Tensor Models for Black Hole Probe

Size: px
Start display at page:

Download "Tensor Models for Black Hole Probe"

Transcription

1 Tensor Models for Black Hole Probe IAP, Paris, 15th Workshop on Non-Perturbative Quantum Chromodynamics June 12, 2018 Swapnamay Mondal LPTHE, UPMC(Sorbonne Université) (based on arxiv: with Nick Halmagyi)

2 Summary Recently there have been models of near extremal black holes (and possibly examples of NAdS_2/NCFT_1). Such black holes Hawking radiate. Model for a probe interacting with such black holes? We propose a class of tensor models as models of black hole interacting with a probe. Non- trivial features: symmetries of near horizon geometry, black hole (partially) inflicts maximal chaos into the probe.

3 Outline Introduction Our Model Future directions

4 Introduction

5 Near-extremal black holes A. Pattern of symmetry breaking: Near horizon geometry of extremal black holes contains a AdS_2 factor. Near horizon geometry of near-extremal black holes contains a near-ads_2 AdS_2 => Asymptotic symmetries are all reparameterizations of asymptotic boundary circle, but AdS_2 metric preserves only a SL(2, R) subgroup of this. => Spontaneous breaking of reparameterization to SL(2,R). Near AdS_2 => spontaneous and explicit breaking of reparameterization symmetry. B. Maximal Chaos: (Non-extremal) black holes are maximally chaotic systems. explicit breaking of reparameterization symmetry should be related to maximal chaos.

6 <latexit sha1_base64="jrwog46q3nkbz2m79o6iz0w3c9i=">aaacohicbvdlsgmxfm3uv62vqks3wsj1vwdqqtdcszuiobx6gryomttthmyejbmhhpksn36go3hjqhg3fohpa7xva4fzz7mxm3uckfehtfpjscwsli2vjfdta+sbm1vp7z26cckosq0hlobnbwncqe9qkkpgmienyhmyatid0shv3beuaobx5takhq/1fopsjksw7pr12val6mu1hmew7xke1uwscle36vgoh8ewhqpqk+tgh5rf2e8i68wuwrzb6yyzm8eaf4k1jrkwrcvop7a7ay484kvmkbatywxlryeukwyktrujqukeb6hhwpr6ycoio8ahx/bak13oblw/x8kx+ntciu+ioefotg/jvpj3ruj/xius7mlhut+mjphxzjebmsgdoeordiknwlkhjghzqv8kcr/p+ktooqvdsozp/kvq+zxl5qybqqz4po0jcfbapjgefjgbrvagfvadgnydz/ak3owh48v4nz4mrqljormlzmb8fgguc6uv</latexit> <latexit sha1_base64="jrwog46q3nkbz2m79o6iz0w3c9i=">aaacohicbvdlsgmxfm3uv62vqks3wsj1vwdqqtdcszuiobx6gryomttthmyejbmhhpksn36go3hjqhg3fohpa7xva4fzz7mxm3uckfehtfpjscwsli2vjfdta+sbm1vp7z26cckosq0hlobnbwncqe9qkkpgmienyhmyatid0shv3beuaobx5takhq/1fopsjksw7pr12val6mu1hmew7xke1uwscle36vgoh8ewhqpqk+tgh5rf2e8i68wuwrzb6yyzm8eaf4k1jrkwrcvop7a7ay484kvmkbatywxlryeukwyktrujqukeb6hhwpr6ycoio8ahx/bak13oblw/x8kx+ntciu+ioefotg/jvpj3ruj/xius7mlhut+mjphxzjebmsgdoeordiknwlkhjghzqv8kcr/p+ktooqvdsozp/kvq+zxl5qybqqz4po0jcfbapjgefjgbrvagfvadgnydz/ak3owh48v4nz4mrqljormlzmb8fgguc6uv</latexit> <latexit sha1_base64="jrwog46q3nkbz2m79o6iz0w3c9i=">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</latexit> <latexit sha1_base64="jrwog46q3nkbz2m79o6iz0w3c9i=">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</latexit> Tensor models for near-extremal black holes Certain tensor models exhibit the same pattern of symmetry breaking and maximal chaos, in large N limit and deep IR. Simplest such tensor model is Carozza-Tanasa-Klebanov- Tarnopolsky (CTKT) Model H CTKT = abc J 4N 3/2 is a real fermion. a,b,c = 1,,N abc ab 0 c 0 a 0 bc 0 a 0 b 0 c

7 Two point function in CTKT Model Simplest leading correction to free propagator Replace any propagator by the above diagram

8 Two point functions in CTKT model (contd.) Schwinger Dyson eqn: large N ) (t 1,t 2 )=J 2 G(t 1,t 2 ) 3 1 deep IR ) G(!) = i! (!) Z large N and deep IR ) J 2 dt G(t 1,t)G(t, t 2 ) 3 = (t 1 t 2 ) Reparameterization symmetry: G(t 1,t 2 )! df (t 1) dt 1 df (t 2 ) dt 2 1/4 G(f(t1 ),f(t 2 )) spontaneously broken down to SL(2,R) by solution G(t) = 1 sgn(t) (4 J 2 ) 1/4 t 1/2

9 Four point functions in CTKT model connected four point function 1 N 6 h abc(t 1 ) abc (t 2 ) a0 b 0 c 0 (t 3 ) a0 b 0 c 0 (t 4 )i = G(t 1,t 2 )G(t 3,t 4 )+ 1 N 3 F(t 1,t 2 ; t 3,t 4 ) Z F n+1 K F n where K = commutes with SL(2,R) gen. F =(1+K + K )F 0 = 1 1 K F 0 K has an eigenvalue 1, when evaluated in conformal limit. For this eigenspace, K must be evaluated away from conformal limit, thus reparameterization symmetry is explicitly broken.

10 Spectrum of primaries K commutes with SL(2,R) generators. Utilise conformal symmetry: F(t 1,t 2 ; t 3,t 4 )=G (t 12 )G (t 34 )F( ), where = t 12t 34 t 13 t 24 In the limit! 0, F( ) primary of dimension h n ) bulk scalar of mass m 2 n = h n (h n 1) NOT a sparse spectrum. No truncation to SUGRA expected. (see , for discussion on holographic dual) 1X m=1 c 2 m h m

11 A Tensor Model for Black Hole Probe

12 Guessing a probe model Had these tensors been matrices, (which they are not), one would think of the black hole as a bound state of D0 branes and them matrices describing strings stretched between D0 branes. An external D0 brane would be a probe. probes would be described by vectors. Naive tensor analog: probes could be tensors of lower rank.

13 Desirable properties for the Black Hole Probe Probe does not affect the black hole dynamics to leading order. Emergent reparameterization symmetry and the pattern of its breaking should be intact. non trivial because this symmetry is not visible in the Lagrangian. Infliction of maximal chaos.

14 <latexit sha1_base64="pua2idvegsfwpvnx+t6dk5iis7y=">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</latexit> <latexit sha1_base64="pua2idvegsfwpvnx+t6dk5iis7y=">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</latexit> <latexit sha1_base64="pua2idvegsfwpvnx+t6dk5iis7y=">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</latexit> <latexit sha1_base64="pua2idvegsfwpvnx+t6dk5iis7y=">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</latexit> Our Model removing an open line do not change the N dependence. One can go on inserting this diagram in internal propagators to get new leading diagrams. These diagrams can come from a vertex like Above method generates all leading diagrams Suggests the Hamiltonian H = H CTKT + g 1 N 3/2 abc a 0 b 0 capple ab 0apple a 0 b

15 physics intact in large N limit <latexit sha1_base64="17uenevnbgzaf0rc1eqqvr4zn7q=">aaab63icbva9swnbej2lxzf+rs1tfongfe5e0djoyxnbxebyhl3njfmyu3fs7gnhyf+wsvde1j9k579xl7lcex8mpn6bywzelahuro9/e6w19y3nrfj2zwd3b/+genjunngqgbzylgldiahbwrw2llcco4lgkiobj9hknvcfn1abhqsho00wlhsk+jazanoplxjer9b8uj8hwsvbqwpqonmvfvugmuslkssenayb+iknm6otzwjnlv5qmkfsqkfydvrrisbm5rfoyjltbmqya1fkkrn6eykj0pipjfynphzslr1c/m/rpnz4hwzcjalfxralhqkgnib542tantirpo5qprm7lbax1zrzf0/fhrasv7xk2hf1wk8h95e1xk0rrxlo4btoiyaramadnkefdmbwdk/w5knvxxv3phatja+yoyy/8d5/acq/jko=</latexit> Leading contributions to two and four point functions can be obtained by cutting melons. melons are subleading compared to <latexit sha1_base64="qasuf/1ialaqb3i2yf1c2veixku=">aaab7xicbvdlsgnbeoynrxhfuy9ebopgkeykomegf48rzaosjfrojsmy2dlhzlyis/7biwdfvpo/3vwbj8kenlggoajqprsruoib6/vfxmftfwnzq7hd2tnd2z8ohx41tzjqyho0eylur2iy4ji1llectzvmgeectalx7cxvptftecif7esxmmah5ano0tqp2r2jutgrv/yqpwdzjufokpcj3it/dfsjtwmmlrvotcfwlq0z1jztwaalbmqyqjrgies4kjfmjszm107jmvp6zjbov9ksufp7ispymekcuc4y7cgsezpxp6+t2sf1mhgpusskxswapilyhmxej32ugbvi4ghszd2thi5qi7uuojilivh+ezu0l6qbxw3ulyu1mzyoipzakzxdafdqgzuoqwmopmizvmkbl3gv3rv3swgtepnmmfyb9/kdliyphw==</latexit> <latexit <latexit sha1_base64="17uenevnbgzaf0rc1eqqvr4zn7q=">aaab63icbva9swnbej2lxzf+rs1tfongfe5e0djoyxnbxebyhl3njfmyu3fs7gnhyf+wsvde1j9k579xl7lcex8mpn6bywzelahuro9/e6w19y3nrfj2zwd3b/+genjunngqgbzylgldiahbwrw2llcco4lgkiobj9hknvcfn1abhqsho00wlhsk+jazanoplxjer9b8uj8hwsvbqwpqonmvfvugmuslkssenayb+iknm6otzwjnlv5qmkfsqkfydvrrisbm5rfoyjltbmqya1fkkrn6eykj0pipjfynphzslr1c/m/rpnz4hwzcjalfxralhqkgnib542tantirpo5qprm7lbax1zrzf0/fhrasv7xk2hf1wk8h95e1xk0rrxlo4btoiyaramadnkefdmbwdk/w5knvxxv3phatja+yoyy/8d5/acq/jko=</latexit> melons.

16 Propagators New diagrams give subleading contribution to propagators. G (t) = 1 sgn(t) (4 g0 2)1/4 t 1/2 G apple satisfy same (up to constants) Schwinger Dyson equation as G G apple (t) = g 0 g 1 G (t)

17 h i 1 1 h ab (t1 ) ab (t2 ) ab (t3 ) ab (t4 )i = G (t12 )G (t34 ) + 3 F (t1, t2 ; t3, t4 ) 6 N N Diagrams contributing to F are 2 g 1 0 F = 2 F0 1 g1 1 3 K <latexit sha1_base64="2c5xwmqtqi3xnrql43r2nup55gm=">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</latexit> No breaking of conformal symmetry. F ( 1,..., 4 ) = G ( 12 )G ( 34 )F ( ) 1 X 2 e lim F ( ) = e c m hm <latexit sha1_base64="x/7ysxmmoadirygusj8bou+ztfw=">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</latexit>!0 m=1 Primaries of different dimensions, but in natural correspondence with those of the black hole.

18 1 X h 5 N h i 1 F abc (t1 ) abc (t2 ) a0 b0 (t3 ) a0 b0 (t4 )i = G (t1, t2 )G (t3, t4 ) + 3 N F <latexit sha1_base64="kdecz23w6cy7vgs5lfpl1xvzoj0=">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</latexit> 2g0 = 3g1 (1 K K)(1 F0 1 3 K) F ( 2, 2, 3, 4 ) = F ( ) + F conf non conf ( 1, 2, 3, 4 ) G ( 12 )G ( 34 ) 1 h i X e lim Fconf ( )= c2m hm e c2m hm <latexit sha1_base64="kt8spu49ixjc3vg1u1yr/jqlps0=">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</latexit>!0 m=1 primaries of same dimensions appear.

19 e t Chaos Replace position and momenta by general operators and separate two commutators along thermal circle. )h[p(0),q(t)] 2 i e t tr [V (t +3i /4) W (i /2) V (t + i /4) W (0)] This is an Out of Time Order Correlator (OTOC). For us case 1: V =,W = case 2: V = apple,w = apple case 3: V =,W = apple

20 Chaos continues For four point functions are of the form f (K) F= F0 l (1 K) <latexit sha1_base64="g+/objjvd1nsi4u1knnujzbk8i8=">aaacgnicbvdlssnafj34rpuvdelmsajtwpkiobuhkijqtqx7gcawyxtsdp1mwsxekchf4czfcencexfixr9x0mzrww8mhm45l7n3ebgjulnwj7g0vlk6tl7ykg5ube/smnv7lrngapmmdlkooh6shffomooqrjqricjwggl7o+vmbz8siwni79u4im6abpz6fcolpz5powfsq4xycppcs+j4auhel9cravk2t+qvb5bcmujpgj2zzfwtceaisxnsajkapfpl6yc4dghxmcepu7yvktdbqlhmsfp0ykkihedoqlqachqq6sat01j4rju+9eohh1dwos5ojciqchx4opltkee9tpzp68bkv3atyqnyey6nh/kxgyqewu+wtwxbio01qvhqvsveq6tbubrnoi7bnj95kbroq7zvte/osrwrvi4coarhoaxsca5q4by0qbng8arewbt4n56nv+pd+jxgl4x85gd8gfh9c9whn3c=</latexit> corresponding OTOC is maximally chaotic. F, F are maximally chaotic. F turns out to be non-chaotic. <latexit sha1_base64="galvdm9dde3qxyls1sir0/sdkq4=">aaacinicbvdlsgmxfm3uv62vqks3wsk4kdijgrorcukygn1azyx30kwbmpkjsuyow3ylg3/fjqtfxql+jjm2i9p6iha4597k5picm6vt+9sqlc2vrk4v10sbm1vbo+xdvaake0log8q8lm0ffousog3nnkdtismepqctf3id+61hkhwlo3s9etqlor+xgbhqruqwl90q9iaat2+yb1codpk641ttnyc0w7n2mvvyhyiqkgxdcswu2mpgrejmsqvnue+wp91etjkqrppwukrj2ej7kujnckdzyu0ufucg0kcdqymiqflsczgmhxmlh4nymhnppfznn1iilrqfvpnme6t5lxf/8zqjdi68leui0tqik4echgmd47wv3goses1hhgcrzgtfzaasidatlkwjzvyxf0nztoryvefurfk7mtzrrafoeb0jb52jgrpfddrabd2hf/sg3q1n69x6sl4mowvrurop/sd6+qxkcqw5</latexit> <latexit sha1_base64="ia+rc35bi+ev/o2m5yprao92otu=">aaab+3icbvdlssnafj34rpuv69jnsaiusikcloucukxgh9decjodtemnk2fmipaqx3hjqhg3/og7/8zjm4w2hhg4nhmv98wjbanku+63tbk6tr6xwdmqbu/s7u3bb7woslkjsrsnljg9ebrhljo2ppqrnpae4pcrbji5lvzui5gkjvxetwujyhhxglem2kgdu+bhomcywhatp/gteaigdt1tudm4y8qrsr2vaa3sl3+y4dqmxgmgsvu9v+gga6kpzisv+qkiavaerqrvkieyqccbzc+de6mmnsir5nhtzntfgxnesk3j0ewwsdwiv4j/ef1ur5dbrrlinef4fihkmamtpyjcgvjjsgztqwblari6eawssdz1vu0j3ukxl0nnrog5de/uvn68kuuoocn0je6rhy5qe92ifmojjj7qm3pfb1zuvvjv1sd8dmuqdw7rh1ifp1asljo=</latexit>

21 Some Cousin Models Restoring permutation symmetry Adding vector fields Coloured probe model

22 Disordered probe model (arxiv: 1806.???? )

23 Probe fields are n in number. 1<<n<<N. 0 H HSY K + j q p p <latexit sha1_base64="dduxeavdupcxq84efhtyq4m9zxm=">aaacehicbvdlssnafj3uv62vqes3g0uqicurqzdfnwu3fe1dmjrmptn27cqzzyzccfken/6kgxekuhxpzr9x2mah1qmxdufcy733+jxrqszry8jnzs8sluwxcyura+sb5uzwq0axwksoixajlo8kytqkduuviy0ucap8rpr+8hzsn++jkdqkr9wiezda/zd2kezks55zqkjh0gbwvetq5ikfb/c25hbjo8ndiu+hm0scow6hnlm0ytye8c+xm1iegwqe+el0ixwhjfsyisnbtswvmychkgykltixjbzhieqttqyhcoh0k8ldkdztshf2iqervhci/pxiucdlkpb1z4duqm56y/e/rx2r3qmb0jdhior4uqgxm6gioe4hdqkgwlgrjgglqm+feiaewkpnwnah2lmv/ywno7jtle3l42lllisjd3baltghnjgbfvafnvahgdyaj/acxo1h49l4m96nrtkjm9kgv2b8fam3b5tz</latexit> F and F are maximally chaotic. has Lyapunov coefficient. smaller than, but F order of the maximal value, 2 T. <latexit sha1_base64="2ejtlzqzhonrazotelyguiabrre=">aaacanicbzdlssnafiynxmu8rv2jm8fscfusexrzfirlcvyctvom00k7ddizzizcccwnr+lghsjufqp3vo3tnatt/whg4z/ncob8owbuadf9tlzw19y3nktb9vbo7t6+c3dyukkqmwnihcwyeyjfgowkqalmpcmkqxhisdsc38zq7qcifu34vz4iesroyglemdlg6jvh9z4vfiv2bdz7wy7+gambpn2n7fbdxhazvalkofcj73z5gwsnmeeam6ru13ofdjikncwmtg0/vuqgpezd0jxiuuxukountghfoamyjdi8rmhu/p7iukzuja5nz4z0sc3wzuz/tw6qo6sgo1ykmna8xxsldooezvkaayoj1mxiagfjzv8hhigjsdap2syeb/hkzwidvz236t1dlgvxrrwlcajowrnwwcwogvvqae2awsn4bq/gzxqyxqx362peumivm0fgj6zph28fli0=</latexit> <latexit sha1_base64="0gyjjdao1cmfyzraydghtbckq9e=">aaacanicbzdlssnafiynxmu8rv2jm8fscfusexrzfirlcvyctvom00k7ddizzizcccwnr+lghsjufqp3vo3tnatt/whg4z/ncob8owbuadf9tlzw19y3nktb9vbo7t6+c3dyukkqmwnihcwyeyjfgowkqalmpcmkqxhisdsc38zq7qcifu34vz4iesroyglemdlg6jvhlxrpf4pcg9z7wu7+gambpn2n7fbdxhazvalkofcj73z5gwsnmeeam6ru13ofdjikncwmtg0/vuqgpezd0jxiuuxukountghfoamyjdi8rmhu/p7iukzuja5nz4z0sc3wzuz/tw6qo6sgo1ykmna8xxsldooezvkaayoj1mxiagfjzv8hhigjsdap2syeb/hkzwidvz236t1dlgvxrrwlcajowrnwwcwogvvqae2awsn4bq/gzxqyxqx362peumivm0fgj6zph23rli0=</latexit> <latexit sha1_base64="isivi+nr6bxhkxk5imzgucgsxri=">aaab/xicbvdlssnafj34rpevhzs3g6xgqiqi6liofjcv7apatnxmj+3qstlmtiqair/ixouibv0pd/6n0zylbt1w4xdovdx7tya4u9p1v62v1bx1jc3clr29s7u37xwcnlsssklrjogjbawgkgcxrwumow0jssekog0go5up33ygurekvtdjqf0ibjelgqftpj5zxkp2o0ixbonqn+umqaiy9jyiw3znwmvey0kr5aj1nk9opyfprgnnocjv9lyh/qykzottid1jfrvarjcgbunjikjys9n1e1wysh+hitqvazxtf09keck1jgltgyeeqkvvkv7ntvmdxvkzi0wqauzmi8kuy53gars4zyqlmo8naskzurwtiugg2grmmxc8xzexseo87lll7+6iwlno4yige3skzpchllef3aiaqiochtezekvv1pp1yr1bh/pwfsufouj/yh3+anzlldm=</latexit> <latexit sha1_base64="9thokael5wd3phcpotqrybpvl50=">aaab7nicbvdlsgnbeoz1gemr6thlyba8hd0g6dhoxwoevcbzwuxkkgyznr1meoww5co8efdeq9/jzb9xkuxbewsaiqpuursilyvf3//2nja3tnd2c3vf/ypdo+psywnljqlhvmksmzhorc2xqvemcps8ow2ncsr5o5rcz/32ezdwjkqbu83dmi6ugapg0untkulpqrr9utmv+auqdrlkpaw56v3sv2+qsdtmcpmk1nydx2oyuyocst4r9lllnwutoujdrxwnuq2zxbkzcumuarkmxpvcslb/t2q0tnyar64zpji2q95c/m/rpji8dtohdipcsewiysojjmt+oxkiwxnkqsougefujwxmdwxoeiq6eilvl9djq1oj/erwef2u3evxfoacluakaribgjxahzrayalp8apvnvzevhfvy9m64euzz/ah3ucpe/wouw==</latexit> p In the limit q! 1,! 1 q ALL four point functions are maximally chaotic. <latexit sha1_base64="8eeambhz+kv7tpgc7t2u0ems6cs=">aaace3icbvbns8naej34wetx1koxxskisele0gpri8ck9goaudbbtbt0s0l3n0oj/q9e/ctepcji1ys3/43bngfb+mdg8d4mm/ochdolhefhwlpewv1bl2wun7e2d3btvf26ilnjai3epjbnacvkmaa1ztsnzurshawcnol+zdhvpfcpwczu9tchfos7gowmyg2ktn06qj5k3z7gusapyd1dxigxyzjrnhjnwm275jsdcdaicxnsghzvtv3tdwksrlrowrfslddjtj9hqrnhdft0ukuttpq4s1ugchxr5wetn0bo2cgdfmbslnboov6dyhck1daktgeedu/ne2pxp6+v6vdkz5hiuk0fms4ku450jmyboq6tlgg+naqtycytipswyusbgismbhf+5uvspy+7ttm9uyhvrvm4cnair3acllxcbw6hcjug8aqv8abv1rp1an1yn9pwjsufoyazwf+/pdgeaq==</latexit> Probe primaries make a copy of the BH primaries.

24 Scorecard Our models satisfy the non trivial requirement of symmetry breaking and partially fulfil that of maximal chaos. Probe spectrum is in natural correspondence with black hole spectrum. Significant improvement for disordered probe model.

25 Future Directions

26 Study thermalisation, i.e. test ETH. Higher point functions.

27 Merci Beaucoup!

Large N fermionic tensor models in d = 2

Large N fermionic tensor models in d = 2 Large N fermionic tensor models in d = 2 Sylvain Carrozza Quantum spacetime and the Renormalization roup 2018 Bad Honnef Sylvain Carrozza Large N fermionic tensor models Bad Honnef 20/6/2018 1 / 17 Context

More information

arxiv: v1 [hep-th] 13 Nov 2017

arxiv: v1 [hep-th] 13 Nov 2017 Tensor Models for Black Hole Probes Nick Halmagyi and Swapnamay Mondal arxiv:1711.04385v1 [hep-th] 13 Nov 017 Sorbonne Universités, UPMC Paris 06, UMR 7589, LPTHE, 75005, Paris, France and CNRS, UMR 7589,

More information

Black Holes, Matrix Models and Large D

Black Holes, Matrix Models and Large D Black Holes, Matrix Models and Large D Frank FERRARI Université Libre de Bruxelles International Solvay Institutes Quantum Gravity in Paris IHP, Paris, March 23th, 2017 Plan of the talk 1. Building Quantum

More information

Partial deconfinement phases in gauged multi-matrix quantum mechanics.

Partial deconfinement phases in gauged multi-matrix quantum mechanics. Partial deconfinement phases in gauged multi-matrix quantum mechanics. David Berenstein, UCSB based on arxiv:1806.05729 Vienna, July 12, 2018 Research supported by gauge/gravity Gauged matrix quantum mechanics

More information

Brief course of lectures at 18th APCTP Winter School on Fundamental Physics

Brief course of lectures at 18th APCTP Winter School on Fundamental Physics Brief course of lectures at 18th APCTP Winter School on Fundamental Physics Pohang, January 20 -- January 28, 2014 Motivations : (1) Extra-dimensions and string theory (2) Brane-world models (3) Black

More information

10 Interlude: Preview of the AdS/CFT correspondence

10 Interlude: Preview of the AdS/CFT correspondence 10 Interlude: Preview of the AdS/CFT correspondence The rest of this course is, roughly speaking, on the AdS/CFT correspondence, also known as holography or gauge/gravity duality or various permutations

More information

Introduction to AdS/CFT

Introduction to AdS/CFT Introduction to AdS/CFT Who? From? Where? When? Nina Miekley University of Würzburg Young Scientists Workshop 2017 July 17, 2017 (Figure by Stan Brodsky) Intuitive motivation What is meant by holography?

More information

Black Holes, Holography, and Quantum Information

Black Holes, Holography, and Quantum Information Black Holes, Holography, and Quantum Information Daniel Harlow Massachusetts Institute of Technology August 31, 2017 1 Black Holes Black holes are the most extreme objects we see in nature! Classically

More information

A Solvable Irrelevant

A Solvable Irrelevant A Solvable Irrelevant Deformation of AdS $ / CFT * A. Giveon, N. Itzhaki, DK arxiv: 1701.05576 + to appear Strings 2017, Tel Aviv Introduction QFT is usually thought of as an RG flow connecting a UV fixed

More information

Chaotic Information Processing by Extremal Black Holes

Chaotic Information Processing by Extremal Black Holes 1 Chaotic Information Processing by Extremal Black Holes Stam Nicolis CNRS Laboratoire de Mathématiques et Physique Théorique (UMR7350) Fédération de Recherche Denis Poisson (FR2964) Département de Physique,

More information

A Holographic Description of Black Hole Singularities. Gary Horowitz UC Santa Barbara

A Holographic Description of Black Hole Singularities. Gary Horowitz UC Santa Barbara A Holographic Description of Black Hole Singularities Gary Horowitz UC Santa Barbara Global event horizons do not exist in quantum gravity: String theory predicts that quantum gravity is holographic:

More information

Disordered metals without quasiparticles, and charged black holes

Disordered metals without quasiparticles, and charged black holes HARVARD Disordered metals without quasiparticles, and charged black holes String Theory: Past and Present (SpentaFest) International Center for Theoretical Sciences, Bengaluru January 11-13, 2017 Subir

More information

Black Hole Entropy and Gauge/Gravity Duality

Black Hole Entropy and Gauge/Gravity Duality Tatsuma Nishioka (Kyoto,IPMU) based on PRD 77:064005,2008 with T. Azeyanagi and T. Takayanagi JHEP 0904:019,2009 with T. Hartman, K. Murata and A. Strominger JHEP 0905:077,2009 with G. Compere and K. Murata

More information

On higher-spin gravity in three dimensions

On higher-spin gravity in three dimensions On higher-spin gravity in three dimensions Jena, 6 November 2015 Stefan Fredenhagen Humboldt-Universität zu Berlin und Max-Planck-Institut für Gravitationsphysik Higher spins Gauge theories are a success

More information

Holographic renormalization and reconstruction of space-time. Kostas Skenderis Southampton Theory Astrophysics and Gravity research centre

Holographic renormalization and reconstruction of space-time. Kostas Skenderis Southampton Theory Astrophysics and Gravity research centre Holographic renormalization and reconstruction of space-time Southampton Theory Astrophysics and Gravity research centre STAG CH RESEARCH ER C TE CENTER Holographic Renormalization and Entanglement Paris,

More information

Supergravity from 2 and 3-Algebra Gauge Theory

Supergravity from 2 and 3-Algebra Gauge Theory Supergravity from 2 and 3-Algebra Gauge Theory Henrik Johansson CERN June 10, 2013 Twelfth Workshop on Non-Perturbative Quantum Chromodynamics, l Institut d Astrophysique de Paris Work with: Zvi Bern,

More information

Insight into strong coupling

Insight into strong coupling Insight into strong coupling Many faces of holography: Top-down studies (string/m-theory based) focused on probing features of quantum gravity Bottom-up approaches pheno applications to QCD-like and condensed

More information

Holography and (Lorentzian) black holes

Holography and (Lorentzian) black holes Holography and (Lorentzian) black holes Simon Ross Centre for Particle Theory The State of the Universe, Cambridge, January 2012 Simon Ross (Durham) Holography and black holes Cambridge 7 January 2012

More information

Holographic Second Laws of Black Hole Thermodynamics

Holographic Second Laws of Black Hole Thermodynamics Holographic Second Laws of Black Hole Thermodynamics Federico Galli Gauge/Gravity Duality 018, Würzburg, 31 July 018 Based on arxiv: 1803.03633 with A. Bernamonti, R. Myers and J. Oppenheim Second Law

More information

Insight into strong coupling

Insight into strong coupling Thank you 2012 Insight into strong coupling Many faces of holography: Top-down studies (string/m-theory based) Bottom-up approaches pheno applications to QCD-like and condensed matter systems (e.g. Umut

More information

Planar diagrams in light-cone gauge

Planar diagrams in light-cone gauge Planar diagrams in light-cone gauge M. Kruczenski Purdue University Based on: hep-th/0603202 Summary Introduction Motivation: large-n, D-branes, AdS/CFT, results D-brane interactions: lowest order, light-cone

More information

Eternal traversable worm hole in 2D

Eternal traversable worm hole in 2D Eternal traversable worm hole in 2D Xiao-Liang Qi Stanford University Strings2018, OIST, 6/27/2018 Ref: J. Maldacena & XLQ, arxiv: 1804.00491 Goal: dual Coupled SYK Global AdS2 Outline: 1. Overview of

More information

Non-relativistic holography

Non-relativistic holography University of Amsterdam AdS/CMT, Imperial College, January 2011 Why non-relativistic holography? Gauge/gravity dualities have become an important new tool in extracting strong coupling physics. The best

More information

Black holes and random matrices

Black holes and random matrices Black holes and random matrices Stephen Shenker Stanford University Strings 2017 Stephen Shenker (Stanford University) Black holes and random matrices Strings 2017 1 / 17 A question What accounts for the

More information

Talk based on: arxiv: arxiv: arxiv: arxiv: arxiv:1106.xxxx. In collaboration with:

Talk based on: arxiv: arxiv: arxiv: arxiv: arxiv:1106.xxxx. In collaboration with: Talk based on: arxiv:0812.3572 arxiv:0903.3244 arxiv:0910.5159 arxiv:1007.2963 arxiv:1106.xxxx In collaboration with: A. Buchel (Perimeter Institute) J. Liu, K. Hanaki, P. Szepietowski (Michigan) The behavior

More information

Black Hole Collapse in Large-C CFT

Black Hole Collapse in Large-C CFT Black Hole Collapse in Large-C CFT Julian Sonner Oxford 13 July 2016 Tarek Anous (MIT) Thomas Hartman (Cornell) Antonin Rovai (Geneva) Introduction The black hole as movie star: Gargantua Gargantua, C.

More information

Symmetric Surfaces of Topological Superconductor

Symmetric Surfaces of Topological Superconductor Symmetric Surfaces of Topological Superconductor Sharmistha Sahoo Zhao Zhang Jeffrey Teo Outline Introduction Brief description of time reversal symmetric topological superconductor. Coupled wire model

More information

Chern-Simons Theories and AdS/CFT

Chern-Simons Theories and AdS/CFT Chern-Simons Theories and AdS/CFT Igor Klebanov PCTS and Department of Physics Talk at the AdS/CMT Mini-program KITP, July 2009 Introduction Recent progress has led to realization that coincident membranes

More information

strings, symmetries and holography

strings, symmetries and holography strings, symmetries and holography Discrete 08 VALENCIA J.L.F. Barbon IFT UAM/CSIC (Madrid) 1 THE ROLE OF SYMMETRY PRINCIPLES IN THE CONSTRUCTION OF STRING THEORY WAS NEVER UNDERESTIMATED 2 Examples of

More information

One Loop Tests of Higher Spin AdS/CFT

One Loop Tests of Higher Spin AdS/CFT One Loop Tests of Higher Spin AdS/CFT Simone Giombi UNC-Chapel Hill, Jan. 30 2014 Based on 1308.2337 with I. Klebanov and 1401.0825 with I. Klebanov and B. Safdi Massless higher spins Consistent interactions

More information

Emergent Quantum Criticality

Emergent Quantum Criticality (Non-)Fermi Liquids and Emergent Quantum Criticality from gravity Hong Liu Massachusetts setts Institute te of Technology HL, John McGreevy, David Vegh, 0903.2477 Tom Faulkner, HL, JM, DV, to appear Sung-Sik

More information

MITOCW watch?v=nw4vp_upvme

MITOCW watch?v=nw4vp_upvme MITOCW watch?v=nw4vp_upvme The following content is provided under a Creative Commons license. Your support will help MIT OpenCourseWare continue to offer high quality educational resources for free. To

More information

BLACK HOLES IN 3D HIGHER SPIN GRAVITY. Gauge/Gravity Duality 2018, Würzburg

BLACK HOLES IN 3D HIGHER SPIN GRAVITY. Gauge/Gravity Duality 2018, Würzburg BLACK HOLES IN 3D HIGHER SPIN GRAVITY Gauge/Gravity Duality 2018, Würzburg What is a Black Hole? What is a Black Hole? In General Relativity (and its cousins): Singularity What is a Black Hole? In General

More information

Thomas Klose Uppsala University J u n e, S t r i n g s , U p p s a l a

Thomas Klose Uppsala University J u n e, S t r i n g s , U p p s a l a Thomas Klose Uppsala University 2 7. J u n e, S t r i n g s 2 0 1 1, U p p s a l a The space-time dependence of two- and three-point functions of Scalar Conformal Primary Operators is fixed by conformal

More information

Theory of Quantum Matter: from Quantum Fields to Strings

Theory of Quantum Matter: from Quantum Fields to Strings Theory of Quantum Matter: from Quantum Fields to Strings Salam Distinguished Lectures The Abdus Salam International Center for Theoretical Physics Trieste, Italy January 27-30, 2014 Subir Sachdev Talk

More information

Black Hole Entropy: An ADM Approach Steve Carlip U.C. Davis

Black Hole Entropy: An ADM Approach Steve Carlip U.C. Davis Black Hole Entropy: An ADM Approach Steve Carlip U.C. Davis ADM-50 College Station, Texas November 2009 Black holes behave as thermodynamic objects T = κ 2πc S BH = A 4 G Quantum ( ) and gravitational

More information

The Schwarzian and black hole physics

The Schwarzian and black hole physics The Schwarzian and black hole physics Thomas Mertens Ghent University Based on arxiv:1606.03438 with J. Engelsöy and H. Verlinde arxiv:1705.08408 with G.J. Turiaci and H. Verlinde arxiv:1801.09605 arxiv:1804.09834

More information

The ground state wave function of Matrix Theory

The ground state wave function of Matrix Theory KITP January 30, 2014 The ground state wave function of Matrix Theory Revisited Xi Yin Harvard University work in progress with Ying-Hsuan Lin It has become increasingly evident that to understand semi-classical

More information

The Strong Interaction and LHC phenomenology

The Strong Interaction and LHC phenomenology The Strong Interaction and LHC phenomenology Juan Rojo STFC Rutherford Fellow University of Oxford Theoretical Physics Graduate School course Lecture 2: The QCD Lagrangian, Symmetries and Feynman Rules

More information

Three-Charge Black Holes and ¼ BPS States in Little String Theory I

Three-Charge Black Holes and ¼ BPS States in Little String Theory I Three-Charge Black Holes and ¼ BPS States in Little String Theory I SUNGJAY LEE KOREA INSTITUTE FOR ADVANCED STUDIES UNIVERSITY OF CHICAGO Joint work (1508.04437) with Amit Giveon, Jeff Harvey, David Kutasov

More information

Gauge/Gravity Duality: Applications to Condensed Matter Physics. Johanna Erdmenger. Julius-Maximilians-Universität Würzburg

Gauge/Gravity Duality: Applications to Condensed Matter Physics. Johanna Erdmenger. Julius-Maximilians-Universität Würzburg Gauge/Gravity Duality: Applications to Condensed Matter Physics. Johanna Erdmenger Julius-Maximilians-Universität Würzburg 1 New Gauge/Gravity Duality group at Würzburg University Permanent members 2 Gauge/Gravity

More information

Entropy of asymptotically flat black holes in gauged supergravit

Entropy of asymptotically flat black holes in gauged supergravit Entropy of asymptotically flat black holes in gauged supergravity with Nava Gaddam, Alessandra Gnecchi (Utrecht), Oscar Varela (Harvard) - work in progress. BPS Black Holes BPS Black holes in flat space

More information

Half BPS solutions in type IIB and M-theory

Half BPS solutions in type IIB and M-theory Half BPS solutions in type IIB and M-theory Based on work done in collaboration with Eric D Hoker, John Estes, Darya Krym (UCLA) and Paul Sorba (Annecy) E.D'Hoker, J.Estes and M.G., Exact half-bps type

More information

Black hole thermodynamics under the microscope

Black hole thermodynamics under the microscope DELTA 2013 January 11, 2013 Outline Introduction Main Ideas 1 : Understanding black hole (BH) thermodynamics as arising from an averaging of degrees of freedom via the renormalisation group. Go beyond

More information

Three-Charge Black Holes and ¼ BPS States in Little String Theory

Three-Charge Black Holes and ¼ BPS States in Little String Theory Three-Charge Black Holes and ¼ BPS States in Little String Theory SUNGJAY LEE KOREA INSTITUTE FOR ADVANCED STUDIES Joint work (JHEP 1512, 145) with Amit Giveon, Jeff Harvey, David Kutasov East Asia Joint

More information

Bubbling Geometries for Half BPS Wilson Lines. Satoshi Yamaguchi (IHES) S. Yamaguchi, hep-th/ S. Yamaguchi, to appear

Bubbling Geometries for Half BPS Wilson Lines. Satoshi Yamaguchi (IHES) S. Yamaguchi, hep-th/ S. Yamaguchi, to appear Bubbling Geometries for Half BPS Wilson Lines Satoshi Yamaguchi (IHES) S. Yamaguchi, hep-th/0601089 S. Yamaguchi, to appear 1. Overview AdS5 CFT4 AdS5 x S5 Goal deform Supergravity Solutions 4dim N=4 Super

More information

Spin Models and Gravity

Spin Models and Gravity Spin Models and Gravity Umut Gürsoy (CERN) 6th Regional Meeting in String Theory, Milos June 25, 2011 Spin Models and Gravity p.1 Spin systems Spin Models and Gravity p.2 Spin systems Many condensed matter

More information

QUANTUM QUENCH ACROSS A HOLOGRAPHIC CRITICAL POINT

QUANTUM QUENCH ACROSS A HOLOGRAPHIC CRITICAL POINT QUANTUM QUENCH ACROSS A HOLOGRAPHIC CRITICAL POINT Sumit R Das (w/ Pallab Basu) (arxiv:1109.3909, to appear in JHEP) Quantum Quench Suppose we have a quantum field theory, whose parameters (like couplings

More information

Nonlocal Effects in Quantum Gravity

Nonlocal Effects in Quantum Gravity Nonlocal Effects in Quantum Gravity Suvrat Raju International Centre for Theoretical Sciences 29th Meeting of the IAGRG IIT Guwahati 20 May 2017 Collaborators Based on work with 1 Kyriakos Papadodimas

More information

The Trailing String in Confining Holographic Theories

The Trailing String in Confining Holographic Theories The Trailing String in Confining Holographic Theories p. 1 The Trailing String in Confining Holographic Theories Francesco Nitti APC, U. Paris VII Twelfth Workshop on Non-Perturbative Quantum Chromodynamics

More information

Random Matrices, Black holes, and the Sachdev-Ye-Kitaev model

Random Matrices, Black holes, and the Sachdev-Ye-Kitaev model Random Matrices, Black holes, and the Sachdev-Ye-Kitaev model Antonio M. García-García Shanghai Jiao Tong University PhD Students needed! Verbaarschot Stony Brook Bermúdez Leiden Tezuka Kyoto arxiv:1801.02696

More information

Holography and Unitarity in Gravitational Physics

Holography and Unitarity in Gravitational Physics Holography and Unitarity in Gravitational Physics Don Marolf 01/13/09 UCSB ILQG Seminar arxiv: 0808.2842 & 0808.2845 This talk is about: Diffeomorphism Invariance and observables in quantum gravity The

More information

Causal Evolution of Bulk localized Excitations in AdS from CFT

Causal Evolution of Bulk localized Excitations in AdS from CFT Causal Evolution of Bulk localized Excitations in AdS from CFT Kanato Goto The University of Tokyo, Komaba Particle Theory Group based on arxiv:1605.02835 KG and M.Miyaji and T.Takayanagi Kanato Goto (Tokyo

More information

Complex entangled states of quantum matter, not adiabatically connected to independent particle states. Compressible quantum matter

Complex entangled states of quantum matter, not adiabatically connected to independent particle states. Compressible quantum matter Complex entangled states of quantum matter, not adiabatically connected to independent particle states Gapped quantum matter Z2 Spin liquids, quantum Hall states Conformal quantum matter Graphene, ultracold

More information

Supersymmetric Gauge Theories in 3d

Supersymmetric Gauge Theories in 3d Supersymmetric Gauge Theories in 3d Nathan Seiberg IAS Intriligator and NS, arxiv:1305.1633 Aharony, Razamat, NS, and Willett, arxiv:1305.3924 3d SUSY Gauge Theories New lessons about dynamics of quantum

More information

String/Brane charge & the non-integral dimension

String/Brane charge & the non-integral dimension Jian-Xin Lu (With Wei and Xu) The Interdisciplinary Center for Theoretical Study (ICTS) University of Science & Technology of China September 28, 2012 Introduction Introduction Found four laws of black

More information

BPS states, permutations and information

BPS states, permutations and information BPS states, permutations and information Sanjaye Ramgoolam Queen Mary, University of London YITP workshop, June 2016 Permutation centralizer algebras, Mattioli and Ramgoolam arxiv:1601.06086, Phys. Rev.

More information

Zhong-Zhi Xianyu (CMSA Harvard) Tsinghua June 30, 2016

Zhong-Zhi Xianyu (CMSA Harvard) Tsinghua June 30, 2016 Zhong-Zhi Xianyu (CMSA Harvard) Tsinghua June 30, 2016 We are directly observing the history of the universe as we look deeply into the sky. JUN 30, 2016 ZZXianyu (CMSA) 2 At ~10 4 yrs the universe becomes

More information

The intricate interplay between integrability and chaos for the dynamics of the probes of extremal black hole spacetimes

The intricate interplay between integrability and chaos for the dynamics of the probes of extremal black hole spacetimes The intricate interplay between integrability and chaos for the dynamics of the probes of extremal black hole spacetimes Stam Nicolis CNRS Laboratoire de Mathématiques et Physique Théorique (UMR7350) Fédération

More information

SYK model, Coadjoint orbits and Liouville bulk dual

SYK model, Coadjoint orbits and Liouville bulk dual SYK model, Coadjoint orbits and Liouville bulk dual Gautam Mandal String theory: past and present SpentaFest ICTS, Bangalore, 11 January 2017 Ongoing work with Pranjal Nayak and Spenta Scanned by CamScanner

More information

Symmetries, Horizons, and Black Hole Entropy. Steve Carlip U.C. Davis

Symmetries, Horizons, and Black Hole Entropy. Steve Carlip U.C. Davis Symmetries, Horizons, and Black Hole Entropy Steve Carlip U.C. Davis UC Davis June 2007 Black holes behave as thermodynamic objects T = κ 2πc S BH = A 4 G Quantum ( ) and gravitational (G) Does this thermodynamic

More information

3d GR is a Chern-Simons theory

3d GR is a Chern-Simons theory 3d GR is a Chern-Simons theory An identity in three dimensions p g R + 1`2 = abc (R ab e c + 1`2 ea e b e c )= A a da a + 13 abca a A b A Ā c a dā a + 13 abcāa Ā b Ā c + db with 1 ` ea = A a Ā a, a bc

More information

Flavor quark at high temperature from a holographic Model

Flavor quark at high temperature from a holographic Model Flavor quark at high temperature from a holographic Model Ghoroku (Fukuoka Institute of Technology) Sakaguchi (Kyushu University) Uekusa (Kyushu University) Yahiro (Kyushu University) Hep-th/0502088 (Phys.Rev.D71:106002,2005

More information

Chris Verhaaren Joint Theory Seminar 31 October With Zackaria Chacko, Rashmish Mishra, and Simon Riquelme

Chris Verhaaren Joint Theory Seminar 31 October With Zackaria Chacko, Rashmish Mishra, and Simon Riquelme Chris Verhaaren Joint Theory Seminar 31 October 2016 With Zackaria Chacko, Rashmish Mishra, and Simon Riquelme It s Halloween A time for exhibiting what some find frightening And seeing that it s not so

More information

Complexity and Spacetime

Complexity and Spacetime Complexity and Spacetime 1612.05439, 1706.03788 + to appear, with Alan Reynolds Simon Ross Centre for Particle Theory, Durham University 13 September 2017 Simon Ross (Durham) Complexity and Spacetime McGill

More information

Non-associative Deformations of Geometry in Double Field Theory

Non-associative Deformations of Geometry in Double Field Theory Non-associative Deformations of Geometry in Double Field Theory Michael Fuchs Workshop Frontiers in String Phenomenology based on JHEP 04(2014)141 or arxiv:1312.0719 by R. Blumenhagen, MF, F. Haßler, D.

More information

Perturbative Integrability of large Matrix Theories

Perturbative Integrability of large Matrix Theories 35 th summer institute @ ENS Perturbative Integrability of large Matrix Theories August 9 th, 2005 Thomas Klose Max-Planck-Institute for Gravitational Physics (Albert-Einstein-Institute), Potsdam, Germany

More information

Knot Homology from Refined Chern-Simons Theory

Knot Homology from Refined Chern-Simons Theory Knot Homology from Refined Chern-Simons Theory Mina Aganagic UC Berkeley Based on work with Shamil Shakirov arxiv: 1105.5117 1 the knot invariant Witten explained in 88 that J(K, q) constructed by Jones

More information

Quark-gluon plasma from AdS/CFT Correspondence

Quark-gluon plasma from AdS/CFT Correspondence Quark-gluon plasma from AdS/CFT Correspondence Yi-Ming Zhong Graduate Seminar Department of physics and Astronomy SUNY Stony Brook November 1st, 2010 Yi-Ming Zhong (SUNY Stony Brook) QGP from AdS/CFT Correspondence

More information

Holographic Techni-dilaton

Holographic Techni-dilaton Holographic Techni-dilaton Maurizio Piai Swansea University D. Elander, MP, arxiv: 1212.2600 D. Elander, MP arxiv: 1112.2915 - NPB R. Lawrance, MP arxiv: 1207.0427 D. Elander, MP arxiv: 1208.0546 - NPB

More information

Holographic Wilsonian Renormalization Group

Holographic Wilsonian Renormalization Group Holographic Wilsonian Renormalization Group JiYoung Kim May 0, 207 Abstract Strongly coupled systems are difficult to study because the perturbation of the systems does not work with strong couplings.

More information

Boundaries, Interfaces and Dualities

Boundaries, Interfaces and Dualities Boundaries, Interfaces and Dualities Dualities I Complementary weakly coupled descriptions in a space of exactly marginal couplings T1 T5 T2 T4 T3 Dualities II IR free effective description of asymptotically

More information

Spatially Modulated Phases in Holography. Jerome Gauntlett Aristomenis Donos Christiana Pantelidou

Spatially Modulated Phases in Holography. Jerome Gauntlett Aristomenis Donos Christiana Pantelidou Spatially Modulated Phases in Holography Jerome Gauntlett Aristomenis Donos Christiana Pantelidou Spatially Modulated Phases In condensed matter there is a variety of phases that are spatially modulated,

More information

Holography for Black Hole Microstates

Holography for Black Hole Microstates 1 / 24 Holography for Black Hole Microstates Stefano Giusto University of Padua Theoretical Frontiers in Black Holes and Cosmology, IIP, Natal, June 2015 2 / 24 Based on: 1110.2781, 1306.1745, 1311.5536,

More information

9 Symmetries of AdS 3

9 Symmetries of AdS 3 9 Symmetries of AdS 3 This section consists entirely of exercises. If you are not doing the exercises, then read through them anyway, since this material will be used later in the course. The main goal

More information

Solvable model for a dynamical quantum phase transition from fast to slow scrambling

Solvable model for a dynamical quantum phase transition from fast to slow scrambling Solvable model for a dynamical quantum phase transition from fast to slow scrambling Sumilan Banerjee Weizmann Institute of Science Designer Quantum Systems Out of Equilibrium, KITP November 17, 2016 Work

More information

Quantum Gravity and the Renormalization Group

Quantum Gravity and the Renormalization Group Nicolai Christiansen (ITP Heidelberg) Schladming Winter School 2013 Quantum Gravity and the Renormalization Group Partially based on: arxiv:1209.4038 [hep-th] (NC,Litim,Pawlowski,Rodigast) and work in

More information

Dynamics of heavy quarks in charged N = 4 SYM plasma

Dynamics of heavy quarks in charged N = 4 SYM plasma Dynamics of heavy quarks in charged N = 4 SYM plasma Aleksi Vuorinen University of Washington, Seattle & Technical University of Vienna C. Herzog and AV, arxiv:0708:0609 [hep-th] Outline N = 4 SYM and

More information

Yukawa Institute Workshop Strings and Fields Developments in String Theory and Quantum Field Theory. Conic D-branes

Yukawa Institute Workshop Strings and Fields Developments in String Theory and Quantum Field Theory. Conic D-branes Yukawa Institute Workshop Strings and Fields Developments in String Theory and Quantum Field Theory Conic D-branes Shunichiro Kinoshita (Chuo University) K. Hashimoto (Osaka), K. Murata (Keio) Based on

More information

21 July 2011, USTC-ICTS. Chiang-Mei Chen 陳江梅 Department of Physics, National Central University

21 July 2011, USTC-ICTS. Chiang-Mei Chen 陳江梅 Department of Physics, National Central University 21 July 2011, Seminar @ USTC-ICTS Chiang-Mei Chen 陳江梅 Department of Physics, National Central University Outline Black Hole Holographic Principle Kerr/CFT Correspondence Reissner-Nordstrom /CFT Correspondence

More information

Introduction to AdS/CFT

Introduction to AdS/CFT Introduction to AdS/CFT D-branes Type IIA string theory: Dp-branes p even (0,2,4,6,8) Type IIB string theory: Dp-branes p odd (1,3,5,7,9) 10D Type IIB two parallel D3-branes low-energy effective description:

More information

Holographic Cosmology Beyond Inflation? Mark Trodden! University of Pennsylvania

Holographic Cosmology Beyond Inflation? Mark Trodden! University of Pennsylvania Holographic Cosmology Beyond Inflation? Mark Trodden! University of Pennsylvania Workshop: Status and Future of Inflationary Theory! University of Chicago, August 22-24, 2014 Questions Haven t been thinking

More information

Chiral Haldane-SPT phases of SU(N) quantum spin chains in the adjoint representation

Chiral Haldane-SPT phases of SU(N) quantum spin chains in the adjoint representation Chiral Haldane-SPT phases of SU(N) quantum spin chains in the adjoint representation Thomas Quella University of Cologne Presentation given on 18 Feb 2016 at the Benasque Workshop Entanglement in Strongly

More information

Recent developments in Monte Carlo studies of superstring theory

Recent developments in Monte Carlo studies of superstring theory Recent developments in Monte Carlo studies of superstring theory Jun Nishimura (KEK & SOKENDAI) 12-16 August, 2013 Current Themes in High Energy Physics and Cosmology Niels Bohr Institute, Copenhagen Large-N

More information

Higher Spin Black Holes from 2d CFT. Rutgers Theory Seminar January 17, 2012

Higher Spin Black Holes from 2d CFT. Rutgers Theory Seminar January 17, 2012 Higher Spin Black Holes from 2d CFT Rutgers Theory Seminar January 17, 2012 Simplified Holography A goal Find a holographic duality simple enough to solve, but complicated enough to look like gravity in

More information

8.821 F2008 Lecture 12: Boundary of AdS; Poincaré patch; wave equation in AdS

8.821 F2008 Lecture 12: Boundary of AdS; Poincaré patch; wave equation in AdS 8.821 F2008 Lecture 12: Boundary of AdS; Poincaré patch; wave equation in AdS Lecturer: McGreevy Scribe: Francesco D Eramo October 16, 2008 Today: 1. the boundary of AdS 2. Poincaré patch 3. motivate boundary

More information

Classical AdS String Dynamics. In collaboration with Ines Aniceto, Kewang Jin

Classical AdS String Dynamics. In collaboration with Ines Aniceto, Kewang Jin Classical AdS String Dynamics In collaboration with Ines Aniceto, Kewang Jin Outline The polygon problem Classical string solutions: spiky strings Spikes as sinh-gordon solitons AdS string ti as a σ-model

More information

Modelling the evolution of small black holes

Modelling the evolution of small black holes Modelling the evolution of small black holes Elizabeth Winstanley Astro-Particle Theory and Cosmology Group School of Mathematics and Statistics University of Sheffield United Kingdom Thanks to STFC UK

More information

Quantum mechanics and the geometry of spacetime

Quantum mechanics and the geometry of spacetime Quantum mechanics and the geometry of spacetime Juan Maldacena PPCM Conference May 2014 Outline Brief review of the gauge/gravity duality Role of strong coupling in the emergence of the interior Role of

More information

On a holographic quantum quench with a finite size effect

On a holographic quantum quench with a finite size effect On a holographic quantum quench with a finite size effect Tomonori Ugajin (U. Tokyo KITP) Based on work in progress with G.Mandal, R.Sinha Holographic Vistas on gravity and strings YITP, 2014 Introduction

More information

Universal Dynamics from the Conformal Bootstrap

Universal Dynamics from the Conformal Bootstrap Universal Dynamics from the Conformal Bootstrap Liam Fitzpatrick Stanford University! in collaboration with Kaplan, Poland, Simmons-Duffin, and Walters Conformal Symmetry Conformal = coordinate transformations

More information

Geometry and Physics. Amer Iqbal. March 4, 2010

Geometry and Physics. Amer Iqbal. March 4, 2010 March 4, 2010 Many uses of Mathematics in Physics The language of the physical world is mathematics. Quantitative understanding of the world around us requires the precise language of mathematics. Symmetries

More information

One-loop Partition Function in AdS 3 /CFT 2

One-loop Partition Function in AdS 3 /CFT 2 One-loop Partition Function in AdS 3 /CFT 2 Bin Chen R ITP-PKU 1st East Asia Joint Workshop on Fields and Strings, May 28-30, 2016, USTC, Hefei Based on the work with Jie-qiang Wu, arxiv:1509.02062 Outline

More information

dynamics of broken symmetry Julian Sonner Non-Equilibrium and String Theory workshop Ann Arbor, 20 Oct 2012

dynamics of broken symmetry Julian Sonner Non-Equilibrium and String Theory workshop Ann Arbor, 20 Oct 2012 dynamics of broken symmetry Julian Sonner Non-Equilibrium and String Theory workshop Ann Arbor, 20 Oct 2012 1207.4194, 12xx.xxxx in collaboration with Jerome Gauntlett & Toby Wiseman Benjamin Simons Miraculous

More information

New Compressible Phases From Gravity And Their Entanglement. Sandip Trivedi, TIFR, Mumbai Simons Workshop, Feb 2013

New Compressible Phases From Gravity And Their Entanglement. Sandip Trivedi, TIFR, Mumbai Simons Workshop, Feb 2013 New Compressible Phases From Gravity And Their Entanglement Sandip Trivedi, TIFR, Mumbai Simons Workshop, Feb 2013 Collaborators: Kevin Goldstein, Nori Iizuka, Shamit Kachru, Nilay Kundu, Prithvi Nayaran,

More information

Recent Developments in Holographic Superconductors. Gary Horowitz UC Santa Barbara

Recent Developments in Holographic Superconductors. Gary Horowitz UC Santa Barbara Recent Developments in Holographic Superconductors Gary Horowitz UC Santa Barbara Outline 1) Review basic ideas behind holographic superconductors 2) New view of conductivity and the zero temperature limit

More information

Symmetries, Groups Theory and Lie Algebras in Physics

Symmetries, Groups Theory and Lie Algebras in Physics Symmetries, Groups Theory and Lie Algebras in Physics M.M. Sheikh-Jabbari Symmetries have been the cornerstone of modern physics in the last century. Symmetries are used to classify solutions to physical

More information

Chapter 3: Duality Toolbox

Chapter 3: Duality Toolbox 3.: GENEAL ASPECTS 3..: I/UV CONNECTION Chapter 3: Duality Toolbox MIT OpenCourseWare Lecture Notes Hong Liu, Fall 04 Lecture 8 As seen before, equipped with holographic principle, we can deduce N = 4

More information

Holographic methods for cosmology. Gonzalo Torroba Stanford University

Holographic methods for cosmology. Gonzalo Torroba Stanford University Holographic methods for cosmology Gonzalo Torroba Stanford University Observations and Theoretical Challenges in Primordial Cosmology KITP, UCSB, April 2013 Members of the collaboration Matt Dodelson Shunji

More information

String theory effects on 5D black strings

String theory effects on 5D black strings String theory effects on 5D black strings Alejandra Castro University of Michigan Work in collaboration with J. Davis, P. Kraus and F. Larsen hep-th/0702072, hep-th/0703087, 0705.1847[hep-th], 0801.1863

More information