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Plans for an accelerator that produces a secondary beam of \({\rm{K}}\)-mesons to scatter from nuclei, for the purpose of studying the strong force, call for them to have a kinetic energy of \({\rm{500 MeV}}\).

(a) What would the relativistic quantity \(\gamma {\rm{ = }}\frac{{\rm{1}}}{{\sqrt {{\rm{1 - }}{{{{\rm{\nu }}^{\rm{2}}}} \mathord{\left/{\vphantom {{{{\rm{\nu }}^{\rm{2}}}} {{{\rm{c}}^{\rm{2}}}}}} \right. \\} {{{\rm{c}}^{\rm{2}}}}}} }}\) be for these particles?

(b) How long would their average lifetime be in the laboratory?

(c) How far could they travel in this time?

Short Answer

Expert verified

(a) The relativistic quantity\(\gamma = \frac{1}{{\sqrt {1 - {v^2}/{c^2}} }}\)for the particles is\(\gamma = 2.013\).

(b) The average lifetime of the particles in the laboratory will be\(\Delta t = 2.50 \times {10^{ - 8}}\;{\rm{s}}\).

(c) The particles could travel a distance of \(d = 6.51{\rm{\;m}}\) in the time \(\Delta t = 2.50 \times {10^{ - 8}}\;{\rm{s}}\).

Step by step solution

01

Concept Introduction

The relation between mass and energy is given by the energy expression,

\(E = \Delta m{c^2}\)

Here\(E\)is the energy of the physical system,\(m\)is the mass of the system and\(c\)is the speed of the light in vacuum.

02

Calculation for relativistic quantity

(a)

Kinetic energy can be calculated as,

\({E_{kin{\rm{ }}}} = (\gamma - 1)m{c^2}\)……. (i)

Where\(m\)is the kaon’s rest mass. As one is creating an accelerator beam, the particles needs to be charged to be accelerated, so consider a\({K^ + }\)or\({K^ - }\)meson (this is relevant because the mass of\({K^ \pm }\)differs from\({K^0}\)). Inverting\({\rm{(1)}}\)to express\(\gamma \)and inputting the known values, it is obtained as,

\(\begin{aligned}{}\gamma &= \frac{{{E_{kin{\rm{ }}}}}}{{m{c^2}}} + 1\\ &= \frac{{{\rm{(500 MeV)}}}}{{\left( {{\rm{493}}{\rm{.67 MeV/}}{{\rm{c}}^{\rm{2}}}} \right){{\rm{c}}^{\rm{2}}}}}{\rm{ + 1}}\\ &= {\rm{2}}{\rm{.013}}\end{aligned}\)

Therefore, the value for relativistic quantity is obtained as \(\gamma = 2.013\).

03

Lifetime of the particle

(b)

The proper lifetime of the kaon’s is \(\Delta {t_0} = 1.24 \times {10^{ - 8}}{\rm{\;s}}\) so to calculate its average lifetime in the laboratory \({\rm{\Delta t}}\)

\(\begin{aligned}{}\Delta t &= \gamma \Delta {t_0}\\ &= (2.013) \cdot \left( {1.24 \times {{10}^{ - 8}}\;{\rm{s}}} \right)\\ &= 2.50 \times {10^{ - 8}}{\rm{\;s}}\end{aligned}\)

Therefore, the value for time is obtained as \({\rm{\Delta t = 2}}{\rm{.50 \times 1}}{{\rm{0}}^{{\rm{ - 8}}}}{\rm{\;s}}\).

04

Calculation for distance

(c)

The equation for the relativistic quantity is given by,

\(\gamma = \frac{1}{{\sqrt {1 - \frac{{{v^2}}}{{{c^2}}}} }}\)

And invert this equation to get –

\(v = c\sqrt {1 - \frac{1}{{{\gamma ^2}}}} \)

The distance travelled\(d\)is given by,

\(\begin{aligned}{}d &= v\Delta t\\ &= c\sqrt {1 - \frac{1}{{{\gamma ^2}}}} \Delta t\\ &= \left( {{\rm{3 \times 1}}{{\rm{0}}^{\rm{8}}}{\rm{\;m}}{{\rm{s}}^{{\rm{ - 1}}}}} \right)\sqrt {{\rm{1 - }}\frac{{\rm{1}}}{{{\rm{2}}{\rm{.01}}{{\rm{3}}^{\rm{2}}}}}} \cdot \left( {{\rm{2}}{\rm{.50 \times 1}}{{\rm{0}}^{{\rm{ - 8}}}}{\rm{\;s}}} \right)\\ &= 6.51\;{\rm{m}}\end{aligned}\)

Therefore, the value for distance is obtained as \(d = 6.51\;{\rm{m}}\).

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Most popular questions from this chapter

In supernovas, neutrinos are produced in huge amounts. They were detected from the \({\rm{1987 A}}\) supernova in the Magellanic Cloud, which is about \({\rm{120,000}}\) light years away from the Earth (relatively close to our Milky Way galaxy). If neutrinos have a mass, they cannot travel at the speed of light, but if their mass is small, they can get close.

(a) Suppose a neutrino with a \({\rm{7 - eV/}}{{\rm{c}}^{\rm{2}}}\) mass has a kinetic energy of \({\rm{700 KeV}}\). Find the relativistic quantity \(\gamma {\rm{ = }}\frac{{\rm{1}}}{{\sqrt {{\rm{1 - }}{{{{\rm{\nu }}^{\rm{2}}}} \mathord{\left/ {\vphantom {{{{\rm{\nu }}^{\rm{2}}}} {{{\rm{c}}^{\rm{2}}}}}} \right. \\} {{{\rm{c}}^{\rm{2}}}}}} }}\) for it.

(b) If the neutrino leaves the \({\rm{1987 A}}\) supernova at the same time as a photon and both travel to Earth, how much sooner does the photon arrive? This is not a large time difference, given that it is impossible to know which neutrino left with which photon and the poor efficiency of the neutrino detectors. Thus, the fact that neutrinos were observed within hours of the brightening of the supernova only places an upper limit on the neutrino’s mass. (Hint: You may need to use a series expansion to find \({\rm{v}}\) for the neutrino, since it \(\gamma \) is so large.)

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(b) What is the analogous decay process for the antiproton?

If a GUT is proven, and the four forces are unified, it will still be correct to say that the orbit of the moon is determined by the gravitational force. Explain why.

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(a) Verify from its quark composition that the \({\rm{\Delta + }}\)particle could be an excited state of the proton.

(b) There is a spread of about \({\rm{100 MeV}}\) in the decay energy of the \({\rm{\Delta + }}\), interpreted as uncertainty due to its short lifetime. What is its approximate lifetime?

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