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    Relativistic Quantum Mechanics

    Dr.K.P.SatheeshPrincipal

    Government College, Ambalapuzha

    November 5, 2010

    (following is a lecture on elementary level introduction to Relativisticquantum mechanics which has been used in various seminars for studentsdoing MSc. in Physics. Main reference is the text book on Advanced quan-tum Mechanics - Zakurai)

    Relativistic notation - Initial attempts in Relativistic Quantum mechanics- Klein Gordon Equation - Probability conservation - Derivation of Dirac

    Equation - Conserved current - Representation independence

    1 Introduction

    It is well known that free particle Hamiltonian is notp2

    2m

    when rela-

    tivistic effects are taken into consideration. Consequently Schrodinger equa-

    tion obtained from this Hamiltonian by operator replacement has to be mod-ified. Attempts to modify the Schrodinger equation by using the relativisticexpression for energy (ie) E = (p2c2+ m2c4)

    1

    2 possess certain undesirable fea-tures. One unattractive feature has been the appearance of different typesof space and time operators which is against the spirit of relativity theory in

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    which space and time are considered to be the components of same four vec-

    tor (ie) E i t , p i would lead to it = (2c22 + m2c4)1

    2 .Moreover the meaning of the operator (2c22 + m2c4)

    1

    2 itself is not quiteclear. Even though the interpretation of square root operator can be madetransparent by transforming to momentum space the procedure fails if wewere to consider p (p eA

    c) which is required in the presence of elec-

    tromagnetic field. attempts to develop a relativistic quantum mechanics wasinitiated by Schrodinger himself immediately after his development of wavemechanics. In order to avoid the difficulties associated with the square rootof a linear operator he tried to develop the basic equation by effecting theoperator replacement in the expression for E2. Consequently he developed

    the equation now known as Klein Gordon equation.Actually Schrodinger con-sidered the relativistic equation unsatisfactory and did not pursue it further.Physical implications of this equation was taken up by Klein and Gordon.Meanwhile Dirac succeeded in obtaining a first order wave equation elimi-nating many of the apparent defects attributed to Klein Gordon equation.All these interim attempts later lead to a full fledged Relativistic QuantumMechanics which gradually took a satisfactory shape now known as Rela-tivistic Quantum Field Theory. In this theory both Klein Gordon and Diracequations are perfectly respectable equations.

    2 Klein Gordon Equation

    Operator replacement is made in the relativistic energy equation toobtain the following

    E2 = p2c2 + m2c4 (1)

    2

    2m

    2

    t2= (2c22 + m2c4) (2)

    1

    c22

    t2 2 +

    mc

    2 = 0 (3)

    This equation is known as Klein Gordon equation. This equation can bewritten in a compact and convenient form using the relativistic notationdescribed below.

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    3 Relativistic Notation

    In the four vector notation (that is going to be used throughout) four vector

    b with = 1, 2, 3, 4 stands for b = (b1, b2, b3, b4) = (

    b , ib0), b1, b2 and b3are real and b4 = ib0 is purely imaginary. In general Greek indices , , . . .run from 1 to 4 where as i, j, k . . . run from 1 to 3. The coordinate vector

    x = (x1, x2, x3, x4) = (x,ict). Symbol x, y, z may also be used in the place

    ofx1, x2 and x3. All the repeated indices are summed unless otherwise statedexplicitly.Under a Lorentz transformation we have x = ax (repeated indices aresummed)a satisfy the following relations:

    aa = (4)

    (a1) = a (5)

    a = (a1)x

    = ax

    (6)

    The DAlembertian operator (Box operator) is defined as

    2 1

    c22

    t2(7)

    Also = with =

    xIn this notation the Klein Gordon equation

    can be written as =

    mc

    2 (8)

    In natural units = c = 1 and hence

    ( m2) = 0 (9)

    is the Klein Gordon equation.

    4 Defects of Klein Gordon equation

    When Klein Gordon equation is treated as the field equation of ascalar particle (like a meson) it is a perfectly respectable and valid equa-tion. More over it is manifestly Lorentz covariant. But in single particlerelativistic quantum mechanics it was treated unsatisfactory. These defectswere historically the main motivation for the development of Dirac equationin relativistic quantum mechanics. Main defects are listed below.

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    1. According to the dynamical postulate of quantum mechanics an equa-

    tion of motion should be first order in time. Klein Gordon equation isnot.

    2. Equation gives the possibility of negative energy states which is notproperly accounted for.

    3. The equation is not capable of predicting or handling the spin of aparticle

    4. Unlike Schrodinger equation the definition of a positive definite proba-bility density and probability current density is not normally possible

    in Klein Gordon Equation

    Apparent defects of Klein Gordon equation listed above motivated Dirac todevelop a first order relativistic wave equation because he identified that theabove mentioned defects are due to to the root cause that wave equation issecond order. Attempt of Dirac met with tremendous success theoreticallyand experimentally.

    5 Probability Conservation in RQM

    In conventional quantum mechanics ||2

    d3

    x is interpreted as the prob-ability of finding the particle with wave function in the volume elementd3x. The probability density P and the flux density S are given by

    P = ||2 > 0 (10)

    S =

    i

    2m

    ( ) (11)

    By the elementary methods using Schrodinger equation the continuity equa-tion is obtained as

    P

    t+ .S = 0 (12)

    By proper normalization of we can set

    P d3x = 1. This integral overall space is a constant of motion. Now the question is how to construct arelativistic analogue of the non relativistic equation of continuity? Followingare the main requirements.

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    Construction of bilinear forms which can be interpreted as the proba-

    bility density and the flux density satisfying the equation of continuity

    According to the fundamental hypothesis of quantum mechanics theprobability density must be positive definite

    According to the requirements of Special theory of relativity ProbabilityP should transform as the fourth component of a four vector density.

    In the covariant form the continuity equation has to be written asS = 0 with S (S, icP)

    We use all the above ideas in RQM based on Klein Gordon equation. The

    four vector current density is defined asS A(

    ) (13)

    Where is the solution of the Klein Gordon equation. Taking the derivativewe get

    Sx

    S = A( +

    )

    = A[ [(

    ) ] ] (14)

    According to the Klein Gordon equation this quantity vanishes giving

    S = 0 (15)Now consider a particle obeying Klein Gordon equation which is

    moving with non-relativistic velocities with energy E mc2. the solu-tion of the Klein Gordon equation and Schrodinger equation are related by emc

    2t/. and are respectively the solutions of Schrodinger andKlein Gordon equation.The components of the four vector density s cannow be determined using equation [13].

    s0 = is4

    2imc

    A||2 (16)

    s = A[ ()] (17)s and s0 will respectively be the flux density and c times the probabilitydensity of Schrodinger theory if we set A = i

    2m. Thus a four vector den-

    sity obtained from the solution of Klein Gordon equation has the followingproperties.

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    1. The current density satisfies the continuity equation

    2. The components of the current density coincide with the flux densityand c times the probability density in the non relativistic limit.

    Using s = (S, icP) and x = (x,ict) the probability density P can be writtenas

    P =i

    2mc2

    t

    t

    (18)

    In contrast to Schrodinger theory Klein Gordon theory has a seriousdifficulty in interpreting the above equation. Since Klein Gordon equationis second order in time both and d

    dtcould be arbitrarily fixed. this spoils

    the positive definite feature of P given by eqn.[18]. Clearly this difficulty canbe avoided by writing a wave equation which is linear in time. This is whatDirac did in 1928. Using the equation which is linear in

    tDirac succeeded in

    deriving the zeroth component of current density which is positive definite.the difficulty associated with probability density was thus removed in Diracstheory. Because of this reason Dirac equation was considered to be the onlycorrect relativistic wave equation during the period 1928 to 1934. In 1934Pauli and Weisskopf revived Klein Gordon equation and interpreted s asthe charge density (instead of probability current density) which need not bepositive definite. The interpretation is more appropriate when the solution

    of Klein Gordon equation is interpreted as a quantized field operator insteadof a single particle wave function.

    6 Derivation of Dirac Equation

    As indicated earlier the derivation of Dirac1 equation was motivatedby the apparent defects of Klein Gordon equation. Klein Gordon equationdo not naturally incorporate spin. A study of the method of incorporationof spin in non relativistic quantum mechanics can be used as a spring boardfor finding the procedure for incorporating spin in relativistic quantum me-

    chanics. The method developed by Pauli to account for the interaction ofelectron magnetic moment with the magnetic field in non relativistic quantummechanics is to add term H(spin) =

    e2mc

    .B to the usual Hamiltonian.

    1This approach based on the necessity of including spin is different from the original

    approach of Dirac who tried to make the equation linear so that probability function

    becomes positive definite.

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    Where B is the applied magnetic field and are the Pauli spin matrices.

    This ad-hoc procedure appears unsatisfactory since we believe that funda-mental electromagnetic interactions are those which can be generated by thereplacement of mechanical momentum by electromagnetic momentum (ie)p p

    eAc

    . this fact motivates the introduction of another procedure for

    the introduction of spin. Instead of using kinetic energy operator H(KE) = p2

    2m

    in the absence of a vector potential we use H(KE) = (p)(p)2m

    which is essen-tially same when there is no vector potential by virtue of the equation

    ( A)( B) = A B + i (A B) (19)

    But the equation is different if we make the substitution p p eAc

    Then we have1

    2m

    p

    eA

    c

    p

    eA

    c

    =1

    2m

    p

    eA

    c

    2+

    i

    2m

    p

    eA

    c

    p

    eA

    c

    =1

    2m

    p

    eA

    c

    2

    e

    2mc B (20)

    Note:Whenever operator product involving derivatives are used remember

    this. Always imagine that the product is applied to a quantity and apply theproduct rule. Therefore we have p (A) = i[( A) + A ].Therefore p A = i( A) A p. (In deriving [eqn. 20] use of thisidea is made)

    The procedure used for incorporating electron spin in a non relativistictheory can be used for developing relativistic theory of a spin half particle.(ie) the replacement p p is made in the relativistic energy equation

    E2

    c2

    = p2 + m2c2 E(op)

    c

    pE(op)

    c

    + p = mc2 (21)

    The operators are E(op) = i t

    = ic x0

    ;p = i This operator replace-ments gives a second order differential equation first written by B.L. van derWaerden for a free electron.

    i

    x0+ i

    i

    x0 i

    = mc2 (22)

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    In the above equation is a two component wave function.

    In order to convert [eqn.22] to a first order differential equation we definebelow two two component wave functions (R) and (L)

    (R) =1

    mc

    i

    x0

    i( )

    , (L) = (23)

    We can now consider [eqn.22] as equivalent to two first order equations

    [i( ) i (/x0)] (L) = mc(R)

    [i( ) i (/x0)] (R) = mc(L) (24)

    For massive particles the equations given above couple (L) and (R). Eventhough these equations are equivalent to Dirac equation we can write it inthe form originally written by Dirac by adding and subtracting them.

    i( )((R) (L)) i (/x0) ((R) + (L)) = mc((R) + (L))(25)

    i( )((R) + (L)) + i (/x0) ((R) (L)) = mc((R) (L))(26)

    Let us now define ((R) + (L)) A and ((R) (L)) B and write the

    above set of coupled differential equations in the form

    i (/x0) i i i (/x0)

    AB

    = mc

    AB

    (27)

    Where the four component wave function (Diracs four component spinor)is defined by the relation

    AB

    =

    (R) + (L)

    (R) + (L)

    (28)

    By defining the Dirac matrices and using the relativistic notation we canwrite the above matrix equation in a more compact manner.

    + 4

    (ix0)

    + mc

    = 0 (29)

    or using the summation convention

    (x) +

    mc

    = 0 (30)

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    The matrices with = 1, 2, 3, 4 are the 4 4 matrices usually known

    as Dirac matrices and can be written as a 2 2 matrix using the Puli spinmatrices defined as follows.Note:The standard form of Pauli 2 2 spin matrices will be used throughout.

    1

    0 11 0

    , 2

    0 ii 0

    , 3

    1 00 1

    , I

    1 00 1

    I is the unit matrix. The space component (k) and the time component (4)of the Dirac Gamma matrices are given by

    k

    0 ikik 0

    , 4

    I 00 I

    (31)

    For clarity we write explicitly two of the gamma matrices below.

    3

    0 0 i 00 0 0 ii 0 0 00 i 0 0

    , 4

    1 0 0 00 1 0 00 0 1 00 0 0 1

    , etc. (32)

    [eqn.30] represents the celebrated Dirac equation which can be more com-

    pactly written in the natural units as

    ( + m) = 0 (33)

    It should be noted that the Dirac equation is actually a set of four differentialequations that couple the four components of the bispinor or dirac spinor which can be represented by a column matrix

    =

    123

    4

    (34)

    The entity is called a spinor because its transformation properties under theLorentz transformation is different from that of an ordinary four vector.

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    7 Properties of Gamma Matrices

    The 4 4 matrices called the Gamma matrices or Dirac matricespossess the following genral properties.

    1. The square of Gamma matrices are unity (ie) 2 = 1

    24 =

    I 00 I

    2=

    I 00 I

    2k =

    0 ik

    ik 0

    0 ik

    ik 0

    =

    2k 00 2k

    =

    I 00 I

    2. and satisfy the following anticommutation relations

    {, } = + = 2 (35)

    For example

    12 + 21 =

    0 i1

    i1 0

    0 i2

    i2 0

    +

    0 i2

    i2 0

    0 i1

    i1 0

    =

    12 + 21 0

    0 12 + 21

    = 0

    3. Gamma matrices are Hermitian (ie) =

    4. Gamma matrices are traceless (ie) the sum of the diagonal elementsvanish as can be easily verified.

    8 Dirac equation in Hamiltonian form

    Originally Dirac wrote the equation satisfied by a relativistic particlein the Hamiltonian form H = i(/t) with the Hamiltonian called DiracHamiltonian satisfying the relation H = ic + mc2 where and ,are 4 4 matrices. They are defined by the relations

    = 4 =

    I 00 I

    , k = i4k =

    0 k

    k 0

    Alpha and Beta matrices are also traceless hermitian matrices having proper-ties similar to gamma matrices {k, } = 0,

    2 = 1, {k, l} = 2kl Conservedcurrent-Representation independence

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    9 Conserved current

    The main motivation behind the derivation of Dirac equation hasbeen the fact the Klein Gordon equation is not giving a positive definiteprobability density as required by the basic postulates of quantum mechanics.In the following we show that Dirac equation actually gives a positive definiteprobability density. An adjoint Dirac spinor () in contrast to the Hermitianconjugate spinor () is defined by = 4. They can be represented asthe following row matrices.

    = (1, 2,

    3,

    4), = (

    1,

    2,

    3,

    4) (36)

    Normally is considered to be an independent spinor different from . Toobtain its wave equation first of all the Hermitian conjugate of Dirac equationis taken.

    xkk +

    xk4 +

    mc

    = 0 (37)

    The adjoint Dirac equation is obtained by multiplying the above equationfrom the right by 4

    x +

    mc

    = 0 (38)

    As in the case of non-relativistic quantum mechanics we multiply the original

    Dirac equation from the left by and the adjoint equation from the rightby and subtract to get

    x

    () = 0 (39)

    The flux density four vector in Dirac theory can therefore be written as

    s = ic = (c, ic) (40)

    which satisfies the continuity equation

    sx

    = s = 0. (41)

    It is clear that the quantity

    = =

    4=1

    (42)

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    is positive definite unlike the case of Klein Gordon theory. Thus in Dirac

    theory the problem of negative probability density is eliminated. The prob-ability density is 4 =

    and the quantity sk = ick = ck is

    the flux density.

    10 Representation independence

    Representation independence of Dirac equation means that Dirac equa-tions with different form of gamma matrices are equivalent if the gammamatrices satisfy the defining property (ie.) anti-commutation. Let the Diracequation be written in the form

    x+

    mc

    = 0 (43)

    In the above equation satisfies the defining property of gamma matrices(ie.)they are 4 4 matrices satisfying {,

    } = 2 with = 1 . . . 4. By

    representation independence we mean the assertion that the equation given

    above is equivalent to

    x+ mc

    = 0 which is the original Dirac equa-

    tion. Different possible sets of 44 matrices satisfying the anti-commutationrelation given above are said to be sets of gamma matrices in different repre-

    sentations. The representation independence can be proved by using Paulisfundamental theorem which states that two sets of 4 4 matrices satisfyingthe anti-commutation relations {, } = 2 and {

    ,

    } = 2 with

    , = 1 . . . 4 there exists a nonsingular 4 4 matrix S such that

    SS1 = (44)

    where the matrix S is unique (up to a multiplicative constant). The Diracequation in the new representation can now be written as

    SS

    1

    x +

    mc

    SS

    1

    = 0 (45)

    Multiplying from the left by S1 we get

    x+

    mc

    S1 = 0 (46)

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    which is same as the original Dirac equation with the solution given by S.

    therefor equation [8] is equivalent to the Dirac equation and the wave func-tions in both representations are related by

    = S (47)

    According to Paulis fundamental theorem S can be chosen to be unitary if are Hermitian. The unitarity of the matrix S implies the equivalence ofprobability density and flux density in both representations as seen below.

    = 4

    = SS4S1S

    S1S

    = (48)

    This clearly shows that all the physical consequences are same in both repre-sentations. But the wave functions in different representations look different.Most common gamma matrices used are the following

    1. The standard Dirac Pauli representation used in the present treatment.

    2. The Weyl representation in which k and 4 are off diagonal matrices.

    3. The Majorana representation in which k are purely real and 4 is

    purely imaginary.

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