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Any two states s,t are either the same (s=t), or different (s t), and that's all ... Given any set S H of system states, Whether all mutually distinguishable, or not, ... – PowerPoint PPT presentation

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Title: EEL%205930%20sec.%205,%20Spring%20


1
EEL 5930 sec. 5, Spring 05Physical Limits of
Computing
http//www.eng.fsu.edu/mpf
  • Slides for a course taught byMichael P. Frankin
    the Department of Electrical Computer
    Engineering

2
Basics of Quantum Theory
3
Systems and Subsystems
  • Intuitively speaking, a physical system consists
    of a region of spacetime all the entities (e.g.
    particles fields) contained within it.
  • The universe (over all time) is a physical system
  • Transistors, computers, people also phys. systs.
  • One physical system A is a subsystem of another
    system B (write A?B) iff A is completely
    contained within B.
  • Later, we will make these definitions more
    formal precise.

B
A
4
Closed vs. Open Systems
  • A subsystem is closed to the extent that no
    particles, information, energy, or entropy (terms
    to be defined) enter or leave the system.
  • The universe is (presumably) a closed system.
  • Subsystems of the universe may be almost closed
  • Often in physics we consider statements about
    closed systems.
  • These statements may often be perfectly true only
    in a perfectly closed system.
  • However, they will often also be approximately
    true in any nearly closed system (in a
    well-defined way)

5
Concrete vs. Abstract Systems
  • Usually, when reasoning about or interacting with
    a system, an entity (e.g. a physicist) has in
    mind a description of the system.
  • A description that contains every property of the
    system is an exact or concrete description.
  • That system (to the entity) is a concrete system.
  • Other descriptions are abstract descriptions.
  • The system (as considered by that entity) is an
    abstract system, to some degree.
  • We nearly always deal with abstract systems!
  • Based on the descriptions that are available to
    us.

6
System Descriptions
  • Classical physics
  • A system could be completely described by giving
    a single state S out of the set ? of all possible
    states.
  • Statistical mechanics
  • Instead, give a probability distribution function
    p??0,1 stating that the system is in state S
    with probability p(S).
  • Quantum mechanics
  • Give a complex-valued wavefunction ?? ? C,
    ?(S)?1, implying the system is instate S with
    probability ?(S)2.

7
States State Spaces
  • A possible state S of an abstract system A
    (described by a description D) is any concrete
    system C that is consistent with D.
  • I.e., it is possible that the system in question
    could be completely described by the description
    of C.
  • The state space of A is the set of all possible
    states of A.
  • So far, the concepts weve discussed can be
    applied to either classical or quantum physics
  • Now, lets get to the uniquely quantum stuff

8
Distinguishability of States
  • Classical quantum mechanics differ crucially
    regarding the distinguishability of states.
  • In classical mechanics, there is no issue
  • Any two states s,t are either the same (st), or
    different (s?t), and thats all there is to it.
  • In quantum mechanics (i.e. in reality)
  • There are pairs of states s?t that are
    mathematically distinct, but not 100 physically
    distinguishable.
  • Such states cannot be reliably distinguished by
    any number of measurements, no matter how
    precise.
  • But you can know the real state (with high
    probability), if you prepared the system to be in
    a certain state.

9
State Vectors Hilbert Space
  • Let S be any maximal set of distinguishable
    possible states s, t, of an abstract system A.
  • I.e., no possible state that is not in S is
    perfectly distinguishable from all members of S.
  • Identify the elements of S with unit-length,
    mutually-orthogonal (basis) vectors in an
    abstract complex vector space H.
  • The systems Hilbert space
  • Postulate 1 Each possible state ? ofsystem A
    can be identified with a unit-length vector in
    the Hilbert space H.

t
s
?
10
(Abstract) Vector Spaces
  • A concept from abstract linear algebra.
  • A vector space, in the abstract, is any set of
    objects that can be combined like vectors, i.e.
  • You can add them
  • Addition is associative commutative
  • Identity law holds for addition to zero vector 0
  • You can multiply them by scalars (incl. ?1)
  • Associative, commutative, and distributive laws
    hold
  • Note There is no inherent basis (set of axes)
  • The vectors themselves are the fundamental
    objects,rather than being just lists of
    coordinates

11
Hilbert spaces
  • A Hilbert space H is a vector space in which the
    scalars are complex numbers, with an inner
    product (dot product) operation ? HH ? C
  • See Hirvensalo p. 107 for defn. of inner product
  • x?y (y?x) ( complex conjugate)
  • x?x ? 0
  • x?x 0 if and only if x 0
  • x?y is linear, under scalar multiplication
    and vector addition within both x and y

Componentpicture
y
Another notation often used
x
bracket
x?y/x
12
Review The Complex Number System
  • It is the extension of the real number system via
    closure under exponentiation.
  • (Complex) conjugate
  • c (a bi) ? (a ? bi)
  • Magnitude or absolute value
  • c2 cc a2b2

The imaginaryunit
i
c
b

?
a
Real axis
Imaginaryaxis
?i
13
Review Complex Exponentiation
  • Powers of i are complex units
  • Note
  • e?i/2 i
  • e?i ?1
  • e3? i /2 ? i
  • e2? i e0 1

e?i
i
?
?1
1
?i
14
Vector Representation of States
  • Let Ss0, s1, be any maximal set of
    mutually distinguishable states, indexed by i.
  • A basis vector vi identified with the ith such
    state can be represented as a list of numbers
  • s0 s1 s2 si-1 si si1
  • vi (0, 0, 0, , 0, 1, 0, )
  • Arbitrary vectors v in the Hilbert space H can
    then be defined by linear combinations of the vi
  • And the inner product is given by

15
Diracs Ket Notation
  • Note The inner product definition is the
    same as the matrix product of x, as a
    conjugated row vector, times y, as a normal
    column vector.
  • This leads to the definition, for state s, of
  • The bra ?s means the row matrix c0 c1
  • The ket s? means the column matrix ?
  • The adjoint operator takes any matrix Mto its
    conjugate transpose M ? MT, so?s can be
    defined as s?, and x?y xy.

Bracket
16
Distinguishability of States, again
  • State vectors s and t are (perfectly)
    distinguishable or orthogonal (write s?t)
    iff st 0. (Their inner product is zero.)
  • State vectors s and t are perfectly
    indistinguishable or identical (write st)
    iff st 1. (Their inner product is one.)
  • Otherwise, s and t are both non-orthogonal, and
    non-identical. Not perfectly distinguishable.
  • We say, the amplitude of state s, given state t,
    is st. Note amplitudes are complex numbers.

17
Probability and Measurement
  • A yes/no measurement is an interaction
    designed to determine whether a given system
    is in a certain state s.
  • The amplitude of state s, given the actual state
    t of the system determines the probability
    of getting a yes from the measurement.
  • Postulate 2 For a system prepared in state t,
    any measurement that asks is it in state s?
    will say yes with probability P(st) st2
  • After the measurement, the state is changed, in a
    way we will define later.

18
A Simple Example
  • Suppose abstract system S has a set of only 4
    distinguishable possible states, which well
    call s0, s1, s2, and s3, with corresponding ket
    vectors s0?, s1?, s2?, and s0?.
  • Another possible state is then the unit vector
  • Which is equal to the column matrix
  • If measured to see if it is in state s0, we
    have a 50 chance of getting a yes.

19
Schrödingers Cat
  • A thought experiment that illustrates the weird
    nature of quantum states.
  • An apparatus is set up tokill a cat if an atom
    decays in a certain time (50 prob.).
  • The system enters the quantum superposition
    state live cat? dead cat?.
  • We cant say that the cat is really either
    alive or dead until we open the box and observe
    it.
  • Even then, the true state can validly be
    considered to be we see live cat? we see
    dead cat?.
  • Outwardly-spreading entanglement ? Many-worlds
    picture

20
Linear Operators
  • V,W Vector spaces.
  • A linear operator A from V to W is a
    linear function AV?W. An operator on V is
    an operator from V to itself, AV?V.
  • Given bases for V and W, we can represent linear
    operators as matrices.
  • An Hermitian operator H on V is a linear operator
    that is self-adjoint (HH).
  • Its diagonal elements are real.

21
Eigenvalues Eigenvectors
  • v is called an eigenvector of linear operator A
    iff A just multiplies v by a scalar a, i.e. Avav
  • eigen (German) means characteristic
  • a, the eigenvalue corresponding to
    eigenvector v, is just the scalar that A
    multiplies v by
  • a is degenerate if it is shared by 2
    eigenvectors that are not scalar multiples of
    each other
  • Any Hermitian operator has all real-valued eigenv
    ectors, which form an orthogonal set

22
Observables
  • A Hermitian operator H on the set V is called an
    observable if there is an orthonormal (all
    unit-length, and mutually orthogonal) subset of
    its eigenvectors that forms a basis of V.
  • Postulate 3 Every measurable physical property
    of a system can be described by a corresponding
    observable H. Measurement outcomes correspond to
    eigenvalues of H.
  • The measurement can also be thought of as a set
    of yes-no tests that compares the state with each
    of the observables normalized eigenvectors.

23
Wavefunctions
  • Given any set S?H of system states,
  • Whether all mutually distinguishable, or not,
  • a quantum state vector v can be translated to a
    wavefunction ?S?C, giving, for each state s?S,
    the amplitude ?(s) of that state.
  • When s is some other state vector, and the
    actual state is v, then ?(s) is just sv.
  • Whenever S includes a basis set, ? also
    determines v.
  • ? is called a wavefunction because its dynamics
    takes the form of a wave equation when S ranges
    over a space of positional states.

24
Unitary Transformations
  • A matrix (or linear operator) U is unitary iff
    its inverse equals its adjoint U?1 U
  • Some nice properties of unitary transformations
  • Invertible, bijective, one-to-one.
  • The set of row vectors comprises an orthonormal
    basis.
  • Ditto for the set of column vectors.
  • Preserves vector length U? ?
  • Therefore also preserves total probability over
    all states
  • Implements a change of basis,
  • from one orthonormal basis to another.
  • Can be thought of as a kind of generalized
    rotation of? in Hilbert space.

25
Time Evolution
  • Postulate 4 (Closed) systems evolve (change
    state) over time via unitary transformations.
  • ?t2 Ut1?t2 ?t1
  • Note that since U is linear, a small-factor
    change in the amplitude of a particular state at
    t1 leads to a correspondingly small change in the
    amplitude of the corresponding state at t2!
  • Chaotic sensitivity to initial conditions
    requires an ensemble of initial states that are
    different enough to be distinguishable (in the
    sense we defined)
  • Indistinguishable initial states never beget
    distinguishable outcomes
  • ? true chaotic/analog computing is physically
    impossible

U-1 U
26
Schrödinger's Wave Equation
  • Start w. classical Hamiltonian energy
    equation H K P (K kinetic, P
    potential)
  • Express K in terms of momentum K ½mv2 p2/2m
  • Substitute H i??t and p -i??x
  • Apply to wavefunction ? over position states x

(Where ?a ? ?/?a)
27
Multidimensional Form
  • For a system with states given by (x,t) where t
    is a global time coordinate, and x describes N/3
    particles (p0,,pN/3-1) with masses (m0,,mN/3-1)
    in a 3-D Euclidean space, where each pi is
    located at coordinates (x3i, x3i1, x3i2), and
    where particles interact with potential energy
    function P(x,t), the wavefunction ?(x,t) obeys
    the following (2nd-order, linear, partial)
    differential equation

28
Features of the wave equation
  • Particles momentum state p is encoded by their
    wavelength ?, as per ph/?
  • The energy of a state is given by the frequency
    f of rotation of the wavefunction in
    the complex plane Ehf.
  • By simulating this simple equation, one can
    observe basic quantum phenomena, such as
  • Interference fringes
  • Tunneling of wave packets through potential
    energy barriers
  • Demo of SCH simulator

29
Gaussian wave packet moving to the rightArray
of small sharp potential-energy barriers
30
Initial reflection/refraction of wave packet
31
A little later
32
Aimed a little higher
33
A faster-moving particle
34
Relativistic Wave Equations
  • Unfortunately, despite its many practical
    successes, the literal Schrödingers equation is
    not relativistically invariant.
  • That is, it does not retain the same form in a
    boosted frame.
  • However, solutions to the free Schrödingers
    equation (where V0) can be given a
    self-consistent relativistic interpretation.
  • Let p -i??x be relativistic momentum,
  • Let m i??t be rest mass in the particles frame
    of ref.
  • Taking the derivative along an isospatial, the
    proper time t axis
  • Let E i??t be relativistic energy of the
    particle
  • Then, E2 p2 m2 is easily shown to be true for
    plane-wave solutions
  • Lines of constant phase angle are the isochrones
    of the moving particle.
  • And everything transforms properly to a new
    reference frame.
  • In fact, the solutions to the free Schrödingers
    equation closely correspond to solutions to the
    relativistic Klein-Gordon equation ?µ?µ
    m2f(xµ) 0.
  • This describes a free, massive scalar particle.

35
Compound Quantum Systems
  • Let CAB be a system composed of two separate
    subsystems A,B with vector spaces A,B with bases
    ai?,bj?.
  • The state space of C is a vector space CA?B
    given by the tensor product of spaces A and B,
    with basis states labeled as aibj? ai?bj?.
  • E.g., if A has state ?aca0a0 ? ca1
    a1?,while B has state ?bcb0b0 ? cb1 b1?,
    thenC has state ?c ?a??b ca0cb0a0b0?
    ca0cb1a0b1? ca1cb0a1b0? ca1cb1a1b1?

(Use distributive law)
36
Entanglement
  • If the state of compound system C can be
    expressed as a tensor product of states of two
    independent subsystems A and B, ?c ?a??b,
  • then, we say that A and B are not entangled, and
    they have definite individual states.
  • E.g. 00?01?10?11?(0?1?)?(0?1?)
  • Otherwise, A and B are entangled (quantumly
    correlated) their states are not independent.
  • E.g. 00?11?

(State has entropy 0 but mutual information 2!)
37
Size of Compound State Spaces
  • Note that a system composed of many separate
    subsystems has a very large state space.
  • Say it is composed of N subsystems, each with k
    basis states
  • The compound system has kN basis states!
  • Many possible states of the compound system will
    have nonzero amplitude in all these kN basis
    states!
  • In such states, all the distinguishable basis
    states are (simultaneously) possible outcomes
  • each with some corresponding probability
  • This illustrates the many worlds nature of
    quantum mechanics.
  • And the enormous number of possible worlds
    involved.

38
After a Measurement?
  • After a system or subsystem is measured from
    outside, its state appears to collapse to exactly
    match the measured outcome
  • the amplitudes of all states perfectly
    distinguishable from states consistent w. that
    outcome drop to zero
  • states consistent with measured outcome can be
    considered renormalized so their probs. sum to
    1
  • This collapse appears nonunitary ( nonlocal)
  • However, this behavior is now explicable as the
    expected consensus phenomenon that would be
    experienced even by entities within a closed,
    perfectly unitarily-evolving world (Everett,
    Zurek).

39
Pointer States
  • For a given system interacting with a given
    environment,
  • The system-environment interactions can be
    considered measurements of a certain observable
    of the system by the environment, and vice-versa.
  • Any each observable, there are certain basis
    states that are characteristic of that
    observable.
  • These are just the eigenstates of the observable.
  • A pointer state of a system is an eigenstate of
    the system-environment interaction observable.
  • The pointer states are the inherently stable
    states.

40
Key Points to Remember
  • An abstractly-specified system may have many
    possible states not all pairs are
    distinguishable.
  • A quantum state/vector/wavefunction ? assigns a
    complex-valued amplitude ?(s) to each state s.
  • The probability of state s is ?(s)2, the square
    of ?(s)s length in the complex plane.
  • Quantum states evolve over time via unitary
    (invertible, length-preserving) transformations.

41
Quantum Information
  • Generalizing classical information theory
    concepts to fit quantum reality

42
Density Operators
  • For any given state ??, the probabilities of all
    the basis states si are determined by an
    Hermitian operator or matrix ? (called the
    density matrix)
  • Note that the diagonal elements ?i,i are just the
    probabilities of the basis states i.
  • The off-diagonal elements are called
    coherences.
  • They describe the quantum entanglements that
    exist between basis states.
  • The density matrix describes the state ??
    exactly!
  • It (redundantly) expresses all of the quantum
    info. in ??.

43
Mixed States
  • Suppose the only thing one knows about the true
    state of a system that it is chosen from a
    statistical ensemble or mixture of state vectors
    vi (called pure states), each with a derived
    density matrix ?i, and a probability Pi.
  • In such a situation, in which ones knowledge
    about the true state is expressed as probability
    distribution over pure states, we say the system
    is in a mixed state.
  • Such a situation turns out to be completely
    described, for all physical purposes, by simply
    the expectationvalue (weighted average) of the
    vis density matrices
  • Note Even if there were uncountably many vi
    going into the calculation, the situation remains
    fully described by O(n2) complex numbers, where n
    is the number of basis states!

44
Von Neumann Entropy
  • Suppose our probability distribution over states
    comes from the diagonal elements of some density
    matrix ?.
  • But, we will generally also have additional
    information about the state hidden in the
    coherences.
  • The off-diagonal elements of the density matrix.
  • The Shannon entropy of the distribution along the
    diagonal will generally depend on the basis used
    to index the matrix.
  • However, any density matrix can be (unitarily)
    rotated into another basis in which it is
    perfectly diagonal!
  • This means, all its off-diagonal elements are
    zero.
  • The Shannon entropy of the diagonal probability
    distribution is always minimized in the diagonal
    basis, and so this minimum is selected as being
    the true (basis-independent) entropy of the mixed
    quantum state ?.
  • It is called the von Neumann entropy.

45
V.N. entropy, more formally
  • The trace Tr M just means the sum of Ms diagonal
    elements.
  • The ln of a matrix M just denotes the inverse
    function to eM. See the logm function in
    Matlab
  • The exponential eM of a matrix M is defined via
    the Taylor-series expansion ?i0 Mi/i!

(Shannon S)
(Boltzmann S)
46
Quantum Information Subsystems
  • A density matrix for a particular subsystem may
    be obtained by tracing out the other
    subsystems.
  • Means, summing over state indices for all systems
    not selected.
  • This process discards information about any
    quantum correlations that may be present between
    the subsystems!
  • Entropies of the density matrices so obtained
    will generally sum to gt that of the original
    system. (Even if the original state was pure!)
  • Keeping this in mind, we may make these
    definitions
  • The unconditioned, reduced or marginal quantum
    entropy S(A) of subsystem A is the entropy of
    the reduced density matrix ?A.
  • The conditioned quantum entropy S(AB)
    S(AB)-S(B).
  • Note this may be negative! (In contrast to the
    classical case.)
  • The quantum mutual information I(AB)
    S(A)S(B)-S(AB).
  • As in the classical case, this measures the
    amount of quantum information that is shared
    between the subsystems
  • Each subsystem knows this much information
    about the other.

47
Tensors and Index Notation
  • For our purposes, a tensor is just a generalized
    matrix that may have more than one row and/or
    column index.
  • We can also define a tensor recursively as a
    number or a matrix of tensors.
  • Tensor signature An (r,c) tensor has r row
    indices and c column indices.
  • Convention Row indices are shown as subscripts,
    and column indices as superscripts.
  • Tensor product An (l,k) tensor T times an (n,m)
    tensor U is a (ln,km) tensor V formed from all
    products of an element of T times an element of
    U
  • Tensor trace The trace of an (r,c) tensor T with
    respect to index k (where 1 k r,c) is given
    by contracting (summing over) the kth row index
    together with the kth column index

Example a (2,2)tensor T in which all 4indices
take on values from the set 0,1
(I is the set of legal values of indices rk and
ck) ?
48
Quantum Information Example
AB AB
  • Consider the state vAB 00?11? of compound
    system AB.
  • Let ?AB vv.
  • Note that the reduced density matrices ?A ?B are
    fully classical
  • Lets look at the quantum entropies
  • The joint entropy S(AB) S(?AB) 0 bits.
  • Because vAB is a pure state.
  • The unconditioned entropy of subsystem A is S(A)
    S(?A) 1 bit.
  • The entropy of A conditioned on B is S(AB)
    S(AB) - S(A) -1 bit!
  • The mutual information I(AB) S(A) S(B) -
    S(AB) 2 bits!

00? 01? 10? 11?
49
Quantum vs. Classical Mutual Info.
  • 2 classical bit-systems have a mutual information
    of at most one bit,
  • Occurs if they are perfectly correlated, e.g.,
    00, 11
  • Each bit considered by itself appears to have 1
    bit of entropy.
  • But taken together, there is really only 1 bit
    of entropy shared between them
  • A measurement of either extracts that one bit of
    entropy,
  • Leaves it in the form of 1 bit of incompressible
    information (to the measurer).
  • The real joint entropy is 1 bit less than the
    apparent total entropy.
  • Thus, the mutual information is 1 bit.
  • 2 quantum bit-systems (qubits) can have a mutual
    info. of two bits!
  • Occurs in maximally entangled states, such as
    00?11?.
  • Again, each qubit considered by itself appears to
    have 1 bit of entropy.
  • But taken together, there is no entropy in this
    pure state.
  • A measurement of either qubit leaves us with no
    entropy, rather than 1 bit!
  • If done carefully see next slide.
  • The real joint entropy is thus 2 bits less than
    the apparent total entropy.
  • Thus the mutual information is (by definition) 2
    bits.
  • Both of the apparent bits of entropy vanish if
    either qubit is measured.
  • Used in a communication tech. called quantum
    superdense coding.
  • 1 qubits worth of prior entanglement between two
    parties can be used to pass 2 bits of classical
    information between them using only 1 qubit!

50
Why the Difference?
  • Scenario Entity A hasnt yet measured B and C,
    which (A knows) are initially correlated with
    each other, quantumly or classically
  • A has measured B and is now correlated with both
    B and C
  • A can use his new knowledge to uncompute
    (compress away) the bits from both B and C,
    restoring them to a standard state

OrderABC
Classical
Quantum
Knowing he is in state 0?1?, A can unitarily
rotate himself back to state 0?. Look ma, no
entropy!
A, being in a mixed state, still holds a bit of
information that is either unknown (external
view) or incompressible (As internal view), and
thus is entropy, and can never go away (by the
2nd law of thermo.).
51
Simulating the Schroedinger Wave Equation
  • A Perfectly Reversible Discrete Numerical
    Simulation Technique

52
Simulating Wave Mechanics
  • The basic problem situation
  • Given
  • A (possibly complex) initial wavefunction
    in an N-dimensional position basis,
    and
  • a (possibly complex and time-varying) potential
    energy function ,
  • a time t after (or before) t0,
  • Compute
  • Many practical physics applications...

53
The Problem with the Problem
  • An efficient technique (when possible)
  • Convert V to the corresponding Hamiltonian H.
  • Find the energy eigenstates of H.
  • Project ? onto eigenstate basis.
  • Multiply each component by .
  • Project back onto position basis.
  • Problem
  • It may be intractable to find the eigenstates!
  • We resort to numerical methods...

54
History of Reversible Schrödinger Sim.
See http//www.cise.ufl.edu/mpf/sch
  • Technique discovered by Ed Fredkin and student
    William Barton at MIT in 1975.
  • Subsequently proved by Feynman to exactly
    conserve a certain probability measure
  • Pt Rt2 It?1It1
  • 1-D simulations in C/Xlib written by Frank at MIT
    in 1996. Good behavior observed.
  • 1 2-D simulations in Java, and proof of
    stability by Motter at UF in 2000.
  • User-friendly Java GUI by Holz at UF, 2002.

(Rreal, Iimag., ttime step index)
55
Difference Equations
  • Consider any system with state x that evolves
    according to a diff. eq. that is 1st-order in
    time x f(x)
  • Discretize time to finite scale ?t, and use a
    difference equation instead x(t ?t) x(t)
    ?t f(x(t))
  • Problem Behavior not always numerically stable.
  • Errors can accumulate and grow exponentially.

56
Centered Difference Equations
  • Discretize derivatives in a symmetric fashion
  • Leads to update rules like x(t ?t) x(t ?
    ?t) 2?t f(x(t))
  • Problem States at odd- vs. even-numbered time
    steps not constrainedto stay close to each other!

2?tf
x1
g

x2
g
x3

g
x4

57
Centered Schrödinger Equation
  • Schrödingers equation for 1 particle in 1-D
  • Replace time ( also space) derivatives with
    centered differences.
  • Centered difference equation has realpart at odd
    times that depends only onimaginary part at even
    times, vice-versa.
  • Drift not an issue - real imaginaryparts
    represent different state components!

R1
g
?
I2
g
R3

g
I4
?
58
Proof of Stability
  • Technique is proved perfectly numerically stable
    convergent assuming V is 0 and ?x2/?t gt ?/m
    (an angular velocity)
  • Elements of proof
  • Lax-Richmyer equivalence convergence?stability.
  • Analyze amplitudes of Fourier-transformed basis
  • This is sufficient due to Parsevals relation
  • Use theorem (cf. Strikwerda) equating stability
    to certain conditions on the roots of an
    amplification polynomial ?(g,?), which are
    satisfied by our rule.
  • Empirically, technique looks perfectly stable
    even for more complex potential energy funcs.

59
Phenomena Observed in Model
  • Perfect reversibility
  • Wave packet momentum
  • Conservation of probability mass
  • Harmonic oscillator
  • Tunneling/reflection at potential energy barriers
  • Interference fringes
  • Diffraction

60
Interesting Features of this Model
  • Can be implemented perfectly reversibly, with
    zero asymptotic spacetime overhead
  • Every last bit is accounted for!
  • As a result, algorithm can run adiabatically,
    with power dissipation approaching zero
  • Modulo leakage frictional losses
  • Can map it to a unitary quantum algorithm
  • Direct mapping
  • Classical reversible ops only, no quantum speedup
  • Indirect (implicit) mapping
  • Simulate p particles on kd lattice sites using pd
    lg k qubits
  • Time per update step is order pd lg k instead of
    kpd
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