Editing 2034: Equations

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:<math>SU(2)U(1)\times{}SU(U(2))</math>
 
:<math>SU(2)U(1)\times{}SU(U(2))</math>
 
;All {{w|quantum gravity}} equations
 
;All {{w|quantum gravity}} equations
Quantum gravity uses mathematical {{w|Group (mathematics)|groups}} denoted by uppercase letters, as shown. {{w|Special unitary group|SU(2)}}, {{w|Unitary group|U(1)}}, and {{w|Unitary group|U(2)}} are all well-studied groups, though 'SU(U(2))' makes no sense.  The lack of relator means this expression isn't an equation.
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Quantum gravity uses mathematical {{w|Group (mathematics)|groups}} denoted by uppercase letters, as shown. {{w|Special unitary group|SU(2)}}, {{w|Unitary group|U(1)}}, and {{w|Unitary group|U(2)}} are all well-studied groups, though 'SU(U(2))' makes no sense.  The lack of relator means this expression isn't an equation.  Here is a possible pun, on "Sue you too... you won"... "Sue you, you too", though it's unclear how it fits in here.
  
:[[File:All gauge theory equations.png]]
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:S<sub>g</sub>=(-1)/(2&epsilon;&#x0304;) i&eth;(&#x302; &xi;<sub>0</sub> &#x2a22; p<sub>&epsilon;</sub> &rho;<sub>v</sub><sup>abc</sup>&sdot;&eta;<sub>0</sub>)&#x302; f&#x0335;<sub>a</sub><sup>0</sup> &lambda;(<span style="display:inline-block; -ms-transform:rotate(180deg); -webkit-transform:rotate(180deg); transform:rotate(180deg);">&xi;</span>) &psi;(0<sub>a</sub>)
 
;All {{w|gauge theory}} equations
 
;All {{w|gauge theory}} equations
 
Gauge theory is a subset of field theory. Most gauge theory equations appear to have many strange-looking constants and variables with odd labels. However, almost none of the symbols used here are found or applicable to gauge theory.
 
Gauge theory is a subset of field theory. Most gauge theory equations appear to have many strange-looking constants and variables with odd labels. However, almost none of the symbols used here are found or applicable to gauge theory.
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Cosmology is the science of the development and ultimate fate of the universe. The joke here may be pertaining to the different models accepted in the field of cosmology. H is the {{w|Hubble's law#Time-dependence of Hubble parameter|Hubble parameter}}, &Omega; is the universal {{w|Friedmann equations#Density parameter|density parameter}}, G is the {{w|gravitational constant}}, and &Lambda; is the {{w|cosmological constant}}.
 
Cosmology is the science of the development and ultimate fate of the universe. The joke here may be pertaining to the different models accepted in the field of cosmology. H is the {{w|Hubble's law#Time-dependence of Hubble parameter|Hubble parameter}}, &Omega; is the universal {{w|Friedmann equations#Density parameter|density parameter}}, G is the {{w|gravitational constant}}, and &Lambda; is the {{w|cosmological constant}}.
  
:[[File:All truly deep physics equations.png]]
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:&#x0124; - u&#x0327;<sub>0</sub> = 0
 
;All truly deep {{w|physics}} equations
 
;All truly deep {{w|physics}} equations
 
The joke about the "truly deep physics equations" is that most of the universal physics equations are simple, almost exceedingly so. In general, many of these equations are types of [https://en.wikipedia.org/wiki/Conservation_law conservation law] equations, which reflect some of the basic truths of the universe. A hallmark of conservation laws is that the total amount of some physical value does not change, and so one side of the equation is zero, as shown in the example. One example is Einstein's ''E = mc²'', which shows conservation of mass-energy. Noether's theorem shows that conservation laws have a one-to-one correspondence with a symmetry of nature, making these equations truly 'deep'.  
 
The joke about the "truly deep physics equations" is that most of the universal physics equations are simple, almost exceedingly so. In general, many of these equations are types of [https://en.wikipedia.org/wiki/Conservation_law conservation law] equations, which reflect some of the basic truths of the universe. A hallmark of conservation laws is that the total amount of some physical value does not change, and so one side of the equation is zero, as shown in the example. One example is Einstein's ''E = mc²'', which shows conservation of mass-energy. Noether's theorem shows that conservation laws have a one-to-one correspondence with a symmetry of nature, making these equations truly 'deep'.  

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