Thorium-230
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Thorium-230
Main isotopes of thorium (90Th)
Iso­tope Decay
abun­dance half-life (t1/2) mode pro­duct
227Th trace 18.68 d ? 223Ra
228Th trace 1.9116 y ? 224Ra
229Th trace 7917 y[1] ? 225Ra
230Th 0.02% 75400 y ? 226Ra
231Th trace 25.5 h ?- 231Pa
232Th 99.98% 1.405×1010 y ? 228Ra
234Th trace 24.1 d ?- 234Pa
Standard atomic weight Ar, standard(Th)

Thorium (90Th) has seven naturally occurring isotopes but none are stable. One isotope, 232Th, is relatively stable, with a half-life of 1.405×1010 years, considerably longer than the age of the Earth, and even slightly longer than the generally accepted age of the universe. This isotope makes up nearly all natural thorium, so thorium was considered to be mononuclidic. However, in 2013, IUPAC reclassified thorium as binuclidic, due to large amounts of 230Th in deep seawater. Thorium has a characteristic terrestrial isotopic composition and thus a standard atomic weight can be given.

Thirty-one radioisotopes have been characterized, with the most stable being 232Th, 230Th with a half-life of 75,380 years, 229Th with a half-life of 7,917 years,[1] and 228Th with a half-life of 1.92 years. All of the remaining radioactive isotopes have half-lives that are less than thirty days and the majority of these have half-lives that are less than ten minutes. One isotope, 229Th, has a nuclear isomer (or metastable state) with a remarkably low excitation energy,[3] recently measured to be 8.28 ± 0.17 eV.[4] It has been proposed to perform laser spectroscopy of the 229Th nucleus and use the low-energy transition for the development of a nuclear clock of extremely high accuracy.[5][6]

The known isotopes of thorium range in mass number from 208[7] to 238.

## List of isotopes

Nuclide
[n 1]
Historic
name
Z N Isotopic mass (u)
[n 2][n 3]
Half-life
[n 4]
Decay
mode

[n 5]
Daughter
isotope

[n 6]
Spin and
parity
[n 7][n 8]
Natural abundance (mole fraction)
Excitation energy Normal proportion Range of variation
208Th[7] 90 118 208.01791(4) 1.7(+1.7-0.6) ms ? 204Ra 0+
209Th[8] 90 119 209.01772(11) 7(5) ms
[3.8(+69-15)]
? 205Ra 5/2-#
210Th 90 120 210.015075(27) 17(11) ms
[9(+17-4) ms]
? 206Ra 0+
?+ (rare) 210Ac
211Th 90 121 211.01493(8) 48(20) ms
[0.04(+3-1) s]
? 207Ra 5/2-#
?+ (rare) 211Ac
212Th 90 122 212.01298(2) 36(15) ms
[30(+20-10) ms]
? (99.7%) 208Ra 0+
?+ (.3%) 212Ac
213Th 90 123 213.01301(8) 140(25) ms ? 209Ra 5/2-#
?+ (rare) 213Ac
214Th 90 124 214.011500(18) 100(25) ms ? 210Ra 0+
215Th 90 125 215.011730(29) 1.2(2) s ? 211Ra (1/2-)
216Th 90 126 216.011062(14) 26.8(3) ms ? (99.99%) 212Ra 0+
?+ (.006%) 216Ac
216m1Th 2042(13) keV 137(4) µs (8+)
216m2Th 2637(20) keV 615(55) ns (11-)
217Th 90 127 217.013114(22) 240(5) µs ? 213Ra (9/2+)
218Th 90 128 218.013284(14) 109(13) ns ? 214Ra 0+
219Th 90 129 219.01554(5) 1.05(3) µs ? 215Ra 9/2+#
?+ (10-7%) 219Ac
220Th 90 130 220.015748(24) 9.7(6) µs ? 216Ra 0+
EC (2×10-7%) 220Ac
221Th 90 131 221.018184(10) 1.73(3) ms ? 217Ra (7/2+)
222Th 90 132 222.018468(13) 2.237(13) ms ? 218Ra 0+
EC (1.3×10-8%) 222Ac
223Th 90 133 223.020811(10) 0.60(2) s ? 219Ra (5/2)+
224Th 90 134 224.021467(12) 1.05(2) s ? 220Ra 0+
?+?+ (rare) 224Ra
225Th 90 135 225.023951(5) 8.72(4) min ? (90%) 221Ra (3/2)+
EC (10%) 225Ac
226Th 90 136 226.024903(5) 30.57(10) min ? 222Ra 0+
227Th Radioactinium 90 137 227.0277041(27) 18.68(9) d ? 223Ra 1/2+ Trace[n 9]
228Th Radiothorium 90 138 228.0287411(24) 1.9116(16) y ? 224Ra 0+ Trace[n 10]
CD (1.3×10-11%) 208Pb
20O
229Th 90 139 229.031762(3) 7.34(16)×103 y ? 225Ra 5/2+ Trace[n 11]
229mTh 8.3(2) eV[4] 7(1) µs[9] IT 229Th 3/2+
230Th[n 12] Ionium 90 140 230.0331338(19) 7.538(30)×104 y ? 226Ra 0+ 0.0002(2)[n 13]
CD (5.6×10-11%) 206Hg
24Ne
SF (5×10-11%) (Various)
231Th Uranium Y 90 141 231.0363043(19) 25.52(1) h ?- 231Pa 5/2+ Trace[n 9]
? (10-8%) 227Ra
232Th[n 14] Thorium 90 142 232.0380553(21) 1.405(6)×1010 y ? 228Ra 0+ 0.9998(2)
?-?- (rare) 232U
SF (1.1×10-9%) (various)
CD (2.78×10-10%) 182Yb
26Ne
24Ne
233Th 90 143 233.0415818(21) 21.83(4) min ?- 233Pa 1/2+
234Th Uranium X1 90 144 234.043601(4) 24.10(3) d ?- 234mPa 0+ Trace[n 13]
235Th 90 145 235.04751(5) 7.2(1) min ?- 235Pa (1/2+)#
236Th 90 146 236.04987(21)# 37.5(2) min ?- 236Pa 0+
237Th 90 147 237.05389(39)# 4.8(5) min ?- 237Pa 5/2+#
238Th 90 148 238.0565(3)# 9.4(20) min ?- 238Pa 0+
1. ^ mTh – Excited nuclear isomer.
2. ^ ( ) – Uncertainty (1σ) is given in concise form in parentheses after the corresponding last digits.
3. ^ # – Atomic mass marked #: value and uncertainty derived not from purely experimental data, but at least partly from trends from the Mass Surface (TMS).
4. ^ Bold half-life – nearly stable, half-life longer than age of universe.
5. ^ Modes of decay:
 CD: Cluster decay EC: Electron capture IT: Isomeric transition
6. ^ Bold symbol as daughter – Daughter product is stable.
7. ^ ( ) spin value – Indicates spin with weak assignment arguments.
8. ^ # – Values marked # are not purely derived from experimental data, but at least partly from trends of neighboring nuclides (TNN).
9. ^ a b Intermediate decay product of 235U
10. ^ Intermediate decay product of 232Th
11. ^ Intermediate decay product of 237Np
12. ^ Used in Uranium-thorium dating
13. ^ a b Intermediate decay product of 238U
14. ^

## Uses

Thorium has been suggested for use in thorium-based nuclear power.

It is radioactive, in many countries the use of thorium in consumer products is banned or discouraged.

It is currently used in cathodes of vacuum tubes, for a combination of physical stability at high temperature and a low work energy required to remove an electron from its surface.

It has, for about a century, been used in mantles of gas and vapor lamps such as gas lights and camping lanterns.

### Low dispersion lenses

Thorium was also used in certain glass elements of Aero-Ektar lenses made by Kodak during World War II. Thus they are mildly radioactive.[10] Two of the glass elements in the f/2.5 Aero-Ektar lenses are 11% and 13% thorium by weight. The thorium-containing glasses were used because they have a high refractive index with a low dispersion (variation of index with wavelength), a highly desirable property. Many surviving Aero-Ektar lenses have a tea colored tint, possibly due to radiation damage to the glass.

As these lenses were used for aerial reconnaissance, the radiation level is not high enough to fog film over a short period. This would indicate the radiation level is reasonably safe. However, when not in use, it would be prudent to store these lenses as far as possible from normally inhabited areas; allowing the inverse square relationship to attenuate the radiation.[11]

## Actinides vs. fission products

Actinides and fission products by half-life
Actinides[12] by decay chain Half-life
range (y)
Fission products of 235U by yield[13]
4n 4n+1 4n+2 4n+3
4.5-7% 0.04-1.25% <0.001%
228RaNo 4-6 + 155Euþ
244Cm? 241Pu? 250Cf 227AcNo 10-29 90Sr 85Kr 113mCdþ
232U? 238Pu? 243Cm? 29-97 137Cs 151Smþ 121mSn
248Bk[14] 249Cf? 242mAm? 141-351

No fission products
have a half-life
in the range of
100-210 k years ...

241Am? 251Cf?[15] 430-900
226RaNo 247Bk 1.3 k - 1.6 k
240Pu 229Th 246Cm? 243Am? 4.7 k - 7.4 k
245Cm? 250Cm 8.3 k - 8.5 k
239Pu? 24.1 k
230ThNo 231PaNo 32 k - 76 k
236Np? 233U? 234UNo ? 99Tc? 126Sn
248Cm 242Pu 327 k - 375 k 79Se?
1.53 M 93Zr
237Np? 2.1 M - 6.5 M 135Cs? 107Pd
236U 247Cm? 15 M - 24 M 129I?
244Pu 80 M

... nor beyond 15.7 M years[16]

232ThNo 238UNo 235U?No 0.7 G - 14.1 G

Legend for superscript symbols
?  has thermal neutron capture cross section in the range of 8-50 barns
fissile
metastable isomer
No  primarily a naturally occurring radioactive material (NORM)
þ  neutron poison (thermal neutron capture cross section greater than 3k barns)
+  range 4-97 y: Medium-lived fission product
?  over 200,000 y: Long-lived fission product

## Notable isotopes

### Thorium-228

228Th is an isotope of thorium with 138 neutrons. It was once named Radiothorium, due to its occurrence in the disintegration chain of thorium-232. It has a half-life of 1.9116 years. It undergoes alpha decay to 224Ra. Occasionally it decays by the unusual route of cluster decay, emitting a nucleus of 20O and producing stable 208Pb. It is a daughter isotope of 232U.

228Th has an atomic weight of 228.0287411 grams/mole.

### Thorium-229

229Th is a radioactive isotope of thorium that decays by alpha emission with a half-life of 7917 years.[1]229Th is produced by the decay of uranium-233, and its principal use is for the production of the medical isotopes actinium-225 and bismuth-213.[17]

#### Thorium-229m

In 1976, gamma ray spectroscopy first indicated that 229Th has a nuclear isomer, 229mTh, with a remarkably low excitation energy.[18] At that time the energy was inferred to be below 100 eV, purely based on the non-observation of the isomer's direct decay. However, in 1990, further measurements led to the conclusion that the energy is almost certainly below 10 eV,[19] making the isomer to be the one of lowest known excitation energy. In the following years, the energy was further constrained to 3.5 ± 1.0 eV, which was for a long time the accepted energy value.[20] Such low energy soon raised some interest as it conceptually allows for direct laser excitation of the nuclear state,[21] which leads to some interesting potential applications, e.g. the development of a nuclear clock of very high accuracy[5][6] or as a qubit for quantum computing.[22]

Nuclear laser excitation of 229mTh and therefore also the development of a nuclear clock has so far been impeded by an insufficient knowledge about the isomeric properties. A precise knowledge of the isomeric energy is of particular importance in this context, as it determines the required laser technology and shortens the scanning times when searching for the direct excitation. This triggered a multitude of investigations, both theoretical and experimental, trying to determine the transition energy precisely and to specify other properties of the isomeric state of 229Th (such as the lifetime and the magnetic moment).[23]

The direct observation of photons emitted in the isomeric decay would significantly help to pin down the isomeric energy value. Unfortunately, until today, there has been no fully conclusive report on the detection of photons emitted in the decay of 229mTh. Instead, improved gamma ray spectroscopy measurements using an advanced high-resolution X-ray microcalorimeter were carried out in 2007, yielding a new value for the transition energy of E = 7.6 ± 0.5 eV,[24] corrected to E = 7.8 ± 0.5 eV in 2009.[25] This shift in isomeric energy from 3.5 eV to 7.8 eV possibly explains why several early attempts to directly observe the transition were unsuccessful. Still, most of the recent searches for light emitted in the isomeric decay failed to observe any signal,[26][27][28][29] pointing towards a potentially strong non-radiative decay channel. A direct detection of photons emitted in the isomeric decay was claimed in 2012[30] and again in 2018.[31] However, both reports are currently subject to controversial discussions within the community.[32][33]

A direct detection of electrons being emitted in the internal conversion decay channel of 229mTh was achieved in 2016.[34] However, at the time the isomer's transition energy could only be weakly constrained to between 6.3 and 18.3 eV. Finally, in 2019, non-optical electron spectroscopy of the internal conversion electrons emitted in the isomeric decay allowed for a determination of the isomer's excitation energy to 8.28 ± 0.17 eV, which poses today's most precise energy value.[4] However, this value appears at odds with the 2018 preprint showing that a similar signal as an 8.4 eV Xenon VUV photon can be shown, but with about 1.3+0.2
-0.1
eV less energy and an 1880 s lifetime.[31] In that paper, 229Th was embedded in SiO2, possibly resulting in an energy shift and altered lifetime, although the states involved are primarily nuclear, shielding them from electronic interactions.

As a peculiarity of the extremely low excitation energy, the lifetime of 229mTh very much depends on the electronic environment of the nucleus. In 229Th ions, the internal conversion decay channel is energetically forbidden, as the isomeric energy is below the energy that is required for further ionization of Th+. This leads to a lifetime that may approach the radiative lifetime of 229mTh, for which no measurement exists, but which has been theoretically predicted to be in the range between 103 to 104 seconds.[35][36] Experimentally, for 229mTh2+ and 229mTh3+ ions, an isomeric lifetime of longer than 1 minute was found.[34] Opposed to that, in neutral 229Th atoms the internal conversion decay channel is allowed, leading to an isomeric lifetime which is reduced by 9 orders of magnitude to about 10 microseconds.[37][35] A lifetime in the range of a few microseconds was indeed confirmed in 2017 for neutral, surface bound 229mTh atoms, based on the detection of the internal conversion decay signal.[9]

In a 2018 experiment, it was possible to perform a first laser-spectroscopic characterization of the nuclear properties of 229mTh.[38] In this experiment, laser spectroscopy of the 229Th atomic shell was conducted using a 229Th2+ ion cloud with 2% of the ions in the nuclear excited state. This allowed to probe for the hyperfine shift induced by the different nuclear spin states of the ground and the isomeric state. In this way, a first experimental value for the magnetic dipole and the electric quadrupole moment of 229mTh could be inferred. In 2019, the isomer's excitation energy was constrained to 8.28 ± 0.17 eV based on the direct detection of internal conversion electrons[4] and a secure population of 229mTh from the nuclear ground state was achieved by excitation of the 29 keV nuclear excited state via synchrotron radiation.[39] The 29189.93 eV excited state of 229Th decays to the isomeric state with a probability of 90%. Both measurements are further important steps towards the development of a nuclear clock. Also gamma spectroscopy experiments confirmed the 8.3 eV energy splitting from the distance to the 29189.93 eV level.[40] 8.28 eV (150 nm) is reachable as a 7th harmonic of an Ytterbium fiber laser by VUV frequency comb.[41][42][43][44] cw phase matching for harmonic generation may be available.[45]

### Thorium-230

230Th is a radioactive isotope of thorium that can be used to date corals and determine ocean current flux. Ionium was a name given early in the study of radioactive elements to the 230Th isotope produced in the decay chain of 238U before it was realized that ionium and thorium are chemically identical. The symbol Io was used for this supposed element. (The name is still used in ionium-thorium dating.)

### Thorium-231

231Th has 141 neutrons. It is the decay product of uranium-235. It is found in very small amounts on the earth and has a half-life of 25.5 hours.[46] When it decays, it emits a beta ray and forms protactinium-231. It has a decay energy of 0.39 MeV. It has a mass of 231.0363043 grams/mole.

### Thorium-232

232Th is the only primordial nuclide of thorium and makes up effectively all of natural thorium, with other isotopes of thorium appearing only in trace amounts as relatively short-lived decay products of uranium and thorium.[47] The isotope decays by alpha decay with a half-life of 1.405×1010 years, over three times the age of the Earth and greater than the age of the universe. Its decay chain is the thorium series, eventually ending in lead-208. The remainder of the chain is quick; the longest half-lives in it are 5.75 years for radium-228 and 1.91 years for thorium-228, with all other half-lives totaling less than 15 days.[48]

232Th is a fertile material able to absorb a neutron and undergo transmutation into the fissile nuclide uranium-233, which is the basis of the thorium fuel cycle.[49] In the form of Thorotrast, a thorium dioxide suspension, it was used as a contrast medium in early X-ray diagnostics. Thorium-232 is now classified as carcinogenic.[50]

### Thorium-233

233Th is an isotope of thorium that decays into protactinium-233 through beta decay. It has a half-life of 21.83 minutes.[51]

### Thorium-234

234Th is an isotope of thorium whose nuclei contain 144 neutrons. 234Th has a half-life of 24.1 days, and when it decays, it emits a beta particle, and in doing so, it transmutes into protactinium-234. 234Th has a mass of 234.0436 atomic mass units (amu), and it has a decay energy of about 270 keV (kiloelectronvolts). Uranium-238 usually decays into this isotope of thorium (although in rare cases it can undergo spontaneous fission instead).

## References

1. ^ a b c Varga, Z.; Nicholl, A.; Mayer, K. (2014). "Determination of the 229Th half-life". Physical Review C. 89 (6): 064310. doi:10.1103/PhysRevC.89.064310.
2. ^ Meija, Juris; et al. (2016). "Atomic weights of the elements 2013 (IUPAC Technical Report)". Pure and Applied Chemistry. 88 (3): 265-91. doi:10.1515/pac-2015-0305.
3. ^ E. Ruchowska (2006). "Nuclear structure of 229Th". Phys. Rev. C. 73 (4): 044326. Bibcode:2006PhRvC..73d4326R. doi:10.1103/PhysRevC.73.044326.
4. ^ a b c d Seiferle, B.; von der Wense, L.; Bilous, P.V.; Amersdorffer, I.; Lemell, C.; Libisch, F.; Stellmer, S.; Schumm, T.; Düllmann, C.E.; Pálffy, A.; Thirolf, P.G. (12 September 2019). "Energy of the 229Th nuclear clock transition". Nature. 573 (7773): 243-246. arXiv:1905.06308. doi:10.1038/s41586-019-1533-4. PMID 31511684.
5. ^ a b Peik, E.; Tamm, Chr. (2003-01-15). "Nuclear laser spectroscopy of the 3.5 eV transition in 229Th" (PDF). Europhysics Letters. 61 (2): 181-186. Bibcode:2003EL.....61..181P. doi:10.1209/epl/i2003-00210-x. Archived from the original (PDF) on 2013-12-16. Retrieved .
6. ^ a b Campbell, C.; Radnaev, A.G.; Kuzmich, A.; Dzuba, V.A.; Flambaum, V.V.; Derevianko, A. (2012). "A single ion nuclear clock for metrology at the 19th decimal place". Phys. Rev. Lett. 108 (12): 120802. arXiv:1110.2490. Bibcode:2012PhRvL.108l0802C. doi:10.1103/PhysRevLett.108.120802. PMID 22540568.
7. ^ a b
8. ^ H. Ikezoe; et al. (1996). "alpha decay of a new isotope of 209Th". Physical Review C. 54 (4): 2043-2046. Bibcode:1996PhRvC..54.2043I. doi:10.1103/PhysRevC.54.2043. PMID 9971554.
9. ^ a b Seiferle, B.; von der Wense, L.; Thirolf, P.G. (2017). "Lifetime measurement of the 229Th nuclear isomer". Phys. Rev. Lett. 118: 042501. arXiv:1801.05205. doi:10.1103/PhysRevLett.118.042501. PMID 28186791.
10. ^ f2.5 Aero Ektar Lenses Some images.
11. ^ Michael S. Briggs (January 16, 2002). "Aero-Ektar Lenses". Archived from the original on August 12, 2015. Retrieved .
12. ^ Plus radium (element 88). While actually a sub-actinide, it immediately precedes actinium (89) and follows a three-element gap of instability after polonium (84) where no nuclides have half-lives of at least four years (the longest-lived nuclide in the gap is radon-222 with a half life of less than four days). Radium's longest lived isotope, at 1,600 years, thus merits the element's inclusion here.
13. ^ Specifically from thermal neutron fission of U-235, e.g. in a typical nuclear reactor.
14. ^ Milsted, J.; Friedman, A. M.; Stevens, C. M. (1965). "The alpha half-life of berkelium-247; a new long-lived isomer of berkelium-248". Nuclear Physics. 71 (2): 299. Bibcode:1965NucPh..71..299M. doi:10.1016/0029-5582(65)90719-4.
"The isotopic analyses disclosed a species of mass 248 in constant abundance in three samples analysed over a period of about 10 months. This was ascribed to an isomer of Bk248 with a half-life greater than 9 y. No growth of Cf248 was detected, and a lower limit for the ?- half-life can be set at about 104 y. No alpha activity attributable to the new isomer has been detected; the alpha half-life is probably greater than 300 y."
15. ^ This is the heaviest nuclide with a half-life of at least four years before the "Sea of Instability".
16. ^ Excluding those "classically stable" nuclides with half-lives significantly in excess of 232Th; e.g., while 113mCd has a half-life of only fourteen years, that of 113Cd is nearly eight quadrillion years.
17. ^ Report to Congress on the extraction of medical isotopes from U-233 Archived 2011-09-27 at the Wayback Machine. U.S. Department of Energy. March 2001
18. ^ Kroger, L.A.; Reich, C.W. (1976). "Features of the low energy level scheme of 229Th as observed in the ? decay of 233U". Nucl. Phys. A. 259: 29-60. doi:10.1016/0375-9474(76)90494-2.
19. ^ Reich, C. W.; Helmer, R. G. (Jan 1990). "Energy separation of the doublet of intrinsic states at the ground state of 229Th". Phys. Rev. Lett. American Physical Society. 64 (3): 271-273. Bibcode:1990PhRvL..64..271R. doi:10.1103/PhysRevLett.64.271. PMID 10041937.
20. ^ Helmer, R. G.; Reich, C. W. (April 1994). "An Excited State of 229Th at 3.5 eV". Physical Review C. 49 (4): 1845-1858. Bibcode:1994PhRvC..49.1845H. doi:10.1103/PhysRevC.49.1845. PMID 9969412.
21. ^ Tkalya, E.V.; Varlamov, V.O.; Lomonosov, V.V.; Nikulin, S.A. (1996). "Processes of the nuclear isomer 229mTh(3/2+, 3.5±1.0 eV) Resonant excitation by optical photons". Physica Scripta. 53 (3): 296-299. doi:10.1088/0031-8949/53/3/003.
22. ^ Raeder, S.; Sonnenschein, V.; Gottwald, T.; Moore, I.D.; Reponen, M.; Rothe, S.; Trautmann, N.; Wendt, K. (2011). "Resonance ionization spectroscopy of thorium isotopes - towards a laser spectroscopic identification of the low-lying 7.6 eV isomer of 229Th". J. Phys. B: At. Mol. Opt. Phys. 44: 165005. arXiv:1105.4646. doi:10.1088/0953-4075/44/16/165005.
23. ^ von der Wense, Lars; Seiferle, Benedict; Thirolf, Peter G. (March 2018). "Towards a 229Th-based nuclear clock". Measurement Techniques. 60 (12): 1178-1192. arXiv:1811.03889. doi:10.1007/s11018-018-1337-1.
24. ^ B. R. Beck; et al. (2007-04-06). "Energy splitting in the ground state doublet in the nucleus 229Th". Physical Review Letters. 98 (14): 142501. Bibcode:2007PhRvL..98n2501B. doi:10.1103/PhysRevLett.98.142501. PMID 17501268.
25. ^ Beck BR, Wu CY, Beiersdorfer P, Brown GV, Becker JA, Moody KJ, Wilhelmy JB, Porter FS, Kilbourne CA, Kelley RL (2009-07-30). Improved value for the energy splitting of the ground-state doublet in the nucleus 229Th (PDF). 12th Int. Conf. on Nuclear Reaction Mechanisms. Varenna, Italy. LLNL-PROC-415170. Archived from the original (PDF) on 2017-01-27. Retrieved .
26. ^ Jeet, Justin (2015). "Results of a Direct Search Using Synchrotron Radiation for the Low-Energy". Physical Review Letters. 114 (25): 253001. arXiv:1502.02189. Bibcode:2015PhRvL.114y3001J. doi:10.1103/physrevlett.114.253001. PMID 26197124.
27. ^ Yamaguchi, A.; Kolbe, M.; Kaser, H.; Reichel, T.; Gottwald, A.; Peik, E. (2015). "Experimental search for the low-energy nuclear transition in 229 Th with undulator radiation". New Journal of Physics. 17 (5): 053053. Bibcode:2015NJPh...17e3053Y. doi:10.1088/1367-2630/17/5/053053. ISSN 1367-2630.
28. ^ von der Wense, L. (2018). On the direct detection of 229mTh (PDF). Springer Theses, Berlin. ISBN 978-3-319-70461-6.
29. ^ Stellmer, S.; Kazakov, G.; Schreitl, M.; Kaser, H.; Kolbe, M.; Schumm, T. (2018). "Attempt to optically excite excite the nuclear isomer in 229Th". Phys. Rev. A. 97: 062506. arXiv:1803.09294. doi:10.1103/PhysRevA.97.062506.
30. ^ Zhao, Xinxin; Yenny Natali Martinez de Escobar; Robert Rundberg; Evelyn M. Bond; Allen Moody; David J. Vieira (2012). "Observation of the Deexcitation of the ^{229m}Th Nuclear Isomer". Physical Review Letters. 109 (16): 160801. Bibcode:2012PhRvL.109p0801Z. doi:10.1103/PhysRevLett.109.160801. ISSN 0031-9007. PMID 23215066.
31. ^ a b Borisyuk, P. V.; Chubunova, E. V.; Kolachevsky, N. N.; Lebedinskii, Yu Yu; Vasiliev, O. S.; Tkalya, E. V. (2018-04-01). "Excitation of 229Th nuclei in laser plasma: the energy and half-life of the low-lying isomeric state". arXiv:1804.00299 [nucl-th].
32. ^ Peik, Ekkehard; Zimmermann, Kai (2013-07-03). "Comment on "Observation of the Deexcitation of the 229mTh Nuclear Isomer"". Physical Review Letters. 111 (1): 018901. Bibcode:2013PhRvL.111a8901P. doi:10.1103/PhysRevLett.111.018901. PMID 23863029.
33. ^ Thirolf, P G; Seiferle, B; von der Wense, L (2019-10-28). "The 229-thorium isomer: doorway to the road from the atomic clock to the nuclear clock". Journal of Physics B: Atomic, Molecular and Optical Physics. 52 (20): 203001. doi:10.1088/1361-6455/ab29b8. ISSN 0953-4075.
34. ^ a b von der Wense, Lars; Seiferle, Benedict; Laatiaoui, Mustapha; Neumayr, Jürgen B.; Maier, Hans-Jörg; Wirth, Hans-Friedrich; Mokry, Christoph; Runke, Jörg; Eberhardt, Klaus; Düllmann, Christoph E.; Trautmann, Norbert G.; Thirolf, Peter G. (5 May 2016). "Direct detection of the 229Th nuclear clock transition". Nature. 533 (7601): 47-51. arXiv:1710.11398. Bibcode:2016Natur.533...47V. doi:10.1038/nature17669. PMID 27147026.
35. ^ a b Tkalya, E.V.; Schneider, C.; Jeet, J.; Hudson, E.R. (2015). "Radiative lifetime and energy of the low-energy isomeric level in 229Th". Phys. Rev. C. 92: 054324. arXiv:1509.09101. doi:10.1103/PhysRevC.92.054324.
36. ^ Minkov, N.; Pálffy, A. (2017). "Reduced transition probabilities for the gamma decay of the 7.8 eV isomer in 229mTh". Phys. Rev. Lett. 118: 212501. arXiv:1704.07919. doi:10.1103/PhysRevLett.118.212501. PMID 28598657.
37. ^ Karpeshin, F.F.; Trzhaskovskaya, M.B. (2007). "Impact of the electron environment on the lifetime of the 229Thm low-lying isomer". Phys. Rev. C. 76 (5): 054313. doi:10.1103/PhysRevC.76.054313.
38. ^ Thielking, J.; Okhapkin, M.V.; Przemyslaw, G.; Meier, D.M.; von der Wense, L.; Seiferle, B.; Düllmann, C.E.; Thirolf, P.G.; Peik, E. (2018). "Laser spectroscopic characterization of the nuclear-clock isomer 229mTh". Nature. 556 (7701): 321-325. arXiv:1709.05325. doi:10.1038/s41586-018-0011-8. PMID 29670266.
39. ^ Masuda, T.; Yoshimi, A.; Fujieda, A.; Fujimoto, H.; Haba, H.; Hara, H.; Hiraki, T.; Kaino, H.; Kasamatsu, Y.; Kitao, S.; Konashi, K.; Miyamoto, Y.; Okai, K.; Okubo, S.; Sasao, N.; Seto, M.; Schumm, T.; Shigekawa, Y.; Suzuki, K.; Stellmer, S.; Tamasaku, K.; Uetake, S.; Watanabe, M.; Watanabe, T.; Yasuda, Y.; Yamaguchi, A.; Yoda, Y.; Yokokita, T.; Yoshimura, M.; Yoshimura, K. (12 September 2019). "X-ray pumping of the 229Th nuclear clock isomer". Nature. 573 (7773): 238-242. arXiv:1902.04823. doi:10.1038/s41586-019-1542-3. PMID 31511686.
40. ^ Yamaguchi, A.; Muramatsu, H.; Hayashi, T.; Yuasa, N.; Nakamura, K.; Takimoto, M.; Haba, H.; Konashi, K.; Watanabe, M.; Kikunaga, H.; Maehata, K. (2019-11-26). "Energy of the $^{229}\mathrm{Th}$ Nuclear Clock Isomer Determined by Absolute $\ensuremath{\gamma}$-ray Energy Difference". Physical Review Letters. 123 (22): 222501. doi:10.1103/PhysRevLett.123.222501.
41. ^ Ozawa, Akira; Zhao, Zhigang; Kuwata-Gonokami, Makoto; Kobayashi, Yohei (2015-06-15). "High average power coherent vuv generation at 10 MHz repetition frequency by intracavity high harmonic generation". Optics Express. 23 (12): 15107. doi:10.1364/OE.23.015107. ISSN 1094-4087.
42. ^ von der Wense, Lars; Zhang, Chuankun (2019-11-19). "Concepts for direct frequency-comb spectroscopy of $^{229\text{m}}$Th and an internal-conversion-based solid-state nuclear clock". arXiv:1905.08060 [physics].
43. ^ Ozawa, Akira; Kobayashi, Yohei (2013-02-19). "vuv frequency-comb spectroscopy of atomic xenon". Physical Review A. 87 (2): 022507. doi:10.1103/PhysRevA.87.022507.
44. ^ Ozawa, Akira; Kobayashi, Yohei (2013-02-19). "vuv frequency-comb spectroscopy of atomic xenon". Physical Review A. 87 (2): 022507. doi:10.1103/PhysRevA.87.022507.
45. ^ Nakazato, Tomoharu; Ito, Isao; Kobayashi, Yohei; Wang, Xiaoyang; Chen, Chuangtian; Watanabe, Shuntaro (2016-07-25). "Phase-matched frequency conversion below 150 nm in KBe_2BO_3F_2". Optics Express. 24 (15): 17149. doi:10.1364/OE.24.017149. ISSN 1094-4087.
46. ^ Knight, G. B.; Macklin, R. L. (1 January 1949). "Radiations of Uranium Y". Physical Review. 75 (1): 34-38. doi:10.1103/PhysRev.75.34.
47. ^ Isotopes Project Home Page, Lawrence Berkeley National Laboratory. "Isotopes of Thorium (Z=90)". Archived from the original on 2010-02-03. Retrieved .
48. ^ Rutherford Appleton Laboratory. "Th-232 Decay Chain". Archived from the original on 2012-04-19. Retrieved .
49. ^ World Nuclear Association. "Thorium". Retrieved .
50. ^ Krasinskas, Alyssa M; Minda, Justina; Saul, Scott H; Shaked, Abraham; Furth, Emma E (2004). "Redistribution of thorotrast into a liver allograft several years following transplantation: a case report". Mod. Pathol. 17 (1): 117-120. doi:10.1038/modpathol.3800008. PMID 14631374.
51. ^ Georges, Audi (2003). "The NUBASE Evaluation of Nuclear and Decay Properties" (PDF). Nuclear Physics A. Atomic Mass Data Center. 729 (1): 3-128. Bibcode:2003NuPhA.729....3A. doi:10.1016/j.nuclphysa.2003.11.001.