The probability amplitude for detecting the neutron in state |+after the second cavity is obtained by i applying the matrix U to the vector 16.5, ii calculating the scalar product of the
Trang 1(c) If |ω0 − ω| ω1, we have, to a good approximation, the differential system
i ˙β+=ω1
2 e
−iωt0β − ; i ˙β −=
ω1
2 e
iωt0β+ ,
whose solution is indeed
β ± (t) = β ± (t0) cosω1 (t − t0)
2 − i e ∓iωt0β ∓ (t0) sinω1 (t − t0)
(d) Defining φ = ω1(t1− t0 )/2 , χ = ω(t1− t0 )/2 , δ = ω(t1+ t0)/2, we
obtain
α+(t1) = e−iχ β
+(t1) = e−iχ"
α+(t0) cos φ − iα − (t0)e−iωt0sin φ#
α − (t1) = eiχ β − (t1) = e+iχ"
α − (t0) cos φ − iα+ (t0)e+iωt0sin φ#
,
and, therefore,
U = e−iχ cos φ −i e −iδ sin φ
−i e iδ sin φ eiχ cos φ
.
Section 16.2: Ramsey Fringes
16.2.1 We assume φ = π/4; the initial conditions are: α+(t0) = 0 , α − (t0) =
1 At time t1 the state is
|ψ(t1) = √1
2
−i e −iδ |n : + + e iχ |n : −
In other words α+(t1) =−ie −iδ / √
2, α − (t1) = eiχ / √
2, and P ± = 1/2.
16.2.2 We set T = D/v The neutron spin precesses freely between the two
cavities during time T , and we obtain
α+ (t
0)
α − (t 0)
=√1
2
−ie −iδe−iω0T /2
eiχe+iω0T /2
16.2.3 By definition, t
0= t1+T and t
1= 2t1−t0+T , therefore the transition
matrix in the second cavity is
U = e−iχ cos φ −ie −iδ
sin φ
−ie iδ
sin φ eiχ
cos φ
with φ = φ = ω1(t1− t0 )/2, χ = χ = ω(t1− t0 )/2 Only the parameter δ is
changed into
δ = ω(t
1+ t
0)/2 = ω(3t1+ 2T − t0 )/2
Trang 216.2.4 The probability amplitude for detecting the neutron in state |+
after the second cavity is obtained by (i) applying the matrix U to the vector
(16.5), (ii) calculating the scalar product of the result with|n : + We obtain
α+(t
1) = 1 2
−ie −i(χ+δ+ω0T /2) − ie −i(δ −χ−ω0T /2)
.
Since
δ + χ = ωt1 δ − χ = ω
2 (3t1+ 2T − t0 − t1 + t0) = ω(t1+ T ) ,
we have
α+(t
1) =−i
2 e
−iω(t1+T /2)
e−i(ω0−ω)T/2+ ei(ω0−ω)T/2
. (16.6) Therefore, the probability that the neutron spin has flipped in the two-cavity system is
P+=|α+ (t
1)|2= cos2(ω − ω0 )T
With the approximation of Sect 1.2c, the probability for a spin flip in a
single cavity is independent of ω, and is equal to 1/2 In contrast, the present
result for two cavities exhibits a strong modulation of the spin flip probability,
between 1 (e.g for ω = ω0) and 0 (e.g for (ω − ω0 )T = π) This modulation
results from an interference process of the two quantum paths corresponding respectively to:
• a spin flip in the first cavity, and no flip in the second one,
• no flip in the first cavity and a spin flip in the second one.
Each of these paths has a probability 1/2, so that the sum of the probability amplitudes (16.6) is fully modulated
16.2.5 (a) Since cos2φ/2 = (1 + cos φ)/2, the averaged probability
distri-bution is
cos2(ω − ω0 )T
2
=1
2 +
1
2e
−(ω−ω0 ) 2τ2/2cos"
(ω − ω0 )T0#
. (16.7)
This form agrees with the observed variation in ω of the experimental signal The central maximum, which is located at ω/2π = 748.8 kHz corresponds
to ω = ω0 For that value, a constructive interference appears whatever the neutron velocity The lateral maxima and minima are less peaked, however, since the position of a lateral peak is velocity dependent The first two
lat-eral maxima correspond to (ω − ω0 )T0 ±2π Their amplitude is reduced,
compared to the central peak, by a factor exp(−2π2τ2/T2)
(b) The angular frequency ω0 is related to the magnetic moment of the neutron by ¯hω0= 2µnB0 which leads to µn= 9.65 × 10 −27 J T−1 The time
T0 can be deduced from the spacing between the central maximum and a
Trang 3lateral one The first lateral maximum occurs at 0.77 kHz from the resonance,
hence T0= 1.3 ms This corresponds to an average velocity v0= 1230 m s−1.
The ratio of intensities between the second lateral maximum and the central one is roughly 0.55 This is approximately equal to exp(−8π2τ2/T2), and gives
τ /T0≈ 0.087, and δv ≈ 110 m s −1.
(c) This experiment can be compared to a Young double slit interference
experiment with polychromatic light.The central fringe (corresponding to the
peak at ω = ω0) remains bright, but the contrast of the interferences de-creases rapidly as one departs from the center In fact, the maxima for some frequencies correspond to minima for others
16.2.6 The probability P++is the product of the two probabilities: the prob-ability to find the neutron in the state|n : + when it leaves the first cavity
(p = 1/2) and, knowing that it is in the state |n : +, the probability to find
it in the same state when it leaves the second cavity (p = 1/2); this gives
P +,+ = 1/4 Similarly P −,+ = 1/4 The sum P +,+ + P −,+ = 1/2 does not
display any interference, since one has measured in which cavity the neutron spin has flipped This is very similar to an electron double-slit interference experiment if one measures which slit the electron goes through
Section 16.3: Detection of the Neutron Spin State
16.3.1 By definition:
|a : ±x = √1
2(|a : + ± |a : −)
|a : ±y = √1
2(|a : + ± i|a : −)
and these states are related to one another by
|a : ±y = 1
2((1± i)|a : +x + (1 ∓ i)|a : −x)
16.3.2 The operators ˆS nz and ˆS ax commute since they act in two different Hilbert spaces; therefore [ ˆS nz , ˆ V ] = 0.
The common eigenvectors of ˆS nz and ˆV , and the corresponding eigenvalues
are
|n : + ⊗ |a : ±x S nz= +¯h/2 V = ±A¯h/2 ,
|n : − ⊗ |a : ±x S nz=−¯h/2 V = ∓A¯h/2
The operators ˆS nz and ˆV form a complete set of commuting operators as far
as spin variables are concerned
16.3.3 Expanding in terms of the energy eigenstates, one obtains for|ψ(0) =
|n : + ⊗ |a : +y :
|ψ(τ) = 1
2|n : + ⊗(1 + i)e−iAτ/2 |a : +x + (1 − i)e iAτ /2 |a : −x ,
Trang 4i.e for Aτ /2 = π/4:
|ψ(τ) = √1
2|n : + ⊗ (|a : +x + |a : −x)
=|n : + ⊗ |a : +
Similarly, if |ψ(0) = |n : − ⊗ |a : +y, then |ψ(τ) = i|n : − ⊗ |a : −.
Physically, this means that the neutron’s spin state does not change since it
is an eigenstate of ˆV , while the atom’s spin precesses around the x axis with
angular frequency A At time τ = π/(2A), it lies along the z axis.
16.3.4 If the initial state is |ψ(0) = (α+|n : + + α − |n : −) ⊗ |a : +y, the
state after the interaction is
|ψ(τ) = α+|n : + ⊗ |a : + + iα − |n : − ⊗ |a : −
The measurement of the z component of the atom’s spin gives +¯ h/2, with
probability|α+|2 and state|n : + ⊗ |a : + after the measurement, or −¯h/2
with probability|α − |2 and state|n : − ⊗ |a : − after the measurement.
In both cases, after measuring the z component of the atom’s spin, the
neutron spin state is known: it is the same as that of the measured atom It is
not necessary to let the neutron interact with another measuring apparatus
in order to know the value of S nz
Section 16.4: A Quantum Eraser
16.4.1 The successive states are:
step (a) √1
2
−ie −iδ |n : + ⊗ |a : +y + e iχ |n : − ⊗ |a : +y
step (b) √1
2
−ie −iδ |n : + ⊗ |a : + + ie iχ |n : − ⊗ |a : −
step (c) √1
2
− ie −i(δ+ω0T /2) |n : + ⊗ |a : +
+iei(χ+ω0T /2) |n : − ⊗ |a : −.
Finally, when the neutron leaves the second cavity (step d), the state of the system is:
|ψ f = 1
2
− ie −i(δ+ω0T /2)
e−iχ |n : + − ie iδ
|n : −⊗ |a : +
+iei(χ+ω0T /2)
−ie −iδ
|n : + + e iχ |n : −⊗ |a : −.
16.4.2 The probability to find the neutron in state |+ is the sum of the
probabilities for finding:
Trang 5(a) the neutron in state + and the atom in state +, i.e the square of the
modulus of the coefficient of|n : + ⊗ |a : + (1/4 in the present case),
(b) the neutron in state + and the atom in state− (probability 1/4 again).
One gets therefore P+ = 1/4 + 1/4 = 1/2: There are no interferences since
the quantum path leading in the end to a spin flip of the neutron can be determined from the state of the atom
16.4.3 One can expand the vectors|a : ± on |a : ±y:
|ψf = 1
2√
2
− ie −i(δ+ω0T /2)
e−iχ |n : + − ie iδ
|n : −
⊗ (|a : +y + |a : −y)
+ei(χ+ω0T /2)
−ie −iδ
|n : + + e iχ |n : −
⊗ (|a : +y − |a : −y)
The probability amplitude that Bob finds +¯h/2 along the z axis while Alice
finds +¯h/2 along the y axis is the coefficient of the term |n : + ⊗ |a : +y in
the above expansion Equivalently, the probability is obtained by projecting the state onto|n : + ⊗ |a : +y, and squaring One obtains
P S nz =¯h
2, S ay=
¯
h
2
= 1 8
−ie −i(δ+χ+ω0T /2) − ie i(χ −δ +ω
0T /2)2
= 1
2cos
2(ω − ω0 )T
which clearly exhibits a modulation reflecting an interference phenomenon Similarly, one finds that
P S nz =¯h
2, S ay=−¯h
2
= 1
2sin
2(ω − ω0 )T
which is also modulated
16.4.4 This result is compatible with the result 4.2 Indeed the sum of the
two probabilities calculated above is 1/2 as in 4.2 If Bob does not know the result found by Alice, or if Alice does not perform a measurement, which is equivalent from his point of view, Bob sees no interferences The interferences
only arise for the joint probability P (S nz , S ay)
16.4.5 (a) This first statement is obviously wrong As seen in question 4.2,
if the atom A is present, Bob no longer sees oscillations (in ω − ω0) of the probability for detecting the neutron in the state|+ This probability is equal
to 1/2 whatever Alice does Notice that if the statement were correct, this would imply instantaneous transmission of information from Alice to Bob
By seeing interferences appear, Bob would know immediately that Alice is performing an experiment, even though she may be very far away
Trang 6(b) This second statement is correct If Alice and Bob put together all
their results, and if they select the subsample of events for which Alice finds +¯h/2, then the number of events for which Bob also finds +¯ h/2 varies like
cos2((ω − ω0 )T /2); they recover interferences for this subset of events In the
complementary set, where Alice has found −¯h/2, the number of Bob’s
re-sults giving +¯h/2 varies like sin2((ω − ω0 )T /2) This search for correlations
between events occurring in different detectors is a common procedure, in particle physics for instance
(c) This third statement, although less precise but more picturesque than
the previous one, is nevertheless acceptable The cos2((ω − ω0 )T /2) signal
found in Sect 2 can be interpreted as the interference of the amplitudes cor-responding to two quantum paths for the neutron spin which is initially in the state |n : −; either its spin flips in the first cavity, or it flips in the
second one If there exists a possibility to determine which quantum path is followed by the system, interferences cannot appear It is necessary to “erase” this information, which is carried by the atom, in order to observe “some”
interferences After Alice has measured the atom’s spin along the y axis, she
has, in some sense “restored” the initial state of the system, and this enables Bob to see some interferences It is questionable to say that information has been erased: one may feel that, on the contrary, extra information has been acquired Notice that the statement in the text does not specify in which physical quantity the interferences appear Notice also that the order of the measurements made by Alice and Bob has no importance, contrary to what this third statement seems to imply
16.4.6 Alice can measure along the axisw = sin η u y +cos η u z , in the (y, z)
plane, for instance Projecting|ψf onto the eigenstate of ˆ S aw with eigenvalue +¯h/2, i.e cos(η/2) |a : ++i sin(η/2) |a : −, a calculation similar to 4.3 leads
to a probability "
1 + sin η cos
(ω − ω0 )T /2 If η = 0 or π (measurement
along the z axis) there are no interferences For η = π/2 and 3π/2 or, more generally, if Alice measures in the (x, y) plane, the contrast of the interferences,
| sin η|, is maximum.
16.6 Comments
Ramsey Fringes with Neutrons The experimental curve given in the text
is taken from J.H Smith et al., Phys Rev 108, 120 (1957) Since then, the
technique of Ramsey fringes has been considerably improved Nowadays one proceeds differently One stores neutrons in a “bottle” for a time of the order
of 100 s and applies two radiofrequency pulses at the begining and at the end
of the storage The elapsed time between the two pulses is 70 s, compared to 1.3 ms here This improves enormously the accuracy of the frequency
measure-ment Such experiments are actually devised to measure the electric dipole
moment of the neutron, of fundamental interest in relation to time-reversal
Trang 7invariance They set a very small upper bound on this quantity (K.F Smith
et al., Phys Lett 234, 191 (1990)).
Non Destructive Quantum Measurements The structure of the
inter-action Hamiltonian considered in the text has been chosen in order to provide
a simple description of the quantum eraser effect Realistic examples of non-destructive quantum measurements can be found in J.P Poizat and P
Grang-ier, Phys Rev Lett 70, 271 (1993), and S.M Barnett, Nature, Vol 362,
p 113, March 1993
Trang 8A Quantum Thermometer
We study here the measurement of the cyclotron motion of an electron The particle is confined in a Penning trap and it is coupled to the thermal radiation which causes quantum transitions of the system between various energy levels
In all the chapter, we neglect spin effects The method and results come from
an experiment performed at Harvard University in 1999
We consider an electron of mass M and charge q (q < 0), confined in a
Penning trap This trap consists in the superposition of a uniform magnetic
field B = Be z (B > 0) and an electric field which derives from the potential
Φ(r) whose power expansion near the origin is:
Φ(r) = M ω
2
z 4q
2z2− x2− y2 . (17.1)
The positive quantity ω zhas the dimension of an angular frequency In all this
chapter we set ω c = |q|B/M (ω c is called the cyclotron angular frequency)
and we assume that ω z ω c
Useful constants: M = 9.1 10 −31 kg ; q = −1.6 10 −19 C; h = 6.63 10 −34 J s; Boltzmann’s constant k B = 1.38 10 −23 J K−1.
17.1 The Penning Trap in Classical Mechanics
We recall that the Lorentz force acting on a charged particle moving in an
electromagnetic field is F = q(E + v × B).
17.1.1 Check that Φ( r) satisfies the Laplace equation ∆Φ = 0 What is the
shape of a surface of constant potential Φ(r) =Const?
17.1.2 Show that the classical equation of motion of the electron in the trap
is:
¨
x + ω c y˙− ω2z
2 x = 0 ¨− ω c x˙− ω z2
2 y = 0 z + ω¨
2
z z = 0
Trang 917.1.3 What is the type of motion along the z axis?
17.1.4 In order to study the component of the motion in the xy plane, we
set α = x + iy.
(a) What is the differential equation satisfied by α(t)?
(b) We seek a solution of this equation of the form α(t) = α0eiωt Show that
ω is a solution of the equation:
ω2− ω c ω + ω
2
z
2 = 0
(c) We note ω r and ω l the two roots of this equation with ω r > ω l Show that:
ω r ω c ω l ω z2
2ω c .
17.1.5 We consider the values B = 5.3 T and ω z /(2π) = 64 MHz.
(a) Show that the most general motion of the electron in the Penning trap
is the superposition of three harmonic oscillator motions
(b) Calculate the frequencies of these motions
(c) Draw the projection on the xy plane of the classical trajectory of the trapped electron, assuming that α r α l (the positive quantities α rand
α l represent the amplitudes of the motions of angular frequencies ω r and ω l)
17.2 The Penning Trap in Quantum Mechanics
We note ˆr and ˆ p the position and momentum operators of the electron The
Hamiltonian of the electron in the Penning trap is, neglecting spin effects:
ˆ
2M (ˆp − qA(ˆ r))2+ qΦ(ˆ r) ,
where the electrostatic potential Φ(r) is given by (17.1) For the magnetic vector potential, we choose the form A(r) = B × r/2.
17.2.1 Expand the Hamiltonian and show that it can be written as ˆH =
ˆ
H xy+ ˆH z, where ˆH xy only involves the operators ˆx, ˆ y, ˆ p x and ˆp y, while ˆH z
only involves the operators ˆz and ˆ p z
Do ˆH xy and ˆH z possess a common eigenbasis?
17.2.2 We are now interested in the motion along the z axis This is called
the axial motion Recall without giving any proof:
(a) the expression of the operators ˆa z and ˆa †
zwhich allow to write ˆH zin the form ˆH z= ¯hω z( ˆN z + 1/2) with ˆ N z= ˆa †
zˆa z and [ˆa z , ˆ a †
z] = 1;
(b) the eigenvalues of ˆN zand ˆH z
Trang 1017.2.3 We now consider the motion in the xy plane under the effect of the
Hamiltonian ˆH xy We set Ω =
ω2
c − 2ω2
z /2 We introduce the right and left
annihilation operators ˆa rand ˆa l:
ˆ
a r=
M Ω
4¯h (ˆx − iˆy) + √ i
4¯hM Ω(ˆp x − iˆp y) ˆ
a l=
M Ω
4¯h (ˆx + iˆ y) +
i
√
4¯hM Ω(ˆp x + iˆ p y )
(a) Show that [ˆa r , ˆ a †
r] = [ˆa l , ˆ a †
l] = 1
(b) Show that any left operator commutes with any right operator, i.e.:
[ˆa r , ˆ a l] = 0 [ˆa r , ˆ a †
l] = 0 [ˆa †
r , ˆ a l] = 0 [ˆa †
r , ˆ a †
l ] = 0
(c) Recall the eigenvalues of ˆn r= ˆa †
rˆa rand ˆn l= ˆa †
lˆa l(no proof is required)
Do ˆn r and ˆn lpossess a common eigenbasis?
(d) Show that the Hamiltonian ˆH xy can be written as:
ˆ
H xy = ¯hω r(ˆn r + 1/2) − ¯hω l(ˆn l + 1/2) , where the angular frequencies ω r and ω l have been introduced in Sect 17.1
(e) Deduce from this the eigenvalues of the Hamiltonian ˆH xy
17.2.4 We note |ψ(t) the state of the system at time t and we define
a r (t) = ψ(t)|ˆa r |ψ(t) and a l (t) = ψ(t)|ˆa l |ψ(t) Using the Ehrenfest
the-orem, calculate da r /dt and da l /dt.
Integrate these equations and calculate the expectation value of the elec-tron’s position (x(t), y(t)) in the xy plane We set a r (0) = ρ r e−iφ r and
a l (0) = ρ leiφ l , where ρ r and ρ l are real and positive
Show that the time evolution of the expectation value of the electron po-sitionr(t) is similar to the classical evolution found in Sect 17.1.
17.2.5 We note|φ0 the eigenstate of ˆ H corresponding to the eigenvalues 0
for each of the operators ˆn r, ˆn land ˆN z
(a) Determine the corresponding wave function φ0(r) (it is not necessary to
normalize the result)
(b) Using the same numerical values as in question 17.1.5, evaluate the
spa-tial extension of φ0(r).
17.2.6 The experiment is performed at temperatures T ranging between
0.1 K and 4 K Compare the characteristic thermal energy k B T to each of the
energy quanta of the “cyclotron”, “axial” and “magnetron” motions (associ-ated respectively with ˆn r, ˆN z and ˆn l) For which of these motions does the discrete nature of the energy spectrum play an important role?
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