Viterbi decoder: Difference between revisions

From formulasearchengine
Jump to navigation Jump to search
en>Mogism
m Applications: Typo fixing and cleanup, typos fixed: etc) → etc.) using AWB
 
en>A D Monroe III
m Undid revision 584792285 by 124.125.66.61 (talk); restore section name
Line 1: Line 1:
{{Unreferenced stub|auto=yes|date=December 2009}}
In [[Quantum gauge theory|quantum gauge theories]], in the [[Hamiltonian (quantum mechanics)|Hamiltonian]] formulation, the [[wave function]] is a [[functional (mathematics)|functional]] of the gauge [[Connection (vector_bundle)|connection]] A and matter fields <math>\,\phi</math>. Being a quantum gauge theory, we have to impose [[first class constraint]]s in the form of functional differential equations—basically, the [[Gauss constraint]].


In flat spacetime, space is noncompact '''R'''<sup>3</sup>. Since the Gauss constraints are local, it suffices to consider [[gauge transformation]]s U which approach 1 at spatial infinity. Alternatively, we can assume space is a very large three sphere S<sup>3</sup> or that space is a compact 3-ball B<sup>3</sup> with a S<sup>2</sup> boundary where the values of the fields are fixed so that the gauge transformations occur only in the interior of the ball. At any rate, we can see that there are gauge transformations U [[homotopic]] to the trivial gauge transformation. These gauge transformations are called [[small gauge transformation]]s. All the other gauge transformations are called [[big gauge transformation]]s, which are classified by the [[homotopy group]] π<sub>3</sub>(G) where G is the gauge group.


Another day I woke up and noticed - I have been single for a while now and after much bullying from pals I today find myself registered for on line dating. They promised me that there are plenty of entertaining, pleasant and normal folks to fulfill, therefore the pitch is gone by here!<br>I try and keep as physically fit as potential being at the fitness center several times per week. I enjoy my athletics and endeavor to play or watch as several a possible. I am going to regularly at Hawthorn matches being winter. Note: Supposing that you will considered shopping a  [http://okkyunglee.com luke bryan information] hobby I do not brain, I've seen the carnage of wrestling matches at stocktake sales.<br>My buddies and  [http://lukebryantickets.hamedanshahr.com luke bryan sold out] family are amazing and spending time with them at tavern gigabytes or dishes is constantly essential. As I see that one can never own a nice dialog with all the noise I have never been in to cabarets. Additionally, I got two definitely cheeky and really [http://Www.Reddit.com/r/howto/search?q=cunning+canines cunning canines] that are [http://www.adobe.com/cfusion/search/index.cfm?term=&invariably+ready&loc=en_us&siteSection=home invariably ready] to meet fresh individuals.<br><br>Also visit my web page: luke bryan 2014 tour ([http://www.cinemaudiosociety.org please click the next page])
The Gauss constraints mean that the value of the wave function functional is constant along the [[orbit]]s of small gauge transformation.
 
i.e.,
 
:<math>\Psi[U\mathbf{A}U^{-1}-(dU)U^{-1},U\phi]=\Psi[\mathbf{A},\phi]</math>
 
for all small gauge transformations U. But this is not true in general for large gauge transformations.
 
It turns out that if G is some [[simple Lie group]], then π<sub>3</sub>(G) is '''Z'''. Let U be any representative of a gauge transformation with [[winding number]] 1.
 
The Hilbert space decomposes into [[superselection sector]]s labeled by a '''theta angle''' θ such that
 
:<math>\Psi[U\mathbf{A}U^{-1}-(dU)U^{-1},U\phi]=e^{i\theta}\Psi[\mathbf{A},\phi]</math>
 
==See also==
* [[Instanton]]
* [[Strong CP problem]]
 
{{DEFAULTSORT:Vacuum Angle}}
[[Category:Quantum field theory]]
[[Category:Quantum chromodynamics]]
 
 
{{Quantum-stub}}

Revision as of 00:09, 7 December 2013

Template:Unreferenced stub In quantum gauge theories, in the Hamiltonian formulation, the wave function is a functional of the gauge connection A and matter fields ϕ. Being a quantum gauge theory, we have to impose first class constraints in the form of functional differential equations—basically, the Gauss constraint.

In flat spacetime, space is noncompact R3. Since the Gauss constraints are local, it suffices to consider gauge transformations U which approach 1 at spatial infinity. Alternatively, we can assume space is a very large three sphere S3 or that space is a compact 3-ball B3 with a S2 boundary where the values of the fields are fixed so that the gauge transformations occur only in the interior of the ball. At any rate, we can see that there are gauge transformations U homotopic to the trivial gauge transformation. These gauge transformations are called small gauge transformations. All the other gauge transformations are called big gauge transformations, which are classified by the homotopy group π3(G) where G is the gauge group.

The Gauss constraints mean that the value of the wave function functional is constant along the orbits of small gauge transformation.

i.e.,

Ψ[UAU1(dU)U1,Uϕ]=Ψ[A,ϕ]

for all small gauge transformations U. But this is not true in general for large gauge transformations.

It turns out that if G is some simple Lie group, then π3(G) is Z. Let U be any representative of a gauge transformation with winding number 1.

The Hilbert space decomposes into superselection sectors labeled by a theta angle θ such that

Ψ[UAU1(dU)U1,Uϕ]=eiθΨ[A,ϕ]

See also


Template:Quantum-stub