Flerovium (Fl) is the name of element 114. Wikipedia has an article which provides a lot of information about the element. This article will focus on things Wikipedia does not stress: heavy isotopes and formation.
The longest lived Fl isotopes are predicted to lie in the band from 298Fl to 292Fl. Peak half-life is predicted to be over 10 days. Those isotopes cannot form. Longest half-lives for isotopes which can form, all of which are heavier than 312Fl, are predicted to be under a second. Any Fl which does form will disappear within 1012 (a trillion) years of the event which led to its formation. This means that the element will be in an environment cool enough for it to interact chemically.
Nuclear properties[]
Information sources[]
This article uses two main resources chosen because of their independence from one another. A third source provides quantitative data over a limited range.
At least one document maps half-life and decay mode for elements below Z = 175 from the neutron dripline down to isotopes which are too neutron-poor to survive any appreciable length of time[1]. Maps on pp 15 & 18 address the entire (Z,N) region covered, but report only the dominant decay mode and report half-lives only to within a band three orders of magnitude wide (0.001 - 1 sec, for example). More detailed estimates of these properties can be extracted from maps on pp 11 & 12, but only for a limited range of Z and N. Half-life data are reported by colors, which makes numerical estimates laborious to produce. This document is connected to Japan's KTUY model.
An independent map of half-lives and decay modes exists.[2] This one is limited to A = 339, as well as to Z = 132. It does not show short-lived isotopes well, and gives half-lives only within rather broad and awkward bands. It does show multiple decay modes for single nuclides. It originates from models used by the Russian agency JINR, so is completely independent of [1].
Japan Atomic Energy Agency (JAEA) maintains an on-line chart of nuclides which includes decay properties of many predicted nuclides[3] - unlike charts published by Korea Atomic Energy Research Institute (KAERI) or the (U.S.) National Nuclear Data Center (NNDC). This chart gives separate numerical values for partial half-lives against fission, beta emission (both β- and β+), and alpha emission. These appear to be systematically too long, but are probably reliable to within an order of magnitude.
Predicted properties[]
Even-N isotopes from the neutron dripline down to 357Fl are predicted to have half-lives in the 0.001 - 1 sec range. (Half-lives aren't reported directly, but the properties of beta decay indicate that half-lives close to 0.001 sec are likely.[4]) In some cases, fission is predicted to be the dominant decay mode, but both fission and beta emission are likely to be significant modes for all isotopes. Odd-N drops in this band decay by neutron emission.
Isotopes in the band 356Fl to 323Fl are predicted to decay by beta emission, with two exceptions. All are predicted to have half-lives in the 0.001 - 1 sec range. The two exceptions, 330Fl and 324Fl have a dominant fission decay mode. Both beta emission and fission are likely to be important in all isotopes, at least at the lower end of this band.
Fission is predicted to become the principal decay mode in the 322Fl to 315Fl band. Half lives are predicted to show a pronounced difference between odd-N and even-N isotopes, and also to decline as A decreases. Heavier odd-N isotopes are predicted to have half-lives exceeding 1 sec, declining to the 10-6 - 0.001 sec range at the band's low-A end. Even-N isotopes are predicted to decay more quickly.
[1] predicts a gap from 314Fl to 306Fl, All isotopes in this band have half-lives under 10-9 sec, and most may not even survive the 10-14 sec needed to qualify as nuclides. [2] predicts all will have half-lives under 10-6, which is as short a time as that document reports. Fission is the predicted decay mode in both cases.
The band 305Fl to 303Fl is a transition region which contains significant differences between the predictions of [1] & [3], and those of [2]. The former predict a rapid rise in half-life as A declines, and a transition to alpha emission as the dominant mode of decay at 303Fl indicating increased stability with respect to fission near N = 184. [2] predicts that fission will dominate throughout the band, and that half-lives will be shorter
Below 303Fl, there have been many studies of decay properties. There does seem to be consensus that fission will not be a significant decay mode, that half-lives will peak just below 300Fl, and that fairly long half-lives will be possible near N = 184. [3] predicts that three alpha-decaying isotopes, 298Fl, 297Fl, and 296Fl will have half-lives exceeding 10 days, and that two others, 293Fl and 292Fl will have half-lives exceeding 1 day. Positive beta (b+ / EC) and alpha are predicted to be about equally important in 293Fl. Further comparison of predicted decay properties or evaluation of likely actual properties is out of scope for this article.
Observed half-lives are found in the band 290Fl to 284Fl. The lighter isotopes have half-lives comparable to the half-lives of adjacent isotopes, as predicted in [3], but 289Fl has an observed half-life around 0.02 times the predicted half-lives for 290Fl and 291Fl. In addition, there is an unconfirmed report that 290Fl has been observed and has a half-life of 19 sec.[5]
The lightest isotope reported by any of [1], [2] or [3] is 273Fl. There may be a few lighter nuclides with half-lives in the 10-14 - 10-9 sec range, but half-lives will quickly decline below the minimum needed for a nuclear drop to qualify as a nuclide.
Occurence[]
Formation[]
Flerovium isotopes exist between the neutron dripline and 319Fl most decay mainly by beta emission; but some, particularly at the light end of the band, decay mainly by fission. All are short-lived. Between 318Fl and 294Fl, beta decay chains end in fission at Z < 114. This band includes relatively long-lived nuclides stabilized by the N = 184 neutron shell closure. Below 294Fl, beta decay chains end in alpha decaying nuclides, but at Z < 114. Material ejected from a disintegrating neutron star is expected to cover the entire A range over which Fl isotopes can form. See Superheavy Island is Deserted for more information.
Neutron capture may be able to produce nuclides up to A around 380 before fission attrition stops further growth. Neutron capture is expected to contribute to formation of almost all Fl isotopes.
Persistence[]
All Fl isotopes which can form have short half-lives and are the result of beta decay of short-lived nuclides. The element is expected to disappear completely less than 1000 sec after a neutron star merger of similar event which led to its formation.
Atomic properties[]
Wikipedia's article "Flerovium" addresses the element's atomic properties and chemistry in some detail. One point it does not make is that, while Fl nuclei can form, they do not persist long enough to reach an environment cool enough to allow chemical processes. The chemistry of Fl is entirely synthetic.
References[]
- ↑ 1.0 1.1 1.2 1.3 1.4 "Decay Modes and a Limit of Existence of Nuclei"; H. Koura; 4th Int. Conf. on the Chemistry and Physics of Transactinide Elements; Sept. 2011.
- ↑ 2.0 2.1 2.2 2.3 2.4 “Systematic Study of Decay Properties of Heaviest Elements.”; Y. M. Palenzuela, L. F. Ruiza, A. Karpov, and W. Greiner; Bulletin of the Russian Academy of Sciences, Physics. Vol . 76, No.11, pp 1165 – 1177; 2012
- ↑ 3.0 3.1 3.2 3.3 3.4 "Chart of the Nuclides, 2014", Japan Atomic Energy Agency; website available using "chart of nuclides" and "JAEA" as internet search terms.
- ↑ "Nuclear Properties for Astrophysical Applications"; P. Moller & J. R. Nix; Los Alamos National Laboratory website; search by "LANL, T2", then "Nuclear Properties for Astrophysical Applications".
- ↑ "Flerovium", Wikipedia article.
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| 1 | 1 H |
2 He | ||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
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| 2 | 3 Li |
4 Be |
5 B |
6 C |
7 N |
8 O |
9 F |
10 Ne | ||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
| 3 | 11 Na |
12 Mg |
13 Al |
14 Si |
15 P |
16 S |
17 Cl |
18 Ar | ||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
| 4 | 19 K |
20 Ca |
21 Sc |
22 Ti |
23 V |
24 Cr |
25 Mn |
26 Fe |
27 Co |
28 Ni |
29 Cu |
30 Zn |
31 Ga |
32 Ge |
33 As |
34 Se |
35 Br |
36 Kr | ||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
| 5 | 37 Rb |
38 Sr |
39 Y |
40 Zr |
41 Nb |
42 Mo |
43 Tc |
44 Ru |
45 Rh |
46 Pd |
47 Ag |
48 Cd |
49 In |
50 Sn |
51 Sb |
52 Te |
53 I |
54 Xe | ||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
| 6 | 55 Cs |
56 Ba |
57 La |
58 Ce |
59 Pr |
60 Nd |
61 Pm |
62 Sm |
63 Eu |
64 Gd |
65 Tb |
66 Dy |
67 Ho |
68 Er |
69 Tm |
70 Yb |
71 Lu |
72 Hf |
73 Ta |
74 W |
75 Re |
76 Os |
77 Ir |
78 Pt |
79 Au |
80 Hg |
81 Tl |
82 Pb |
83 Bi |
84 Po |
85 At |
86 Rn | ||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
| 7 | 87 Fr |
88 Ra |
89 Ac |
90 Th |
91 Pa |
92 U |
93 Np |
94 Pu |
95 Am |
96 Cm |
97 Bk |
98 Cf |
99 Es |
100 Fm |
101 Md |
102 No |
103 Lr |
104 Rf |
105 Db |
106 Sg |
107 Bh |
108 Hs |
109 Mt |
110 Ds |
111 Rg |
112 Cn |
113 Nh |
114 Fl |
115 Mc |
116 Lv |
117 Ts |
118 Og | ||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
| 8 | 119 Uue |
120 Ubn |
121 Ubu |
122 Ubb |
123 Ubt |
124 Ubq |
125 Ubp |
126 Ubh |
127 Ubs |
128 Ubo |
129 Ube |
130 Utn |
131 Utu |
132 Utb |
133 Utt |
134 Utq |
135 Utp |
136 Uth |
137 Uts |
138 Uto |
139 Ute |
140 Uqn |
141 Uqu |
142 Uqb |
143 Uqt |
144 Uqq |
145 Uqp |
146 Uqh |
147 Uqs |
148 Uqo |
149 Uqe |
150 Upn |
151 Upu |
152 Upb |
153 Upt |
154 Upq |
155 Upp |
156 Uph |
157 Ups |
158 Upo |
159 Upe |
160 Uhn |
161 Uhu |
162 Uhb |
163 Uht |
164 Uhq |
165 Uhp |
166 Uhh |
167 Uhs |
168 Uho |
169 Uhe |
170 Usn |
171 Usu |
172 Usb | ||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
| 9 | 173 Ust |
174 Usq | ||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
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