scholarly journals An inverse mass expansion for the mutual information in free scalar QFT at finite temperature

2020 ◽  
Vol 2020 (2) ◽  
Author(s):  
Dimitrios Katsinis ◽  
Georgios Pastras
2012 ◽  
Vol 2012 (01) ◽  
pp. P01023 ◽  
Author(s):  
Johannes Wilms ◽  
Julien Vidal ◽  
Frank Verstraete ◽  
Sébastien Dusuel

2020 ◽  
Vol 2020 (7) ◽  
Author(s):  
Hiroyuki Fujita ◽  
Mitsuhiro Nishida ◽  
Masahiro Nozaki ◽  
Yuji Sugimoto

Abstract We study the time evolution of mutual information (MI) and logarithmic negativity (LN) in two-dimensional free scalar theory with two kinds of time-dependent masses: one time evolves continuously from non-zero mass to zero; the other time evolves continuously from finite mass to finite mass, but becomes massless once during the time evolution. We call the former protocol ECP, and the latter protocol CCP. Through numerical computation, we find that the time evolution of MI and LN in ECP follows a quasi-particle picture except for their late-time evolution, whereas that in CCP oscillates. Moreover, we find a qualitative difference between MI and LN which has not been known so far: MI in ECP depends on the slowly moving modes, but LN does not.


2011 ◽  
Vol 106 (13) ◽  
Author(s):  
Rajiv R. P. Singh ◽  
Matthew B. Hastings ◽  
Ann B. Kallin ◽  
Roger G. Melko

2013 ◽  
Vol 87 (12) ◽  
Author(s):  
Willy Fischler ◽  
Arnab Kundu ◽  
Sandipan Kundu

2020 ◽  
Vol 2020 (11) ◽  
Author(s):  
Pablo Bueno ◽  
Horacio Casini

Abstract We continue our study of reflected entropy, R(A, B), for Gaussian systems. In this paper we provide general formulas valid for free scalar fields in arbitrary dimensions. Similarly to the fermionic case, the resulting expressions are fully determined in terms of correlators of the fields, making them amenable to lattice calculations. We apply this to the case of a (1 + 1)-dimensional chiral scalar, whose reflected entropy we compute for two intervals as a function of the cross-ratio, comparing it with previous holographic and free-fermion results. For both types of free theories we find that reflected entropy satisfies the conjectural monotonicity property R(A, BC) ≥ R(A, B). Then, we move to (2 + 1) dimensions and evaluate it for square regions for free scalars, fermions and holography, determining the very-far and very-close regimes and comparing them with their mutual information counterparts. In all cases considered, both for (1 + 1)- and (2 + 1)-dimensional theories, we verify that the general inequality relating both quantities, R(A, B) ≥ I (A, B), is satisfied. Our results suggest that for general regions characterized by length-scales LA ∼ LB ∼ L and separated a distance ℓ, the reflected entropy in the large-separation regime (x ≡ L/ℓ ≪ 1) behaves as R(x) ∼ −I(x) log x for general CFTs in arbitrary dimensions.


2020 ◽  
Vol 2020 (9) ◽  
Author(s):  
Noburo Shiba

Abstract We consider the (Rényi) mutual information, $$ {I}^{(n)}\left(A,B\right)={S}_A^{(n)}+{S}_B^{(n)}-{S}_{A\cup B}^{(n)} $$ I n A B = S A n + S B n − S A ∪ B n , of distant compact spatial regions A and B in the vacuum state of a free scalar field. The distance r between A and B is much greater than their sizes RA,B. It is known that $$ {I}^{(n)}\left(A,B\right)\sim {C}_{AB}^{(n)}{\left\langle 0\left|\phi (r)\phi (0)0\right|\right\rangle}^2 $$ I n A B ∼ C AB n 0 ϕ r ϕ 0 0 2 . We obtain the direct expression of $$ {C}_{AB}^{(n)} $$ C AB n for arbitrary regions A and B. We perform the analytical continuation of n and obtain the mutual information. The direct expression is useful for the numerical computation. By using the direct expression, we can compute directly I(A, B) without computing SA, SB and SA∪B respectively, so it reduces significantly the amount of computation.


2005 ◽  
Vol 20 (20n21) ◽  
pp. 4995-5007 ◽  
Author(s):  
TOMOHIRO INAGAKI ◽  
DAIJI KIMURA ◽  
TSUKASA MURATA

We investigate scalar and spinor field theories in a constant magnetic field at finite temperature and chemical potential. In an external constant magnetic field the exact solution of the two-point Green functions are obtained by using the Fock–Schwinger proper-time formalism. We extend it to the thermal field theory and find the expressions of the Green functions exactly for the temperature, the chemical potential and the magnetic field. For practical calculations the contour of the proper-time integral is carefully selected. The physical contour is discussed in a constant magnetic field at finite temperature and chemical potential. As an example, behavior of the vacuum self-energy is numerically evaluated for the free scalar and spinor fields.


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