<?xml version="1.0" encoding="utf-8" standalone="yes"?><rss version="2.0" xmlns:atom="http://www.w3.org/2005/Atom"><channel><title>Mathematical Physics on Haifei's Home</title><link>https://haifei-home.pages.dev/en/categories/mathematical-physics/</link><description>Recent content in Mathematical Physics on Haifei's Home</description><generator>Hugo</generator><language>en</language><managingEditor>hfwang132@gmail.com (hfwang132)</managingEditor><webMaster>hfwang132@gmail.com (hfwang132)</webMaster><copyright>This work is licensed under a Creative Commons Attribution-NonCommercial 4.0 International License.</copyright><lastBuildDate>Thu, 07 Mar 2024 16:13:09 +0800</lastBuildDate><atom:link href="https://haifei-home.pages.dev/en/categories/mathematical-physics/index.xml" rel="self" type="application/rss+xml"/><item><title>Baker-Campbell-Hausdorff Formula</title><link>https://haifei-home.pages.dev/en/post_20240307_bch-%E5%85%AC%E5%BC%8F-%E9%87%8F%E5%AD%90%E5%8A%9B%E5%AD%A6%E7%88%86%E7%AE%97%E7%9A%84%E5%A4%A7%E6%9D%80%E5%99%A8/</link><pubDate>Thu, 07 Mar 2024 16:13:09 +0800</pubDate><author>hfwang132@gmail.com (hfwang132)</author><guid>https://haifei-home.pages.dev/en/post_20240307_bch-%E5%85%AC%E5%BC%8F-%E9%87%8F%E5%AD%90%E5%8A%9B%E5%AD%A6%E7%88%86%E7%AE%97%E7%9A%84%E5%A4%A7%E6%9D%80%E5%99%A8/</guid><description>&lt;p&gt;Chinese version &lt;a href="../zh-cn/bch/" rel=""&gt;here&lt;/a&gt;&lt;/p&gt;
&lt;p&gt;&lt;strong&gt;Baker-Campbell-Hausdorff Formula&lt;/strong&gt; can be used to compute operator evolution in the Heisenberg picture:&lt;/p&gt;
&lt;p&gt;$e^X Y e^{-X}=Y+[X,Y]+\frac{1}{2!}[X,[X,Y]]+\frac{1}{3!}[X,[X,[X,Y]]]+\cdots$&lt;/p&gt;
&lt;blockquote&gt;
&lt;p&gt;This formula is actually just a younger sibling of the BCH formula.&lt;/p&gt;
&lt;/blockquote&gt;
&lt;p&gt;Because the evolution rule of operators in the Heisenberg picture is $A\rightarrow UAU^{\dag}$, where $U$ is a unitary evolution operator.&lt;/p&gt;
&lt;p&gt;If $U$ is generated by $H$, then it becomes $A\rightarrow e^{\frac{t}{i\hbar}H}Ae^{-\frac{t}{i\hbar}H}$.&lt;/p&gt;
&lt;blockquote&gt;
&lt;p&gt;&lt;strong&gt;Example 1: Phase Shifter&lt;/strong&gt;
The Hamiltonian is $H=\varphi n$, and the annihilation operator $a$ evolves as:
$\begin{aligned} e^{-i\varphi n} a e^{i\varphi n}&amp;amp;= a + i\varphi [n, a] - \frac{\varphi}{2!} [n,[n,a]] - \cdots \\ &amp;amp;= a (1+i\varphi -\frac{\varphi^2}{2!} - \cdots)\\ &amp;amp;= e^{i\varphi} a \end{aligned}$&lt;/p&gt;</description></item><item><title>What is the relationship between Lie derivative and covariant derivative?</title><link>https://haifei-home.pages.dev/en/post_20230715_%E6%9D%8E%E5%AF%BC%E6%95%B0%E4%B8%8E%E5%8D%8F%E5%8F%98%E5%AF%BC%E6%95%B0%E6%9C%89%E4%BB%80%E4%B9%88%E8%81%94%E7%B3%BB/</link><pubDate>Sat, 15 Jul 2023 16:52:03 +0800</pubDate><author>hfwang132@gmail.com (hfwang132)</author><guid>https://haifei-home.pages.dev/en/post_20230715_%E6%9D%8E%E5%AF%BC%E6%95%B0%E4%B8%8E%E5%8D%8F%E5%8F%98%E5%AF%BC%E6%95%B0%E6%9C%89%E4%BB%80%E4%B9%88%E8%81%94%E7%B3%BB/</guid><description>&lt;h2 id="i-differences-and-similarities-in-properties"&gt;I. Differences and Similarities in Properties&lt;/h2&gt;
&lt;p&gt;Lie derivative $\mathcal{L}_V$ and covariant derivative $\nabla_V$ share many common points:&lt;/p&gt;
&lt;ol&gt;
&lt;li&gt;Both $\mathcal{L}_V$ and $\nabla_V$ preserve the type of tensors, mapping $\mathcal{T}^p_q(M)$ to $\mathcal{T}^p_q(M)$. $\mathcal{T}^p_q(M)$ represents the set of all smooth tensor fields of type (p, q) on $M$.&lt;/li&gt;
&lt;/ol&gt;
&lt;p&gt;Particularly, for (0,0) type tensor fields, i.e., scalar fields $f\in \mathcal{F}(M)$, we have $\mathcal{L}_V f=\nabla_V f=Vf$.&lt;/p&gt;
&lt;ol start="2"&gt;
&lt;li&gt;Both satisfy linearity and the Leibniz rule:&lt;/li&gt;
&lt;/ol&gt;
&lt;p&gt;$ \begin{aligned} \mathcal{L}_V(\mu A + \lambda B) &amp;amp;= \mu \mathcal{L}_V A + \lambda \mathcal{L}_V B, \\ \mathcal{L}_V (A \otimes B) &amp;amp;= (\mathcal{L}_V A)\otimes B + A \otimes (\mathcal{L}_V B) \end{aligned} $&lt;/p&gt;</description></item></channel></rss>