<\/p>\n
+ Bohr’s theory said electrons could begin in some orbit m and end up in some orbit n, or an electron could begin in some orbit n and end up in some orbit m so if a photon<\/strong> hits an electron, its energy will be absorbed, and the electron will move to a higher orbit because of that extra energy.\n<\/p>\n <\/p>\n + This work by Planck asserts that the energy of a photon<\/strong> is proportional to its frequency, and their relation can be put in terms of familiar units such as the joule by using the proportionality constant Planck gave us.\n<\/p>\n <\/p>\n + The longer a photon<\/strong><\/strong> has been traveling, the more expansion it has undergone; hence, older photon<\/strong><\/strong>s from more distant galaxies are the most red-shifted.\n<\/p>\n <\/p>\n + Another property of a photon<\/strong> is its wavelength.\n<\/p>\n <\/p>\n + A photon<\/strong> has a given frequency, which determines its color.\n<\/p>\n <\/p>\n + However, we can never know whether the photon<\/strong> is off-center at that time.\n<\/p>\n + Neutron versus photon<\/strong> irradiation for unresectable salivary gland tumors: final report of an RTOG-MRC randomized clinical trial.\n<\/p>\n <\/p>\n + Pair production happens sometimes in radiation therapy treatments with high-energy photon<\/strong> beams.\n<\/p>\n <\/p>\n + However, all we can say is that the photon<\/strong> must have been at that point when it ended its existence.\n<\/p>\n <\/p>\n + The energy of each photon<\/strong> depends on its frequency.\n<\/p>\n <\/p>\n + Another way to locate a photon<\/strong> is to make it go through a small place.\n<\/p>\n <\/p>\n + If an oscillation leads to a change in dipole in the molecule, then it will absorb a photon<\/strong> which has the same frequency.\n<\/p>\n <\/p>\n + The photon<\/strong> is the only boson that does not decay.\n<\/p>\n <\/p>\n + If the photon<\/strong> has a lot of energy, Compton scattering may take place.\n<\/p>\n <\/p>\n + The energy of a photon<\/strong> causing the photoelectric effect is found through is the work function for the metal.\n<\/p>\n <\/p>\n + Finally, a photon<\/strong> has a property called spin.\n<\/p>\n <\/p>\n + Radiated energy is emitted as photon<\/strong><\/strong>s, and the frequency of a photon<\/strong><\/strong> is proportional to the “punch” it delivers.\n<\/p>\n <\/p>\n + The wave that is part of the description of a photon<\/strong> is, in quantum mechanics, not the same kind of thing as a wave on the surface of the ocean or the regions of compressed air and rarefied air that make up sound waves.\n<\/p>\n <\/p>\n + The Enterprise had 12 Type X phasers and three Photon<\/strong> Torpedo launchers.\n<\/p>\n <\/p>\n + But if we slow the process down and see where each photon<\/strong> lands on the screen we can never tell ahead of time where the next one will show up.\n<\/p>\n <\/p>\n + We either measure the momentum of a photon<\/strong> or electron at one time and then without any more delay than necessary measure its position, or we switch things around and measure position first and momentum second.\n<\/p>\n <\/p>\n + If you saw a giant photon<\/strong> coming straight at you, it could appear as a swath whipping vertically, horizontally, or somewhere in between.\n<\/p>\n <\/p>\n + If the color of the light is infrared, each photon<\/strong> can heat up what it hits.\n<\/p>\n <\/p>\n + The way to calculate the amount of energy of a photon<\/strong> is given by the equation E = h\u03bd.\n<\/p>\n <\/p>\n + For example, an ultraviolet photon<\/strong><\/strong> has more energy than an infrared photon<\/strong><\/strong>.\n<\/p>\n <\/p>\n + That dim spot of light represents the photon<\/strong> or other atomic particle which tunnels through the wall.\n<\/p>\n <\/p>\n + That only happens when a photon<\/strong> of a certain frequency and energy comes in from the outside, is absorbed by the electron and gives it its energy, and that is what makes the electron go out to a higher orbit.\n<\/p>\n <\/p>\n + That is because when a photon<\/strong> goes through a hole like that it experiences diffraction.\n<\/p>\n <\/p>\n + The energy of a photon<\/strong> can be computed from its frequency \u03bd or wavelength \u03bb.\n<\/p>\n <\/p>\n + The smaller the circular hole is made, the closer we come to knowing the exact position of the photon<\/strong> as it goes through it.\n<\/p>\n <\/p>\n + Basically, if an electron with “x” amount of energy goes to a lower state of energy and loses “y” energy, then a photon<\/strong> with energy “y” is emitted by the atom and either becomes light or some other form of radiation.\n<\/p>\n <\/p>\n + The photon<\/strong><\/strong> or photon<\/strong><\/strong>s come out of a very small hole within a well known period of time.\n<\/p>\n <\/p>\n + We can know for sure that it is most likely that a photon<\/strong><\/strong> will hit the center bright band, and that it gets less and less likely that a photon<\/strong><\/strong> will show up at bands farther and farther from the center.\n<\/p>\n <\/p>\n + As noted above, the redshift arises from the metric expansion of space; as the space itself expands, the wavelength of a photon<\/strong> traveling through space likewise increases, decreasing its energy.\n<\/p>\n <\/p>\n + Electromagnetic radiation includes everything from cosmic rays on the high energy photon<\/strong> end, to the visual light spectrum, and on down below the infrared to the extremely low frequency radio waves.\n<\/p>\n <\/p>\n + Any photon<\/strong> with sufficient energy can affect the chemical bonds of a chemical compound.\n<\/p>\n <\/p>\n + Each photon<\/strong> in the ultraviolet range has a lot of energy, enough to hurt skin cells and cause a sunburn.\n<\/p>\n <\/p>\n + If we had very sensitive photographic film that could be darkened by only one photon<\/strong><\/strong>, then we would find a tiny speck of silver where the photon<\/strong><\/strong> ended up.\n<\/p>\n <\/p>\n + When a photon<\/strong> is absorbed by an electron it gives its energy to the electron and disappears.\n<\/p>\n <\/p>\n + Planck suggested that the energy of each photon<\/strong><\/strong> was related to the photon<\/strong><\/strong> frequency by the Planck constant.\n<\/p>\n <\/p>\n + For saffron, absorbance is determined for the crocin-specific photon<\/strong> wavelength of 440 nm in a given dry sample of spice.\n<\/p>\n <\/p>\n + If the mathematical model is an accurate representation of the real world, then no photon<\/strong> or other subatomic particle has either an exact position or a definite momentum.\n<\/p>\n <\/p>\n + If we use this formula, the photon<\/strong> has a mass, which is according to experiments incorrect.\n<\/p>\n <\/p>\n + We would not know where the photon<\/strong> would hit, but we would know exactly how hard it would hit.\n<\/p>\n <\/p>\n + An incoming photon<\/strong> will strike the photocathode surface of the PMT which will emit electrons.\n<\/p>\n <\/p>\n + Chloroplasts also contain various yellow and orange pigments to assist in photon<\/strong> capture for photosynthesis.\n<\/p>\n <\/p>\n + In a neutral atom, the system will emit a photon<\/strong> of the difference in energy.\n<\/p>\n <\/p>\n + On the other hand, the momentum of a photon<\/strong> is mathematically related to the amplitude of its wave.\n<\/p>\n <\/p>\n + Einstein said that the effect was due to a photon<\/strong> striking an electron.\n<\/p>\n <\/p>\n + A single x-ray is very high photon<\/strong> energy and can go right through the human body.\n<\/p>\n <\/p>\n + Quantum mechanics is based on the knowledge that a photon<\/strong><\/strong> of a certain frequency means a photon<\/strong><\/strong> of a certain amount of energy.\n<\/p>\n <\/p>\n + Each photon<\/strong> has a certain amount of energy related to its wavelength.\n<\/p>\n <\/p>\n + And, very surprisingly, a single photon<\/strong> could interfere with itself as though it were a single wave that fit the old wave description.\n<\/p>\n <\/p>\n + For example, for us to “see” an electron, a photon<\/strong> must first interact with it, and this interaction will change the path of that electron.\n<\/p>\n <\/p>\n + The wave that applies to a photon<\/strong> might be a pure sine wave.\n<\/p>\n <\/p>\n + But we never know for sure which photon<\/strong> will go into which band.\n<\/p>\n <\/p>\n + As the diameter of the hole is decreased, the momentum or the direction of the photon<\/strong> as it leaves the hole is more and more greatly changed.\n<\/p>\n <\/p>\n + Another important property of a photon<\/strong> is its polarity.\n<\/p>\n <\/p>\n + If the hole is exactly the same size as the photon<\/strong> it won’t pass through.\n<\/p>\n <\/p>\n + In atomic physics, Rydberg unit of energy, symbol Ry, corresponds to the energy of the photon<\/strong> whose wavenumber is the Rydberg constant, i.e.\n<\/p>\n <\/p>\n + When the electron decays back again, it emits one photon<\/strong> of light.\n<\/p>\n <\/p>\n + A photon<\/strong> has no rest mass, but it has momentum.\n<\/p>\n <\/p>\n + There was a photon<\/strong> with a certain frequency and now it has been taken away.\n<\/p>\n <\/p>\n + It is equal to Avogadro’s number multiplied by the energy of one photon<\/strong> of light.\n<\/p>\n <\/p>\n + A photon<\/strong> is an example of a boson as it has a spin spin of 1 and carries electromagnetism.\n<\/p>\n <\/p>\n + Bohr said that we know nothing about something like a photon<\/strong> or electron until we observe it.\n<\/p>\n <\/p>\n![\"Some](\"https:\/\/englishteststore.net\/blog\/wp-content\/uploads\/2021\/09\/Some-example-sentences-of-photon.jpg\" "\\"Some")
Example sentences of “photon”:<\/h2>\n
+ Neutron versus photon<\/strong> irradiation for unresectable salivary gland tumors: final report of an RTOG-MRC randomized clinical trial.\r\n
+ Pair production happens sometimes in radiation therapy treatments with high-energy photon<\/strong> beams.\r\n
<\/pre>\nMore in-sentence examples of “photon”:<\/h2>\n
+ If the color of the light is infrared, each photon<\/strong> can heat up what it hits.\r\n
+ The way to calculate the amount of energy of a photon<\/strong> is given by the equation E = h\u03bd.\r\n
+ For example, an ultraviolet photon<\/strong><\/strong> has more energy than an infrared photon<\/strong><\/strong>.\r\n
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