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Chapter 44: Q29P (page 1364)

Which hadron in Tables 44-3 and 44-4 corresponds to the quark bundles (a) ssu and (b) the dds?

Short Answer

Expert verified

(a) The quark bundle of $s s u$ is $惟^{o}$ (omega) hadrons.

(b) The quarks bundle $d d s$ is in Sigma hadrons.

Step by step solution

01

(a) Hadron corresponds to the quark bundles ssu.

The quark bundle . $s s u$

The total charge is calculated as,

$\begin{matrix} Q = (鈭� \frac{1}{3}) + (鈭� \frac{1}{3}) + (\frac{2}{3}) \\ = 0 \end{matrix}$

Total strangeness

$\begin{matrix} s = (鈭� 1) + (鈭� 1) + 0 \\ = 鈭� 2 \end{matrix}$

Here the charge and strangeness coincides with the $E^{o}$ baryon.

Hence the quark bundle of $s s u$ is $惟^{o}$ (omega) hadrons.

02

(b) Hadron corresponds to the quark bundles dds.

The given quark $d d s$ is of Baryons families. As the baryons made of an odd number of quarks i.e, usually three quarks.

The quarks bundle $d d s$ is Sigma.

Hence, the quarks bundle $d d s$ is in Sigma hadrons.

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Most popular questions from this chapter

What would the mass of the Sun have to be if Pluto (The outermost 鈥減lanet: most of the time) were to have the same orbital speed that Mercury (the innermost planet) has now? Use data from Appendix C, express your answer in terms of the Sun鈥檚 current mass, $M_{s}$ and assume circular orbits.

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 $z = \frac{螖位}{位_{0}}$

(a)Show that, in termsof, $z$ the recessional speedparameter $尾 = \frac{v}{c}$ isgiven by

$尾 = \frac{z^{2} + 2 z}{z^{2} + 2 z + 2}$ .

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(c) Find the distance to the quasar, assuming that Hubble鈥檚 law is valid to these distances.

A proton has enough mass energy to decay into a shower made

up of electrons, neutrinos, and their antiparticles. Which of the following

conservation laws would necessarily be violated if it did: electron lepton number or baryon number?

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 $R$ is revolving about the center of the galaxy in a circular orbit of radius. $r < R$

(a) Show that the orbital speed $v$ of the star is given by

$v = r \sqrt{\frac{G M}{r^{3}}}$

And therefore that the star鈥檚 period $T$ of revolution is

$T = 2 蟺 \sqrt{\frac{R^{3}}{G M}}$

Independentof. $r$ Ignore any resistive forces.

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

Which conservation law is violated in each of these proposed reactions and decays? (Assume that the products have zero orbital angular momentum.)

$(a) {鈭�}^{0} 鈫� {pK}^{-}; (b) 惟^{-} 鈫� {鈭�}_{}^{-} + 蟺^{0} (S = - 3, q = - 1, m = 162 MeV / c^{2}, and m_{s} = \frac{3}{2} 蹿辞谤惟); (c) K^{-} + p 鈫� 鈭� 0 + 蟺^{+}$

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