Concept of Field: Canonical Formalism in QFT

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SUMMARY

The discussion centers on the canonical formalism of fields in Quantum Field Theory (QFT), emphasizing the transition from classical field theory to QFT. Participants recommend understanding classical field theory, particularly the Lagrangian density and its role in generating field equations, before tackling QFT. 't Hooft's work is highlighted as a valuable introductory resource. Additionally, Mandl and Shaw are suggested as good references for further study in field theory.

PREREQUISITES
  • Classical Field Theory
  • Lagrangian Density
  • Quantum Mechanics
  • Electromagnetism
NEXT STEPS
  • Study 't Hooft's conceptual basis for QFT
  • Read Mandl and Shaw on field theory
  • Master Classical Field Theory before advancing to QFT
  • Review thermodynamics and optics as part of the physics syllabus
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Students and researchers in theoretical physics, particularly those focusing on Quantum Field Theory, classical mechanics, and advanced physics topics.

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can ne 1 explain 2 me the canonical formalism of generalising the concept of field in QFT...i m not 2 sure abt the replacement of generalised coordinates q(i) i=1,2,... n with phi(x)
 
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I'm not sure if this view is popular, but I for one would personally appreciate if you wrote your posts in correct English as it makes it a lot easier for me to read.

I would recommend that you first gain an understanding of the classical field before you attempt to learn about a quantum system which reduces to a classical field theory in a certain limit (which is what QFT is; see 't Hooft's piece on the "conceptual basis for QFT" for further details).

Classical field theory is the generalisation of a system with finite degrees to one with infinite degrees of freedom. This is why we replace co-ordinates with a (usually) function; we have a Lagrangian density {\cal L} (which is a scalar) and we try and extremize the action given by this Lagrangian so that:

\delta \frac{1}{c}\int{\cal L} d^4\vec{x} = 0

and this procedure generates field equations.

Getting to QFT is a lot more complicated, and I would recommend firstly 't Hooft's work as a brief introduction and then to dive into one of the several texts on the topic.
 
thanks for the help ...and i apologise for not writing in the correct english ... could u please tell me more about the references for QFT
 
I'm sorry, but at this stage I'm only just about mastering Classical Field Theory -- EM was relatively simple (no pun intended), and GR took a bit of work. Term has started again, and I have little free time to continue my dalliances in advanced physics. QFT is my next topic of interest, but I have to learn thermodynamics, quantum mechanics and electromagnetism + optics according to the syllabus for my exams this year.

Essentially what I'm trying to say (and doing so badly) is that you'll have to ask someone else.
 
f u want a gd xplanation of th canonical frmlsm then prob just check any field thry bk.

I find Mandl and Shaw and good reference.

chrs.
 
Time reversal invariant Hamiltonians must satisfy ##[H,\Theta]=0## where ##\Theta## is time reversal operator. However, in some texts (for example see Many-body Quantum Theory in Condensed Matter Physics an introduction, HENRIK BRUUS and KARSTEN FLENSBERG, Corrected version: 14 January 2016, section 7.1.4) the time reversal invariant condition is introduced as ##H=H^*##. How these two conditions are identical?

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