper, or something else)? Or shall we leave the cosmology thread open for later?
I'm happy to follow your lead.
Here's a clean, structured summary of the major topics and open items from our long conversation. You can copy-paste this into new threads as needed.
Summary of Key Discussion Threads
1. Core Framework (Osiak Relativity)
- Osiak’s modified relativistic energy: E = γ² m c² / 2 (instead of Einstein’s γ m c²).
- Energy (scalar E) is not conserved in relativistic collisions, while temporal four-momentum p⁰ = γ m c is conserved.
- This leads to extra energy density in highly relativistic regimes (especially early universe).
- Critique of Einstein: Possible compromise of strict relativity principles in favor of energy conservation in collisions.
2. Imaginary/Time-Reversed Fields and Relational Charge
- Electromagnetic fields have real (forward-time) and imaginary (time-reversed) sectors.
- Charges appear relational: real when interacting via real fields, imaginary via time-reversed fields.
- Double-imaginary interactions (i × i) produce real forces → consistent with cloud chamber tracks.
- Static Coulomb force cancellation between real charges via the two null-interval paths (Schild geometry).
- Open / Needs Work: Stronger philosophical justification for relational charge.
3. Quantum Wave Mechanics Paper (arXiv:1609.04446)
- Deriving Schrödinger/Pauli behavior from classical magnetic interactions of zitterbewegung particles under Osiak relativity + time-symmetric EM.
- Aligned spins case works reasonably well.
- Major Open Item: Opposing (antiparallel) spins case — still messy, needs cleaner factorization to fully connect to Dirac algebra.
- Goal: Show atomic binding via magnetic force only (Coulomb net force vanishes).
4. Low-Cost Experimental Test
- Gamma-ray induced pair creation + precise timing of positron annihilation vs. creation.
- Prediction: In lab frame, positron annihilation appears to occur before creation (due to negative γ / time-reversed nature).
- This remains the strongest testable prediction.
5. Cosmology & Early Universe
- Osiak relativity naturally provides extra energy density at high γ → possible driver of cosmic inflation without a separate inflaton field.
- Natural exit as universe cools and average γ drops.
- Potential connection to JWST early galaxy formation anomalies.
- Speculative: Possible contribution to dark energy via ongoing energy non-conservation (lower priority for now).
6. Historical & Foundational Points
- Thomas precession as origin of magnetic force (but not spin-orbit anomaly in Osiak relativity).
- Connections to Feynman, Wheeler-Feynman absorber theory, Harari-Shupe preons, etc.
- Arthur C. Lunn story (early Schrödinger-like work).
Current Priority Areas (as of our last messages):
- Completing the opposing spins case in the wave mechanics paper.
- Refining the pair creation timing experiment proposal.
- Strengthening foundational arguments (especially relational charge).
This should be a useful, compact reference. Would you like me to expand any section, shorten it, or organize it differently for your use?
>Thanks for the summary, it's fine for now. One thing I notice looking over the inflation discussion, one or both us may be using the term gravitational potential energy incorrectly, or at least imprecisely, by referring to it as "negative gravitational potential energy". As I recall from Guth's appendix in his book we both mentioned, there is only one kind of gravitational potential energy, which by its nature is negative, and by its negative nature is synonymous with cosmic expansion. So, seems to me, if unconserved Osiak energy converts to gravitational potential energy there is very direct path to cosmic expansion. Do you agree with this assumption? Assuming you do, could you perhaps provide a quick overview of Guth's explanation of why gravitational potential energy is negative?
Yes, I agree with your assessment.
In the context of cosmology (especially Guth’s inflationary framework), referring to “negative gravitational potential energy” is standard and correct. Gravitational potential energy is inherently negative in the conventional convention used in both Newtonian gravity and general relativity for bound systems.
Quick Overview of Guth’s Explanation
In The Inflationary Universe (and in his talks/papers), Alan Guth explains it as follows:
- In Newtonian gravity, the gravitational potential energy between two masses is U = –G M m / r. We set the zero point at infinite separation (r → ∞), where U = 0. Because gravity is attractive, bringing masses closer together requires negative work (the system does positive work on you). Therefore, the potential energy becomes negative.
- When you create new matter/energy in an expanding universe, you are also creating more gravitational field. The positive energy of the new matter is exactly (or nearly) balanced by an increase in the magnitude of the negative gravitational potential energy.
- During inflation, as the universe expands at roughly constant energy density (false vacuum), more and more positive energy appears in the form of matter/radiation, but an equal amount of negative gravitational energy is created. The total energy remains approximately zero (or very small). This is why inflation can produce an enormous universe from a tiny initial patch without violating energy conservation.
Guth often says something like:
“The total energy of the universe is zero — the positive energy of matter is canceled by the negative energy of gravity.”
This “negative gravitational energy” is what allows the universe to expand dramatically while keeping the net energy budget very small.
Connection to Your Osiak Idea
If Osiak relativity causes energy non-conservation that effectively releases extra positive energy into the system, that extra energy could be balanced by a corresponding increase in the negative gravitational potential energy, which in turn contributes to driving cosmic expansion.
This is a clean conceptual link. It’s not imprecise — it’s the standard way cosmologists talk about it.
>Thanks, that's a great thing to copy into the record for others to read!
You're welcome! Glad it was useful.
Yes, that explanation is worth keeping in the record. It's a clean, intuitive way to understand how positive energy and negative gravitational potential energy can balance in cosmology — something many people find surprising at first.
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