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| Tags: derivation, dopplershifts, energymomentumrelation, equipped, equivalence, formula, galilean, massenergy, relativity, rule, specific, under |
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#1
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In this approach, nonsensical meta-phenomena like
time dilation and length contraction, along with other SR's badly-resolved paradoxes, will be avoided. We can invoke a strictly 3-d flat manifold plus time, described by Galilean relativity equipped with a specific rule for Doppler shifts, where addition of velocities remains purely as Euclidean vectorial sum: 1. Define the frequency Doppler shift z as, f' = f Exp(-v/c), z = (f' - f) / f = Exp(-v/c) - 1, v/c = - ln(z + 1) 2. Consider a thought experiment similar to those carried out by Friedrich Hasenöhrl, as described in his papers of 1904 and 1905. Let two photons of equal frequency f, with combined energy E_0 = 2hf, reflect back and forth on two mirrors at rest, one in front the other, such that each reflection occurs simultanously on each opposite mirror. Now, let the mirrors move with relative speed v. This would mean that a photon is seen as Doppler blue-shifted by a mirror and the other photon is seen as red-shifted. So, according to the definition of Doppler shift, provided above, we get a difference between momenta as p = (hf/c)(Exp(v/c) - Exp(-v/c)), p = (2hf/c) sinh(v/c), and since the combined energy is E_0 = 2hf, we get p = (E_0/c) sinh(v/c) To first order approximation, if v -- 0, then sinh(v/c) -- v/c, so we would get p -- (E_0/c) (v/c) -- E_0 v/c^2 . Also to first order approximation, the momentum of a particle with mass m moving at small v -- 0, tends to p -- mv . Thus, we get E_0 v/c^2 = mv, E_0 /c^2 = m, E_0 = mc^2, which is the famous mass-energy equivalence equation. Since this equivalence must be true for any particle at rest with mass m, it implies that the momentum at speed v, deduced above, p = (E_0 /c) sinh(v/c), must be expressed in function of m, v and c, as p = mc sinh(v/c). Now, total energy E of a particle can be expressed as E = mc^2 + E_k, where E_k is kinetic energy, defined as E_k = mc^2 (cosh(v/c) - 1), thus, we get E = mc^2 + mc^2 (cosh(v/c) - 1) E = mc^2 cosh(v/c) This latter equation means, since cosh(v/c) = sqrt(1 + sinh^2 (v/c)), then E = mc^2 sqrt(1 + sinh^2 (v/c)) so, E^2 = m^2c^4 (1 + sinh^2 (v/c)) E^2 = m^2c^4 + m^2c^4 sinh^2 (v/c), and as we have already attained above that p = mc sinh(v/c), it yields E^2 = (mc^2)^2 + (pc)^2, which is the famous energy-momentum relation. Summarizing: We can see that E = mc^2 and E^2 = (mc^2)^2 + (pc)^2 are correct formulas, but, under Galilean relativity equipped with the above mentioned Doppler shift rule, we can express the momentum as p = mc sinh(v/c), and the kinetic energy as E_k = mc^2 (cosh(v/c) - 1), So, total energy E can be also expressed as E = mc^2 cosh(v/c). Discussion: What's the difference between this approach and the well-known relativistic approach, described in SR? Firstly, both approaches are experimentally undistinguishable. Secondly, we can see that the lorentz factor, gamma = 1/sqrt(1 - v^2/c^2) is replaced by the factor, for some cases, gamma' = (c/v) sinh(v/c), which means that if v -- 0, then sinh(v/c) -- v/c, so it would be gamma' -- (c/v)(v/c) = 1. Therefore, gamma' = (c/v) sinh(v/c) can be used to deduce the momentum p = mv gamma' = mc sinh(v/c), and total energy E^2 = m^2c^4 + m^2c^4 sinh^2 (v/c), E^2 = m^2c^4 + m^2c^4 (v/c)^2 gamma'^2 , E = mc^2 sqrt(1 + ( (v/c) gamma' )^2) , which in the limit gamma'= 1, it yields E = mc^2 sqrt(1 + v^2/c^2), with first order approximation as E = mc^2 + mv^2/2, and second order approximation as E = mc^2 + mv^2/2 - mv^4/8c^2. Under this approach, we can easily afford gravitation issues. For example, if we are wanting to enhance Newtonian gravitation, then the speed c should be replaced by the speed of gravity c_g, so an orbiting test body with mass m, around a massive body, would be endowed with momentum p = m c_g sinh(v/c_g), and angular momentum L would be then L = m r c_g sinh(v/c_g), where r is the radial distance to the center of the massive body. If we compare this angular momentum L with Newtonian L_n = m r v , we see L_n is not preserved when relativistic effects are taken into account due to strong gravitational fields, whereas L must be preserved along any orbit. Let's examine deeply what a momentum p = mc sinh(v/c) means. Newtonian force F is defined as the rate of change of momentum p. So, we get F = dp/dt = m d(c sinh(v/c))/dt. Therefore, d(c sinh(v/c))/dt must be an acceletation, a = d(c sinh(v/c))/dt = c cosh(v/c) d(v/c)/dt = = c cosh(v/c) (1/c)d(v)/dt = = cosh(v/c) d(v)/dt = = cosh(v/c) a_n, where a = a_n is acceleration for the case c = oo, or for the case v -- 0. IOW, a_n is Newtonian acceleration. For Newtonian gravity, it is a_n = GM/r^2, thus a = cosh(v/c) GM/r^2. But now the question is, what is that ratio v/c? Is that c the speed of light?, or is it the speed of gravity considered as superluminal? If we can answer this latter question, then we can answer what the ratio v/c is. If c is defined as the speed of gravity, regarded as a finite superluminal speed, then v must be a real tangential speed of the orbiting body. If c is defined as the speed of light, then v must be an apparent speed deduced through observed Doppler and ranging values. In any case, the force of gravity would be F = cosh(v/c) GMm/r^2. Since experimental astronomical tests are performed by means of light observations and measurements of Doppler and ranging, we should choose c as the speed of light, so v would be the apparent deduced speed. We can now modified the Newtonian equation of the orbit of a test particle, r = (h^2/GM)/(1 + e cos(phi - phi_0)), where h is angular momentum per unit mass, e is orbital eccentricity, r and phi are polar coordinates wrt center of the massive body with mass M, making h = r c sinh(v/c), it yields r = ( r c sinh(v/c))^2 /GM)/(1 + e cos(phi - phi_0)), GM / c^2 = (r sinh^2 (v/c)) / (1 + e cos(phi - phi_0)). Regards |
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#2
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Under this novel approach, we can calculate, for instance,
a escape velocity: Kinetic energy of an orbiting test particle is E_k = mc^2 (cosh(v/c) - 1) And potential energy is E_p = cosh(v/c)GMm/r Now, we equate E_k = E_p, and it yields mc^2 (cosh(v/c) - 1) = cosh(v/c) GMm/r, c^2 (cosh(v/c) - 1) = cosh(v/c) GM/r, cosh(v/c) = 1 / ( 1 - GM/rc^2), v = c arccosh(1 / (1 - GM/rc^2)) A first-order approximation is v_e = sqrt(2GM/r), which is the well-known Newtonian escape velocity. Let's compute, for example, the complete escape velocity (all higher order considered), for the mean position of the Earth in solar system: GM = 132,712,440,018 Km^3/s^2, is Sun's gravitational parameter, R_e = 149597870.691 Km, is mean Earth-Sun distance, and c = 299792.458 km/s, is the speed of light in vacuum, Then v = c arccosh(1/(1 - GM/R_ec^2)), v = 42.1219 Km/s |
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#3
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On Jun 7, 2:21 am, Albert****o wrote:
1. Define the frequency Doppler shift z as, f' = f Exp(-v/c), No reason to define it in such an idiotic way. |
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#4
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On Jun 7, 2:56 pm, Dono wrote:
On Jun 7, 2:21 am, Albert****o wrote: 1. Define the frequency Doppler shift z as, f' = f Exp(-v/c), No reason to define it in such an idiotic way. There are reasons that you will never be capable of understanding, troll. |
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#5
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On Jun 7, 6:01 pm, Albertito wrote:
On Jun 7, 1:38 pm, Albertito wrote: Under this novel approach, we can calculate, for instance, a escape velocity: Kinetic energy of an orbiting test particle is E_k = mc^2 (cosh(v/c) - 1) And potential energy is E_p = cosh(v/c)GMm/r Now, we equate E_k = E_p, and it yields mc^2 (cosh(v/c) - 1) = cosh(v/c) GMm/r, c^2 (cosh(v/c) - 1) = cosh(v/c) GM/r, cosh(v/c) = 1 / ( 1 - GM/rc^2), v = c arccosh(1 / (1 - GM/rc^2)) A first-order approximation is v_e = sqrt(2GM/r), which is the well-known Newtonian escape velocity. Let's compute, for example, the complete escape velocity (all higher order considered), for the mean position of the Earth in solar system: GM = 132,712,440,018 Km^3/s^2, is Sun's gravitational parameter, R_e = 149597870.691 Km, is mean Earth-Sun distance, and c = 299792.458 km/s, is the speed of light in vacuum, Then v = c arccosh(1/(1 - GM/R_ec^2)), v = 42.1219 Km/s Vis viva equation (orbital velocity): Under this novel approach, let m be the mass of the test body. Total energy of the test body in its orbit is the sum of its kinetic and potential energies, E = mc^2 (cosh(v/c) - 1) - cosh(v/c) GMm/r For orbits that are circular or elliptical, the total energy is also given by E = - cosh(v/c) GMm/2a where a is semi-major orbital axis Now, equating - cosh(v/c) GMm/2a = mc^2 (cosh(v/c) - 1) - cosh(v/c) GMm/r, and solving for v, it yields v = c arccosh(1 - GM/rc^2 + GM/2ac^2). For a circular orbit, it is a = r, so v = c arccosh(1 - GM/2rc^2 ), is the velocity of orbiting body Let's compute, for example, the orbital velocity (all higher orders considered), for the mean circular orbit of the Earth in solar system: GM = 132712440018 Km^3/s^2, is Sun's gravitational parameter, R_e = 149597870.691 Km, is mean Earth-Sun distance, and c = 299792.458 km/s, is the speed of light in vacuum, v = c arccosh(1 - GM/2R_ec^2 ), v = 29.7847 Km/s Sorry, there is a typo, I meant equating - cosh(v/c) GMm/2a = mc^2 (cosh(v/c) - 1) - cosh(v/c) GMm/r, and solving for v, it yields v = c arccosh(1/(1 - GM/rc^2 + GM/2ac^2)). For a circular orbit, it is a = r, so v = c arccosh(1/(1 - GM/2rc^2)), is the velocity of orbiting body Let's compute, for example, the orbital velocity (all higher orders considered), for the mean circular orbit of the Earth in solar system: GM = 132712440018 Km^3/s^2, is Sun's gravitational parameter, R_e = 149597870.691 Km, is mean Earth-Sun distance, and c = 299792.458 km/s, is the speed of light in vacuum, v = c arccosh(1/(1 - GM/2E_ec^2)), v = 29.7847 Km/s |
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