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Simplified expansion simulation with arbitrary scale factor function
Because I have a total number equal zero of my own equations to prove. You can't prove the arbitrary scale factor function and the Friedmann's a(t) is already perfectly proved. You totally can't read with comprehension. What institute gave you your degrees?
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Simplified expansion simulation with arbitrary scale factor function
I'm not your mate, pal. I can get the most accurate, explicit form of the equation for a(t) calculated from the Friedmann eq. in Lambda CDM with the most accurate density parameters and I will have the same result for my simulated observer, but you simply don't get it. Don't edit your answers after you were replied.
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Simplified expansion simulation with arbitrary scale factor function
You probably forgot to throw in the multiplication table. "Then you better show your equations if it deviates from GR you have your work cut out for you and believe me I'll be able to tell." Every possible and arbitrary but monotonically increasing function of the scale factor function will have the same result for my simulated observer and I gave the explanation. That's why my explicit form of [math]a(t)[/math] is meaningless and makes no difference.
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Simplified expansion simulation with arbitrary scale factor function
And these comoving coordinates manifest themeselves in the expanding distance between the observer and the photon that he emitted. "hence you would need a different geometry with a different flow of any measurements you take of any particles or objects around you unless you are moving with the coordinates ie fixed coordinate." My geometry is expressed by the same expanding distance and the expanding wavelenght of the photon.
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Simplified expansion simulation with arbitrary scale factor function
Can't you seriously imagine a universe with a single observer with his own reference frame, that is also the only reference frame in this universe?
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Simplified expansion simulation with arbitrary scale factor function
There is no other comoving observer in my simulation, mister. There must be at least two to be comoving.
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Simplified expansion simulation with arbitrary scale factor function
Your answer to my question should be: No, the observable universe radius has never increased with the velocity v<c. So I repeat my previous question: Mister, what exactly is moving with the relative velocity v<c in my universe with a single observer and a single photon that he emitted?
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Simplified expansion simulation with arbitrary scale factor function
Do you understand the definition of the radius of the observable universe? Has it ever increased with the velocity v<c? Don't edit your answers after you were replied.
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Simplified expansion simulation with arbitrary scale factor function
Is the blooming radius of the observable universe shorter than the distance traveled by my only photon emitted by my only observer? If it's not, then it's relative velocity can't be less than c. Is it? Don't edit your answers after you were replied.
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Simplified expansion simulation with arbitrary scale factor function
Mister, what exactly is moving with the relative velocity v<c in my universe with a single observer and a single photon that he emitted?
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Simplified expansion simulation with arbitrary scale factor function
Mister, what exactly is moving with the relative velocity v<c in my universe with a single observer and a single photon that he emitted?
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Simplified expansion simulation with arbitrary scale factor function
So you're basically saying that the cosmological horizon is like the other material observer moving with the relative velocity v<c with respect to my only observer, yes?
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Simplified expansion simulation with arbitrary scale factor function
What is contracting if there is only one observer in the expanding universe? How do you want me to apply Lorentz transformation to a single observer? My responses are not the only garbage in this thread, mister.
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Simplified expansion simulation with arbitrary scale factor function
Think about what you wrote. If it's applicable for a million observers it's also applicable for one.
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Simplified expansion simulation with arbitrary scale factor function
How many observers do you have in my simulation to apply the Lorentz transformation between them? One! Think! Don't edit your answers after you were replied.
kawiusz
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