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Access to Content of deleted edits

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There are 4 deletions on the page of Banu Qurayza, all of which correspond to major edits. The reasons listed on the deletions is that they violate copywrite. The page itself is implicated in an ANI outcome (Incident archive 1159: Kaalakaa on Islam-related topics) where a consensus of uninvolved found that the user @Kaalakaa maintained a collection of NPOV abused pages on Islam related topics, including this page.

I would like to request a copy of the deleted content (3 most recent deletions), all of which were found violating RD1: Copywrite. I would like to salvage the knowledge and assess if portions of it remain relevant. If so, remedy it of its violation to be reintroduced, as long as its citations are of acceptable standard.

Thank you for your time and consideration. Bro The Man (talk) 08:51, 16 October 2024 (UTC)[reply]

@Bro The Man: I cannot provide or reinstate content that was deleted as copyright infringement. Additionally, the additions of infringing content were immediately reverted, so they had no long-term impact on the overall accuracy and neutrality.
The deletion log entries include some of the sources from which material was copied, though, and you are free to assess the original sources for relevance and write fresh content in your own words. However, I am not familiar enough with the subject matter to point you to the best available sources. I see that you also started a thread on the article's talk page and I hope that you find assistance there. Thanks, Complex/Rational 16:33, 16 October 2024 (UTC)[reply]
So it was just blocks of copy-pastes? If that's so, then that's useless, lmao. Please, let me know if i understood you correctly. Bro The Man (talk) 18:27, 16 October 2024 (UTC)[reply]
I haven't checked it thoroughly, but in general, copyright infringement refers to improper verbatim copy-and-paste or close paraphrasing. So yes, you'll find essentially the same material in the original sources as you would in the deleted version. Complex/Rational 19:59, 16 October 2024 (UTC)[reply]

Invitation to participate in a research

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Hello,

The Wikimedia Foundation is conducting a survey of Wikipedians to better understand what draws administrators to contribute to Wikipedia, and what affects administrator retention. We will use this research to improve experiences for Wikipedians, and address common problems and needs. We have identified you as a good candidate for this research, and would greatly appreciate your participation in this anonymous survey.

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BGerdemann (WMF) (talk) 19:23, 23 October 2024 (UTC) [reply]

since you mentioned "perhaps the full article has still more" regarding Lv

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The full article is available from Lund University. :) Double sharp (talk) 17:06, 24 October 2024 (UTC)[reply]

@Double sharp: Thanks for sharing! Complex/Rational 17:08, 24 October 2024 (UTC)[reply]

6-year editaversary

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Sdkbtalk 05:32, 28 October 2024 (UTC)[reply]

@Sdkb: Thank you! Here's to another trip around the Sun! Complex/Rational 12:46, 28 October 2024 (UTC)[reply]

Happy First Edit Day!

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@DaniloDaysOfOurLives: Thank you! Complex/Rational 22:53, 28 October 2024 (UTC)[reply]

Silicon-45 and 46 discovered

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New paper. Also of interest to Nucleus hydro elemon. :) Double sharp (talk) 04:26, 1 November 2024 (UTC)[reply]

@Double sharp: Cool, thanks! Fortunately this one is open-access. Complex/Rational 13:50, 1 November 2024 (UTC)[reply]
Another exciting discovery, thanks! It seems like all the recent discoveries are light nuclides. For the heavier nuclides, it seems like light isotopes perform better in synthesizing Uue. Nucleus hydro elemon (talk) 13:53, 1 November 2024 (UTC)[reply]
@Nucleus hydro elemon: I suspect people stick to the heavy ones because they want the half-life of the product to be long enough to detect. ;) Double sharp (talk) 03:49, 2 November 2024 (UTC)[reply]
doi:10.1142/S0218301320500536 predicts among 284-308Uue, 296,300,302Uue have a half-life of >100 μs. (297,308Uue may reach this bar or not depends on prediction used) Only 296Uue is a reasonable long-lived isotope to be synthesized among them. 297Uue requires either 2n channel, 250Cm, or einsteinium, while even heavier isotopes are more unlikely to produce.
On the other hand, I found lighter isotopes 292,293Uue interesting because the whole decay chain is unknown. However, their predicted half-lives of ~30 μs is troublesome. Nucleus hydro elemon (talk) 08:22, 2 November 2024 (UTC)[reply]
If only 241Am+48Ca and 231Pa+48Ca would get studied. :( Double sharp (talk) 12:06, 2 November 2024 (UTC)[reply]
It does indeed seem that even-Z SHEs have been getting much of the attention lately. Meanwhile, the gap between cold and hot fusion persists for odd-Z elements, and Mt and Rg each have one isotope that has been directly synthesized... decades ago. Complex/Rational 16:32, 2 November 2024 (UTC)[reply]
Since you mention 266Mt from 1982: Peter Armbruster and Gottfried Münzenberg both died this year. :( (Sigurd Hofmann died in 2022.) Double sharp (talk) 16:36, 2 November 2024 (UTC)[reply]
I guess the even-Z gap gets studied more because it looks like 120 is going to be easier than 119. Maybe once 120 is discovered, we'll see a renaissance of interest in the odd ones. Double sharp (talk) 16:43, 2 November 2024 (UTC)[reply]
@Double sharp: I stumbled upon this, which mentions a proposed search for 276Rg and 272Mt (along with 250Lr and 254Db) – though neither a reaction nor an experimental timeframe are described. If year 1 was 2020, we're in year 5, and I haven't found anything more recent, so I wonder what became of this.
There was also an SHE-related conference earlier this year at FRIB, though I don't know if the conference proceedings have been uploaded anywhere. Complex/Rational 02:06, 11 November 2024 (UTC)[reply]
Well, the 50Ti agenda happened quite similarly to the plan of those slides, with the 244Pu+50Ti reaction having succeeded. Perhaps the other things happened, or perhaps it was decided that going for 120 was more exciting. Yeah, that's kind of a non-answer. ;) Double sharp (talk) 04:29, 11 November 2024 (UTC)[reply]

242Pu+50Ti

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New presentation from JINR! With 289Lv! And 280Cn! And a p2n channel leading to 289Mc!! Double sharp (talk) 15:19, 2 November 2024 (UTC)[reply]

@Nucleus hydro elemon: Since you just noted that lately it had mostly been light nuclides getting discovered! :D Double sharp (talk) 15:20, 2 November 2024 (UTC)[reply]
@Double sharp: Thanks for sharing the exciting news! I suppose the new isotopes could be added, but I'm not sure that WP:CALC permits computing half-lives in the absence of aggregated data and complete analysis... so a more detailed update will likely have to wait. Complex/Rational 15:34, 2 November 2024 (UTC)[reply]
Yeah, I've confined myself to just adding their existence. (Well, I guess their colour in the Table of nuclides can be handwaved as obvious; computing the detailed half-life is too much, but it's too obvious that it must be <1 d. :D) Double sharp (talk) 15:34, 2 November 2024 (UTC)[reply]
As the decay chain of 289Lv passes through 269Sg, its half-life must be revised. Perhaps the most stable isotope of Sg will become 269Sg again. Nucleus hydro elemon (talk) 06:52, 3 November 2024 (UTC)[reply]
Wow, one more nuclide with Z:N = 2:3 found, whoopee! Discovering 295Og in the future would complete this huge family from 5He to 295Og, spanning from the beginning to the end of the periodic table. 129.104.65.2 (talk) 00:06, 3 November 2024 (UTC)[reply]
I'm looking forward to synthesis of 295,296Og with 250,251,252Cf + 48Ca and 248Cm + 50Ti. Besides that, I'm also hoping for the discovery of 293Og to clean up Ninov's mess completely. Nucleus hydro elemon (talk) 06:59, 3 November 2024 (UTC)[reply]
@Nucleus hydro elemon: You know what else I want? A sustained search for the pxn channel from 248Cm+48Ca to get heavier Mc isotopes (to see if they really electron-capture their way to the middle of the island), plus sustained looks at 242Cm+48Ca to get even lighter Lv isotopes. And the odd-Z cases too, but you already know that. I guess the dream of using 250Cm will have to languish in limbo for a long while. :)
I guess a sustained 249Cf+48Ca campaign might well actually find 293Og in the 4n channel. Double sharp (talk) 07:03, 3 November 2024 (UTC)[reply]
248Cm(48Ca,p3n)292Mc has extremely bad cross section (12 fb).[1] I found nothing about 242Cm+48Ca, probably because 242Cm is too unstable, even more unstable than 249Bk. I think 238-240Pu+50Ti makes more sense, but there exists only a prediction 43 years ago, which states 238Pu(48Ca,4n)284Lv has a cross section of a few pb.[2]
I have a complicated feeling towards nuclides at the island of stability, especially if they have a half-life in centuries or millennia. After formed from the EC chain, the atom will outlive any SHE researcher, so no one can know its decay properties. It might be hard to detect the existence of this long-lived atom. I don't think chemistry can be done, as chemistry done in a single atom relies on its radioactive decay, which this long-lived atom will never do in a reasonable timeframe. Nucleus hydro elemon (talk) 08:06, 3 November 2024 (UTC)[reply]
@Nucleus hydro elemon: True, but I guess an ER that has no plausible SF event following it would be quite a sign that the island's been reached at least. And yeah, 242Cm is perhaps a bit ambitious, but at least 243Cm has a half-life of a few decades and will get us most of the way. :) Double sharp (talk) 08:11, 3 November 2024 (UTC)[reply]
Found a prediction about 243Cm+46,48Ca.[3] It also predicts 245Cm+46Ca, but this reaction is worse than 243Cm+48Ca in all channels, so I ignored it. Cross sections are square bracketed and in pb.
  • 243Cm(48Ca,3n)288Lv [1.53]
  • 243Cm(48Ca,4n)287Lv [0.36]
  • 243Cm(48Ca,5n)286Lv [0.29]
  • 243Cm(46Ca,3n)286Lv [1.69]
  • 243Cm(46Ca,4n)285Lv [0.27]
  • 243Cm(46Ca,5n)284Lv [0.17]
Nucleus hydro elemon (talk) 09:59, 3 November 2024 (UTC)[reply]
The funny thing is that 244Pu+50Ti (0.44+0.58
−0.28
 pb
) seems to have a larger cross-section than 208Pb+70Zn (0.078+0.179
−0.065
 pb
). If not for the serendipitous 294Og atom produced in 2012 during a Ts campaign (when the 249Bk target had significantly decayed), I wonder if it might've been tried last decade, as it would both confirm 118 by producing its daughter 290Lv, and provide useful experience with 50Ti back when people were already thinking about 119 and 120. Though looking at the trend, it seems distressingly plausible that current technology levels have simply made 119 and 120 go from "it's not gonna happen" to "sure, if you're willing to spend years and years like RIKEN did with 113"... Double sharp (talk) 08:14, 3 November 2024 (UTC)[reply]
The source I added to moscovium also discusses αxn channels, and suggests they may be more favorable to produce heavier Mc isotopes from 249Bk and 48Ca. On the other side, some of the neutron deficient even–even isotopes may have very short SF half-lives (predicted by several sources and supported by observations of 284Fl, 282Cn, and now 280Cn), so they may not be readily detectable even with cross sections within experimental detection limits. Complex/Rational 15:08, 3 November 2024 (UTC)[reply]

I'm kind of wondering how we should handle the successful pxn – it doesn't fit quite well with how the superheavy "isotopes of X" pages are currently handled. Well, what a happy problem to have! Double sharp (talk) 15:53, 2 November 2024 (UTC)[reply]

@Double sharp: And a happy problem to solve! Time to update island of stability next while we await detailed results. Complex/Rational 16:08, 2 November 2024 (UTC)[reply]

References

  1. ^ Wu, Zhi-Han; Zhu, Long; Li, Fan; Yu, Xiao-Bin; Su, Jun; Guo, Chen-Chen (2018-06-11). "Synthesis of neutron-rich superheavy nuclei with radioactive beams within the dinuclear system model". Physical Review C. 97 (6). American Physical Society (APS). doi:10.1103/physrevc.97.064609. ISSN 2469-9985.
  2. ^ Magda, M T; Pop, A; Poenaru, D; Sandulescu, A; Greiner, W (1981). "Synthesis of superheavy elements in heavy-ion fusion reactions". Journal of Physics G: Nuclear Physics. 7 (3). IOP Publishing: 359–370. doi:10.1088/0305-4616/7/3/011. ISSN 0305-4616.
  3. ^ Zhu, Long; Su, Jun; Zhang, Feng-Shou (2016-06-22). "Influence of the neutron numbers of projectile and target on the evaporation residue cross sections in hot fusion reactions". Physical Review C. 93 (6). American Physical Society (APS). doi:10.1103/physrevc.93.064610. ISSN 2469-9985.

Administrators' newsletter – November 2024

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News and updates for administrators from the past month (October 2024).

Administrator changes

readded
removed

CheckUser changes

removed Maxim

Oversighter changes

removed Maxim

Guideline and policy news

Technical news

  • Mass deletions done with the Nuke tool now have the 'Nuke' tag. This change will make reviewing and analyzing deletions performed with the tool easier. T366068

Arbitration

Miscellaneous


Plutonium-226

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@ComplexRational and Nucleus hydro elemon: JINR preprint (in Russian). See p. 7: it alpha decays with a lower half-life limit of 1 ms. :) Double sharp (talk) 08:04, 9 November 2024 (UTC)[reply]

Interesting :) Its predicted alpha half-life is 1.3 ms (doi:10.1016/j.physletb.2022.137569), which is consistent with the experimental half-life >1 ms. The prediction also predicts its double alpha half-life will be 537 ms.
Looking forward to the publication and additional discoveries. Also hoping that some of the missing or poorly-studied isotopes described in NUBASE2020 are the subject of future work. Complex/Rational 01:57, 11 November 2024 (UTC)[reply]
By the way, 222Rn is also listed in the list of nuclides predicted with shortest double alpha half-lives. With a predicted half-life of 3 years, this decay mode is observable. Unfortunately, I'm not sure is there a way to separate 222Rn→218Po→214Pb and direct 222Rn→214Pb. Nucleus hydro elemon (talk) 11:15, 9 November 2024 (UTC)[reply]
If I'm understanding correctly, there should be a measurable time delay if 218Po is produced as an intermediate product, whereas double alpha decay would feature both alphas emitted simultaneously. I haven't read many articles about this, but I'd instead think it would be harder to distinguish double alpha decay from 8Be cluster emission. Complex/Rational 01:57, 11 November 2024 (UTC)[reply]
According to the predictions, double alpha decays (if we have method to distinguish them from two separate alpha decays) of 148Sm and 152Gd are clearly observable! (Perhaps also 150Gd and 154Dy, if these two nuclides are available). 129.104.241.5 (talk) 23:12, 13 November 2024 (UTC)[reply]

November 22 + 26: Free Culture Friday and Wikicurious photo event!

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Reminder to participate in Wikipedia research

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BGerdemann (WMF) (talk) 00:18, 13 November 2024 (UTC) [reply]