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  1. Question: By examining strangeness, determine which of the following decays or reactions proceed via the strong interaction: (a) K0π++π- (b) Λ0+pΣ++n(c) Λ0p+π-(d)K-+pΛ0+π0.

Short Answer

Expert verified
  1. Strangeness is not conversed.
  2. Strangeness is not conversed.
  3. Strangeness is not conversed.
  4. Strangeness is conversed.

Step by step solution

01

(a) Strangeness of K0→π++π-.

The strangeness of K0is +1and the strangeness ofπ+is 0 and strangeness of π-is0.

Thus, strangeness is not conversed.

Hence, it does not proceed via strong interaction.

02

(b) Strangeness of Λ0+p→∑++n.

The strangeness ofΛ0 is-1 andp is 0and the strangeness +of is 1 and strangeness ofnis 0.

Thus, strangeness is not conversed.

Hence, it does not proceed via strong interaction.

03

(c) Strangeness of Λ0→p+π- .

The strangeness ofΛ0 is -1and the strangeness of pis 0andπ- is 0.

Thus, strangeness is not conversed.

Hence, it does not proceed via strong interaction.

04

(d) Strangeness of K-+p→Λ0+π0 ..

The strangeness ofK- is-1 andp is0 and the strangeness ofΛ0 is-1 andπ0 is0 .

Thus, strangeness is conversed.

Hence, it proceed via strong interaction.

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Most popular questions from this chapter

The wavelength at which a thermal radiator at temperature Tradiates electromagnetic waves most intensely is given by Wien’slaw:localid="1663130298382" λmax=(2898μm.K)/T(a) Show that the energyEof a photon corresponding to that wavelength can be computed from

E=(4.28×1010MeVK)T

(b) At what minimum temperature can this photon create an electron-positron pair(as discussed in Module 21-3)?

Does the proposed decay Λ0p+K- conserve (a) electric charge, (b) spin angular momentum, and (c) strangeness? (d) If theoriginal particle is stationary, is there enough energy to create thedecay products?

Suppose that the matter (stars, gas, dust) of a particular galaxy, of total mass M, is distributed uniformly throughout a sphere of radius.A star of mass Ris revolving about the center of the galaxy in a circular orbit of radius.r<R

(a) Show that the orbital speedv of the star is given by

v=rGMr3

And therefore that the star’s period Tof revolution is

T=2πR3GM

Independentof.rIgnore any resistive forces.

(b) Next suppose that the galaxy’s mass is concentrated near the galactic center, within a sphere of radius less than . What expression then gives the star’s orbital period?

Calculate the disintegration energy of the reactions

(a)π++p++K+and(b)K-+pΛ0+π0

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.)

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