<?xml version="1.0"?>
<feed xmlns="http://www.w3.org/2005/Atom" xml:lang="hi">
	<id>https://hi.bharatpedia.org/w/index.php?action=history&amp;feed=atom&amp;title=%E0%A4%B8%E0%A4%BE%E0%A4%B9%E0%A4%BE_%E0%A4%B8%E0%A4%AE%E0%A5%80%E0%A4%95%E0%A4%B0%E0%A4%A3</id>
	<title>साहा समीकरण - अवतरण इतिहास</title>
	<link rel="self" type="application/atom+xml" href="https://hi.bharatpedia.org/w/index.php?action=history&amp;feed=atom&amp;title=%E0%A4%B8%E0%A4%BE%E0%A4%B9%E0%A4%BE_%E0%A4%B8%E0%A4%AE%E0%A5%80%E0%A4%95%E0%A4%B0%E0%A4%A3"/>
	<link rel="alternate" type="text/html" href="https://hi.bharatpedia.org/w/index.php?title=%E0%A4%B8%E0%A4%BE%E0%A4%B9%E0%A4%BE_%E0%A4%B8%E0%A4%AE%E0%A5%80%E0%A4%95%E0%A4%B0%E0%A4%A3&amp;action=history"/>
	<updated>2026-08-25T14:04:52Z</updated>
	<subtitle>विकि पर उपलब्ध इस पृष्ठ का अवतरण इतिहास</subtitle>
	<generator>MediaWiki 1.43.6</generator>
	<entry>
		<id>https://hi.bharatpedia.org/w/index.php?title=%E0%A4%B8%E0%A4%BE%E0%A4%B9%E0%A4%BE_%E0%A4%B8%E0%A4%AE%E0%A5%80%E0%A4%95%E0%A4%B0%E0%A4%A3&amp;diff=5749&amp;oldid=prev</id>
		<title>imported&gt;EatchaBot: बॉट: पुनर्प्रेषण ठीक कर रहा है</title>
		<link rel="alternate" type="text/html" href="https://hi.bharatpedia.org/w/index.php?title=%E0%A4%B8%E0%A4%BE%E0%A4%B9%E0%A4%BE_%E0%A4%B8%E0%A4%AE%E0%A5%80%E0%A4%95%E0%A4%B0%E0%A4%A3&amp;diff=5749&amp;oldid=prev"/>
		<updated>2020-03-02T05:17:53Z</updated>

		<summary type="html">&lt;p&gt;बॉट: पुनर्प्रेषण ठीक कर रहा है&lt;/p&gt;
&lt;p&gt;&lt;b&gt;नया पृष्ठ&lt;/b&gt;&lt;/p&gt;&lt;div&gt;&amp;#039;&amp;#039;&amp;#039;साहा समीकरण&amp;#039;&amp;#039;&amp;#039; का विकाश सुप्रसिद्ध [[भारत|भारतीय]] खगोलविज्ञानी (एस्ट्रोफिजिसिस्ट्) [[मेघनाद साहा]] ने [[१९२०|1920]] में किया था। इसके द्वारा [[वर्णपट्ट]] के आधार पर [[तारा|तारों]] के वर्गीकरण की व्याख्या की गई है। For a gas composed of a single atomic species, the Saha equation is written:&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;\frac{n_{i+1}n_e}{n_i} = \frac{2}{\Lambda^3}\frac{g_{i+1}}{g_i}\exp\left[-\frac{(\epsilon_{i+1}-\epsilon_i)}{k_BT}\right]&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
where:&lt;br /&gt;
&lt;br /&gt;
* &amp;lt;math&amp;gt;n_i\,&amp;lt;/math&amp;gt; is the density of atoms in the &amp;#039;&amp;#039;i&amp;#039;&amp;#039;-th state of ionization, that is with &amp;#039;&amp;#039;i&amp;#039;&amp;#039; electrons removed.&lt;br /&gt;
* &amp;lt;math&amp;gt;g_i\,&amp;lt;/math&amp;gt; is the [[Degenerate energy level|degeneracy]] of states for the &amp;#039;&amp;#039;i&amp;#039;&amp;#039;-ions&lt;br /&gt;
* &amp;lt;math&amp;gt;\epsilon_i\,&amp;lt;/math&amp;gt; is the energy required to remove &amp;#039;&amp;#039;i&amp;#039;&amp;#039; electrons from a neutral atom, creating an &amp;#039;&amp;#039;i&amp;#039;&amp;#039;-level ion.&lt;br /&gt;
* &amp;lt;math&amp;gt;n_e\,&amp;lt;/math&amp;gt; is the [[electron density]]&lt;br /&gt;
* &amp;lt;math&amp;gt;\Lambda\,&amp;lt;/math&amp;gt; is the [[thermal de Broglie wavelength]] of an electron&lt;br /&gt;
::&amp;lt;math&amp;gt;\Lambda \ \stackrel{\mathrm{def}}{=}\  \sqrt{\frac{h^2}{2\pi m_ek_BT}}&amp;lt;/math&amp;gt;&lt;br /&gt;
* &amp;lt;math&amp;gt;m_e\,&amp;lt;/math&amp;gt; is the [[Mass of electron#Properties and behavior|mass of an electron]]&lt;br /&gt;
* &amp;lt;math&amp;gt;T\,&amp;lt;/math&amp;gt; is the [[temperature]] of the gas&lt;br /&gt;
* &amp;lt;math&amp;gt;k_B\,&amp;lt;/math&amp;gt; is the [[Boltzmann constant]]&lt;br /&gt;
* &amp;lt;math&amp;gt;h\,&amp;lt;/math&amp;gt; is [[Planck&amp;#039;s constant]]&lt;br /&gt;
&lt;br /&gt;
In the case where only one level of ionization is important, we have &amp;lt;math&amp;gt;n_1=n_e&amp;lt;/math&amp;gt; and defining the total density &amp;#039;&amp;#039;n&amp;#039;&amp;#039;&amp;amp;nbsp; as &amp;lt;math&amp;gt;n=n_0+n_1&amp;lt;/math&amp;gt;, the Saha equation simplifies to:&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;\frac{n_e^2}{n-n_e} = \frac{2}{\Lambda^3}\frac{g_1}{g_0}\exp\left[\frac{-\epsilon}{k_BT}\right]&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
where &amp;lt;math&amp;gt;\epsilon&amp;lt;/math&amp;gt; is the energy of ionization.&lt;br /&gt;
&lt;br /&gt;
The Saha equation is useful for determining the ratio of particle densities for two different ionization levels. The most useful form of the Saha equation for this purpose is&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;\frac{Z_i}{N_i} = \frac{Z_{i+1}Z_e}{N_{i+1}N_e}&amp;lt;/math&amp;gt;, &lt;br /&gt;
&lt;br /&gt;
where &amp;#039;&amp;#039;Z&amp;#039;&amp;#039; denotes the [[partition function (statistical mechanics)|partition function]]. The Saha equation can be seen as a restatement of the equilibrium condition for the [[chemical potential]]s:&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;\mu_i = \mu_{i+1} + \mu_e\,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
[[श्रेणी:भौतिकी]]&lt;/div&gt;</summary>
		<author><name>imported&gt;EatchaBot</name></author>
	</entry>
</feed>