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Tin-121m (121m Sn) is a radioisotope and nuclear isomer of tin with a half-life of 43.9 years. In a normal thermal reactor, it has a very low fission product yield; thus, this isotope is not a significant contributor to nuclear waste. Fast fission or fission of some heavier actinides will produce tin-121 at higher yields. For example, its yield ...
This is a list of radioactive nuclides (sometimes also called isotopes), ordered by half-life from shortest to longest, in seconds, minutes, hours, days and years. Current methods make it difficult to measure half-lives between approximately 10 −19 and 10 −10 seconds. [1]
The single-row parameters, commented "!"=could be required; ..1 – 4 refer to the decay mode dm#= {{Isotopes/main/isotope | mn =! massnumber | sym =! symbol | link = isotope page: uranium-232 | ref = reference for the isotope-row | na =! natural abundancy (can be: synth, trace) | hl =! half-life (can be: stable) | dm1 =! decay mode #1 ...
The unstable tin isotopes have half-lives of less than a year except for tin-126, which has a half-life of about 230,000 years. Tin-100 and tin-132 are two of the very few nuclides with a "doubly magic" nucleus which despite being unstable, as they have very uneven neutron–proton ratios, are the endpoints beyond which tin isotopes lighter ...
Isotopes of tin. Main isotopes [9] Decay; abundance half-life (t 1/2) mode product; 112 Sn 0.970% stable: 114 Sn 0.66% stable 115 Sn 0.34% stable 116 Sn 14.5%
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Instead, the half-life is defined in terms of probability: "Half-life is the time required for exactly half of the entities to decay on average". In other words, the probability of a radioactive atom decaying within its half-life is 50%. [2] For example, the accompanying image is a simulation of many identical atoms undergoing radioactive decay.
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