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Predict the type of radioactive decay process for the following radionuclides: (a) 58 B, (b) 2968Cu, (c) phosphorus-32, (d) chlorine-39. 21.20 Each of the following nuclei undergoes either beta decay or positron emission. Predict the type of emission for each: (a) tritium, 13H, (b) 3889Sr, (c) iodine-120, (d) silver-102.

Short Answer

Expert verified
The predicted decay types for the given radionuclides are: (a) 58B: Positron emission (β+) (b) 2968Cu: Beta decay (β) (c) Phosphorus-32: Beta decay (β) (d) Chlorine-39: Beta decay (β) For the second part of the exercise, the predicted type of emission for each is: (a) Tritium, 13H: Beta decay (β) (b) 3889Sr: Positron emission (β+) (c) Iodine-120: Positron emission (β+) (d) Silver-102: Positron emission (β+)

Step by step solution

01

Determine the isotope's stability

There are 5 protons and 3 neutrons in this isotope, meaning it has too many protons compared to neutrons. Therefore, it will undergo a decay to convert one of the protons into a neutron.
02

Predict the decay type

As the isotope has too many protons, it is likely to undergo positron emission, which will convert a proton to a neutron and decrease the atomic number by 1. The predicted decay type is positron emission (β+). (b) 2968Cu
03

Determine the isotope's stability

This isotope has 29 protons and 39 neutrons. Since Cu-63 and Cu-65 are the stable isotopes of copper, this isotope has too many neutrons compared to protons.
04

Predict the decay type

As this isotope has too many neutrons compared to protons, it is likely to undergo beta decay. This would convert a neutron to a proton, thereby increasing the atomic number by 1. The predicted decay type is beta decay (β). (c) Phosphorus-32
05

Determine the isotope's stability

This isotope has 15 protons and 17 neutrons. The most stable isotope of phosphorus is P-31, so this isotope has one too many neutrons compared to protons.
06

Predict the decay type

With too many neutrons, this isotope is predicted to undergo beta decay, converting a neutron to a proton and increasing the atomic number by 1. The predicted decay type is beta decay (β). (d) Chlorine-39
07

Determine the isotope's stability

This isotope has 17 protons and 22 neutrons. The stable isotopes of chlorine are Cl-35 and Cl-37, which means this isotope has too many neutrons compared to protons.
08

Predict the decay type

Having too many neutrons, this isotope is likely to undergo beta decay, converting a neutron to a proton and therefore increasing the atomic number by 1. The predicted decay type is beta decay (β). Now, let's predict the type of emission for the second part of the exercise: (a) Tritium, 13H
09

Determine the isotope's stability

This isotope has 1 proton and 2 neutrons, while the stable isotope of hydrogen is H-1, which means this isotope has too many neutrons compared to protons.
10

Predict the decay type

Since tritium has too many neutrons, it is predicted to undergo beta decay, converting a neutron to a proton and hence increasing the atomic number by 1. The predicted decay type is beta decay (β). (b) 3889Sr
11

Determine the isotope's stability

This isotope has 38 protons and 51 neutrons. The stable isotopes of strontium are Sr-88, Sr-87, Sr-86, and Sr-84, which means this isotope has too many protons compared to neutrons.
12

Predict the decay type

As this isotope has too many protons, it is likely to undergo positron emission, converting a proton to a neutron and decreasing the atomic number by 1. The predicted decay type is positron emission (β+). (c) Iodine-120
13

Determine the isotope's stability

This isotope has 53 protons and 67 neutrons. Since the stable isotopes of iodine are around I-127, iodine-120 has too few neutrons compared to protons.
14

Predict the decay type

With too few neutrons and too many protons, the isotope is expected to undergo positron emission, converting a proton to a neutron and decreasing the atomic number by 1. The predicted decay type is positron emission (β+). (d) Silver-102
15

Determine the isotope's stability

This isotope has 47 protons and 55 neutrons. The stable isotopes of silver are Ag-107 and Ag-109, which means this isotope has too few neutrons compared to protons.
16

Predict the decay type

Since this isotope has too few neutrons and too many protons, it is predicted to undergo positron emission, converting a proton to a neutron and decreasing the atomic number by 1. The predicted decay type is positron emission (β+).

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Key Concepts

These are the key concepts you need to understand to accurately answer the question.

Beta Decay
Beta decay is a common type of radioactive decay where an unstable nucleus transforms, releasing energy in the form of radiation. This process involves a neutron in the nucleus changing into a proton and emitting a beta particle, which is an electron. Let's examine how this affects the atom:

  • The atomic number of the element increases by one because a neutron changes into a proton. This transformation turns the atom into a different element.
  • The mass number, however, remains unchanged because the transformation is within the nucleus and doesn't add or remove an overall nucleon.
  • The beta particle released is the electron. Although small, it carries away kinetic energy, reducing the overall energy of the nucleus and making it more stable.
Through beta decay, elements like phosphorus-32 with excess neutrons convert them into protons, thereby moving closer to a stable state. Elements with too many neutrons relative to protons can undergo beta decay to reach a more balanced and stable configuration.
Positron Emission
Positron emission is another form of radioactive decay, which occurs when a proton in an unstable nucleus transforms into a neutron. This process emits a positron, which is the antimatter counterpart of an electron. Here’s how positron emission functions:

  • Since a proton is converting into a neutron, the atomic number of the element decreases by one. This results in the transformation of the atom into a new element.
  • The mass number remains the same as no nucleons are lost; only their composition has changed within the nucleus.
  • The positron emitted is similar to an electron but with a positive charge. When emitted, it can encounter electrons, leading to mutual annihilation and releasing energy in the form of gamma radiation.
Isotopes that exhibit an excess of protons—like 58extB—may undergo positron emission to convert one of these protons into a neutron, stabilizing the atomic composition of the element. The release of the positron helps in balancing the overall charge and energy of the atom.
Isotope Stability
Isotope stability refers to how likely an isotope of an element will remain unchanged or undergo radioactive decay over time. Stability is influenced by the ratio of neutrons to protons in the nucleus. Key factors for understanding isotope stability include:

  • An ideal balance of neutrons and protons fosters a stable nucleus. The strong nuclear forces must adequately counteract the repulsion between positively charged protons.
  • Isotopes that deviate significantly from the neutron-to-proton ratio typical for stability are likely to undergo forms of radioactive decay such as beta decay or positron emission.
  • Radioactive isotopes, which are less stable, will transform over time through these decay processes until a stable isotope or element is formed.
For example, isotopes like 13extH (tritium) highlight the principles of isotope stability. Tritium has more neutrons compared to the stable hydrogen-1, leading it to undergo beta decay over time. Understanding which isotopes are stable gives chemists and physicists insight into the behavior of elements under various conditions and helps in tailoring isotopes for practical applications such as medical imaging, radiometric dating, and nuclear power generation.

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Most popular questions from this chapter

(a) Which of the following statements about the uranium used in nuclear reactors is or are true? (i) Natural uranium has too little 295U to be used as a fuel. (ii) 24U cannot be used as a fucl because it forms a supereritical mass too casily. (iii) To be used as fuel, uranium must be enriched so that it is more than 50%2.35U in composition. (iv) The neutron-induced fission of 235U releases more neutrons per nucleus than fission of 2.85U. (b) Which of the following statements about the plutonium shown in the chapter-opening photograph explains why it cannot be used for nuclear power plants or nuclear weapons? (i) None of the isotopes of Pu possess the characteristics needed to support nuclear fission chain reactions. (ii) The orange glow indicates that the only radioactive decay products are heat and visible light. (iii) The particular isotope of plutonium used for RTGs is incapable of sustaining a chain reaction. (iv) Plutonium can be used as a fuel, but only atter it decays to uranium.

In 2010, a team of scientists from Russia and the U.S. reported creation of the first atom of element 117 , which is not yet named and is denoted [117]. The synthesis involved the collision of a target of 249 Bk with accelerated ions of an isotope which we will denote Q. The product atom, which we will call 97249Bk+QZ117294[117]+301n

How much energy must be supplied to break a single 21Ne nucleus into separated protons and neutrons if the nucleus has a mass of 20.98846 amu? What is the nuclear binding energy for 1 mol of 21Ne ?

Indicate the number of protons and neutrons in the following nuclei: (a) 2456Cr, (b) 193Tl, (c) argon-38.

Calculations Involving Radioactive Decay and Time If we start with 1.000 g of strontium- 90,0.953 g will remain after 2.00yr. (a) What is the half-life of strontium- 90 ? (b) How much strontium- 90 will remain after 5.00yr ? (c) What is the initial activity of the sample in becquerels and curies? SOLUTION (a) Analyze We are asked to calculate a half-life, t1/2 based on data that tell us how much of a radioactive nucleus has decayed in a time interval t=2.00yr and the information N0=1.000 g,Nt=0.953 g. Plan We first calculate the rate constant for the decay, k, and then use that to compute t1/2. Solve Equation 21.19 is solved for the decay constant, k, and then Equation 21.20 is used to calculate half-life, t1/2 : k=1tlnNfN0=12.00yrln0.953 g1.000 g=12.00yr(0.0481)=0.0241yr1t1/2=0.693k=0.6930.0241yr1=28.8yr (b) Analyze We are asked to calculate the amount of a radionuclide remaining after a given period of time. Plan We need to calculate Nb the amount of strontium present at time t, using the initial quantity, N0, and the rate constant for decay, k, calculated in part (a). Solve Again using Equation 21.19, with k=0.0241yr1, we have lnNtN0=kt=(0.0241yr1)(5.00yr)=0.120 Nt/N0 is calculated from ln(Nt/N0)=0.120 using the ex or INV LN function of a calculator: NtN0=e1.120=0.887 Because N0=1.000 g, we have Nt=(0.887)N0=(0.887)(1.000 g)=0.887 g (c) Analyze We are asked to calculate the activity of the sample in becquerels and curies. Plan We must calculate the number of disintegrations per atom per second and then multiply by the number of atoms in the sample. Solve The number of disintegrations per atom per second is given by the decay constant, k : k=(0.0241yr)(1yr365 days )(1 day 24 h)(lh3600 s)=7.64×1010 s1 To obtain the total number of disintegrations per second, we calculate the number of atoms in the sample. We multiply this quantity by k, where we express k as the number of disintegrations per atom per second, to obtain the number of disintegrations per second: (1.000 g90Sr)(1 mol90Sr90 g90Sr)(6.022×1023atomsSr1 mol90Sr)=6.7×1021 atoms 90Sr Total disintegrations/s =(7.64×1010 disintegrations  atom 2 s)(6.7×1021 atoms )=5.1×1012 disintegrations/s  Because 1 Bq is one disintegration per second, the activity is 5.1×1012 Bq. The activity in curies is given by (5.1×1012 disintegrations/s )(1Ci3.7×1010 disintegrations/s )=1.4×102Ci We have used only two significant figures in products of these calculations because we do not know the atomic weight of 90Sr to more than two significant figures without looking it up in a special source.

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