Problem 2. Assuming the scale factor a(t) evolves as a power law with time as - (-:-)^, where the power law index I > 0, and to is the age of the universe. 1. Derive an expression for the Hubble parameter H(z) as a function of to, I, and the redshift z at time t. 2. What is the age of the universe if I = 1/2 and Ho = 70 km/s/Mpc ? 3. For what value of I is the age of the universe equal to the Hubble time?
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- 1. Given questions about reviewing the quark model a. With six different quark flavors, how many different meson pairings are possible? Let's say they come in the flavors u, d, c, s, t, and d. Please explain these combination ! b. With six different quark flavors, how many different Baryon pairings are possible? Let's say they come in the flavors u, d, c, s, t, and d. Please explain these combination !13If the mass density of the universe is above the critical density as it appears to be with the mass detected so far, then the universe is a. flat b. negatively curved C. in steady state d. positively curved
- The matter density in the Universe today is Pm = -27 kg m-3. What would 2.7 x 10 be the value of the density parameter, 2o, if the Hubble constant had the value Ho = 38 km/s/Mpc? Assume the Universe does not contain dark energy and choose the option below that best matches your answer. Select one: O a. 0.1 O b. 2. О с. 1. O d. 0.7 О е. 0.5Please answer within 90 minutes.Please answer all three parts! Thank you. Stanford has a linear particle accelerator (SLAC) which is 3 km long that produces electrons with a total energy of 50 GeV. These electrons lead exciting (albeit brief) lives, zooming along the accelerator before slamming into a target to produce other high-energy particles. a. Consider the viewpoint of one of the electrons. From the electron’s point of view, how long is the accelerator? Note that it is possible to answer this question without calculating the electron’s velocity. b. Let’s figure out how fast the electrons are traveling. Start by solving for β = u/c in terms of 1/γ following the trick we used in class. Use the binomial expansion if that is helpful. At what speed does a 50 GeV electron travel? c. The Large Hadron Collider (LHC) at CERN presently accelerates protons to a total energy of 6.5 TeV. Imagine a pulse of light, a 50 GeV electron, and a 6.5 TeV proton race each other along a 3 km distance. The light pulse will surely win…
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- There are two new equa3ons we need to learn about in this assignment (so that we can usethem in class on Wednesday). No need to derive or prove them – just look up the twoequa3ons in the book and then use them as explained below. If there’s a symbol in theequa3on you’re not sure about, read that part of the book carefully to see what it means.A) Find and report the equa3on for the Electric field due to a long line of charge. The keypart of the book is in sec3on 21.5, example 21.10. Keep in mind that we’re interested inthe limit of a very long (infinitely long) charged wire, where the equa3on looks simpler.B) Use the equa3on from A) to calculate the electric field 2mm radially out from the centerof a long thin charged wire. Assume the wire has a uniform charge of 3nC per meterlength. Make sure you give both the magnitude and the direc3on of the E-field at thispoint, rela3ve to the wire.C) Next, find and report the equa3on for the Electric Field due to a large plate of charge(spread over…The density of the universe is a. equal to the critical density if the universe is closed. b. equal to the critical density if the universe is flat. c. greater than the critical density if the universe is flat. d. greater than the critical density if the universe is open. e. none of the above.There are two parts to this question. I need to know the years for both. I have tried 14,000,000,000, 17,908,900,000, 17.29 x 10^9, and 17.9089 x 10^9 for the hubble time and all those are wrong. I have tried 17,908,900,000, 17.29 x 10^9, and 17.9089 x 10^9 for the second question and those are wrong too.