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		<title>en&gt;Waacstats: /* References */Add persondata short description using AWB</title>
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		<updated>2014-01-01T12:12:22Z</updated>

		<summary type="html">&lt;p&gt;&lt;span class=&quot;autocomment&quot;&gt;References: &lt;/span&gt;Add persondata short description using &lt;a href=&quot;/w/index.php?title=Testwiki:AWB&amp;amp;action=edit&amp;amp;redlink=1&quot; class=&quot;new&quot; title=&quot;Testwiki:AWB (page does not exist)&quot;&gt;AWB&lt;/a&gt;&lt;/p&gt;
&lt;p&gt;&lt;b&gt;New page&lt;/b&gt;&lt;/p&gt;&lt;div&gt;{{Multiple issues|{{copy edit|date=November 2013}}{{citation style|date=November 2013}}{{technical|date=November 2013}}}}&lt;br /&gt;
&lt;br /&gt;
== Non-extensive self-consistent thermodynamics ==&lt;br /&gt;
&lt;br /&gt;
The non-extensive self-consistent thermodynamical theory keeps the concept of [[Fireball concept|fireball]] for high-energy particle collisions at the same time that uses the [[Constantino Tsallis|Tsallis]] [[Tsallis statistics|non-extensive thermodynamics]].&amp;lt;ref&amp;gt;A. Deppman, Physica A 391 (2012) 6380.&amp;lt;/ref&amp;gt;&lt;br /&gt;
Fireballs lead naturally to the bootstrap-idea, or self-consistency principle, just as it happens in the case of the Boltzmann statistics used by [[Rolf Hagedorn|Hagedorn]].&amp;lt;ref&amp;gt;R. Hagedorn, Suppl. Al Nuovo Cimento 3 (1965) 147.&amp;lt;/ref&amp;gt; Assuming that the distribution function gets modifications due to possible symmetrical change, [[Abdel Nasser Tawfik]] applied the non-extensive concepts on high-energy particle production.&amp;lt;ref&amp;gt;A. Tawfik, Int. J. Theor. Phys, 51, 1396-1407 (2012); arXiv:1011.6622 [hep-ph].&amp;lt;/ref&amp;gt;&amp;lt;ref&amp;gt;A. Tawfik, Prog. Theor. Phys. 126, 279-292 (2011)&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
The motivation to use the non-extensive statistics from Tsallis&amp;lt;ref&amp;gt;C. Tsallis,  J Stat Phys 52, 479-487, 1988.&amp;lt;/ref&amp;gt; comes from the results obtained by Bediaga et al.,&amp;lt;ref&amp;gt;I. Bediaga, E.M.F. Curado and J.M. de Miranda, Physica A 286 (2000) 156.&amp;lt;/ref&amp;gt; who showed that with the substitution of the [[Boltzmann]] [[Boltzmann factor|factor]] which appears in the Hagedorn&amp;#039;s theory by the [[Tsallis_statistics#q-exponential|q-exponential function]], it was possible to recover the good agreement between calculation and experiment, even at energies as high as those achieved at [[LHC]], with &amp;lt;math&amp;gt;q&amp;gt;1&amp;lt;/math&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
==Non-extensive entropy for ideal quantum gas==&lt;br /&gt;
The starting point for the theory is entropy for a non-extensive quantum gas of bosons and fermions, as proposed by Conroy, Miller and Plastino,&amp;lt;ref&amp;gt;J.M. Conroy, H.G. Miller, A.R. Plastino, Phys. Lett. A 374 (2010) 4581–4584.&amp;lt;/ref&amp;gt; which is given by &amp;lt;math&amp;gt;S_q=S_q^{FD}+S_q^{BE}&amp;lt;/math&amp;gt; where &amp;lt;math&amp;gt;S_q^{FD}&amp;lt;/math&amp;gt; is the non-extensive version of the [[Fermi-Dirac statistics|Fermi-Dirac]] entropy and &amp;lt;math&amp;gt;S_q^{BE}&amp;lt;/math&amp;gt; is the non-extensive version of the [[Bose–Einstein statistics|Bose-Einstein]] entropy.&lt;br /&gt;
&lt;br /&gt;
As shown by Conroy, Miller and Plastino&amp;lt;ref&amp;gt;J.M. Conroy, H.G. Miller and A.R. Plastino, Physics Letters A 374 (2010) 4581–4584.&amp;lt;/ref&amp;gt; and also by Cleymans and Worku,&amp;lt;ref&amp;gt;J. Cleymans and D. Worku, J. Phys. G 39 (2012) 025006.&amp;lt;/ref&amp;gt; the entropy just defined leads to occupation numbers formulaes&lt;br /&gt;
that reduces to the one used by Bediaga et al. and by C. Beck,&amp;lt;ref&amp;gt;C. Beck, Physica A 286 (2000) 164–180.&amp;lt;/ref&amp;gt; and shows the power-like tails present in the distributions found in High Energy Physics experiments.&lt;br /&gt;
&lt;br /&gt;
== Non-extensive partition function for ideal quantum gas ==&lt;br /&gt;
Using the entropy defined above, the [[Partition function (statistical mechanics)|partition function]] results to be&lt;br /&gt;
:&amp;lt;math&amp;gt; \ln[1+Z_q(V_o,T)]=\frac{V_o}{2\pi^2}\sum_{n=1}^{\infty}\frac{1}{n}\int_0^{\infty}dm \int_0^{\infty}dp \, p^2 \rho(n;m)[1+(q-1)\beta \sqrt{p^2+m^2}]^{-\frac{nq}{(q-1)}} \,.&amp;lt;/math&amp;gt;&lt;br /&gt;
Since experiments have shown that &amp;lt;math&amp;gt;q&amp;gt;1&amp;lt;/math&amp;gt;, this restriction is adopted.&lt;br /&gt;
&lt;br /&gt;
Another way to write the non-extensive partition function for a fireball is&lt;br /&gt;
:&amp;lt;math&amp;gt; Z_q(V_o,T)=\int_0^{\infty}\sigma(E)[1+(q-1)\beta E]^{-\frac{q}{(q-1)}} dE\,,&amp;lt;/math&amp;gt;&lt;br /&gt;
where &amp;lt;math&amp;gt;\sigma(E)&amp;lt;/math&amp;gt; is the density of states of the fireballs.&lt;br /&gt;
&lt;br /&gt;
==Self-consistency principle==&lt;br /&gt;
The self-consistency implies that both forms of partition functions must be asymptotically equivalent and that the mass spectrum and the [[density of states]] must be related to each other by&lt;br /&gt;
:&amp;lt;math&amp;gt; log[\rho(m)]= log[\sigma(E)] &amp;lt;/math&amp;gt;,&lt;br /&gt;
in the limit of &amp;lt;math&amp;gt;m,E&amp;lt;/math&amp;gt; sufficiently large.&lt;br /&gt;
&lt;br /&gt;
The self-consistency can be asymptotically achieved by choosing&amp;lt;ref&amp;gt;A. Deppman, Physica A 391 (2012) 6380.&amp;lt;/ref&amp;gt;&lt;br /&gt;
:&amp;lt;math&amp;gt; m^{3/2} \rho(m)=\frac{\gamma}{m}\big[1+(q_o-1) \beta _o m\big]^{\frac{1}{q_o -1}}=\frac{\gamma}{m}[1+(q&amp;#039;_o-1)  m]^{\frac{\beta _o}{q&amp;#039;_o -1}}&amp;lt;/math&amp;gt;&lt;br /&gt;
and&lt;br /&gt;
:&amp;lt;math&amp;gt;\sigma(E)=bE^a\big[1+(q&amp;#039;_o-1)E\big]^{\frac{\beta _o}{q&amp;#039;_o -1}}\,,&amp;lt;/math&amp;gt;&lt;br /&gt;
where &amp;lt;math&amp;gt;\gamma&amp;lt;/math&amp;gt; is a constant and &amp;lt;math&amp;gt;q&amp;#039;_o-1=\beta _o (q_o-1)&amp;lt;/math&amp;gt;. Here, &amp;lt;math&amp;gt;a,b,\gamma&amp;lt;/math&amp;gt; are arbitrary constants. For &amp;lt;math&amp;gt;q&amp;#039; \rightarrow 1&amp;lt;/math&amp;gt; the two expressions above approach the corresponding expressions in the Hagedorn&amp;#039;s theory.&lt;br /&gt;
&lt;br /&gt;
==Main results==&lt;br /&gt;
With the mass spectrum and density of states given above, the asymptotic form of the partition function results to be&lt;br /&gt;
:&amp;lt;math&amp;gt; Z_q(V_o,T) \rightarrow \bigg(\frac{1}{\beta - \beta _o }\bigg)^{\alpha}&amp;lt;/math&amp;gt;&lt;br /&gt;
where&lt;br /&gt;
:&amp;lt;math&amp;gt;\alpha=\frac{\gamma V_o}{2\pi^2 \beta^{3/2}}\,,&amp;lt;/math&amp;gt;&lt;br /&gt;
with&lt;br /&gt;
:&amp;lt;math&amp;gt; a+1=\alpha=\frac{\gamma V_o}{2\pi^2 \beta^{3/2}} \,.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
One immediate consequence of the expression for the partition function is the existence of a limiting temperature &amp;lt;math&amp;gt;T_o=1/\beta _o&amp;lt;/math&amp;gt;. This result is equivalent to the important result obtained by Hagedorn.&amp;lt;ref&amp;gt;R. Hagedorn, Suppl. Al Nuovo Cimento 3 (1965) 147.&amp;lt;/ref&amp;gt; With these results it is expected that at sufficiently high energy collisions the fireball will present not only a constant temperature, but also constant entropic factor.&lt;br /&gt;
&lt;br /&gt;
==Experimental evidences==&lt;br /&gt;
&lt;br /&gt;
Experimental evidences of the existence of a limiting temperature and of a limiting entropic index can be found in the papers by J. Cleymans and collaborators,&amp;lt;ref&amp;gt;J. Cleymans and D. Worku, J. Phys. G: Nucl. Part. Phys. 39 (2012)&lt;br /&gt;
025006.&amp;lt;/ref&amp;gt;&amp;lt;ref&amp;gt;J. Cleymans, G.I. Lykasov, A.S. Parvan, A.S. Sorin, O.V. Teryaev and&lt;br /&gt;
D. Worku, arXiv:1302.1970 (2013).&amp;lt;/ref&amp;gt; by Isaac Sena and A. Deppman.&amp;lt;ref&amp;gt;I. Sena and A. Deppman, Eur. Phys. J. A 49 (2013) 17.&amp;lt;/ref&amp;gt;&amp;lt;ref&amp;gt;I. Sena and A. Deppman, AIP Conf. Proc. 1520, 172 (2013) -&lt;br /&gt;
arXiv:1208.2952v1.&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
==References==&lt;br /&gt;
{{Reflist}}&lt;br /&gt;
&lt;br /&gt;
[[Category:Particle physics]]&lt;br /&gt;
[[Category:Nuclear physics]]&lt;br /&gt;
[[Category:Principles]]&lt;/div&gt;</summary>
		<author><name>en&gt;Waacstats</name></author>
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