Does There Exist Only One Solution of the Dyson-Schwinger Equation for the Quark Propagator in the Case of Non-Zero Current Quark Mass


    C H IN .P H Y S.L E T T V o1.22N o.12 (2005)3036
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    It is sh o w n o n g en era l g ro un d th a t th er e ex ist tw o q ua lita tiv ely d is tin ct so lu tio n s of th e D y son S ch w in g er eq u a tion
    for th e q u ark p rop a ga tor in th e case o f n on —z ero c urren t q ua rk m a ss .O n e so lu tion c orresp on d s to th e 'N am b u —
    G olds ton e’’p h ase an d th e o th er on e corresp on d s to th e W ig n erp h ase in th e ch ira l lim it.
    P A C S : 1 1 .1 5 .T k 1 2 .3 8 .A w 12 .3 8 .L g 12 .3 9 . x
    It is g e n era lly b e liev ed th a t w ith in crea sin g t em —
    p e ra tu re a n d b a ry o n n u m b er d e n sity th e h a d ro n ic
    m a tte r u n d e rgo es a p h a se tran sitio n to th e q u ark ——
    gluon plasm a (q c P ) w hich is expected to appear in
    u ltra reia tiv istic h e av y io n co llisio n s.T h ese tw o p h a ses
    a re g en era lly refe rred to a s th e N a m b u — G o ld sto n e
    p hase fch aracterized by d yn am ical ch iral sym m etry
    b reaking and con fin em ent of d ressed quarks) and th e
    W ignerphase (corresponding to Q G P w here chi—
    r al sy m m etry is resto red a n d q u a rk s a re n o t co n fi n e—
    m ent1.T heoretically th ese tw o p hases are describ ed
    by tw o d ifi erent solu tion s fth e N am bu G old ston e
    a n d th e W ig n e r so lu tio n of th e q u a rk p ro p a g a —
    to r an d th e ex iste n ce o f th e se tw o so lu tio n s in th e
    ch ira l lim it h a s b ee n rig o ro u sly p ro v en in th e fra m e—
    w ork of D ysonSchw inger equation (D SE ) approach
    of Q C D .H ow everit is a general view in th e litera—
    tu re th a t w h en th e c u rren t q u a rk m a ss is n o n —ze ro
    th e D y so n S ch w in g er eq u a tio n fo r t h e q u ark p rop a —
    g a to r h a s o n ly o n e so lu tio n w h ich c o rre sp o n d s to th e
    N a m b u — G o ld sto n e p h a se .w h ile th e so lu tio n co rre—
    sp o n d in g to th e W ig n e r p h a se d o e s n o t ex ist
    H o w ev era s fa r a s w e k n o w th is cla im h a s n ev er b e en
    p ro v ed .D o e s th ere rea lly ex ist on ly o n e so lu tio n of th e
    D y so n S ch w in g er eq u a tio n fo r th e q u a rk p ro p a g a to r
    in th e ca se o f n o n —z ero c u rren t q u a rk m a ss
    In or d e r to in v e stig a te th is p ro b le m .1et u s fi rst re—
    ca ll th e u su a l a rg u m en ts w h ic h ex c lu d e th e ex iste n c e
    o f th e W ig n e r so lu tio n o f th e D y so n S ch w in g er
    e q u a tio n fo r th e q u a rk p ro p a g a to r in th e ca se of n o n
    z ero cu rren t q u a rk m a ss . T h e D S E sa tisfi e d b y th e
    q u a rk selfen erg y is
    X (pm )

    d 4q
    夕 2 ab (
    7ut9 (qm ) (pq) (1)
    w here 夕 2 a b(p) and (pg) are the fullnonp er·
    tu rb a tiv e g lu o n p ro p a g at or a n d th e q u a rk ·g lu o n v e r’
    te x re sp ect iv e ly a a n d b a re th e c o lo u r in d ic es w ith
    t: f0r the standard G ellM ann SU (3) represen 0
    tationand is the current quark m ass.
    T he quark propagator 9 (pm ) and the quark self
    energy X (pm ) are related by
    9 (pm ) 三io'·P + m + X (pm )
    i7 .pA (p )+ (p )+ m (2)
    w here A (p ) and S (P ) are the quark self energy func—
    tio n s in th e c a se o f n o n .zer o cu rre n t q u a rk m a ss.If m
    is set to be zero9 (pm ) goes into the dressed quark
    propagator in the chiral lim it G (p) 三 9 (pm 0)
    w h ich h a s th e d ec o m p o sitio n
    G (p)三i7 .P + X (P仇 0) i7 ·pA (p )+ B (p)
    In order to handle E q.(1) it is necessary to m ake
    ce rta in sim p lifi ca tio n s a n d tru n ca tion s . O n e c o m —
    m only used truncation of E q.(1)called the rainbow
    a p p ro x im a tio n in v o lv es rep la cin g th e fu ll v e rt ex in
    Eq.(1) by the bare vertex
    (pq)
    In th is ca se th e q u a rk selfen erg y fu n c tio n s
    B (p )are determ ined by the rainbow D SE
    ra l lim it:I1— 3
    [A (p )1]p 4
    3 /. y s J /(2丌)
    (4)
    A (p)and
    in th e ch i.
    S u p p o r te d in p a rt b y t h e N at io n a l N a t u ra l S c ie n c e F o u n d a tio n o f C h in a u n d e r G ra n t N o s 1 0 17 5 0 3 3 1 0 1 3 5 0 3 0 a n d 1 0 5 7 5 0 5 0
    a n d th e R es e a rc h F u n d fo r t h e D o ct o r a l P ro g r a m o f H ig h e r d u c a t io n u n d er G r a n t N o 2 0 0 3 0 2 8 4 0 0 9 .
    E m ail:z0n gh s@ ch enw an g .n ju .edu .cn
    ⑥ 200 5 C hin ese P hy sical S ociety a nd IO P P ub lish in g L td
    维普资讯 httpwwwcqvipcom
    N o .12 Z O N G H o n g —S h i e t a l 3 0 3 7
    A (q)
    qA (q) + B (q)
    lP ·q + 2 L P ·(P — q)q ·(P — q)
    (P — q)
    B∽4/ d4q 2(p'q)
    B (q) qA (q)+ B (q)’ (5)
    w h ere w e h a v e u se d L a n d a u g a u g e .It is rea d ily seen
    that B (p ) in E q.(5)has tw o qualitatively distinct so—
    lu tio n s .T h e N a m b u — G o ld sto n eso lu tio n .fo r w h ich
    B (p ) ≠ 0describes a phasein w hich (1) chiral
    sy m m etry is d y n a m ic ally b ro k en .b eca u se o n e h a s a
    n onzero qu ark m ass fun ction and f21 th e dressed
    qu a rk s a re co n fi n ed b e ca u se th e p ro p ag a to r d e scrib e d
    b y th e se fu n ctio n s d o es n o t h av e a L e h m a n n rep —
    re sen ta tio n . T h e o th er so lu tio n .th e W ig n er on e .
    B (p ) 三0describ es a phasein w hich the chiral sym —
    m etry is n o t b ro k en a n d th e d ressed —q u a rk s a re n ot
    confined.[23H ow everw hen 仇 ≠ 0the selfenergy
    functions A (p ) and S (p) are determ ined by the fol—
    lo w in g ra in b ow D S E :
    )'l 罟/ g2~D(p—q) (q) q (q)+[ (q)+m
    IP ·q + 2 P ·(P — q)q ·(P — q)
    (P — q)
    (p):4 t/.研d4q 2(p
    (q)+ m q (q)+ [ (q)+ m (6)
    Com paring E q.(6) w ith Eq.(5)it is apparent that
    (p2) 三 0 is not a solution to E q.(6). From this
    ob serv a tio n o n e o ften co n c lu d e s th a t in th e c a se o f
    non—zero current quark m ass E q.(6) has only one so—
    lution (B (p ) ≠0)w hich corresponds to the N am bu—
    G o ld sto n e p h a se in th e ch ira l lim it.w h ile th e so lu tio n
    co rresp o n d in g to th e W ig n er p h a se sim p ly d o es n o t
    ex ist. It sh o u ld b e n o ted th a t in o b ta in in g th is co n —
    clu sio n o n e h a s a ssu m e d th a t th e d re ss ed g lu o n p ro p —
    a ga to rs in th ese tw o p h a ses a re th e sa m e . H o w e ve r
    sin ce th e fe a tu res o f th ese tw o p h ase s ar e so d iff ere n t
    it is re a son a b le to e x p ect th a t th e b e h a v io u r o f th e
    d resse d g lu o n p ro p a g a tors in th e se tw o p h a ses s h o u ld
    also b e di ren t.In ad dition .th e fa ct that g (p 1 三0
    is not a solu tion to E q .f61 does n ot necessarily m ean
    that there exists only one solution ( (p ) ≠ 0) fo r
    Eq.(6). A s is show n in the fo llow ingthere do ex—
    ist tw o qualitatively distinct B (p ) ≠ 0 solutions in
    Eq.(6). .
    In o rd e r to d em o n stra te th is p o in tle t u s sep a —
    ra te t h e co n trib u tio n s o f d y n a m ica l a n d ex p licit ch ira l
    sym m etry breaking (driven by current quark m ass m )
    ex p lic itly .B y d iff e ren tia tin g th e d re sse d q u a rk p ro p —
    agator 9 (Pm ) w ith respect to 仇w e find that the
    d resse d q u ark p ro p a g a to r is rela ted to th e v ertex fo r
    th e sca lar o p e ra tor q b y
    (pm ) —a0 1(p m )
    In te g ra tin g th is eq u a tio n w e h a v e
    01(pm) 9 (Pm + 厂 (p0m m
    0
    G (p)+ 9云 (pm ) (8)
    w here G (p)an integration constantis the contri—
    b u tio n of d y n a m ic al ch ira l sy m m etry b re ak in g a n d is
    independent ofthe current quark m ass m 9云 (Pm )is
    th e c o n trib u tio n o f ex p licit ch ira l sy m m e try b reak in g
    a n d v a n ish e s if t h e c u rren t q u a rk m a ss 仇 e q u a ls z ero .
    W ithout loss of generality9 (Pm ) can be w ritten
    a S
    9云 (pm ) m [i~/·pE (p)+ F (p). (9)
    Substituting E qs.(8) and (9)into Eq.(2)w e have
    A (p) 三A (p)+ m E (p)
    (p) 三B (p)+ m F (p)m
    P utting E q.(10) into E q
    fled by E (p) and F (p)
    (6)w e have the D SE satis—
    B(p2)+m )m4/研d4q 2(p'q)
    B (q)+ m F (q)
    q2[A (q)+ m E (q)+ [B (q) + m F (q)’
    [A (p) + m E (p) lip
    4 I d4q
    3 (27r)
    g2D (p — q)[A (q) + m E (q)
    q2[A (q)+ m E (q)+ [B (q)+ m F (q)
    p.q+2 ]
    w here A (p ) and B (p ) are determ ined by E q.(5).
    For a given m odel gluon propagator g J[)(p)w e
    can solve consistently E qs.(5) and (1 1) to obtain the
    four scalar functions A (p)B (p)E (p)and F (p).
    In the treatm ents of the previous literature[1—6] one
    o fte n a d o p ts th e sa m e fo rm o f th e m o d e l g lu o n p ro p —
    a g a to r a s in p u t to so lv e fo r th e se sc a la r fu n ctio n s co r—
    r esp on d in g to d ifi eren t p h a ses . A s w a s p o in ted o u t
    b e fo re th is is p ro b lem a tic .T h e co rrect w ay is to u se
    d iff eren t m o d el g lu o n p ro p ag a to rs as in p u t in so lv in g
    fo r different phases.To be specificwe use g~D (p — q)
    to d e n o te th e d re ssed g lu o n p rop a g a to r in th e N a m b u
    G oldstone phase and g82 J[) (p — q) to the dressed gluon
    p ro p a ga to r in th e W ig n e r p h a se .
    A s is sh o w n a b o v e th ere ex ists tw o so lu tion s
    to E q.(5)i.e. the N am bu—G oldstone solution
    1 ●● ●● J
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    3 0 3 8 Z O N G H o n g —S h i e t a l V o 1.2 2
    (B (p) ≠o) and the W ignersolution (B (p) 三0).
    Substituting these two solutions into Eq.(11)w e can
    obtain tw o different solutions for E (p) and F (p).
    For exam plesubstituting B (p) 三 0 and the m odel
    gluon propagator g D (p q)into E qs.(5)and (11)w e
    have the W ignersolution A )E ) and F (p)
    an d
    [A (p)1]p d4q 2
    D'(p_q)[p.q
    — q) q ·(P — q)]
    (p — q) J q2A '(q)’ (12)
    p)14/ d4q g p_q)
    F (q)
    q[A (q)+ m E (q)]+ [m F (q)]
    (p)+ (p)_1]p2 4/ d4q
    g D (p — q)[A (q) + m E (q)]
    q[A (q) + m E (q)]+ [m F (q)]
    p.q+2 ].(13
    S o fa r at th e ra in b o w a p p rox im a tio n to th e D S E
    w e h a v e co m p le ted th e d e riv a tio n o f th e d ep en d e n c e
    of (Pm ) on m in the N am buG oldstoneand
    W ig n erp h a se s sep a ra tely
    (ⅣG) (pm ) i7 .P A (p)+ B (p)
    + m [i~/·pE (p)+ F (p)]fo r B (p) ≠0
    (14)
    ( ) (p m ) i7 .P A (p)+ m .pE (p)
    + F(p)1 for B(p)≠0. (15) J
    Just as is show n by E qs.(14)(15)there does exist
    tw o qualitatively distinct solutions w ith ( ) ≠ 0 in
    th e c ase o f n o n —ze ro c u rren t q u ark m a ss .In a d d itio n
    w e w a n t to stress th at th e a b o v e a p p ro a ch is g en e ra l
    in th e sen se th at it d o es n o t d ep e n d o n th e ra in b ow
    a p p rox im a tio n u se d h e re . It ca n a lso b e a p p lied to
    th e c ase o f th e B a ll C h iu [71 an d C u rtis— P en n in g to n [ l
    v e rtice s.
    In o rd e r to h av e a q u a lita tiv e u n d ersta n d in g o f th e
    a b o v e tw o q u a lita tiv e ly d istin c t so lu tio n s a p a rtic—
    u la rly sim p le an d u sefu l m o d el o f th e d re ssed g lu o n
    tw o —p o in t fu n ctio n [9j in th e N a m b u ~G o ld sto n e p h a se
    is e m p lo y ed :
    g D (p — q) 47r 町
    ( )(P — q)
    (P ~q) (p ]
    (P — g)
    w h e re th e sca le p a ra m eter r/ is a m e a su re o f th e
    stre n g th o f th e in fra red slav ery eff ec t. T h is m o d e l
    h a s th e a d v a n ta g e th a t th e in teg ra l eq u a tio n o f D S E
    re d u c es to alg e b ra ic eq u a tio n s.
    H e re w e sh o u ld also sp ec ifv t h e d ressed g lu o n tw o —
    p o in t fu n c tio n in th e W ig n er p h ase . 昭 h av e n o a p ri·
    or i k n ow le d g e o f th is fu n c tio n e x ce p t th at it sh o u ld b e
    d ifrere n t fro m th e o n e in th e N a m b u G o ld ston e p h a se .
    In o rd er to sh o w th a t th e re d o e x is t tw o q u a lita tiv ely
    d istin c t so lu tio n s o f th e D y so n ——S ch w in g er eq u a tio n fo r
    th e q u a rk p ro p a g a to r in th e c as e o f n o n —ze ro c u rren t
    q u a rk m ass w e c h o o se th e fo llow in g a n sa tz
    gD (p — q)4丌 町 5
    . ( )(P — q)
    (P — g) g)
    (P — q)0
    w ith a sca le p a ra m e ter r/ d iff e ren t fro m 町.H ere w e
    em p h a size th a t w e ch o o se th e a b o v e an sa tz o n ly fo r
    co n v en ien ce a n d th is w ill n o t aff ect o u r m a in co n clu —
    sio n .
    Substituting E q.(16) into E q.(5)w e have the
    N a m b u — G o ld sto n e so lu tio n in ch ira l lim it
    8 (p) (町~4p)
    A (p) 2 fo r P<
    B (p) 0
    叩2
    4
    ( +
    Sim ilarlysubstituting E q.(17)into E q.(12)w e have
    th e W ig n e r so lu tio n in ch ira l lim it
    B (pz)三A (pz): 1[1+(1+2pr/2/~ ].(19)
    W ith th e m o d el o f th e d res sed g lu o n p ro p a g ato r
    specified in E qs.(16)and (1 7)and the explicit expres—
    sion fo r A (p)B (p)and A (p)given in E qs.(18)and
    (19)E qs.(11)and (13)entail that the scalar functions
    u (p) and F (p) satisfy
    A (p)+ rnE (p) 2[B (p)+ m F (p)
    B (p)+ m F (p) + m
    +mFcp m { 竽
    +[B(p)+mF(p)])町 (20)
    and the scalar functions E (p) and F (p) satisfy
    A (p)+ m E (p)
    )1]{ +rn2F'( )
    8
    1

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    2 p
    r
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    l 2
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    N o .1 2 Z O N G H o n g —S h i e t a l 3 0 3 9
    U sin g M a th e m a tica it is n o t d iffi cu lt to v e rify th at th e
    solutions of E q s.(20) an d f2 1) do ex ist.T h e fuU ex—
    pressions for E (p )F (p)E (p)and F )are too
    len g th y a n d w ill n o t b e g iv en in th is stu d y .It sh o u ld
    be noted that the m odel gluon propagator (16) is an
    in fra red —d o m in a n t m o d e l th a t d o es n o t rep re sen t w e ll
    the behaviour of g J[) (p) aw ay from P 0.N ev—
    erth elessth is sim p le m o d el ca n p ro v id e a rea so n ab le
    g u id e to th e n o n D e rtu rb ativ e p rop erties o f m ore so —
    p h istic ate d D S E —m o d el o f O C D .
    In su m m a ry w e sh o w on g en era l g ro u n d th at th e re
    ex ist tw o q u alita tive ly d is tin ct so lu tio n s o f th e D y son ——
    S ch w in g er eq u a tio n fo r th e q u a rk p ro p ag a to r in th e
    case of non—zero current quark m ass (one of w hich
    co rresp o n d s to th e N a m b u ——G o ld sto n e p h a se a n d th e
    oth er c o rresp o n d s to th e W ig n er p h a se in th e ch ira l
    lim it).T h is app roach h as the a dvan tage th at w e can
    a n aly se th e effect s of ex p lic it a n d d y n am ic a l ch ira l
    sy m m etry b rea k in g se p a ra tely . T h e b a sic e q u a tio n s
    u sed here are E q s.f5) an d f11).In order to have a
    q u a lita tiv e u n d e rs tan d in g o f th e a b o v e tw o q u a lit a
    tiv ely d istin ct so lu tio n s w e ch o o se a sim p le co n fi n —
    ing m odel (16) in solving E qs.(5) and (11). From
    th is th e d re sse d q u ar k p ro p a g a to r in th e N am b u
    G o ld ston e p h a se an d th e W ig n e r p h a se are d erive d .
    W ith th ese tw o p h a ses ch a ra cte riz ed b y q u a lita —
    tiv e ly d iff e ren t m om en tu m —d ep en d en t q u a rk p ro p a g a
    torsone can stud y th e Q C D p hase stru ctu re in a d ef
    in ite w a y .
    R e fe r e n c e s
    1C ahill R T and R oberts C D 1985 P hysR D 32 2419
    [2] T andy P C 1997 P rog.P art. N uc1.P hys.39 1 17 and
    re fe re n c es t h e r ein
    l3 l R ob erts C D a nd W illiam s A G 1994 P rog.尸art. Ⅳcf.
    P h y s .3 3 4 7 7 a n d re fer e n c e s t h er ein
    [4] R oberts C D and Schm idt S M 2000 P rog.P art.肌 cf.
    P h y s .4 5 S 1 1 a n d re fere n ce s t h e re in
    [5] Zong H SP ing J L Y ang H T L x F and W ang F 2003
    P h y s .R e u .D 6 7 0 7 4 0 0 4
    Z on g H S Q i S C h en W S un W M a nd Z hao E G 200 3
    P h y s .L ett.B 5 7 6 2 8 9
    Y a n g H T Z o n g H S P in g J L a n d W a n g F 2 0 0 3 P h y s .
    L e tt.B 5 5 7 3 3
    [6] Zong H SC hang L H ou F Y Sun W M and Liu Y X 2005
    P h y s .R e u .C 7 1 0 1 5 2 0 5
    Z o n g H S H o u F Y S u n W M P in g J L a n d Z h ao E G
    2 0 0 5 P h y s R e .C 7 2 0 3 5 2 0 2
    H o u F Y C h a n g L S u n W M Z o n g H S a n d L iu Y X 2 0 0 5
    P h y s .R e .C 7 2 0 3 4 9 0 1
    7l B all J S and C hiu T W 1980 P hys.R eu.D 22 2542
    [8l C urtis D C and Pennington M R 1990 Phys.R eu.D 42
    4 1 6 5
    9I M unczek H J and N em irovsky A M 1983 P hys.Reu.D 28
    8
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