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Natural Radioactivity Natural Radioactivity was discovered at the end of the 19th centaury. Protons and neutrons we consider today as occupants of a nucleus. The electron flays out from a nuclei as a particle, is not occupant of nuclei. Simply is to show it use of the Heisenberg uncertainty principle: The electron cannot be in nuclei. Energy of the electron should be about 200 MeV, but such particles we do not observe in nature. One previous apparatus to investigate radioactivity can be seen in Fig 1. A magnetic field is perpendicular to the surface of the figure. Fig.1 A reader of this book should get explanations. One of the important physical laws is the Heisenberg uncertainty principle. This principle refers us we can’t localise particle because its momentum is equal to infinite. Instead, energy very often we take momentum of a particle. The momentum, which is multiplication of its mass and velocity, is a vector and we can give this quantity direction. After Heisenberg, we say: x Or for energy and time: p ≤ h/2, E If: ≤ h/2 x - uncertainty of location (dimension of a nuclei ~10-17 m), p - uncertainty of a momentum and h - Universal Plank’s constant (6.63 x 10-34 J s) At 1918, the Plank got the Nobel Price. In the second equation: E and are uncertainties of energy and time, respectively. Proton we marked as 1p1 and neutron as 1n0, (sometime we write down markers on one side of letters). The 1p1 (we called) proton has a charge one (q = +1 (1.6 x 10-19 Coulomb), and a mass equal to one. A proton has mass equal to 1.007825AM (average atomic mass) exactly. A neutron has no charge. Its big magnetic momentum indicates a neutron has internal charges. A 1p1 particle is one of nuclear particles. A particle is a polarised electron. A polarised electron means the electron, which has angular momentum and velocity correlated. Angular momentum is often called spin. particles move very fast, often with speed closely to the speed of light (3 x 10 8 m/s). The Einstein relativistic laws should apply to any calculation. Einstein was the Nobel price winner from 1931. Nobody understood his General Relativistic Theory and he got the Nobel Price for external photo-effect. Energy of disintegration we can calculate from a range in metals, for instance in Al (Aluminium). Sometimes, we write down the number and symbol of an atom. For example, 1H or 3H means 1Hydrogen and 3Hydrogens (Tritium), respectively. An Isotope we call a nucleus that has different numbers of neutrons. Mathematical shorthanded are often in use. I will say nothing about Auger’s electrons (read Oze) and internal conversion of . I will apply all shorts to secundus as example. We call ; Ts equal to 1012s called terra-seconds G =|= 109s =|= giga-seconds Ms =|= 106s =|= mega-seconds ks =|= 103s =|= kilo-seconds s =|= second =|= second ms =|= 10-3s =|= mili-seconds μs =|= 10-6s =|= micro-seconds ns =|= 10-9s =|= nano-seconds ps =|= 10-12s= | = pico-seconds For example, for another unity, we will call Volt and write down: nV, GV V or pV and so on. What is the primary and what is the secondary particle, we can discuss. Protons and neutrons have in Quarks, but these “particles” not exists alone. Quarks have charges but fractional of the primary charge, only. Feynman used to say, “As far as we know.” N = A – Z are number of neutrons in nucleus; A – Atomic Mass Z – Atomic Numbers All above are taking from the table of elements. Instead of Joule (J) as unity of energy in nuclear physic, we frequently use electronvolt (eV). One unit 1 eV is there if charge of one electron is moving across Potential Difference of one Volta. 1 eV = q x 1V = 1.6 x 10-19J Hydrogen has two “brothers.” The first “brother” called Deuterium and the second one called Tritium. The following figure shows two “brothers” of the Hydrogen. We call these isotopes. Fig.2 Tritium is radioactive and has virtually long Half Life Time; you can obtain it only in Nuclear Reaction. Half Life Time (T½) we called such period, after which half mass of radioactive material (radioactive isotope), left only. Life Time ( of radioactive material (isotope) is longer than T½. = T½ / Radioactive disintegrations have general formula. You can calculate many things from this. I = I0e- If: - disintegration constant (decay constant) I – radiation intensities after time () I0 –beginning intensity and are tree natural disintegrations of radioactivity. The last one is always a companion to or radiations. We know only one example so called “clean” decay. disintegration is nuclei of Helium, which consists of two protons and two neutrons. “Why Helium” we can ask? I will not explain a theory even many books have been written in this subject. Radioactive element, which produce particle, coming back in table of element two unities and its atomic mass diminished four units. Figure 3 shows creation of the particle. Fig.3 A recoil nucleus (A-4YZ-2) is usually at excited state, after emission of particle. A recoil nucleus when becoming normal, produce particle. Normal obtain from natural radioactivity not coming through piece of paper. particle strong ionised environment. Ionising means produce many ions (atoms with orbital electrons added o subtracted from atoms). Recoil nucleus often is radioactive it self. Next generations of and offcourse can be produces. Radioactive element, which produce particle going forward one place in a table of elements and its atomic mass, remains the same. The figure 4 shows creation of particle. Fig. 4 Both of radioactive decays and particle. This is shown in Figure 5 Fig. 5. K capture and positronium emissions belong to artificial radioactivity. K capture is taking off an electron from orbita of k (the first one) and capture it into a nucleus. Only a neutrino flays from a nucleus. At emission of the positronium, we observe positive electron (antiparticle to an electron). An element created going back one place at table of element and this atomic mass does not changed. This is shown in Figure 6. Fig. 6. An element produces positronium going back one place at table of element and this atomic mass does not changed. During production of positronium, neutrino is created. Positronium creation shows next figure. Fig.7. An element can stand on the top with radioactive “family” if it has very long live time. These are related to both decays and . All created elements (isotopes) are radioactive and all are finish with isotope of Lead, which are not radioactive. An isotope of a Lead means Lead with different atomic masses (different numbers of neutrons inside). We have tree radioactive series (family) of elements on the earth. In the first family or series on the top of its family is an isotope of a 238 U92 (238 Uranium), decayed to an isotope of 234 Th90 (234 Thorium) with a very long lifetime and equal to approximately 4.51 x 109 years. A mass of those “sisters” and “brothers” maybe calculated from the equation of 4n + 2, where n is equals to positive integers (1, 2, 3… and so on). In the second family on the top, is an isotope of decays to particle and 231 235 U92 (235 Uranium), Th90 (231Thorium) with a lifetime equal to 7.53 x 109 years. All members of this family have Atomic Mass calculated as 4n + 3. Next and last family is family of isotope of isotope of 228 232 Th90 (232Thorium), decays to Ra88 (228Radon) and particle with a lifetime of 1.39 x 1010 years. All members of this family have Atomic Mass calculated as 4n. We had another “family” in pas, but all members of this family decays and they should have Atomic mass equal to 4n+1. The longest lifetime from this family had isotope of Neptune and on the bottom of this family should bee isotope of 205 Tl81 (209Talium). Members of this family may be created in Nuclear Reactions. We have radioactive elements do not belong to families such as of 40K, 50V, 196Hg, 204Pb and all Transuranic (bigger than Uranium). Atomic Numbers (Z) we don’t write down very often. Instead of writing down the full name of an elements such as 205 Tl81 or different, we simple write down 205Tl. Thallium have 124 neutrons (205 - 81 = 124). and radiations are always companions to particle, as I have mentioned. If a nucleus that been created is in exciting state, this event produces particle, which is similar to light. This Phenomenon is similar to a light creation but with bigger energy (hν), where h – Plank constant and - frequency. Figure 8 shows this phenomenon, where * - recoil nucleus in exciting state and - normal state. Fig.8 Energy is equal distributed between particle and a coil nucleus. Is not equally distributed in a decay of particle, where the spectrum of energy is different. We say this energy spectrum is continuous (see chapter about neutrinos). Different counter can applied to radioactive particles. Standard counter is a G-M counter. We have also other counters like scintillating counter and semi-conductor counter, respectively. G-M counters profits ionisation by ionising particles entering volume of ionising chamber. Separate problems are quenching of avalanche of ions in the G-M counter, so counter can recorded next ionising particle. Very small scintillation time, can record tiny scintillations and record these by special electronic device called a multiplier. Each sort of radiation has different a scintillator. Semi conductor counters works tis way that ionised p-n junction in counters by entering of ionized radiation. I do not describe counters. Intensity of radiations we can measure using Becquerel (Bq) or kiore (Ci). 1 Bq = 1 disintegration/secund 1 Ci = 3.7 x 1010 disintegration/secund is equal to Radon, which is in balance with 1 g of Radium. 1 Ci = 3.7 x 1010 Bq. Ci is not a standard unit, but is widely recognised in the world. By applying an external magnetic or electric field, we can also observe momentum of a particle. Momentum of a particle giving as more information than energy of a particle, because also is giving its direction. We do it in a Wilson Chamber or in a Glaser bubble chamber. Wilson Chamber applied to superheated steam and bubble chamber applied to supercooled liquid (liquid hydrogen). Any ionising particles we can trace in both chambers. Superheated steam is over heated steam and supercooled liquid is over cooled liquid. The Glaser bubble chamber applied to high-energy particles because bigger density than the Wilson Chamber. Becquerel and couple of Curie were Nobel Price winners at the 1903. Maria Skłodowska (original name) did a PhD thesis and married P. Curie, taking his name. Her husband, Pierre, had horse carriage accident and died soon after. Marie Curie was the Nobel Price winner again, 1911, in Chemistry for discovery Polonium. She was one of the first causality of radiation. C.T.R. Wilson, F. Heisenberg and D. Glaser got a Nobel Prices in 1927, 1932 and 1957, respectively. R. P. Feynman got the Nobel Price at 1967.