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    1

    MAGNETISM A Few BasicsA. HISTORY

    Magnetite or lodestone (FeIIOFeIII2O3)mineral in its natural state often has a strong attraction for iron and steel...mined in magnesiabut Pliny says it was named for the discoverer, a shepherd, magnes, "the nails of whose shoes

    and the tip of whose staff stuck fast in a magnetick field while he pastured his flocks."

    Lodestone appears in Greek writings by 800 B.C.First magnetic technological invention compass: in China, sometime between 2637 B.C. and

    1100 A.D. (!)others say it was introduced to China in 1200s by Italians or Arabs

    Early theories and experiments on magnetism were developed by the great minds of all times Gilbert, Descartes, Coulomb, Poisson, Green, Oertsted, Ampere, Davy, Freesnel, Faraday,Maxwell...

    But: Quantum Mechanics is necessary to develop a viable model, and the model continues toevolve: MAGNETISM IS NOT A SOLVED PROBLEM

    B. BASICSAll materials respond to an external magnetic field (H). The magnetization (M) of a sample isproportional to H:

    M = H. The proportionality constant, , is the magnetic susceptibility

    C. TYPES OF MAGNETISM - see chartThe Big five1. Diamagnetism

    electrons in closed shells cause a material to be repelled by H ( < 0).Typically, m = -1x10-6 emu/molusually a very small contribution to expexp = dia + para + Paulidia diamagnetic term due to closed-shell (core) electrons. ALL materials have this. For our

    systems, which will probably have a very small , the diamagnetic correction is non-trivial can be obtained from atom/group additivities or the Curie plot (see below).

    dia is temperature and field independent.para is due to unpaired electrons (= p)Pauli is typically seen in metals and other conductors - due to mixing excited states that are not

    thermally populated into the ground (singlet) state - temperature independent. Presumably notimportant in our systems.

    ALL OTHER TYPES OF MAGNETISM REQUIRE UNPAIRED SPINS (MOMENTS) THEINTERACTIONS AMONG SPINS DETERMINES THE TYPE OF MAGNETISM

    2. Paramagnetismrandomly oriented, rapidly reorienting moments; no permanent, spontaneous magnetic moment

    (M = 0 if H = 0)spins are non-interacting (non-cooperative)all other forms of magnetism have a critical temperature, TC, below which there is some

    interaction of moments. Above TC paramagnetp varies with T empirically according to the Curie Law:

    p

    = CT

    C = Curie constant

    or the Curie-Weiss Law:

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    2

    p

    = CT = Weiss constant

    is indicative ofintermolecularinteractions among the moments> 0 - ferromagnetic interactions (NOT ferromagnetism)< 0 - antiferromagnetic interactions (NOT antiferromagnetism)

    DIAMAGNETISM INCIPIENTFERROMAGNETISM

    METAMAGNETISM

    ANTI-FERROMAGNETISM

    FERRIMAGNETISM

    FERROMAGNETISM

    SUPER-PARAMAGNETISM

    SPERIMAGNETISM

    PARAMAGNETISMARAMAGNETISM

    SPEROMAGNETISM ASPEROMAGNETISM

    SPIN GLASS HELIMAGNETISM

    MICTOMAGNETISM

    Using the Curie Plot:

    exp

    = CT + T (T = dia + Pauli = temperature independent contribution)

    exp

    = CT

    +T

    (at high temperature if is small)

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    Plot exp vs 1/T

    0

    0.05

    0.1

    0.15

    0.2

    0.25

    0.3

    0.35

    0.4

    0 0.1 0.2 0.3 0.4 0.5

    para

    ferro

    antiferro

    ParamagneticSusce

    ptibility

    1/ Temperature (1/ K)

    slope = C; intercept = T; exp - T = p...then plot 1/p vs. T

    0

    10

    20

    30

    40

    50

    0 5 10 15 20

    = 0

    = +2

    = -2

    ParamagneticSusce

    ptibility

    1/ Temperature (1/ K)

    slope = 1/C; intercept = /CA magnetometer measures M which gives . Do the first plot to get T. Then at all T and H, p

    = exp - T

    The magnetization plotFor an atom with spin ms, its energy in H is:

    E(ms) = m

    sg

    BH = -msgB

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    4

    B is Bohr magneton (= 9.27x10-24J/T); g is the Lande constant (= 2.0023192778)Consider N particles, with ni in ith level

    ni

    i = N

    P i =

    ni

    N =

    exp

    i

    kT

    exp

    i

    kT

    i

    M = N i

    i P

    i

    now, consider two spin states (ms = 1/2),

    M = N

    msg

    B( )expm

    sg

    BH

    kT

    ms=1/2

    +1/2

    expm

    sg

    BH

    kT

    ms=1/2

    +1/2

    =Ng

    B

    2

    expg

    BH

    2kT

    exp

    gB

    H

    2kT

    expg

    BH

    2kT

    + exp

    gB

    H

    2kT

    =Ng

    B

    2tanh

    gB

    H

    2kT

    since tanh(y) = (ey-e-y)/(ey+e-y)

    if y

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    5

    a) For x >> 1, BS

    x( ) = 1S

    S+ 12( )

    12

    = 1

    x =g

    BH

    kT>> 1 means H

    T>> k

    gB

    = 1.38x1023 J / K

    2x9.27x10 24 J/ T= 0.7T / K

    b) For x

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    6

    0

    1

    2

    3

    4

    5

    6

    7

    8

    9

    10

    0 1 2 3 4 5 6 7

    S=1/2S=1S=3/2S=2S=5/2S=3S=7/2S=4S=9/2S=5

    M

    molar

    (B)

    H/T (Tesla/Kelvin)

    The effective magnetic momentdirectly relates to number of spins:

    eff= g[S(S+1)]1/2BS eff/B1/2 1.731 2.832 4.89

    related to molar susceptibility (m = emu/mol)

    m

    =N

    eff2

    3kT= C'

    T

    Therefore,

    eff= 3kC'

    N= 2.82 C'

    eff = 2.824 mT3. Ferromagnetismmoments throughout a material in 3-D tend to align parallelcan lead to a spontaneous permanent M (in absence of H)but, in a macroscopic system, it is energetically favorable for spins to segregate into regions

    calledDOMAINS- domains need not be aligned with each other

    A Domain

    may or may not have spontaneous Mapplication of H causes aligned domains to grow at the expense of misaligned

    domains...alignment persists when H is removed

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    7Ferromagnetism is a critical phenomenon, involving a phase transition that occurs at a critical

    temperature, Tc = Curie Temperature. Above Tc paramagnetTC is directly proportional to S(S+1)It takes energy to move domain walls - hysteresis:

    MR = Remnant Magnetization (M at Happ = 0)

    Msat = Saturation Magnetization (Msat= NgBS)

    HC = Coercive Field (Happ required to flip M)

    "Hard" magnetic material = high Coercivity"Soft" magnetic material = low Coercivity

    Electromagnets High MR and Low HC

    Electromagnetic Relays High Msat, Low MR, and Low HC

    Magnetic Recording Materials High MR and relatively High HC

    Permanent Magnets High MR and High HC

    (-) (+)

    (+)

    (-)

    Sample Magnetization

    Applied Field MR

    2HC

    M

    M

    HappHapp

    Msat

    M = Happ

    Msat = gBS

    Remanence: Magnetization of sample after H is removedCoercive field: Field required to flip M (+M to -M)

    4. Antiferromagnetismspins tend to align antiparallel in 3-Dno spontaneous Mno permanent Mcritical temperature: TN (Neel Temperature)

    above TN paramagnet

    5. Ferrimagnetismrequires two chemically distinct species with different momentsthey couple antiferomagnetically:no M; critical T = TC (Curie Temperature)

    bulk behavior very similar to ferromagnetismMagnetite is a ferrimagnet

    6. Other types

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    DIAMAGNETISM

    INCIPIENTFERROMAGNETISM

    METAMAGNETISM

    Low T; temporary alignment of momentsof ions & itinerant electrons

    Field-induced transition to magnetic

    state;must be below Neel temperature

    ANTI-FERROMAGNETISM

    FERRIMAGNETISM

    FERROMAGNETISM

    SUPER-

    PARAMAGNETISM

    SPERIMAGNETISM

    PARAMAGNETISM

    Small particle size allows singledomain fluctuation; destroyed by

    cooling below blocking temperature

    Two species frozen as in speromagnet;

    often net magnetication

    SPEROMAGNETISM ASPEROMAGNETISM

    SPIN GLASSHELIMAGNETISM

    Local moments licked into randomorientation;no net magnetiztion

    Magnetic ions cooled in a nonmagnetic host;usually dilute; RKKY coupling only (?)

    As in speromagnetism, but some orientation;net magnetization

    Crystalline asperomagnet

    MICTOMAGNETISMCluster glass; local correlations dominant

    D. SPECIAL TOPICS1. Magnetooptical Disks

    a. ReadingMagnetic materials rotate plane polarized lightin transmission: Faraday effectin reflection: Kerr effect (used in devices)Direction of rotation depends on polarization of M

    b. Writingactually a thermo-magnetic process since a high-powered laser is used to heat the sample1) Curie point writing-heat above TC, then cool in applied field2) Threshold (or compensation point) writing - if material has a temperature dependentcoercive field heat to point where H > Hc, then on cooling H < Hc

    c. MaterialsTypically rare-earth transition metal alloys (RE-TM) RE: Gd, Tb; TM: Fe, Co

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    9Many factors to tune: Tc, Hc, Magnetic anisotropy, reflectivity, Kerr rotation, stability, etc.

    2. Spin Glasses one of the more intriguing new forms of magnetismmay be a new state of matter, maybe notprototypical SG is an alloy, with 1-10% of a paramagnetic impurity (e.g., Fe or Mn) in adiamagnetic metal (e.g. Cu or Au)Spin coupling is mediated through the conduction electrons through the RKKY interaction(Ruderman, Kittel, Kasuya, Yosida) - oscillatory in nature

    This leads to frustration:

    A

    B

    C

    ferromagnetic coupling

    antiferromagnetic coupling

    spin center

    frustrated

    unfrustrated

    unfrustrated frustrated

    A critical consequence of Frustration is a highly degenerate ground state - there areMANY equally probable, equally acceptable combinations of spins

    Therefore, even at 0 Kelvin, many states are populated - novel thermodynamic andmagnetic properties

    Experimentally, the hallmark of a SG is a cusp in the AC susceptibility - defines a criticaltemperature - TSG

    Heat capacity measurements do not reveal the some critical temperatureSG do show remanence and hysteresis effectsSG theory has been adopted to other problems, including:

    combinatorial optimization (traveling salesman) problemsneural networkspre-biotic evolution

    E. MISCELLANY1. Units and fundamental constants

    N = 6.022 x 1023 mol-1

    g = 2.0023

    k = 1.3807 x 10-23 J/K

    B = 9.274 x 10-24 J/TNB2/k = 0.375 emu K/molgB/k = 1.3449 K/TG = g1/2 cm-1/2 s-1

    T = 104 G

    T2 = 10 J/emu2. Saturation behavior of S-only paramagnets

    M = Msat BS(gBH/kT)BS(x) = (1/S)((S + 1/2)x coth(S + 1/2)x - (x/2) coth(x/2))

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    Msat = NgBS= 11.18245 SJ/molT = 1.118245 x 104 S emuG/mol3. Curie Law for paramagnets

    M = H

    T = C =Ng2

    B2 S(S+1)

    3k= 0.125g2S(S+1) emuK/mol

    eff= (g2S(S+1)1/2 = (8T)1/2

    4. Relation between saturation and Curie behaviors

    C emu K( )

    Msat

    emu G( )=

    Ng2B2 S(S+1)

    3kNgB

    S=

    gB

    (S +1)

    3k=

    2.00239.274x10 28 J/ G

    31.3807x10 23 J / K(S +1) = 4.4831x10 5 K

    G(S +1)

    F. MAGNETIC DIMERS THE HEISENBERG-DIRAC-VAN VLECK HAMILTONIAN1. Introduction

    In section C.2 we examined primary magnetochemistry relationships for paramagnets

    species with non-interacting spins. The magnetic properties of such materials can be describedby the Curie-Weiss law (for small values of H/T), or more generally by:

    M = NgBSBS

    However, in the next simplest case a molecule with two exchange-coupled unpairedelectrons the magnetic properties cannot usually be described by this relation except at verylow temperatures. This will be the case when the exchange coupling creates thermally accessiblestates of different spin multiplicity. Such is the case for most organic biradicals.

    The Heisenberg-Dirac-Van Vleck (HDVV) Hamiltonian, eq 1, is an empirical operator thatmodels interaction (coupling) of unpaired electrons. The form of the Hamiltonian suggests that

    coupling arises through interaction of spin angular momentum operators. The magnitude of theinteraction depends on the interaction parameter, Jij (called the exchange parameter). The Jijterm embodies all of the interactions that determine the ground state spin preference. Theproduct of spin operators is a reasonable component since interaction of species containingunpaired electrons results in either a decrease (antiferromagnetic coupling) or increase(ferromagnetic coupling) in spin angular momentum. For example, two doublets can couple toyield a singlet and a triplet, the relative energies of which depend on Jij. By definition, forferromagnetic (high-spin) coupling Jij > 0, while for antiferromagnetic coupling, Jij < 0.

    Hij

    = 2Jij

    SiS

    j(1)

    The product of spin angular momentum operators may be expressed in terms of component

    and product (total) spin angular momentum operators,

    STot2 = S

    i+ S

    j

    2

    = Si2 + S

    j2 + 2S

    iS

    j(2)

    therefore, SiS

    j= 1

    2S

    Tot2 S

    i2 S

    j2

    (3)

    Since the eigenvalue ofS2 is S S +1( ) , the energy of the state with spin STot

    resulting from

    interaction of species with spins Si

    and Sj

    is given by,

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    11

    ETot

    = Jij

    STot

    STot

    +1( ) S i S i +1( ) Sj Sj +1( )[ ] (4)

    Thus for two doublets (2 x multiplicity 2 = 4 states), coupling results in a triplet and a singlet(multiplicity 3 and multiplicity 1 = 4 states). In the case of ferromagnetic coupling (J > 0), theenergy of the triplet state (S = 1) is,

    ET = J 11 +1( ) 12

    12 +1( ) 12 12 +1( )[ ]= J 2 34 34[ ] = J2 (6)

    The energy of the singlet state (S = 0) is,

    ES

    = J 0 0 +1( ) 12

    12

    +1( ) 1212

    +1( )[ ] = J 0 34 34[ ] =

    3J

    2(7)

    The singlet triplet gap, EST, is given by,

    EST

    = ES

    ET

    = 3J2

    J2( ) = 2J (8)

    The energy level diagram for ferromagnetic coupling is shown below.

    S = 1/2S = 1/2

    Triplet, S = 1

    Singlet, S = 0

    EST

    The energy level diagram for antiferromagnetic coupling is shown below.

    S = 1/2S = 1/2

    Triplet, S = 1

    Singlet, S = 0

    EST

    Note that by definition of the Hamiltonian, J< 0 describes antiferromagnetic coupling and J> 0. Had we defined the Hamiltonian as Hij = 2J ijSiSj , then J < 0 would be for

    ferromagnetically coupled spins. Therefore, when reading the literature, always note the form ofthe Hamiltonian to be sure of the nature of the type of exchange coupling.

    2. Measuring Jby Electron Paramagnetic Resonance SpectroscopyThe intensity of the EPR signal is directly proportional to the paramagnetism which can be

    given by the Curie Law,

    IEPR

    = CT

    (9)

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    12

    Although the paramagnetism of the triplet follows the Curie Law, the concentration of tripletis temperature dependent and is given by the Boltzmann distribution,

    nT

    nT

    + nS

    = TRIPLET[ ] rel =

    3exp

    T

    RT

    3exp

    T

    RT

    + exp

    S

    RT

    (10)

    Multiplication of the numerator and denominator by exp

    S

    RT

    , and letting T - S = EST gives,

    TRIPLET[ ] rel =

    3expE

    ST

    RT

    1 + 3expE

    ST

    RT

    (11)

    Thus, the EPR signal intensity is given by,

    IEPR

    = CT

    TRIPLET[ ] rel =CT

    3expE

    ST

    RT

    1 +3expE

    ST

    RT

    (12)

    A plot of EPR signal intensity versus 1/T for different singlet-triplet gaps is shown below. Notethat very little change in the slope of the plot occurs as the triplet becomes more stable.

    0

    0.05

    0.1

    0.15

    0.2

    0.25

    0

    IEPR

    0.1275 0.255 0.3825 0.51

    E = 50 cal

    E = 20 cal

    E = 10 cal

    1/T (1/K)

    EPR Signal Intensity vs 1/ T for Several Values of ETS

    E = 5 cal

    E = -5 calE = -10 cal

    E = -20 cal

    E = -50 cal

    3. Measuring Jby Magnetometry1

    Van Vleck derived a general equation for calculating paramagnetic susceptibility as a

    function of temperature.2 Use of the equation requires knowledge of the energy levels, whichwe calculate with the HDVV Hamiltonian (see previous section). Van Vleck began the

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    13derivation by letting the energy levels of the system be developed as a power series expansion inthe applied field.

    E n = E n0 + HEn

    (1) + H2E n(2) + H3E n

    (3) +... (13)

    The term which is independent of H is the zero-order term (and has units of J, the exchangeparameter), while the term linear in H is the first-order Zeeman term, and the term that scales as

    H2

    is the second-order Zeeman term, and so on. Neglecting Zero-field splitting, and assumingisotropic g, the total magnetic moment, M, for the system is:

    M = Nn exp E n kBT( )n

    exp E n kBT( )n(14)

    Where n is the magnetic moment of state n (n = - En/H). Now,

    exp

    E nkBT( ) = exp

    En0 + HE

    n(1) + H2E

    n(2) +...( )

    kBT

    = expE n

    0

    kBT

    expHE n

    (1)

    kBT

    ... (15)

    Ignoring H2 and higher-order exponentials, and recalling that for small x,

    exp(x) 1 xThen,

    expE n

    kBT( ) = expE n

    0

    kBT

    exp

    HE n(1)

    kBT

    ... 1

    HEn(1)

    kBT

    exp

    E n0

    kBT

    (16)

    (This assumes that first-order Zeeman splitting is much smaller than exchange coupling.) and,

    n = E nH

    = E n(1) 2HE n

    (2) +... (17)

    From the approximation and substitution we obtain,

    M = N

    En(1) 2HE

    n(2)( )

    n 1

    HEn(1)

    kBT

    exp

    En0

    kBT

    1HEn

    (1)

    kBT

    exp

    En0

    kBT

    n

    (18)

    If we limit the derivation to paramagnetic substances, such that M=0 at H=0, then

    E n(1)

    expE n

    0

    kBT

    n = 0 (19)

    Retaining only terms linear in H, and ignoring second-order energy terms, we obtain,

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    14

    M = NH

    En(1)( )

    2

    kBTn exp

    E n0

    kBT

    expE

    n0

    kBT

    n

    (20)

    Since =M/H, then

    = N

    En(1)( )2

    kBTn exp

    E n0

    kBT

    expE

    n0

    kBT

    n

    (21)

    Recall that,

    E n(1) = msg B and ms

    2

    S

    +S = 1

    3S S +1( ) 2S +1( ) (22)

    and adding degeneracy terms gives,

    =Ng2

    B2

    3kBT

    S S +1( ) 2S +1( )S exp ES kBT

    2S +1( )expE

    SkBT

    S

    (23)

    Plugging in the constants gives,

    =0.125g2emuK / mol

    T

    S S+ 1( ) 2S +1( )S expE

    S kBT

    2S +1( )expE

    SkBT

    S

    (24)

    Where ES is the energy of the exchange-coupled spin states determined using the HDVVHamiltonian. The energies of the states (in units ofJ) are relative to the lowest state, which istaken as zero. The denominator can be modified according to the Curie-Weiss law to give:

    = 0.125g2

    emuK/molT( )

    S S+1( ) 2S+ 1( )S

    exp ESkBT

    2S+1( )expE

    SkBT

    S

    (25)

    Below are plots of T vs T for = -0.01 K and -500 cm-1J +500 cm-1.

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    15

    0

    0.2

    0.4

    0.6

    0.8

    1

    0 500 1000 1500 2000 2500

    -500-250-150-50-10-5+5+10+50+150+250+500

    paraT(emuK

    /mol)

    Temperature (Kelvin)

    Below are plots of vs T for = -0.01 K and -500 cm-1J +500 cm-1. Note that forferromagnetic coupling, increases asymtotically as the temperature is lowered, while for

    antiferromagnetic coupling, exhibits a maximum at Tmax.

    0

    0.001

    0.002

    0.003

    0.004

    0.005

    0 500 1000 1500 2000 2500

    -500-250-150-50-10-5+5+10+50+150+250+500

    para

    (emu/mol)

    Temperature (Kelvin)

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    16The exchange coupling parameter is related to Tmax by:

    |J| = 0.8 kTmax (26)

    Thus, a maximum in the plot of vs. T is the signature of antiferromagnetic coupling.

    References1)Kahn, O.Molecular Magnetism; VCH: New York, 1993.

    2)Van Vleck, J. H. The Theory of Electric and Magnetic Susceptibilities; Oxford UniversityPress: Oxford, 1932.