Isotopes of americium: Difference between revisions
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! <br />isotopic mass (u)<br /> |
! <br />isotopic mass (u)<br /> |
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! rowspan="2" | half-life |
! rowspan="2" | half-life |
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! rowspan="2" | decay<br>mode(s)<ref>http://www.nucleonica.net/unc.aspx</ref><ref group="n">Abbreviations:<br>CD: [[Cluster decay]]<br>EC: [[Electron capture]]<br>IT: [[Isomeric transition]]<br>SF: [[Spontaneous fission]]</ref> |
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! rowspan="2" | daughter<br>isotope(s) |
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! rowspan="2" | nuclear<br />spin |
! rowspan="2" | nuclear<br />spin |
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|- |
|- |
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! colspan="3" | excitation energy |
! colspan="3" | excitation energy |
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|- |
|- |
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| <sup>231</sup>Am |
| rowspan=2|<sup>231</sup>Am |
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| style="text-align:right" | 95 |
| rowspan=2 style="text-align:right" | 95 |
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| style="text-align:right" | 136 |
| rowspan=2 style="text-align:right" | 136 |
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| 231.04556(32)# |
| rowspan=2|231.04556(32)# |
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| 30# s |
| rowspan=2|30# s |
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| [[beta decay|β<sup>+</sup>]] |
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| |
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| <sup>231</sup>Pu |
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| rowspan=2| |
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|- |
|- |
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| [[alpha decay|α]] (rare) |
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| <sup>232</sup>Am |
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| <sup>227</sup>Np |
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| style="text-align:right" | 95 |
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| style="text-align:right" | 137 |
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| 232.04659(32)# |
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| 79(2) s |
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| |
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|- |
|- |
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| <sup> |
| rowspan=3|<sup>232</sup>Am |
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| style="text-align:right" | 95 |
| rowspan=3 style="text-align:right" | 95 |
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| style="text-align:right" | |
| rowspan=3 style="text-align:right" | 137 |
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| |
| rowspan=3|232.04659(32)# |
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| 3 |
| rowspan=3|79(2) s |
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| β<sup>+</sup> (98%) |
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| |
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| <sup>233</sup>Pu |
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| rowspan=3| |
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|- |
|- |
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| α (2%) |
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| <sup>234</sup>Am |
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| <sup>228</sup>Np |
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| style="text-align:right" | 95 |
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| style="text-align:right" | 139 |
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| 234.04781(22)# |
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| 2.32(8) min |
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| |
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|- |
|- |
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| <sup> |
| β<sup>+</sup>, [[Spontaneous fission|SF]] (.069%) |
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| (various) |
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| style="text-align:right" | 95 |
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| style="text-align:right" | 140 |
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| 235.04795(13)# |
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| 9.9(5) min |
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| 5/2-# |
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|- |
|- |
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| <sup> |
| rowspan=2|<sup>233</sup>Am |
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| style="text-align:right" | 95 |
| rowspan=2 style="text-align:right" | 95 |
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| style="text-align:right" | |
| rowspan=2 style="text-align:right" | 138 |
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| |
| rowspan=2|233.04635(11)# |
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| 3. |
| rowspan=2|3.2(8) min |
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| β<sup>+</sup> |
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| |
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| <sup>233</sup>Pu |
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| rowspan=2| |
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|- |
|- |
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| α |
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| <sup>237</sup>Am |
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| <sup>229</sup>Np |
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| style="text-align:right" | 95 |
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| style="text-align:right" | 142 |
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| 237.05000(6)# |
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| 73.0(10) min |
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| 5/2(-) |
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|- |
|- |
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| <sup> |
| rowspan=3|<sup>234</sup>Am |
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| style="text-align:right" | 95 |
| rowspan=3 style="text-align:right" | 95 |
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| style="text-align:right" | |
| rowspan=3 style="text-align:right" | 139 |
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| rowspan=3|234.04781(22)# |
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| 238.05198(5) |
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| |
| rowspan=3|2.32(8) min |
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| β<sup>+</sup> (99.95%) |
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| 1+ |
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| <sup>234</sup>Pu |
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| rowspan=3| |
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|- |
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| α (.04%) |
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| <sup>230</sup>Np |
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|- |
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| β<sup>+</sup>, SF (.0066%) |
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| (various) |
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|- |
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| rowspan=2|<sup>235</sup>Am |
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| rowspan=2 style="text-align:right" | 95 |
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| rowspan=2 style="text-align:right" | 140 |
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| rowspan=2|235.04795(13)# |
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| rowspan=2|9.9(5) min |
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| β<sup>+</sup> |
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| <sup>235</sup>Pu |
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| rowspan=2|5/2-# |
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|- |
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| α (rare) |
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| <sup>231</sup>Np |
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|- |
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| rowspan=2|<sup>236</sup>Am |
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| rowspan=2 style="text-align:right" | 95 |
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| rowspan=2 style="text-align:right" | 141 |
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| rowspan=2|236.04958(11)# |
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| rowspan=2|3.6(1) min |
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| β<sup>+</sup> |
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| <sup>236</sup>Pu |
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| rowspan=2| |
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|- |
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| α |
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| <sup>232</sup>Np |
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|- |
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| rowspan=2|<sup>237</sup>Am |
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| rowspan=2 style="text-align:right" | 95 |
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| rowspan=2 style="text-align:right" | 142 |
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| rowspan=2|237.05000(6)# |
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| rowspan=2|73.0(10) min |
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| β<sup>+</sup> (99.97%) |
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| <sup>237</sup>Pu |
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| rowspan=2|5/2(-) |
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|- |
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| α (.025%) |
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| <sup>233</sup>Np |
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|- |
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| rowspan=2|<sup>238</sup>Am |
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| rowspan=2 style="text-align:right" | 95 |
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| rowspan=2 style="text-align:right" | 143 |
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| rowspan=2|238.05198(5) |
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| rowspan=2|98(2) min |
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| β<sup>+</sup> |
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| <sup>238</sup>Pu |
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| rowspan=2|1+ |
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|- |
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| α (1E-4%) |
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| <sup>234</sup>Np |
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|- |
|- |
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| style="text-indent:1em" | <sup>238m</sup>Am |
| style="text-indent:1em" | <sup>238m</sup>Am |
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| colspan="3" style="text-indent:2em" | 2500(200)# keV |
| colspan="3" style="text-indent:2em" | 2500(200)# keV |
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| 35(10) µs |
| 35(10) µs |
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| |
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| |
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| |
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|- |
|- |
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| <sup>239</sup>Am |
| rowspan=2|<sup>239</sup>Am |
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| style="text-align:right" | 95 |
| rowspan=2 style="text-align:right" | 95 |
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| style="text-align:right" | 144 |
| rowspan=2 style="text-align:right" | 144 |
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| 239.0530245(26) |
| rowspan=2|239.0530245(26) |
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| 11.9(1) h |
| rowspan=2|11.9(1) h |
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| [[Electron capture|EC]] (99.99%) |
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| (5/2)- |
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| rowspan=2|(5/2)- |
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|- |
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| α (.01%) |
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| <sup>235</sup>Np |
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|- |
|- |
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| style="text-indent:1em" | <sup>239m</sup>Am |
| style="text-indent:1em" | <sup>239m</sup>Am |
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| colspan="3" style="text-indent:2em" | 2500(200) keV |
| colspan="3" style="text-indent:2em" | 2500(200) keV |
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| 163(12) ns |
| 163(12) ns |
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| |
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| |
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| (7/2+) |
| (7/2+) |
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|- |
|- |
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| <sup>240</sup>Am |
| rowspan=2|<sup>240</sup>Am |
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| style="text-align:right" | 95 |
| rowspan=2 style="text-align:right" | 95 |
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| style="text-align:right" | 145 |
| rowspan=2 style="text-align:right" | 145 |
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| 240.055300(15) |
| rowspan=2|240.055300(15) |
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| 50.8(3) h |
| rowspan=2|50.8(3) h |
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| β<sup>+</sup> |
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| (3-) |
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| <sup>240</sup>Pu |
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| rowspan=2|(3-) |
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|- |
|- |
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| α (1.9E-4%) |
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| [[Americium-241|<sup>241</sup>Am]] |
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| <sup>236</sup>Np |
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| style="text-align:right" | 95 |
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|- |
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| style="text-align:right" | 146 |
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| rowspan=3|<sup>241</sup>Am |
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| 241.0568291(20) |
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| rowspan=3| style="text-align:right" | 95 |
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| 432.2(7) a |
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| rowspan=3 style="text-align:right" | 146 |
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| 5/2- |
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| rowspan=3|241.0568291(20) |
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| rowspan=3|432.2(7) a |
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| α |
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| <sup>237</sup>Np |
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| rowspan=3|5/2- |
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|- |
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| SF (4.3E-10%) |
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| (various) |
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|- |
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| [[Cluster decay|CD]] (7.4E-10%) |
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| <sup>207</sup>Tl, <sup>34</sup>Si |
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|- |
|- |
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| style="text-indent:1em" | <sup>241m</sup>Am |
| style="text-indent:1em" | <sup>241m</sup>Am |
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| colspan="3" style="text-indent:2em" | 2200(100) keV |
| colspan="3" style="text-indent:2em" | 2200(100) keV |
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| 1.2(3) µs |
| 1.2(3) µs |
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| |
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| |
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| |
| |
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|- |
|- |
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| |
| rowspan=2|<sup>242</sup>Am |
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| style="text-align:right" | 95 |
| rowspan=2 style="text-align:right" | 95 |
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| style="text-align:right" | 147 |
| rowspan=2 style="text-align:right" | 147 |
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| 242.0595492(20) |
| rowspan=2|242.0595492(20) |
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| 16.02(2) h |
| rowspan=2|16.02(2) h |
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| β<sup>-</sup> (82.7%) |
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| 1- |
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| <sup>242</sup>Cm |
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| rowspan=2|1- |
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|- |
|- |
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| EC (17.3%) |
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| style="text-indent:1em" | <sup>242m1</sup>Am |
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| <sup>242</sup>Pu |
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| colspan="3" style="text-indent:2em" | 48.60(5) keV |
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|- |
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| 141(2) a |
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| rowspan=3 style="text-indent:1em" | <sup>242m1</sup>Am |
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| 5- |
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| rowspan=3 colspan="3" style="text-indent:2em" | 48.60(5) keV |
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| rowspan=3|141(2) a |
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| [[Isomeric transition|IT]] (99.54%) |
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| <sup>242</sup>Am |
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| rowspan=3|5- |
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|- |
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| α (.46%) |
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| <sup>238</sup>Np |
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|- |
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| SF (1.5E-8%) |
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| (various) |
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|- |
|- |
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| style="text-indent:1em" | <sup>242m2</sup>Am |
| style="text-indent:1em" | <sup>242m2</sup>Am |
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| colspan="3" style="text-indent:2em" | 2200(80) keV |
| colspan="3" style="text-indent:2em" | 2200(80) keV |
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| 14.0(10) ms |
| 14.0(10) ms |
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| |
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| |
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| (2+,3-) |
| (2+,3-) |
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|- |
|- |
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| |
| rowspan=2|<sup>243</sup>Am |
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| style="text-align:right" | 95 |
| rowspan=2 style="text-align:right" | 95 |
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| style="text-align:right" | 148 |
| rowspan=2 style="text-align:right" | 148 |
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| 243.0613811(25) |
| rowspan=2|243.0613811(25) |
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| 7.37(4)E+3 a |
| rowspan=2|7.37(4)E+3 a |
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| |
| α |
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| <sup>239</sup>Np |
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| rowspan=2|5/2- |
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|- |
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| SF (3.7E-9%) |
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| (various) |
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|- |
|- |
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| <sup>244</sup>Am |
| <sup>244</sup>Am |
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Line 208: | Line 299: | ||
| 244.0642848(22) |
| 244.0642848(22) |
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| 10.1(1) h |
| 10.1(1) h |
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| β<sup>-</sup> |
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| <sup>244</sup>Cm |
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| (6-)# |
| (6-)# |
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|- |
|- |
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| style="text-indent:1em" | <sup>244m</sup>Am |
| rowspan=2 style="text-indent:1em" | <sup>244m</sup>Am |
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| colspan="3" style="text-indent:2em" | 86.1(10) keV |
| rowspan=2 colspan="3" style="text-indent:2em" | 86.1(10) keV |
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| 26(1) min |
| rowspan=2|26(1) min |
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| β<sup>-</sup> (99.96%) |
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| 1+ |
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| <sup>244</sup>Cm |
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| rowspan=2|1+ |
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|- |
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| EC (.0361%) |
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| <sup>244</sup>Pl |
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|- |
|- |
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| <sup>245</sup>Am |
| <sup>245</sup>Am |
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Line 220: | Line 318: | ||
| 245.066452(4) |
| 245.066452(4) |
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| 2.05(1) h |
| 2.05(1) h |
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| β<sup>-</sup> |
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| <sup>245</sup>Cm |
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| (5/2)+ |
| (5/2)+ |
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|- |
|- |
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Line 227: | Line 327: | ||
| 246.069775(20) |
| 246.069775(20) |
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| 39(3) min |
| 39(3) min |
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| β<sup>-</sup> |
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| <sup>246</sup>Cm |
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| (7-) |
| (7-) |
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|- |
|- |
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| style="text-indent:1em" | <sup>246m1</sup>Am |
| rowspan=2 style="text-indent:1em" | <sup>246m1</sup>Am |
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| colspan="3" style="text-indent:2em" | 30(10) keV |
| rowspan=2 colspan="3" style="text-indent:2em" | 30(10) keV |
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| 25.0(2) min |
| rowspan=2|25.0(2) min |
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| β<sup>-</sup> (99.99%) |
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| 2(-) |
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| <sup>246</sup>Cm |
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| rowspan=2|2(-) |
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|- |
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| IT (.01%) |
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| <sup>246</sup>Am |
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|- |
|- |
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| style="text-indent:1em" | <sup>246m2</sup>Am |
| style="text-indent:1em" | <sup>246m2</sup>Am |
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| colspan="3" style="text-indent:2em" | ~2000 keV |
| colspan="3" style="text-indent:2em" | ~2000 keV |
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| 73(10) µs |
| 73(10) µs |
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| |
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|- |
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Line 244: | Line 353: | ||
| 247.07209(11)# |
| 247.07209(11)# |
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| 23.0(13) min |
| 23.0(13) min |
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| β<sup>-</sup> |
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| <sup>247</sup>Cm |
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| (5/2)# |
| (5/2)# |
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|- |
|- |
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Line 251: | Line 362: | ||
| 248.07575(22)# |
| 248.07575(22)# |
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| 3# min |
| 3# min |
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| β<sup>-</sup> |
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| <sup>248</sup>Cm |
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| |
| |
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|- |
|- |
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Line 258: | Line 371: | ||
| 249.07848(32)# |
| 249.07848(32)# |
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| 1# min |
| 1# min |
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| β<sup>-</sup> |
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| <sup>249</sup>Cm |
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|} |
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<references group="n" /> |
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=== Notes === |
=== Notes === |
Revision as of 08:38, 20 May 2011
Actinides[1] by decay chain | Half-life range (a) |
Fission products of 235U by yield[2] | ||||||
---|---|---|---|---|---|---|---|---|
4n | 4n + 1 | 4n + 2 | 4n + 3 | 4.5–7% | 0.04–1.25% | <0.001% | ||
228Ra№ | 4–6 a | 155Euþ | ||||||
244Cmƒ | 241Puƒ | 250Cf | 227Ac№ | 10–29 a | 90Sr | 85Kr | 113mCdþ | |
232Uƒ | 238Puƒ | 243Cmƒ | 29–97 a | 137Cs | 151Smþ | 121mSn | ||
248Bk[3] | 249Cfƒ | 242mAmƒ | 141–351 a |
No fission products have a half-life | ||||
241Amƒ | 251Cfƒ[4] | 430–900 a | ||||||
226Ra№ | 247Bk | 1.3–1.6 ka | ||||||
240Pu | 229Th | 246Cmƒ | 243Amƒ | 4.7–7.4 ka | ||||
245Cmƒ | 250Cm | 8.3–8.5 ka | ||||||
239Puƒ | 24.1 ka | |||||||
230Th№ | 231Pa№ | 32–76 ka | ||||||
236Npƒ | 233Uƒ | 234U№ | 150–250 ka | 99Tc₡ | 126Sn | |||
248Cm | 242Pu | 327–375 ka | 79Se₡ | |||||
1.53 Ma | 93Zr | |||||||
237Npƒ | 2.1–6.5 Ma | 135Cs₡ | 107Pd | |||||
236U | 247Cmƒ | 15–24 Ma | 129I₡ | |||||
244Pu | 80 Ma |
... nor beyond 15.7 Ma[5] | ||||||
232Th№ | 238U№ | 235Uƒ№ | 0.7–14.1 Ga | |||||
|
Americium (Am) has no stable isotopes. A standard atomic mass cannot be given.
19 radioisotopes of americium have been characterized, with the most stable being 243Am with a half-life of 7370 years, and 241Am with a half-life of 432.7 years. All of the remaining radioactive isotopes have half-lives that are less than 51 hours, and the majority of these have half-lives that are less than 100 minutes. This element also has 8 meta states, with the most stable being 242mAm (t½ 141 years). The isotopes of americium range in atomic weight from 231.046 u (231Am) to 249.078 u (249Am).
Some notable isotopes
Americium-241
![](http://upload.wikimedia.org/wikipedia/commons/thumb/1/16/Americium-241.jpg/150px-Americium-241.jpg)
Americium-241 is the most prevalent isotope of americium in nuclear waste.[6] It is the americium isotope used in smoke detectors based on ionization chambers. It is a potential fuel for long-lifetime radioisotope thermoelectric generators.
Parameter | Value |
---|---|
Atomic mass | 241.056823 u |
Mass excess | 52930 keV |
Beta decay energy | -767 keV |
Spin | 5/2- |
Half life | 432.2 years |
Spontaneous fissions | 1200 per kg/s |
Decay heat | 114 watts/kg |
Possible parent nuclides: beta from Pu-241, electron capture from Cm-241, alpha from Bk-245
Americium-241 decays by alpha emission, with a by-product of gamma rays. Its presence in plutonium is determined by the original concentration of plutonium-241 and the sample age. Because of the low penetration of alpha radiation, Americium-241 only poses a health risk when ingested or inhaled. Older samples of plutonium containing plutonium-241 contain a buildup of Am-241. A chemical removal of americium from reworked plutonium, e.g. during reworking of plutonium pits, may be required.
Americium-242m
![](http://upload.wikimedia.org/wikipedia/commons/thumb/c/cc/Sasahara.svg/375px-Sasahara.svg.png)
Fission percentage is 100 minus shown percentages.
Total rate of transmutation varies greatly by nuclide.
245Cm–248Cm are long-lived with negligible decay.
Probability | Decay mode | Decay energy | Decay product |
---|---|---|---|
99.54% | isomeric transition | 0.05 MeV | 242Am |
0.46% | alpha decay | 5.64 MeV | 238Np |
(1.5±0.6)×10−10[8] | spontaneous fission | ~200 MeV | fission products |
Americium-242m is one of the isotopes of americium, with 95 protons and electrons and 147 neutrons and a mass of 242.0595492 g/mol. It is one of the rare cases, like tantalum-180m, where a higher-energy nuclear isomer is more stable than the lower-energy one, Americium-242.[9]
242mAm is fissile (because it has an odd number of neutrons) and has a low critical mass, comparable to that of plutonium-239.[10] It has a very high cross section for fission, and if in a nuclear reactor is destroyed relatively quickly. Another report claims that 242mAm has a much lower critical mass, can sustain a chain reaction even as a thin film, and could be used for a novel type of nuclear rocket.[11]
Probability | Decay mode | Decay energy | Decay product |
---|---|---|---|
82.70% | beta decay | 0.665 MeV | 242Cm |
17.30% | electron capture | 0.751 MeV | 242Pu |
Americium-243
Americium-243 is a radioactive isotope of americium having 95 electrons and protons and 148 neutrons and has a mass of 243.06138 g/mol.
It has a half-life of 7370 years, the longest lasting of all americium isotopes, however, it is still not found in nature. It is formed in the nuclear fuel cycle by neutron capture on plutonium-242 followed by beta decay. [12] Production increases exponentially with increasing burnup as a total of 5 neutron captures on uranium-238 are required.
It either decays by emitting an alpha particle (the decay energy is 5.27MeV)[13] to turn into neptunium-239, which then quickly decays to plutonium-239, or infrequently, by spontaneous fission. [14]
Americium-243 is a hazardous substance, because it can cause cancer. Neptunium-239, which is formed from Americium-243, emits dangerous gamma rays, making Americium-243 the most dangerous isotope of Americium. [15]
Table
nuclide symbol |
Z(p) | N(n) | isotopic mass (u) |
half-life | decay mode(s)[16][n 1] |
daughter isotope(s) |
nuclear spin |
---|---|---|---|---|---|---|---|
excitation energy | |||||||
231Am | 95 | 136 | 231.04556(32)# | 30# s | β+ | 231Pu | |
α (rare) | 227Np | ||||||
232Am | 95 | 137 | 232.04659(32)# | 79(2) s | β+ (98%) | 233Pu | |
α (2%) | 228Np | ||||||
β+, SF (.069%) | (various) | ||||||
233Am | 95 | 138 | 233.04635(11)# | 3.2(8) min | β+ | 233Pu | |
α | 229Np | ||||||
234Am | 95 | 139 | 234.04781(22)# | 2.32(8) min | β+ (99.95%) | 234Pu | |
α (.04%) | 230Np | ||||||
β+, SF (.0066%) | (various) | ||||||
235Am | 95 | 140 | 235.04795(13)# | 9.9(5) min | β+ | 235Pu | 5/2-# |
α (rare) | 231Np | ||||||
236Am | 95 | 141 | 236.04958(11)# | 3.6(1) min | β+ | 236Pu | |
α | 232Np | ||||||
237Am | 95 | 142 | 237.05000(6)# | 73.0(10) min | β+ (99.97%) | 237Pu | 5/2(-) |
α (.025%) | 233Np | ||||||
238Am | 95 | 143 | 238.05198(5) | 98(2) min | β+ | 238Pu | 1+ |
α (1E-4%) | 234Np | ||||||
238mAm | 2500(200)# keV | 35(10) µs | |||||
239Am | 95 | 144 | 239.0530245(26) | 11.9(1) h | EC (99.99%) | (5/2)- | |
α (.01%) | 235Np | ||||||
239mAm | 2500(200) keV | 163(12) ns | (7/2+) | ||||
240Am | 95 | 145 | 240.055300(15) | 50.8(3) h | β+ | 240Pu | (3-) |
α (1.9E-4%) | 236Np | ||||||
241Am | style="text-align:right" | 95 | 146 | 241.0568291(20) | 432.2(7) a | α | 237Np | 5/2- |
SF (4.3E-10%) | (various) | ||||||
CD (7.4E-10%) | 207Tl, 34Si | ||||||
241mAm | 2200(100) keV | 1.2(3) µs | |||||
242Am | 95 | 147 | 242.0595492(20) | 16.02(2) h | β- (82.7%) | 242Cm | 1- |
EC (17.3%) | 242Pu | ||||||
242m1Am | 48.60(5) keV | 141(2) a | IT (99.54%) | 242Am | 5- | ||
α (.46%) | 238Np | ||||||
SF (1.5E-8%) | (various) | ||||||
242m2Am | 2200(80) keV | 14.0(10) ms | (2+,3-) | ||||
243Am | 95 | 148 | 243.0613811(25) | 7.37(4)E+3 a | α | 239Np | 5/2- |
SF (3.7E-9%) | (various) | ||||||
244Am | 95 | 149 | 244.0642848(22) | 10.1(1) h | β- | 244Cm | (6-)# |
244mAm | 86.1(10) keV | 26(1) min | β- (99.96%) | 244Cm | 1+ | ||
EC (.0361%) | 244Pl | ||||||
245Am | 95 | 150 | 245.066452(4) | 2.05(1) h | β- | 245Cm | (5/2)+ |
246Am | 95 | 151 | 246.069775(20) | 39(3) min | β- | 246Cm | (7-) |
246m1Am | 30(10) keV | 25.0(2) min | β- (99.99%) | 246Cm | 2(-) | ||
IT (.01%) | 246Am | ||||||
246m2Am | ~2000 keV | 73(10) µs | |||||
247Am | 95 | 152 | 247.07209(11)# | 23.0(13) min | β- | 247Cm | (5/2)# |
248Am | 95 | 153 | 248.07575(22)# | 3# min | β- | 248Cm | |
249Am | 95 | 154 | 249.07848(32)# | 1# min | β- | 249Cm |
- ^ Abbreviations:
CD: Cluster decay
EC: Electron capture
IT: Isomeric transition
SF: Spontaneous fission
Notes
- Values marked # are not purely derived from experimental data, but at least partly from systematic trends. Spins with weak assignment arguments are enclosed in parentheses - ( ).
- Uncertainties are given in concise form in parentheses after the corresponding last digits. Uncertainty values denote one standard deviation, except isotopic composition and standard atomic mass from IUPAC which use expanded uncertainties.
See also
References
- ^ 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.
- ^ Specifically from thermal neutron fission of uranium-235, e.g. in a typical nuclear reactor.
- ^ 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 [years]. No growth of Cf248 was detected, and a lower limit for the β− half-life can be set at about 104 [years]. No alpha activity attributable to the new isomer has been detected; the alpha half-life is probably greater than 300 [years]." - ^ This is the heaviest nuclide with a half-life of at least four years before the "sea of instability".
- ^ 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 eight quadrillion years.
- ^ "Americium". Argonne National Laboratory, EVS. Retrieved 25 December 2009.
- ^ Sasahara, Akihiro; Matsumura, Tetsuo; Nicolaou, Giorgos; Papaioannou, Dimitri (April 2004). "Neutron and Gamma Ray Source Evaluation of LWR High Burn-up UO2 and MOX Spent Fuels". Journal of NUCLEAR SCIENCE and TECHNOLOGY. 41 (4): 448–456. doi:10.3327/jnst.41.448.
- ^ Phys. Rev. 155 (1967): J. T. Caldwell, S. C. Fultz, C. D. Bowman, and R. W. Hoff - Spontaneous Fission Half-Life of 242mAm (halflife (9.5±3.5)×1011
- ^ 95-Am-242
- ^ http://typhoon.jaea.go.jp/icnc2003/Proceeding/paper/6.5_022.pdf
- ^ Extremely Efficient Nuclear Fuel Could Take Man To Mars In Just Two Weeks
- ^ "Americium-243". Oak Ridge National Laboratory. Retrieved 25 December 2009.
- ^ "Americium-243". Oak Ridge National Laboratory. Retrieved 25 December 2009.
- ^ "Isotopes of the Element Americium". Jefferson Lab Science Education. Retrieved 25 December 2009.
- ^ "Americium". Argonne National Laboratory, EVS. Retrieved 25 December 2009.
- ^ http://www.nucleonica.net/unc.aspx
- Isotope masses from:
- G. Audi, A. H. Wapstra, C. Thibault, J. Blachot and O. Bersillon (2003). "The NUBASE evaluation of nuclear and decay properties" (PDF). Nuclear Physics A. 729: 3–128. doi:10.1016/j.nuclphysa.2003.11.001.
{{cite journal}}
: CS1 maint: multiple names: authors list (link)
- G. Audi, A. H. Wapstra, C. Thibault, J. Blachot and O. Bersillon (2003). "The NUBASE evaluation of nuclear and decay properties" (PDF). Nuclear Physics A. 729: 3–128. doi:10.1016/j.nuclphysa.2003.11.001.
- Isotopic compositions and standard atomic masses from:
- J. R. de Laeter, J. K. Böhlke, P. De Bièvre, H. Hidaka, H. S. Peiser, K. J. R. Rosman and P. D. P. Taylor (2003). "Atomic weights of the elements. Review 2000 (IUPAC Technical Report)". Pure and Applied Chemistry. 75 (6): 683–800. doi:10.1351/pac200375060683.
{{cite journal}}
: CS1 maint: multiple names: authors list (link) - M. E. Wieser (2006). "Atomic weights of the elements 2005 (IUPAC Technical Report)". Pure and Applied Chemistry. 78 (11): 2051–2066. doi:10.1351/pac200678112051.
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ignored (help)
- J. R. de Laeter, J. K. Böhlke, P. De Bièvre, H. Hidaka, H. S. Peiser, K. J. R. Rosman and P. D. P. Taylor (2003). "Atomic weights of the elements. Review 2000 (IUPAC Technical Report)". Pure and Applied Chemistry. 75 (6): 683–800. doi:10.1351/pac200375060683.
- Half-life, spin, and isomer data selected from the following sources. See editing notes on this article's talk page.
- G. Audi, A. H. Wapstra, C. Thibault, J. Blachot and O. Bersillon (2003). "The NUBASE evaluation of nuclear and decay properties" (PDF). Nuclear Physics A. 729: 3–128. doi:10.1016/j.nuclphysa.2003.11.001.
{{cite journal}}
: CS1 maint: multiple names: authors list (link) - National Nuclear Data Center. "NuDat 2.1 database". Brookhaven National Laboratory. Retrieved September 2005.
{{cite web}}
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(help) - N. E. Holden (2004). "Table of the Isotopes". In D. R. Lide (ed.). CRC Handbook of Chemistry and Physics (85th ed.). CRC Press. Section 11. ISBN 978-0849304859.
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- G. Audi, A. H. Wapstra, C. Thibault, J. Blachot and O. Bersillon (2003). "The NUBASE evaluation of nuclear and decay properties" (PDF). Nuclear Physics A. 729: 3–128. doi:10.1016/j.nuclphysa.2003.11.001.