Bismuth-209 (209Bi) is the isotope of bismuth with the longest known half-life of any radioisotope that undergoes α-decay (alpha decay). It has 83 protons and a magic number[2] of 126 neutrons,[2] and an atomic mass of 208.9803987 amu (atomic mass units). Primordial bismuth consists entirely of this isotope.
Bismuth-209 was long thought to have the heaviest stable nucleus of any element, but in 2003, a research team at the Institut d’Astrophysique Spatiale in Orsay, France, discovered that 209Bi undergoes alpha decay with a half-life of approximately 19 exayears (1.9×1019, approximately 19 quintillion years),[3][4] over a billion times longer than the current estimated age of the universe.[5] The heaviest nucleus considered to be stable is now lead-208 and the heaviest stable monoisotopic element is gold as the 197Au isotope.
Theory had previously predicted a half-life of 4.6×1019 years. It had been suspected to be radioactive for a long time.[6] The decay event produces a 3.14 MeV alpha particle and converts the atom to thallium-205.[3][4]
Bismuth-209 occurs in the neptunium series decay chain.
Bismuth-209 will eventually form 205Tl if unperturbed:
If perturbed, it would join in lead-bismuth neutron capture cycle from lead-206/207/208 to bismuth-209, despite low capture cross sections. Even thallium-205, the decay product of bismuth-209, reverts to lead when fully ionized.[8]
Due to its extraordinarily long half-life, for nearly all applications 209Bi can still be treated as if it were non-radioactive. Its radioactivity is much less than that of human flesh, so it poses no meaningful hazard from radiation. Although 209Bi holds the half-life record for alpha decay, bismuth does not have the longest half-life of any radionuclide to be found experimentally—this distinction belongs to tellurium-128 (128Te) with a half-life estimated at 7.7 × 1024 years by double β-decay (double beta decay).[9][10][11]
The half-life of bismuth-209 was confirmed in 2012 by an Italian team in Gran Sasso who reported (2.01±0.08)×1019 years. They also reported an even longer half-life for alpha decay of bismuth-209 to the first excited state of thallium-205 (at 204 keV), was estimated to be 1.66×1021 years.[12] Even though this value is shorter than the measured half-life of tellurium-128, both alpha decays of bismuth-209 hold the record of the thinnest natural line widths of any measurable physical excitation, estimated respectively at ΔΕ~5.5×10−43 eV and ΔΕ~1.3×10−44 eV in application of the uncertainty principle of Heisenberg[13] (double beta decay would produce energy lines only in neutrinoless transitions, which has not been observed yet).
Applications
Because primordial bismuth is entirely bismuth-209, bismuth-209 is used for all of the normal applications attributed to bismuth, such as being used as a replacement for lead,[14][15] in cosmetics,[16][17] in paints,[18] and in several medicines such as Pepto-Bismol.[5][19][20] Alloys containing bismuth-209 such as bismuth bronze have been used for thousands of years.[21]
Synthesis of other elements
210Po can be manufactured by bombarding 209Bi with neutrons in a nuclear reactor.[22] Only around 100 grams of 210Po are produced each year.[23][22]209Po and 208Po can be made through the proton bombardment of 209Bi in a cyclotron.[24]Astatine can also be produced by bombarding forms of 209Bi with alpha particles.[25][26][27] Traces of 209Bi have also been used to creategold in nuclear reactors.[28][29]
Bismuth-209 is created in the final part of the s-process.[lower-alpha 1]
In the red giant stars of the asymptotic giant branch, the s-process (slow process) is ongoing to produce bismuth-209 and polonium-210 by neutron capture as the heaviest elements to be formed,[44] and the latter quickly decays.[44] All elements heavier than it are formed in the r-process, or rapid process, which occurs during the first fifteen minutes of supernovas.[45][44] Bismuth-209 is also created during the r-process.[44]
↑Red horizontal lines with a circle in their right ends represent neutron captures; blue arrows pointing up-left represent beta decays; green arrows pointing down-left represent alpha decays; cyan/light-green arrows pointing down-right represent electron captures.
↑ 4.04.1Marcillac, Pierre de; Noël Coron; Gérard Dambier; Jacques Leblanc; Jean-Pierre Moalic (April 2003). "Experimental detection of α-particles from the radioactive decay of natural bismuth". Nature422 (6934): 876–878. doi:10.1038/nature01541. PMID12712201. Bibcode: 2003Natur.422..876D.
↑ 5.05.1Kean, Sam (2011). The Disappearing Spoon (and other true tales of madness, love, and the history of the world from the Periodic Table of Elements). New York/Boston: Back Bay Books. pp. 158–160. ISBN978-0-316-051637.
↑Carvalho, H. G.; Penna, M. (1972). "Alpha-activity of The element Chemistry:Bismuth does not exist.". Lettere al Nuovo Cimento3 (18): 720. doi:10.1007/BF02824346.
↑J.W. Beeman (2012). "First Measurement of the Partial Widths of 209Bi Decay to the Ground and to the First Excited States". Physical Review Letters108 (6): 062501. doi:10.1103/PhysRevLett.108.062501. PMID22401058.
↑Maile, Frank J.; Pfaff, Gerhard; Reynders, Peter (2005). "Effect pigments—past, present and future". Progress in Organic Coatings54 (3): 150. doi:10.1016/j.porgcoat.2005.07.003.
↑Larsen, R. H.; Wieland, B. W.; Zalutsky, M. R. J. (1996). "Evaluation of an Internal Cyclotron Target for the Production of 211At via the 209Bi (α,2n)211At reaction". Applied Radiation and Isotopes47 (2): 135–143. doi:10.1016/0969-8043(95)00285-5. PMID8852627.
↑ 30.030.1Munzenberg; Hofmann, S.; Heßberger, F. P.; Reisdorf, W.; Schmidt, K. H.; Schneider, J. H. R.; Armbruster, P.; Sahm, C. C. et al. (1981). "Identification of element 107 by α correlation chains". Z. Phys. A300 (1): 107–108. doi:10.1007/BF01412623. Bibcode: 1981ZPhyA.300..107M.
↑Hessberger, F. P.; Münzenberg, G.; Hofmann, S.; Agarwal, Y. K.; Poppensieker, K.; Reisdorf, W.; Schmidt, K.-H.; Schneider, J. R. H. et al. (1985). "The new isotopes 258105,257105,254Lr and 253Lr". Z. Phys. A322 (4): 4. doi:10.1007/BF01415134. Bibcode: 1985ZPhyA.322..557H.
↑Hofmann, S.; Heßberger, F. P.; Ninov, V. et al. (1997). "Excitation function for the production of 265108 and 266109". Zeitschrift für Physik A358 (4): 377–378. doi:10.1007/s002180050343. Bibcode: 1997ZPhyA.358..377H.
↑Hofmann, S.; Ninov, V.; Heßberger, F. P.; Armbruster, P.; Folger, H.; Münzenberg, G.; Schött, H. J.; Popeko, A. G. et al. (1995). "The new element 111". Zeitschrift für Physik A350 (4): 281–282. doi:10.1007/BF01291182. Bibcode: 1995ZPhyA.350..281H.
↑Hofmann, S.; Heßberger, F. P.; Ackermann, D.; Münzenberg, G.; Antalic, S.; Cagarda, P.; Kindler, B.; Kojouharova, J. et al. (2002). "New results on elements 111 and 112". The European Physical Journal A14 (2): 147–157. doi:10.1140/epja/i2001-10119-x. Bibcode: 2002EPJA...14..147H.
↑Morita, K.; Morimoto, K. K.; Kaji, D.; Goto, S.; Haba, H.; Ideguchi, E.; Kanungo, R.; Katori, K. et al. (2004). "Status of heavy element research using GARIS at RIKEN". Nuclear Physics A734: 101–108. doi:10.1016/j.nuclphysa.2004.01.019. Bibcode: 2004NuPhA.734..101M.
↑Morita, Kosuke; Morimoto, Kouji; Kaji, Daiya; Akiyama, Takahiro; Goto, Sin-Ichi; Haba, Hiromitsu; Ideguchi, Eiji; Kanungo, Rituparna et al. (2004). "Experiment on the Synthesis of Element 113 in the Reaction 209Bi(70Zn, n)278113". Journal of the Physical Society of Japan73 (10): 2593–2596. doi:10.1143/JPSJ.73.2593. Bibcode: 2004JPSJ...73.2593M.
↑Barber, Robert C.; Karol, Paul J; Nakahara, Hiromichi; Vardaci, Emanuele; Vogt, Erich W. (2011). "Discovery of the elements with atomic numbers greater than or equal to 113 (IUPAC Technical Report)". Pure and Applied Chemistry83 (7): 1485. doi:10.1351/PAC-REP-10-05-01.
↑K. Morita; Morimoto, Kouji; Kaji, Daiya; Haba, Hiromitsu; Ozeki, Kazutaka; Kudou, Yuki; Sumita, Takayuki; Wakabayashi, Yasuo et al. (2012). "New Results in the Production and Decay of an Isotope, 278113, of the 113th Element". Journal of the Physical Society of Japan81 (10): 103201. doi:10.1143/JPSJ.81.103201. Bibcode: 2012JPSJ...81j3201M.