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首页量子真空中的纠缠波包与黑洞纯化效应
在本文《真空中纠缠的波包》中,作者Joris Kattemölla、band Ben Freivogel针对黑洞防火墙问题提出了一个独特的视角。该问题起源于量子引力理论中的一个争议,即在黑洞事件视界附近,量子信息似乎被永久地摧毁,引发了所谓的“黑洞信息悖论”。为了探索这个问题,研究者们转向量子场论,寻找可能的解决方案。 文章的核心发现是发现了高度纠缠的空间局部模式对,这些模式在量子场论的背景下出现。这些波包并非均匀分布,而是被设计为在事件视界之外的特定位置进行局域化。研究者证明,这些波包在外侧被一种“镜像”效应所净化,即它们与事件视界内的“镜像”波包形成了强烈纠缠。这种纠缠使得外侧的波包在一定程度上恢复了纯度,即使它们与黑洞内部的状态密切相关。 作者不仅关注波包的纠缠性质,还进一步计算了Minkowski真空中单个局部波包的纠缠熵。这是一种衡量量子系统纯度和复杂性的物理量,它揭示了波包的量子态在空间上的分布及其纯度之间的关系。随着波包的区域逐渐扩大,量子状态趋于纯化,这表明在某种程度上,波包的局部化程度与量子纯度之间存在着一种动态平衡。 关键词“Black Holes”、“Effective Field Theories”和“Models of Quantum Gravity”强调了这项工作与黑洞物理学、有效场论以及量子引力模型的关联。整体来看,这篇文章深入探讨了量子场论中的纠缠现象,如何影响黑洞边缘附近的物理过程,并尝试通过纠缠波包的研究来理解黑洞信息悖论,为量子引力理论的未来发展提供了新的洞察。
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JHEP10(2017)092
2.1 Particles in the vacuum
Consider the free massless scalar field. The field operator
ˆ
φ can be expanded over the basis
of Minkowski plane waves f
p
as
ˆ
φ =
Z
dp (f
p
ˆa
p
+ f
∗
p
ˆa
†
p
),
thus associating the mode operator ˆa
p
with the Minkowski plane wave f
p
. The Minkowski
vacuum |0i
M
is defined as the state for which
ˆa
p
|0i
M
= 0 for all p. (2.1)
Alternatively, the field could be expanded over a basis {g
k
},
ˆ
φ =
Z
dk (g
k
ˆ
b
k
+ g
∗
k
ˆ
b
†
k
).
Here k need not be momentum, but should be thought of as an index that labels the basis
modes. Thus the operator
ˆ
b
k
is associated with the mode g
k
. This operator can be written
in terms of the mode operators ˆa
p
as
ˆ
b
k
=
Z
dp
α
∗
kp
ˆa
p
− β
∗
kp
ˆa
†
p
, (2.2)
where α
kp
and β
kp
are the so-called Bogolyubov coefficients. These coefficients can be
computed by
α
kp
= (g
k
, f
p
), β
kp
= −(g
k
, f
∗
p
), (2.3)
where
∗
is complex conjugation, and the inner product (·, ·) is given by the Klein-Gordon
inner product. In Minkowski space it reads
(g, f) = −i
Z
dx [ g ∂
t
f
∗
− (∂
t
g)f
∗
] . (2.4)
Now by using (2.1) and (2.2), we see that the expectation value of the number operator
of the new modes equals
h
ˆ
b
†
k
ˆ
b
k
i
M
=
Z
dp |β
kp
|
2
. (2.5)
So, even though the overall state is the vacuum with respect to the modes f
p
, the modes
g
k
are in an excited state. As will become clear in due course, the modes g
k
will separately
often be in a mixed state due to entanglement with other modes. Thus they will have
some non-zero von Neumann entropy. Since the overall state |0i
M
is pure, this entropy is
solely due to entanglement, and we will therefore refer to this quantity as the entanglement
entropy of the mode.
In this paper, the overall state is always the Minkowski vacuum, so we will henceforth
drop the subscript M .
– 5 –
JHEP10(2017)092
2.2 Gaussian states
The Minkowski vacuum is in fact a Gaussian state (see [3, 9] for a proof.) We will here
show how Gaussian states and continuous variable quantum information theory can be
used to calculate various quantities. More detail can be found in [6–9].
In the phase space formulation of quantum mechanics, any state - be it mixed or pure -
is fully described by the characteristic function χ. There is a specific one-to-one relation
between the density matrices and the characteristic functions [7], but its actual form is not
of intrest here.
Now let X = (q
1
, p
1
, . . . , q
N
, p
N
)
T
be a vector in the 2N -dimensional phase space of an
N-mode system with mode operators
ˆ
b
m
. A Gaussian state then, is a state with a Gaussian
characteristic function,
χ(x) ∼ e
−
1
2
x
T
σx
. (2.6)
Here σ is the covariance matrix,
[σ]
kp
=
1
2
h{
ˆ
R
k
,
ˆ
R
p
}i − h
ˆ
R
k
ih
ˆ
R
p
i, (2.7)
with {·, ·} the anti-commutator,
ˆ
R = (ˆq
1
, ˆp
1
, . . . , ˆq
N
, ˆp
N
)
T
, and (ˆq
m
, ˆp
m
) the quadrature
operators
ˆq
m
=
1
√
2
(
ˆ
b
m
+
ˆ
b
†
m
), ˆp
m
=
1
i
√
2
(
ˆ
b
m
−
ˆ
b
†
m
). (2.8)
Note that in the standard formulation of quantum mechanics, the density matrix is al-
ready infinity dimensional for N = 1, whereas the covariance matrix is only 2N -dimensional
in general.
Since σ contains all information about the Gaussian state it must, in principle, be
possible to express the von Neumann entropy S of that state in terms of the entries of σ
only. Indeed there is a nice formula that does exactly that [8]. It reads
S =
X
j
s
j
+
1
2
log
s
j
+
1
2
−
s
j
−
1
2
log
s
j
−
1
2
, (2.9)
where the s
j
are the positive eigenvalues of the matrix iΩσ, called the symplectic eigen-
values of σ, and
Ω =
N
M
j=1
0 1
−1 0
!
.
Example. Let us write out the entropy of a single mode. For N = 1, the covariance
matrix reads
σ =
hˆq
2
i
1
2
h{ˆq, ˆp}i
1
2
h{ˆq, ˆp}i hˆp
2
i
!
.
It has a single symplectic eigenvalue, s =
p
hˆp
2
ihˆq
2
i − h{ˆq, ˆp}i
2
.
– 6 –
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