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The M/M/+M® Model

The M/M/+M®Model can predict response time components between objects that are moving at very high speeds (relativistic speeds). The M/M/+M®Model or MM+M Model (variation) predicts response time between two points based upon given information on the starting point of the two points and their velocity and direction of motion relative to a stationary observer for various What If assumptions about length contraction. The M/M/+M®Model can also be used to predict aberration of a radio signal (or aberration of starlight) due to the velocity of the receiver and the direction of the signal source relative to the direction of motion of the receiver. The M/M/+M® Model is a more accurate predictor of response time components and aberration due to relativistic speeds than competitive models such as those that are based upon Special Relativity or the Lorentz Transform. The M/M/+M®Model Version 1 Beta Test Release (V1R0) is available as a Microsoft Excel® file to qualified researcher's for research purposes at no cost and may be acquired upon request by an e-mail to ken-more@ken-more.com.

To select this topic click "M/M/+M Model" here or at the top of the page.

Relativistic Stellar Aberration

The M/M/+M® Model V2 with its Best Equations are derivatives of the M/M/+M® Model V1 and are a precise predictor of relativistic stellar aberration. The V2 Model and the Best Equations are offered as Proof of Concept. The Concept is that the Relative Response Time (RRT) Hypothesis and the algorithms of the M/M/+M® models are the most reliable predictors of relativistic phenomena that will be observed by a traveler (the Traveler) due to the Traveler's velocity within an observer's (the Observer's) inertial frame. The Proof of the Concept will show that the Best Equations and the Best Model is a more precise predictor of stellar aberration than the stellar aberation equation that was a derivative of Special Relativity Theory (1905) or the leading stellar aberration equation currently used by astronomers to predict the location of a star at a given future date and time.

To select this topic click "Stellar Aberration" here or at the top of this page. .

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