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Let us assume that we have a large gravitational field, then the gravitational redshift can be expressed as,
$$\frac {v_{\infty}} {v_e} = (1-r_s/R_e)^{1/2}$$
In this equation ##v_{\infty}## represents the frequency of the light measured by an observer at infinity, ##v_e## is the frequency of the emitted wavelength, ##r_s## is the schwarzschild radius, ##r_S=2GM/c^2##, and finally ##R_e## is the radius which photon is emitted.
And I argue that when we ##R_e## get closer to ##r_s## the wavelength of photon will decrease.
And at ##r_s=R_e## the energy of the photon will be zero, at the surface of the event horizon
"When the photon is emitted at a distance equal to the Schwarzschild radius, the redshift will be infinitely large, and it will not escape to any finite distance from the Schwarzschild sphere."
https://en.wikipedia.org/wiki/Gravi..._equivalence_principle_and_general_relativity
At this point I argue that the energy of the photon also decreases. I find an experiment that explains the energy decrease, https://en.wikipedia.org/wiki/Pound–Rebka_experiment and the math of it
http://hyperphysics.phy-astr.gsu.edu/hbase/Relativ/gratim.html
At this point, can someone else argue that "Light doesn't lose energy as it ascends. It was emitted with less energy at a lower elevation." ? I didnt understand what it means and also how it explains the experiment that I shared. Thanks
$$\frac {v_{\infty}} {v_e} = (1-r_s/R_e)^{1/2}$$
In this equation ##v_{\infty}## represents the frequency of the light measured by an observer at infinity, ##v_e## is the frequency of the emitted wavelength, ##r_s## is the schwarzschild radius, ##r_S=2GM/c^2##, and finally ##R_e## is the radius which photon is emitted.
And I argue that when we ##R_e## get closer to ##r_s## the wavelength of photon will decrease.
And at ##r_s=R_e## the energy of the photon will be zero, at the surface of the event horizon
"When the photon is emitted at a distance equal to the Schwarzschild radius, the redshift will be infinitely large, and it will not escape to any finite distance from the Schwarzschild sphere."
https://en.wikipedia.org/wiki/Gravi..._equivalence_principle_and_general_relativity
At this point I argue that the energy of the photon also decreases. I find an experiment that explains the energy decrease, https://en.wikipedia.org/wiki/Pound–Rebka_experiment and the math of it
http://hyperphysics.phy-astr.gsu.edu/hbase/Relativ/gratim.html
At this point, can someone else argue that "Light doesn't lose energy as it ascends. It was emitted with less energy at a lower elevation." ? I didnt understand what it means and also how it explains the experiment that I shared. Thanks