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Unstable nuclei attain stability through...

Unstable nuclei attain stability through disintegration. The nuclear stability is related to neutron proton ratio `(n//p)`. For stable nuclei `n//p` ratio lies close to unity for elements with low atmoic numbers (20 or less) but it is more than 1 for nuclei having higher atomic numbers. Nuclei having `n//p` ratio either very high or low undergo nuclear transformation. When `n//p` ratio is higher than required for stability, the nuclei have the tendency to emit `beta`-rays. while when `n//p` ratio is lower than required for stability, the nuclei either emits `alpha`-particles or a positron or capture `K`-electron.

A

`Cu_(68)`

B

`Cu^(59)`

C

`Cu^(68)`

D

`Cu^(67)`

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The correct Answer is:
D
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Unstable nuclei attain stability through disintegration. The nuclear stability is related to neutron proton ratio (n/p). For stable nuclei n/p ratio lies close to unity for elements with low atomic numbers (20 or less) but it is more than 1 for nuclei having higher atomic numbers. Nuclei having n/p ratio either very high or low undergo nuclear transformation. when n/p ratio is higher than required for stabilioty, the nuclei have the tendency to emit beta -rays. While when n/p ratio is lower than required for stability, the nucleieither emits alpha -particles or a position or capture K-electron. The order of radioactive disinigration is

Unstable nuclei attain stability through disintegration. The nuclear stability is related to neutron proton ratio (n/p). For stable nuclei n/p ratio lies close to unity for elements with low atomic numbers (20 or less) but it is more than 1 for nuclei having higher atomic numbers. Nuclei having n/p ratio either very high or low undergo nuclear transformation. when n/p ratio is higher than required for stabilioty, the nuclei have the tendency to emit beta -rays. While when n/p ratio is lower than required for stability, the nucleieither emits alpha -particles or a position or capture K-electron. Unstable substance exhibit high radioactivity due to

If n//p ratio is high, the nucleus tends to stabilize by :

An unstable nuclide with N/P ratio more than that required for stability can attain stability by

An unstable nuclide (Z lt 70) with N/P ratio less than that required for stability can attain stability by

A nucleus X^(235) splits into two nuclei having the mass numbers in the ratio 2:1 . The ratio of the radii of those two nuclei is

The n//p ratio for a stable lighter nuclei is about ……………… .

CENGAGE CHEMISTRY-NUCLEAR CHEMISTRY-Exercises Link Comprehension
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  2. Unstable nuclei attain stability through disintegration. The nuclear s...

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  3. Unstable nuclei attain stability through disintegration. The nuclear s...

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  4. Unstable nuclei attain stability through disintegration. The nuclear s...

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  5. In the disintegration of a radioactive element, alpha- and beta-partic...

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  6. In the disintegration of a radioactive element, alpha- and beta-partic...

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  7. In the disintegration of a radioactive element, alpha- and beta-partic...

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  8. In the disintegration of a radioactive element, alpha- and beta-partic...

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  9. In the disintegration of a radioactive element, alpha- and beta-partic...

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  10. In the decay series .(92)U^(238) to .(82)Pb^(206), how many alpha-pari...

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  11. Uranium .(92)U^(238) decayed to .(82)Pb^(206). They decay process is ....

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  12. Uranium .(92)U^(238) decayed to .(82)Pb^(206). They decay process is ....

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  13. Uranium .(92)U^(238) decayed to .(82)Pb^(206). They decay process is ....

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  14. The source of energy of stars is nuclear fusion. Fusion reaction occur...

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  15. The source of energy of stars is nuclear fusion. Fusion reaction occur...

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  16. The source of energy of stars is nuclear fusion. Fusion reaction occur...

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  17. The source of energy of stars is nuclear fusion. Fusion reaction occur...

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  18. The source of energy of stars is nuclear fusion. Fusion reaction occur...

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  19. Radioactive decay follows first-order kinetic. The mean life and half-...

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  20. Radioactive decay follows first-order kinetic. The mean life and half-...

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