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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. 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. 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. 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.
  4. "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".
  5. "Flerovium", Wikipedia article.
9-Period Periodic Table of Elements
1 1
H
2
He
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
Alkali metal Alkaline earth metal Lanthanide Actinide Superactinide Transition metal Post-transition metal Metalloid Other nonmetal Halogen Noble gas
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(10-10-20)