Moscovium (Mc) is the name of element 115. 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 Mc isotopes are predicted to lie in the band from 299Mc to 295Mc. Peak half-life is predicted to be near 1/2 hour. Those isotopes cannot form. Longest half-lives for isotopes which can form, all of which are heavier than 316Mc, are predicted to be under a second. Any Mc which does form will disappear within 1000 sec of the event which led to its formation. This means that the element will never 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 Ref. 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 b- and b+), 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 368Mc 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 367Mc to 333Mc are predicted to decay by beta emission. All are predicted to have half-lives in the 0.001 - 1 sec range.
332Mc to 327Mc is a transition band. Half-lives are all predicted to be in the range 0.001 - 1 s, but the principal decay mode is sometimes beta emission and sometimes fission. Both modes are likely to be important in all isotopes.
Isotopes in the band 326Mc to 319Mc are predicted to decay by fission. All are predicted to have half-lives in the 0.001 - 1 sec range, except for 319Mc, which is predicted to have a half-life in the 10-06 - 0.001 sec range. This may be a minor difference, or may reflect the onset of instability with respect to fission.
Ref 1 predicts a gap from 318Mc to 307Mc, All isotopes in this band have half-lives under 10-06 sec, and most may not even survive the 10-14 sec needed to qualify as nuclides. Ref. 2 predicts all will have half-lives under 10-06, which is as short a time as that document reports. Fission is the predicted decay mode in both cases.
The band 306Mc to 302Mc is a transition region which contains significant differences between the predictions of Ref. 1 & 3, and those of Ref. 2. The former predict a rapid rise in half-life as A declines to a peak near 30 sec, followed by an abrupt drop as N approaches 184. This is similar to the pattern observed above N = 126. Principal decay mode shifts to alpha emission at 304Mc, indicating increased stability with respect to fission near N = 184. Ref. 2 predicts increasing half-life throughout the band, as well predicting that fission will dominate throughout the band.
Below 302Mc, 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 300Mc, and that even the most stable isotopes will have moderate half lives. Ref. 3 predicts that 299Mc will have a half-life exceeding 1500 sec, and that all of 298Mc to 295Mc will have half-lives exceeding 100 sec. There is disagreement on whether b+ / EC will be an important decay mode. Ref. 2 & 3 indicate that it will be, while Ref. 1 indicates that it will not be. Further comparison of predicted decay properties or evaluation of likely actual properties is out of scope for this article.
Observed half-lives in the band 290Mc to 287Mc are an order of magnitude shorter than half-lives of adjacent isotopes predicted in Ref. 3, both above and below the band.
The lightest isotope reported by any of Refs. 1 through 3 is 277Mc. There may be a few lighter nuclides with half-lives in the 10-14 - 10-09 sec range, but half-lives will quickly decline below the minimum needed for a nuclear drop to qualify as a nuclide.
OCCURRENCE
FORMATION
Moscovium isotopes are predicted from the neutron dripline to 319Mc. Most are beta emitters, but a few decay mainly by fission. All are short-lived. Between 318Mc and 294Mc, beta decay chains are truncated by fission at Z < 115. This band includes the relatively long-lived isotopes stabilized by neutron shell closure at N = 184. Below 294Mc, beta decay chains are interrupted by alpha-decaying nuclides, but the effect is the same; no light isotope of Mc can form. Material ejected from a disintegrating neutron star is expected to cover the entire band of possible nuclides, although quantity may be small at high A.
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 all significant Mc isotopes.
PERSISTENCE
All Mc 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 "Moscovium" addresses the element's atomic properties and chemistry in some detail. One point it does not make is that, while Mc nuclei can form, they do not persist long enough to reach an environment cool enough to allow chemical processes. The chemistry of Mc is entirely synthetic.
REFERENCES
1. "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. “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. "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".
| 9-Period Periodic Table of Elements | ||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
| 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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(10-08-20)