A 525 nm photon emitted by a distant galaxy is observed to be 890 nm. Estimate the redshift of the galaxy.
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- Redshift takes place when the source of electromagnetic radiation moves away from the observer. This shifts the wavelength to the red side and will decrease the frequency.
- Redshift can be calculated from wavelength using the following formula,
Here λobs is the observed wavelength and λemit is the emitted wavelength.
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- How does the relativistic landau energy spectrum for a particle in a magnetic field simplify down in the non-relativistic limit?Under the right circumstances, a photon of high enough energy can give rise to an electron-positron pair. What minimum energy photon is required?If pair production of muon-antimuon pair can occur for photons of wavelength = 5.85 x 10-15m or less, what is the mass of a muon?
- To measure the muon magnetic moment a 2.9-T uniform magnetic field is used. How much energy is stored in the field if the experimental chamber where the field is created has dimensions of 65 cm×35 cm×60 cm? The energy, ? How long will it take to “switch on” the field if the experiment uses a 1.5-kW power supply? Time ?Why does the cosmic microwave background (CMB) shine in low-energy microwave wavelengths? O The trapped photons within the plasma of the earliest universe originally had wavelengths in the microwave band due to rapid inflation O The CMB was originally emitted as high-energy gamma rays and x-rays, but the light has redshifted downward to lower-energy microwaves through time When nuclei of H and He first combined with free electrons to create atoms, photons of light were released as microwaves The photons released in the CMB were intensely hot, with energy levels in microwave wavelengths The early universe 380,000 years after the Big Bang was cold (2.7 kelvins) the temperature of microwave energy