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	<title>formulasearchengine - User contributions [en]</title>
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	<updated>2026-09-20T13:46:46Z</updated>
	<subtitle>User contributions</subtitle>
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	<entry>
		<id>https://en.formulasearchengine.com/w/index.php?title=Regular_local_ring&amp;diff=231461</id>
		<title>Regular local ring</title>
		<link rel="alternate" type="text/html" href="https://en.formulasearchengine.com/w/index.php?title=Regular_local_ring&amp;diff=231461"/>
		<updated>2014-03-03T06:23:00Z</updated>

		<summary type="html">&lt;p&gt;117.216.197.134: /* Examples */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;Hi there! :) My name is Stevie, I&#039;m a student studying Modern Languages and Classics from Naringal, Australia.&amp;lt;br&amp;gt;&amp;lt;br&amp;gt;My homepage ... Fifa 15 Coin Generator ([http://Hongbo.me/?document_srl=43594 http://Hongbo.me/?Document_srl=43594])&lt;/div&gt;</summary>
		<author><name>117.216.197.134</name></author>
	</entry>
	<entry>
		<id>https://en.formulasearchengine.com/w/index.php?title=Conservation_of_energy&amp;diff=1946</id>
		<title>Conservation of energy</title>
		<link rel="alternate" type="text/html" href="https://en.formulasearchengine.com/w/index.php?title=Conservation_of_energy&amp;diff=1946"/>
		<updated>2014-01-28T17:14:07Z</updated>

		<summary type="html">&lt;p&gt;117.216.70.17: /* Noether&amp;#039;s theorem */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;{{Infobox ununennium}}&lt;br /&gt;
&#039;&#039;&#039;Ununennium&#039;&#039;&#039;, also known as &#039;&#039;&#039;[[Mendeleev&#039;s predicted elements|eka]]-[[francium]]&#039;&#039;&#039; or element 119, is the temporary name of a [[chemical element]] in the [[periodic table]] that has the temporary symbol &#039;&#039;&#039;Uue&#039;&#039;&#039; and has the [[atomic number]] 119. To date, attempted syntheses of this element have been unsuccessful.  Since it is below the [[alkali metals]] it might have properties similar to those of [[francium]] or [[caesium]] and thus be extremely reactive with water and air (though [[relativistic quantum chemistry|relativistic effects]] might make it less reactive than francium and caesium). A predicted oxidation state is +1; however, unlike all the other alkali metals, it is also predicted to show the +3 oxidation state.&lt;br /&gt;
&lt;br /&gt;
Ununennium would be the first element in the eighth [[periodic table period|period]] of the [[periodic table]].&lt;br /&gt;
&lt;br /&gt;
==Attempts at synthesis==&lt;br /&gt;
The synthesis of ununennium was attempted in 1985 by bombarding a target of [[einsteinium]]-254 with [[calcium]]-48 ions at the superHILAC accelerator at Berkeley, California:&lt;br /&gt;
:&amp;lt;math&amp;gt;\,^{254}_{99}\mathrm{Es} + \,^{48}_{20}\mathrm{Ca} \to \,^{302}_{119}\mathrm{Uue} ^{*} &amp;lt;/math&amp;gt;&lt;br /&gt;
No atoms were identified, leading to a limiting yield of 300 [[barn (unit)|nb]].&amp;lt;ref&amp;gt;{{cite journal|title=Search for superheavy elements using &amp;lt;sup&amp;gt;48&amp;lt;/sup&amp;gt;Ca + &amp;lt;sup&amp;gt;254&amp;lt;/sup&amp;gt;Es&amp;lt;sup&amp;gt;g&amp;lt;/sup&amp;gt; reaction|journal=Physical Reviews C|year=1985|pages=1760–1763|doi=10.1103/PhysRevC.32.1760|volume=32|issue=5|bibcode = 1985PhRvC..32.1760L|last1=Lougheed|first1=R.|last2=Landrum|first2=J.|last3=Hulet|first3=E.|last4=Wild|first4=J.|last5=Dougan|first5=R.|last6=Dougan|first6=A.|last7=Gäggeler|first7=H.|last8=Schädel|first8=M.|last9=Moody|first9=K. |displayauthors=11}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
As of May 2012, plans are under way to attempt to synthesize the isotopes &amp;lt;sup&amp;gt;295&amp;lt;/sup&amp;gt;Uue and &amp;lt;sup&amp;gt;296&amp;lt;/sup&amp;gt;Uue by bombarding a target of [[berkelium]] with [[titanium]] at the [[GSI Helmholtz Centre for Heavy Ion Research]] in [[Darmstadt]], Germany:&amp;lt;ref name=&amp;quot;economist&amp;quot;&amp;gt;[http://www.economist.com/node/21554502 Modern alchemy: Turning a line], [[The Economist]], May 12, 2012.&amp;lt;/ref&amp;gt;&amp;lt;ref&amp;gt;Düllmann, Christoph E. (October 20, 2011). [http://fias.uni-frankfurt.de/kollo/Duellmann_FIAS-Kolloquium.pdf Superheavy Element Research: News from GSI and Mainz]. Johannes Gutenberg University Mainz; GSI Helmholtzzentrum für Schwerionenforschung GmbH; Darmstadt Helmholtz Institute Mainz.&amp;lt;/ref&amp;gt;&lt;br /&gt;
:&amp;lt;math&amp;gt;\,^{249}_{97}\mathrm{Bk} + \,^{50}_{22}\mathrm{Ti} \to \,^{296}_{119}\mathrm{Uue} \,+3\,^{1}_{0}\mathrm{n}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;\,^{249}_{97}\mathrm{Bk} + \,^{50}_{22}\mathrm{Ti} \to \,^{295}_{119}\mathrm{Uue} \,+4\,^{1}_{0}\mathrm{n}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
==Predicted decay characteristics==&lt;br /&gt;
The alpha-decay half-lives of 1700 nuclei with 100 ≤ Z ≤ 130 have been calculated in a quantum tunneling model with alpha-decay Q-values from different mass estimates.&amp;lt;ref name=npa07&amp;gt;{{cite journal|journal=Nucl. Phys. A|volume=789|pages=142–154|year=2007|title=Predictions of alpha decay half lives of heavy and superheavy elements|author=Chowdhury, P. Roy; Samanta, C. and Basu, D. N. |doi=10.1016/j.nuclphysa.2007.04.001|bibcode=2007NuPhA.789..142S|arxiv = nucl-th/0703086 }}&amp;lt;/ref&amp;gt;&amp;lt;ref&amp;gt;{{cite journal|journal=Phys. Rev. C|volume=77|pages=044603|year=2008|title=Search for long lived heaviest nuclei beyond the valley of stability|author=Chowdhury, P. Roy; Samanta, C. and Basu, D. N. |doi=10.1103/PhysRevC.77.044603|issue=4|bibcode=2008PhRvC..77d4603C|arxiv = 0802.3837 }}&amp;lt;/ref&amp;gt;&amp;lt;ref&amp;gt;{{cite journal|journal=At. Data &amp;amp; Nucl. Data Tables|volume=94|pages=781–806|year=2008|title=Nuclear half-lives for α -radioactivity of elements with 100 ≤ Z ≤ 130|author=Chowdhury, P. Roy; Samanta, C. and Basu, D. N. |doi=10.1016/j.adt.2008.01.003|issue=6|bibcode=2008ADNDT..94..781C|arxiv = 0802.4161 }}&amp;lt;/ref&amp;gt; The alpha-decay half-lives predicted for &amp;lt;sup&amp;gt;291–307&amp;lt;/sup&amp;gt;119 are of the order of micro-seconds. The highest value of the alpha-decay half-life predicted in the quantum tunneling model with the mass estimates from a macroscopic-microscopic model is ~485 microseconds for the isotope &amp;lt;sup&amp;gt;294&amp;lt;/sup&amp;gt;119. For &amp;lt;sup&amp;gt;302&amp;lt;/sup&amp;gt;119 it is ~163 microseconds.&lt;br /&gt;
&lt;br /&gt;
==Target-projectile combinations leading to Z=119 compound nuclei==&lt;br /&gt;
The below table contains various combinations of targets and projectiles which could be used to form compound nuclei with an atomic number of 119.&lt;br /&gt;
&lt;br /&gt;
{|class=&amp;quot;wikitable&amp;quot; style=&amp;quot;text-align:center&amp;quot;&lt;br /&gt;
&lt;br /&gt;
!Target!!Projectile!!CN!!Attempt result&lt;br /&gt;
|-&lt;br /&gt;
!&amp;lt;sup&amp;gt;254&amp;lt;/sup&amp;gt;Es&lt;br /&gt;
|&amp;lt;sup&amp;gt;48&amp;lt;/sup&amp;gt;Ca||&amp;lt;sup&amp;gt;302&amp;lt;/sup&amp;gt;Uue||{{no|Failure to date}}&lt;br /&gt;
|-&lt;br /&gt;
!&amp;lt;sup&amp;gt;249&amp;lt;/sup&amp;gt;Bk&lt;br /&gt;
|&amp;lt;sup&amp;gt;50&amp;lt;/sup&amp;gt;Ti||&amp;lt;sup&amp;gt;299&amp;lt;/sup&amp;gt;Uue||{{unk|Planned reaction}}&lt;br /&gt;
|}&amp;lt;!--Please use {{yes|Successful reaction}} for successes, thanks--&amp;gt;&lt;br /&gt;
&lt;br /&gt;
==Theoretical calculations on evaporation cross sections==&lt;br /&gt;
The below table contains various targets-projectile combinations for which calculations have provided estimates for cross section yields from various neutron evaporation channels. The channel with the highest expected yield is given.&lt;br /&gt;
&lt;br /&gt;
DNS = Di-nuclear system; σ = cross section&lt;br /&gt;
&lt;br /&gt;
{|class=&amp;quot;wikitable&amp;quot; style=&amp;quot;text-align:center&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
!Target!!Projectile!!CN!!Channel (product)!!σ &amp;lt;sub&amp;gt;max&amp;lt;/sub&amp;gt;!!Model!!Ref&lt;br /&gt;
|-&lt;br /&gt;
!&amp;lt;sup&amp;gt;254&amp;lt;/sup&amp;gt;Es&lt;br /&gt;
|&amp;lt;sup&amp;gt;48&amp;lt;/sup&amp;gt;Ca||&amp;lt;sup&amp;gt;302&amp;lt;/sup&amp;gt;Uue||3n (&amp;lt;sup&amp;gt;299&amp;lt;/sup&amp;gt;Uue)||0.5 pb||DNS||&amp;lt;ref&amp;gt;{{cite journal|arxiv=0803.1117|doi=10.1016/j.nuclphysa.2008.11.003|title=Production of heavy and superheavy nuclei in massive fusion reactions|year=2009|author=Feng, Z|journal=Nuclear Physics A|volume=816|page=33|last2=Jin|first2=G|last3=Li|first3=J|last4=Scheid|first4=W|bibcode=2009NuPhA.816...33F}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
==Extrapolated chemical properties==&lt;br /&gt;
Ununennium is expected to behave normally for an alkali metal and exhibit a strong +1 [[oxidation state]]. However, the energetic properties of its [[valence electron]] would increase its first [[ionization energy]], making it less reactive than expected and more like [[potassium]] than [[caesium]] chemically. This would also decrease the [[metallic radius|metallic]] and [[ionic radius|ionic radii]] of ununennium.&amp;lt;ref name=EB&amp;gt;{{cite web|author=Seaborg|url=http://www.britannica.com/EBchecked/topic/603220/transuranium-element|title=transuranium element (chemical element)|publisher=Encyclop&amp;amp;aelig;dia Britannica|date=c. 2006|accessdate=2010-03-16}}&amp;lt;/ref&amp;gt; Ununennium is also predicted to be the first alkali metal to display the +3 oxidation state, due to the ionization energy of the 7p&amp;lt;sub&amp;gt;3/2&amp;lt;/sub&amp;gt; electrons, which is predicted to be very low.&amp;lt;ref name=Haire/&amp;gt;&lt;br /&gt;
&lt;br /&gt;
==See also==&lt;br /&gt;
*[[Extended periodic table]]&lt;br /&gt;
&lt;br /&gt;
==References==&lt;br /&gt;
{{clear}}&lt;br /&gt;
{{Reflist|colwidth=30em}}&lt;br /&gt;
&lt;br /&gt;
{{Compact extended periodic table}}&lt;br /&gt;
&lt;br /&gt;
[[Category:Chemical elements]]&lt;br /&gt;
[[Category:Alkali metals]]&lt;br /&gt;
[[Category:Hypothetical chemical elements]]&lt;/div&gt;</summary>
		<author><name>117.216.70.17</name></author>
	</entry>
	<entry>
		<id>https://en.formulasearchengine.com/w/index.php?title=Gross_enrolment_ratio&amp;diff=12746</id>
		<title>Gross enrolment ratio</title>
		<link rel="alternate" type="text/html" href="https://en.formulasearchengine.com/w/index.php?title=Gross_enrolment_ratio&amp;diff=12746"/>
		<updated>2013-12-08T06:31:01Z</updated>

		<summary type="html">&lt;p&gt;117.216.176.13: /* Example */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;{{Unreferenced|date=December 2009}}&lt;br /&gt;
&amp;lt;!-- ==CDF method== will do this later --&amp;gt;&lt;br /&gt;
In [[probability theory]], it is possible to approximate the [[moment (mathematics)|moments]] of a function &#039;&#039;f&#039;&#039; of a [[random variable]] &#039;&#039;X&#039;&#039; using [[Taylor expansion]]s, provided that &#039;&#039;f&#039;&#039; is sufficiently differentiable and that the moments of &#039;&#039;X&#039;&#039; are finite.  This technique is often used by [[statistics|statisticians]].&lt;br /&gt;
&amp;lt;!--&lt;br /&gt;
::{|&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;math&amp;gt;\mu&amp;lt;/math&amp;gt;&lt;br /&gt;
|&amp;lt;math&amp;gt; = \operatorname{E}\left[X\right]&amp;lt;/math&amp;gt;&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;math&amp;gt;\sigma^2&amp;lt;/math&amp;gt; &lt;br /&gt;
|&amp;lt;math&amp;gt; = \operatorname{var}\left[X\right]&amp;lt;/math&amp;gt;&lt;br /&gt;
|}--&amp;gt;&lt;br /&gt;
&lt;br /&gt;
==First moment==&lt;br /&gt;
: &amp;lt;math&amp;gt;&lt;br /&gt;
\begin{align}&lt;br /&gt;
\operatorname{E}\left[f(X)\right] &amp;amp; {} = \operatorname{E}\left[f(\mu_X + \left(X - \mu_X\right))\right] \\&lt;br /&gt;
&amp;amp; {} \approx \operatorname{E}\left[f(\mu_X) + f&#039;(\mu_X)\left(X-\mu_X\right) + \frac{1}{2}f&#039;&#039;(\mu_X) \left(X - \mu_X\right)^2 \right].&lt;br /&gt;
\end{align}&lt;br /&gt;
&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
Noting that &amp;lt;math&amp;gt;E[X-\mu_X]=0&amp;lt;/math&amp;gt;, the 2nd term disappears. Also &amp;lt;math&amp;gt;E[(X-\mu_X)^2]&amp;lt;/math&amp;gt; is &amp;lt;math&amp;gt;\sigma_X^2&amp;lt;/math&amp;gt;. Therefore,&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;\operatorname{E}\left[f(X)\right]\approx f(\mu_X) +\frac{f&#039;&#039;(\mu_X)}{2}\sigma_X^2&amp;lt;/math&amp;gt;&lt;br /&gt;
where &amp;lt;math&amp;gt;\mu_X&amp;lt;/math&amp;gt; and &amp;lt;math&amp;gt;\sigma^2_X&amp;lt;/math&amp;gt; are the mean and variance of X respectively.&lt;br /&gt;
&lt;br /&gt;
It is possible to generalize this to functions of more than one variable using [[Taylor expansion#Taylor series in several variables|multivariate Taylor expansions]]. For example,&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;\operatorname{E}\left[\frac{X}{Y}\right]\approx\frac{\operatorname{E}\left[X\right]}{\operatorname{E}\left[Y\right]} -\frac{\operatorname{cov}\left[X,Y\right]}{\operatorname{E}\left[Y\right]^2}+\frac{\operatorname{E}\left[X\right]}{\operatorname{E}\left[Y\right]^3}\operatorname{var}\left[Y\right]&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
==Second moment==&lt;br /&gt;
Analogously,&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;\operatorname{var}\left[f(X)\right]\approx \left(f&#039;(\operatorname{E}\left[X\right])\right)^2\operatorname{var}\left[X\right] = \left(f&#039;(\mu_X)\right)^2\sigma^2_X.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
The above is using a first order approximation unlike for the method used in estimating the first moment. It will be a poor approximation in cases where &amp;lt;math&amp;gt;f(X)&amp;lt;/math&amp;gt; is highly non-linear. This is a special case of the [[delta method]]. For example,&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;\operatorname{var}\left[\frac{X}{Y}\right]\approx\frac{\operatorname{var}\left[X\right]}{\operatorname{E}\left[Y\right]^2}-\frac{2\operatorname{E}\left[X\right]}{\operatorname{E}\left[Y\right]^3}\operatorname{cov}\left[X,Y\right]+\frac{\operatorname{E}\left[X\right]^2}{\operatorname{E}\left[Y\right]^4}\operatorname{var}\left[Y\right].&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
==See also==&lt;br /&gt;
*[[Propagation of uncertainty]]&lt;br /&gt;
*[[WKB approximation]]&lt;br /&gt;
*http://www.stanford.edu/class/cme308/notes/TaylorAppDeltaMethod.pdf&lt;br /&gt;
&lt;br /&gt;
{{DEFAULTSORT:Taylor Expansions For The Moments Of Functions Of Random Variables}}&lt;br /&gt;
[[Category:Statistical approximations]]&lt;br /&gt;
[[Category:Algebra of random variables]]&lt;/div&gt;</summary>
		<author><name>117.216.176.13</name></author>
	</entry>
	<entry>
		<id>https://en.formulasearchengine.com/w/index.php?title=Skew-Hermitian_matrix&amp;diff=5306</id>
		<title>Skew-Hermitian matrix</title>
		<link rel="alternate" type="text/html" href="https://en.formulasearchengine.com/w/index.php?title=Skew-Hermitian_matrix&amp;diff=5306"/>
		<updated>2013-06-30T05:59:12Z</updated>

		<summary type="html">&lt;p&gt;117.216.34.162: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;&#039;&#039;&#039;LIX&#039;&#039;&#039; is a [[readability test|readability measure]] indicating the difficulty of reading a text&amp;lt;ref&amp;gt;http://reap.cs.cmu.edu/Papers/IASTED-HCI-05-jonbrown.pdf&amp;lt;/ref&amp;gt; developed by [[Swedes|Swedish]] scholar [[Carl-Hugo Björnsson]]. It is computed as follows:&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;\text{LIX} = \frac{A}{B} + \frac{C \cdot 100}{A}&amp;lt;/math&amp;gt;, where&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;A&amp;lt;/math&amp;gt; is the number of words,&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;B&amp;lt;/math&amp;gt; is the number of periods (defined by period, colon or capital first letter), and&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;C&amp;lt;/math&amp;gt; is the number of long words (more than 6 letters).&amp;lt;ref&amp;gt;[http://www.iva.dk/bh/core%20concepts%20in%20lis/articles%20a-z/readability.htm ]&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
==References==&lt;br /&gt;
&amp;lt;references/&amp;gt;&lt;br /&gt;
&lt;br /&gt;
==Further reading==&lt;br /&gt;
* Björnsson, C. H. (1968). Läsbarhet. Stockholm: Liber.&lt;br /&gt;
* Björnsson, C. H. (1971). Læsbarhed. København: Gad.&lt;br /&gt;
&lt;br /&gt;
==External links==&lt;br /&gt;
* {{Official website|http://www.lix.se/ }}&lt;br /&gt;
* [http://www.standards-schmandards.com/exhibits/rix/ Calculator for LIX and other readability indices]&lt;br /&gt;
&lt;br /&gt;
[[Category:Readability tests]]&lt;/div&gt;</summary>
		<author><name>117.216.34.162</name></author>
	</entry>
</feed>