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Calculate the difference in mass, in kilograms, between the muon and pion of Sample Problem 44.01.

Short Answer

Expert verified

The difference in mass between the pion and muon is 6.03×10-29kg.

Step by step solution

01

Given data

The interaction provided is

π+μ++ν

02

Rest mass of muon and pion

The muon rest mass is

m0μ=105.7MeV/c2.......1

The pion rest mass is

role="math" localid="1663137427708" m0π=139.6MeV/c2........2

Here, c is the speed of light in vacuum with value

c=3×108m/s

03

Determining the difference in masses of muon and pion

From equations (I) and (II), the difference in the masses of muon and pion are

m0π-m0μ=139.6MeV/c2-105.7MeV/c2=33.93×1082·1MeV×1.602×10-13kg·m2/s21MeV·11m2/s2=6.03×10-29kg

Thus, the difference is =6.03×10-29kg.

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Most popular questions from this chapter

Show that if, instead of plotting strangenessS versus chargeq for the spin -12baryons in Fig. 44-3a and the spin-zero mesons in Fig.44-3b , we plot the quantity Y=B+Sversus the quantity Tz=q-12(B+S), we get the hexagonal patterns without using sloping axes. (The quantityY is called hypercharge, andTzis related to a quantity called isospin.)

Use Wien’s law (see Problem 37) to answer the following questions: (a) The cosmic background radiation peaks in intensity at a wavelength of.1.1mmTo what temperature does this correspond? (b) About379000y after the big bang, the universe became transparent to electromagnetic radiation. Its temperature then was2970K . What was the wavelength at which the background radiation was then most intense?

There are baryons with spin .Their symbols and quantum numbers for charge and strangeness are as follows:


q S
q S
--10*0
0-1
000*++1-1
+
+10*0-1-2
+++20*00-2
*--1-1Ω--1-3

Make a charge–strangeness plot for these baryons, using the sloping coordinate system of Fig. 44-3. Compare your plot with this figure.

Because the apparent recessional speeds of galaxies and quasars at great distances are close to the speed of light, the relativistic Doppler shift formula (Eq.37-31) must be used. The shift is reported as fractional red shift z=Δλλ0

(a)Show that, in termsof,zthe recessional speedparameterβ=vcisgiven by

β=z2+2zz2+2z+2.

(b) A quasar in 1987 has z=4.43. Calculate its speed parameter.

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If Hubble’s law can be extrapolated to very large distances, at what distance would the apparent recessional speed become equal to the speed of light ?

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