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Computer Systems Engineer with over 30 years experience in Computer Performance Evaluation (CPE) and Mathematical Modeling, Retired. I am interested in knowing if Special Relativity Theory (SRT) can be used to reliably predict the performance of network elements (computer platforms) that are traveling at relativistic speeds with respects to our Local Group of about one million stars. At this point, I am interested in developing a mathematical model that can reliably predict performance metrics such as response time (one way transmission time as well as end-to-end response time) between two platforms moving at relativistic speeds with respects to an Observer (CPE Analyst) who is "stationary" with respects to the stars in our Local Group of stars. I am not interested in modeling the effects of gravity fields. I want to "keep it simple" and predict response times between two platforms that are far enough from massive objects that reliable performance predictions can be made as a function of relative velocity only.
'''Ken Moore''' is an American computer systems engineer, based in Kensington, Maryland. Now retired, he spent more than 30 years working in the fields of Computer Performance Evaluation (CPE) and mathematical modeling. He is known within the dissident-science community for his work applying performance-modeling techniques to questions in [[Relativity]].
 
==Biography==
 
Moore worked as a computer systems engineer for over 30 years, specializing in Computer Performance Evaluation (CPE) and mathematical modeling. He is now retired and resides in Kensington, Maryland, United States.
 
==Work==
 
Moore's principal research interest concerns whether Special Relativity Theory (SRT) can be used to reliably predict the performance of network elements (computer platforms) travelling at relativistic speeds relative to the Local Group of roughly one million stars. He has sought to develop a mathematical model capable of predicting performance metrics such as response time, including both one-way transmission time and end-to-end response time, between two platforms moving at relativistic speeds relative to an observer (a CPE analyst) who is stationary with respect to the stars of the Local Group.
 
Moore's approach deliberately excludes the modeling of gravitational fields. His stated aim is to keep the problem simple by predicting response times between two platforms that are sufficiently distant from massive objects that reliable performance predictions can be made as a function of relative velocity alone.


==Abstracts==
==Abstracts==


* 2011 - "[[The Best Stellar Aberration Model]]" ([http://www.naturalphilosophy.org/pdf/abstracts/abstracts_5983.pdf Read in full])
* 2011 - "[[The Best Stellar Aberration Model]]" ([http://www.naturalphilosophy.org/pdf/abstracts/abstracts_5983.pdf Read in full])
==External links==
* [http://www.naturalphilosophy.org/pdf/abstracts/abstracts_5983.pdf "The Best Stellar Aberration Model" (2011 abstract)]


[[Category:Scientist|Moore Kenneth]]
[[Category:Scientist|Moore Kenneth]]
[[Category:Worldwide List of Dissident Scientists]]

Latest revision as of 16:23, 17 July 2026

Ken Moore
Ken Moore
ResidenceKensington, MD, United States
NationalityUSA
Known forRelativity
Scientific career
FieldsComputer Systems Engineer

Ken Moore is an American computer systems engineer, based in Kensington, Maryland. Now retired, he spent more than 30 years working in the fields of Computer Performance Evaluation (CPE) and mathematical modeling. He is known within the dissident-science community for his work applying performance-modeling techniques to questions in Relativity.

Biography

Moore worked as a computer systems engineer for over 30 years, specializing in Computer Performance Evaluation (CPE) and mathematical modeling. He is now retired and resides in Kensington, Maryland, United States.

Work

Moore's principal research interest concerns whether Special Relativity Theory (SRT) can be used to reliably predict the performance of network elements (computer platforms) travelling at relativistic speeds relative to the Local Group of roughly one million stars. He has sought to develop a mathematical model capable of predicting performance metrics such as response time, including both one-way transmission time and end-to-end response time, between two platforms moving at relativistic speeds relative to an observer (a CPE analyst) who is stationary with respect to the stars of the Local Group.

Moore's approach deliberately excludes the modeling of gravitational fields. His stated aim is to keep the problem simple by predicting response times between two platforms that are sufficiently distant from massive objects that reliable performance predictions can be made as a function of relative velocity alone.

Abstracts

External links