Unpentseptium, Ups, is the temporary name for element 157. Isotopes are predicted between 485Ups and 428Ups. Reported half-lives are all less than 1 hr, and most are under 1 sec. Five isotopes in the band 456Ups to 449Ups can form. Beyond the region for which predictions are available, isotopes in the band 565Ups to 547Ups are likely. It is possible that all of them can form. 456Ups is expected to last for between 1 and 2 days. All other Ups isotopes will be gone less than 1000 sec after the event which led to their formation.
Nuclear properties[]
Between Z = 175 and Z near 130, one set of predictions for half-life and principal decay mode has been published[1]. [1] is publicly available and can be found via a search by paper title. Anyone interested in this element should study pp 15 and 18, which allow a given element to be understood in the context of adjacent nuclides.
These data are limited to nuclides for which N <= 333. Half-lives are presented in bands covering 3 orders of magnitude (0.001 sec to 1 sec, for instance) and are accurate to within +/- 3 orders of magnitude, which seems rather crude until the enormous extrapolation from what is known is taken into account, Minimum half-life is set at 10-9 sec, rather than 10-14 sec; which introduces a little uncertainty, but not a great deal because fission half-lives tend to transition quickly from values well above 10-9 sec to values well below 10-14 sec; and, while alpha-decay half-lives change more slowly, alpha emission is rarely dominant except where fission is suppressed. Significantly, beta-decay half-lives do not decline far below 10-3 sec, even for highly energetic decays, so there is little uncertainty about neutron-rich nuclides.
[1] does have one significant weakness. Nuclides which are beta-stable are identified by black squares, overwriting decay mode and half-life information. In many cases, these data can be estimated from adjacent nuclides.
No predictions exist for N > 333. The liquid-drop sketch developed in "The Final Element" for Z = 176 and above can be used to guess at where nuclides with Z < 175 and N > 333 may exist. Probability criteria for this purpose were set in "Nuclear Guesswork". Below Z = 171, it is necessary to look only at nuclear drops which are not expected to decay by neutron emission and require only normal amounts of structural correction energy in order to suppress spontaneous fission.
Predicted properties[]
[1] predicts isotopes ranging from 485Ups to 428Ups. Format used to display isotope properties is: isotope(s); half-life in seconds; dominant decay mode; comments.
485Ups - 483Ups; 10-9 - 10-6; fission.
482Ups - 480Ups; 10-6 - 0.001; fission.
479Ups; 10-9 - 10-6; fission. The short half-life of this isotope of Ups may reflect an even-N/odd-N effect.
478Ups; 0.001 - 1; fission. There is a jump in half-life of at least 3 orders of magnitude between 479Ups and 478Ups. Results in the band from 478Ups to 475Ups are not unrealistic if there is a shell closure at N = 318[2], but can't be called reliable.
477Ups; 1 - 1000; fission. This half-life seems long since its half-life against beta decay should be short. (also see 478Ups above)
476Ups - 475Ups; 0.001 - 1; fission. (also see 478Ups above)
474Ups - 466Ups; 1 - 1000; alpha. Both half-life and decay mode for these isotopes of Ups are not unrealistic if there are shell closures at both N = 308 and N = 318 and if half-lives are close to 1 sec. Shell closures do not appear to enhance beta-decay half-lives[3]. All nuclides in this band are at least four steps away from beta-stability, so beta decay is probably an important, although not dominant, mode.
465Ups - 459Ups; 0.001 - 1; beta.
458Ups; 1 - 1000; alpha. Beta decay in smaller nuclides does not show significant differences in half-life between odd-N and even-N nuclides[3]. The half-life predicted is realistic if it does not greatly exceed 1 sec.
457Ups 0.001 - 1; beta.
456Ups; 1 - 1000; alpha. As above, this is realistic if half-life is close to 1 sec.
455Ups; 0.001 - 1; beta.
454Ups; 1 - 1000; alpha. As above, this is realistic if half-life is close to 1 sec.
453Ups; 0.001 - 1; beta.
452Ups; 1 - 1000; alpha. As above, this is realistic if half-life is close to 1 sec.
451Ups - 440Ups; 0.001 - 1; alpha.
439Ups - 433Ups; 10-6 - 0.001; alpha, although fission may be a significant decay branch.
432Ups; 10-6 - 0.001; fission.
431Ups; 10-9 - 10-6; fission.
430Ups; 10-6 - 0.001; fission.
429Ups - 428Ups; 10-9 - 10-6; fission.
Below N = 308, this pattern is to be expected, given a neutron shell closure at N = 308. Above this point, predictions become more confusing.
Guessed properties[]
Drops in the band 565Ups to 547Ups are unlikely to decay by neutron emission and are stable against fission. Nuclides in this band are likely. Drops in the band 546Ups to 491Ups are unlikely to decay by neutron emission and require a moderate amount of structural correction energy. Nuclides in this band are unlikely. Below 491Ups, predictions are available.
Occurence[]
Formation[]
565Ups to 547Ups are likely to be nuclides. Depending on the neutron dripline's actual location, nuclei in this A range may form when material over 700 - 800 meters deep is ejected from a neutron star during a merger. (See "Neutron Star".). These can form directly as neutron star material breaks up or by beta-decay chains from lower-Z nuclides. They are outside the range in which half-life predictions exist. They are all very neutron-rich, which implies half-lives under 1 sec[1][3] are likely.
All nuclear drops in the band 485Ups to 428Ups are predicted to be nuclides. They are all too far from the neutron dripline to form directly. All beta-decay chains which would lead to 457Ups or heavier isotopes are terminated at Z < 157 by nuclides which fission so quickly that no beta-decay branch is possible.
In order to determine whether 456Ups and lighter isotopes can form, it is necessary to model the evolution of initial material by radioactive decay. Details of the model are provided in "Nuclear Decay Chains at High A" in this wiki. Per that model, 456Ups, 455Ups, 453Ups, 451Ups, and 449Ups can form.
It is implausible that neutron capture can form any Ups isotope.
Persistence[]
457Ups and heavier isotopes will decay to the vanishing point within 1000 sec after a neutron star merger which led to their formation.
456Ups is predicted to have a half-life in the 1 - 1000 sec range, and to be fed by a chain of beta-decaying nuclides with half-lives predicted to be under 1 sec. It will persist for up to 105 sec under maximum half-life assumptions. It is part of a beta-alpha-fission decay chain that persists for a maximum computed time under 125000 sec, so its own time-to-extinction wasn't tracked closely in the calculations.
455Ups, 453Ups, and 451Ups are each part of a long-lived decay chain, but will vanish quickly themselves.
449Ups has a precursor predicted to have a half-life in the 1 - 1000 sec range. As above, it's worst case time-to-vanish will be on the order of 105 sec.
No other isotopes of Ups persist for a significant time.
Calculations done under maximum half-life assumptions and with all nuclides initially populated still point to all isotopes of Ups vanishing within 105.5 (3.16E05) sec.
Atomic properties[]
Electron structure of Ups has been predicted by several sources (see "Extended Periodic Table" in Wikipedia). However, these predictions should be used with caution. Ups is large enough that nuclear shape may have an effect on electron structure, which might cause different isotopes of Ups to have different electronic structures. (That means it is no longer an element in the chemical sense.)
If this effect is small, Ups will be a f-block metal of the 8th period (possibly d block). As such, it would also be classed as a superactinide. Its electron configuration has been predicted[4] to be [Og] 5g18 6f14 7d3 8s2 8p21/2.
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.
- ↑ “The Highest Limiting Z in the Extended Periodic Table”; Y.K. Gambhir, A. Bhagwat, and M. Gupta; Journal of Physics G: Nuclear and Particle Physics. 42 (12): 125105. DOI:10.1088/0954 3899/42/12/ 125105.
- ↑ 3.0 3.1 3.2 "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".
- ↑ "Extended Periodic Table", Wikipedia.
Other references are found in the wiki articles cited.
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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(06-18-20)