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Which of these elements is not “cooked up” by thermonuclear fusion processes in stellar interiors: carbon, silicon, chromium, bromine?

Short Answer

Expert verified

The Bromine among the given elements cannot be cooked up by thermonuclear fusion in stellar interiors.

Step by step solution

01

Thermonuclear Fusion

The fusion process in which the combination of two lighter nuclei to form heavier nuclei takes place by overcoming the repulsive force of protons due to thermal energy is called thermonuclear fusion. The necessary thermal energy depends on the charge of the atoms.

02

Identification of elements not cooked up by thermonuclear fusion in stellar interiors

Thermonuclear fusion is only possible up to middle-size nuclei. The atomic number 56 is a barrier to thermonuclear fusion, so nuclei of atomic numbers up to 56 undergo thermonuclear fusion.

The atomic number of Bromine is greater than 56, so it cannot be cooked up by thermonuclear fusion in stellar interiors.

Therefore, the Bromine among the given elements cannot be cooked up by thermonuclear fusion in stellar interiors.

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Most popular questions from this chapter

(a) How many atoms are contained in 1.0 kg of pure 235U? (b) How much energy, in joules, is released by the complete fashioning of 1.0 kg of 235U? Assume Q = 200 MeV . (c) For how long would this energy light 100 W a lamp?

Calculate the energy released in the fission reaction

U235+nCs141+Rb93+2n

Here are some atomic and particle masses.

U235235.04392uRb9392.92157uCs141140.91964un1.00866u

Figure 43-15 shows an early proposal for a hydrogen bomb. The fusion fuel is deuterium,H2. The high temperature and particle density needed for fusion are provided by an atomic bomb “trigger” that involves a U235orPu239fission fuel arranged to impress an imploding, compressive shock wave on the deuterium. The fusion reaction is

52H3He+4He+1H+2n

(a) Calculate Q for the fusion reaction. For needed atomic masses, see Problem 42. (b) Calculate the rating (see Problem 16) of the fusion part of the bomb if it contains 500 kg of deuterium, 30.0% of which undergoes fusion.

Question: Assume that immediately after the fission of U236according to Eq. 43-1, the resulting Xe140andSr94nuclei are just touching at their surfaces. (a) Assuming the nuclei to be spherical, calculate the electric potential energy associated with the repulsion between the two fragments. (Hint: Use Eq. 42-3 to calculate the radii of the fragments.) (b) Compare this energy with the energy released in a typical fission event.

In the deuteron–triton fusion reaction of Eq. 43-15, what is the kinetic energy of (a) the alpha particle and (b) the neutron? Neglect the relatively small kinetic energies of the two combining particles.

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