Fundamental Interactions

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Our specializations:

According to our present knowledge there are four fundamental interactions in nature: gravity, electromagnetism, weak and strong interaction with electromagnetism and weak interaction unified in the electroweak theory. Gravity as well as electromagnetism are macroscopic phenomena, immediately present in our everyday life, like falling objects and static electricity. Weak and strong nuclear interactions, on the other hand, become only important on the microscopic, atomic and subatomic level.

The most important aspect of the strong interaction is that it provides stability to the nucleus overcoming electric repulsion, whereas the transmutation of neutrons into protons is the most well-known weak phenomenon. The aim of fundamental physics may be described as obtaining a deeper understanding of these interactions, and penultimately finding a unified framework, which understands the different interactions as different aspects of a single truly fundamental interaction.

[Possible topics for a Bachelor thesis]

Research topics

Quantum field theory and non-commutative geometry

Describing the interactions on a more fundamental level the concepts of relativistic quantum field theories are employed. With the advent of quantum mechanics in the first decades of the 20th century it was realized that the electromagnetic field, including light, is quantized and can be seen as a stream of particles, the photons. This implies that the interaction between matter is mediated by the exchange of photons. The concept of relativistic quantum field theory is very simple, unifying a classical field theory with the concepts of quantum theory and special relativity.

Full propagator of free propagation
Fig.: Full propagator in terms of free propagation and self-energy corrections.

The construction of the perturbative NCQFT leads to new types of infrared (IR) singularities which represent a severe obstacle for the renormalization program at higher order and therefore lead to inconsistencies. The IR singularities are produced by the so-called UV finite nonplanar one-loop graphs (which are expected to be UV divergent by naive power counting) in U(N) gauge models and also in scalar field theories. The interplay between expected UV divergencies and the existence of the IR singularities is the so-called UV/IR mixing problem of NCQFT. One also has to stress that the usual UV divergences may be removed by the standard renormalization procedure.

The present research activities are devoted to find solutions for the UV/IR mixing problem of noncommutative gauge field models. In order to respect the effects of noncommutativity implied by the non-abelian structure a consistent treatment requires the use of the BRS quantization procedure even for a U(1) deformed Maxwell theory.


Gravitation

Since the groundbreaking work of Einstein, gravitation is conceived as defining the geometry of spacetime - even defining the very concepts of time and space itself. Planetary motion as well as the motion of massless particles, that is to say light, become the straightest possible paths in a non-Euclidean geometry.

Light-cone representing causal past and future
Fig.: Light-cone of an event representing its causal past and future.

General relativity is a very successful theory. Its predictions range from the deflection of light by massive bodies which distort spacetime (Einstein-lensing) to that of gravitational radiation carrying away energy in the form of "ripples" in spacetime (Hulse-Taylor binary pulsar), as well as to the expansion of the universe (microwave background radiation). One of the most spectacular predictions of general relativity is the existence of black holes, which by now has been confirmed indirectly by numerous astrophysical observations.

Despite of these successes there are several unresolved problems in the physics of gravitation, some of which are considered as the biggest problems in contemporary theoretical physics:

  • The cosmological constant problem entails a gigantic discrepancy (123 orders of magnitude) between observation and naive theoretical expectation, and so far no satisfying explanation exists that resolves this discrepancy.
  • Numerous astrophysical and cosmological observations reveal discrepancies with the theory of general relativity, unless we postulate the existence of dark matter, which so far has not been detected in particle physics experiments.
  • The elusive theory of quantum gravity still is very much a theory under construction, with several conceptual and technical issues seeking for solutions.
  • General relativity predicts its own failure as a consequence of the famous singularity theorems. Physically this means that spacetime contains regions where the curvature grows without a bound. The most prominent examples are the singularities within black holes as well as the Big Bang singularity.

Deeper insights into the structure of physical systems have often been achieved by the imposition of symmetries. This usually breaks the problem down into simpler building blocks which ideally allow a complete solution. Gravity is no exception to this rule since the prototypic black-hole solution, the Schwarzschild geometry (actually the first exact non-trivial solution of the Einstein-equations), has been found precisely along theses lines, i.e. upon imposing spherical symmetry. It is therefore natural to pursue a similar plan of attack for the quantization of gravity. The corresponding models become gravitational theories in a 1+1 dimensional spacetime coupled to the area of the two-sphere which becomes a dynamical variable in the reduced theory. There are several other ways how lowerdimensional (1+1 and 2+1) models arise from higherdimensional configurations in string theory or general relativity, and the description of gravity in lower dimensions is one of the key research fields of our group.


Quark-Gluon plasma

Quantum chromodynamics (QCD) is the accepted theory of the strong interactions responsible for the binding of quarks into hadrons such as protons and neutrons, and the binding of protons and neutrons into atomic nuclei. The fundamental particles of QCD, the quarks and gluons, carry a new form of charge, which is called color because of its triplet nature in the case of the quarks (e.g. red, green, blue); gluons come in eight different colors which are composites of color and anticolor charges. However, quarks and gluons have never been observed as free particles. Nevertheless, because quarks have also electrical charge, they can literally be seen as constituents of hadrons by deep inelastic scattering using virtual photons. The higher the energy of the probing photon, the more do the quarks appear as particles propagating freely within a hadron. This feature is called "asymptotic freedom". It arises from so-called nonabelian gauge field dynamics, with gluons being the excitations of the nonabelian gauge fields similarly to photons being the excitations of the electromagnetic fields, except that gluons also carry color charges. Asymptotic freedom is well understood, and the Nobel prize was awarded to its main discoverers Gross, Politzer, and Wilczek in 2004.

Much less understood is the phenomenon of "confinement", which means that only color-neutral bound states of quarks and gluons exist. This confinement can in fact be broken in a medium if the density exceeds significantly that of nuclear matter. When hadrons overlap so strongly that they loose their individuality, quarks and gluons come into their own as the elementary degrees of freedom. It is conceivable that such conditions are realized in the cores of certain neutron stars.

phase diagram of quark-gluon matter
Fig.: Qualitative sketch of the phase diagram of quark-gluon matter as a function of temperature T and quark chemical potential µ. Solid lines denote rst-order phase transitions, the dashed line a rapid crossover.


At comparatively low temperatures, quark matter is known to form Cooper pairs and turns into a color superconductor. Also at temperatures just above the superconductivity phase new phenomena appear, which reflect that quark matter has strong deviations from an ideal Fermi liquid. In particular, there is anomalous behaviour in the low-temperature specific heat, which has been calculated for the first time systematically by our group. This has already found application in revised calculations of the cooling behavior of young neutron stars.

String theory

The names of the fundamental forces are related to their strength. The strong force is much stronger than electromagnetism and is thus able to overcome the repulsive force between objects with the same electrical charge (protons or quarks). The weak force is weaker than electromagnetism but still much stronger than gravity. The reason that we almost only recognize gravity in everyday life is that the macroscopic objects are neutral. They don't carry an effective color charge and they carry - if at all - only very small electric charges. For gravity there is no negative charge (negative mass), so that all the small gravitational effects add up to something which is strong enough to move galaxies and build black holes. The seperate description of the forces is quite accurate by now. This is summarized in the standard model of particle physics.

There is only one particle (the Higgs boson), which is predicted by the standard model and has not yet been found. A measure for the strength of a force are the coupling constants of the corresponding theory. They are, however, not constant, but depend on the energy level one is dealing with. If one extrapolates their values to high energies, one discovers that the couplings of electromagnetism, strong and weak force meet at a certain energy level almost in one single point (see Figure 1). This supports the idea that those three forces could be just different aspects of one and the same universal force. There are several theories which try to describe this unification. They are called GUTs, 'grand unified theories'. However, to be really 'grand', such a unification should also include gravity, whose coupling constant is far weaker still at this high energies. The theory, which will manage to unify all forces, including gravity, is sometimes called TOE, "theory of everything". String theory is one candidate, and at present actually the only one for this TOE.

Point particle and closed string interaction
Fig.: Left: Point particle interaction, Right: Closed string interaction, note the smooth interaction surface.


'SUSY' stands for supersymmetry and means that there is an exchange symmetry between fermionic particles (like quarks and electrons) and bosonic ones (like photons and even gravitons, if one includes gravity into the considerations). It does, however, not relate the already known particles, but it predicts new supersymmetric partners to the known particles (called e.g. squarks, selectrons, photinos and gravitinos). So far none of those superparticles has been discovered, but there are a lot of theoretical reasons for believing in supersymmetry. Supersymmetry is an integral part of string theory, or more precisely 'superstring theory'. Within one year now, the new accelerator LHC (large hadron collider) at CERN will start and try to produce the Higgs boson and the superparticles mentioned above and will therefore also be a first test for string theory.

For further information and news on fundamental physics visit:

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This contains the public outreach web pages of the Fachausschuss für Kern- und Teilchenphysik (FAKT) of the ÖPG (Austrian Physical Society), which our institute are hosting.



Preprints

Preprints of the group Fundamental Interactions:

Current year

  • TUW-14-01 M. Gary, D. Grumiller, S. Prohazka, and S.-J. Rey, Lifshitz Holography with Isotropic Scale Invariance hep-th/1406.1468
  • TUW-14-02 S. Detournay, D. Grumiller, F. Schöller and J. Simon, Variational principle and 1-point functions in 3-dimensional flat space Einstein gravity hep-th/1402.3687
  • TUW-14-03 D. Grumiller, R. McNees and J. Salzer, Black holes and thermodynamics - The first half century hep-th/1402.5127
  • TUW-14-04 H. Afshar, T. Creutzig, D. Grumiller, Y. Hikida and P. Ronne, Unitary W-algebras and three-dimensional higher spin gravities with spin one symmetry 1404.0010
  • TUW-14-05 D. Grumiller, M. Riegler and J. Rosseel, Unitarity in three-dimensional flat space higher spin theories hep-th/1403.5297
  • TUW-14-06 V. Keranen, H Nishimura, S. Stricker, O. Taanila, A. Vuorinen, Universality in holographic entropy production 1405.7015
  • TUW-14-07 A. Bagchi, S. Detournay, D. Grumiller, S. Prohazka and M. Riegler, Holographic Chern-Simons Theories 1404.1919
  • TUW-14-08 D. Grumiller, R. McNees and J. Salzer, Cosmological constant as confining U(1) charge in two-dimensional dilaton gravity 1406.7007
  • TUW-14-09 Harald Skarke, The Evolution of an Inhomogeneous Universe 1407.6602
  • TUW-14-10 A. Bagchi, D. Grumiller, J. Salzer, S. Sarkar and F. Schöller, Flat space cosmologies in two dimensions 1408.5337
  • TUW-14-11 P. Anastasopoulos and R. Richter, Light stringy state production 1408.4810
  • TUW-14-12 M. Riegler, Flat space limit of Cardy formula 1408.6831
  • TUW-14-13 R. Baier, H. Nishimura, S. Stricker, Scalar field collapse with negative cosmological constant 1410.3495
  • TUW-14-14 A. Bagchi, R. Basu, D. Grumiller, M. Riegler, Entanglement entropy in Galilean conformal field theories and flat holography 1410.4089
  • TUW-14-15 M. Gary, D. Grumiller, M. Riegler and J. Rosseel, Flat space (higher spin) gravity with chemical potentials 1411.3728
  • TUW-14-15 A. Rebhan, The Witten-Sakai-Sugimoto model: A brief review and some recent results 1410.8858

2013

  • TUW-13-01 D. Grumiller, W. Riedler, J. Rosseel and T. Zojer, Holographic applications of logarithmic conformal field theories hep-th/1302.0280
  • TUW-13-02 M. Attems, A. Rebhan, M. Strickland, Longitudinal thermalization via the chromo-Weibel instability hep-ph/1301.7749
  • TUW-13-03 M. Attems, A. Rebhan, M. Strickland, The chromo-Weibel instability in an expanding background hep-ph/1302.5098
  • TUW-13-04 Roberto Emparan, Daniel Grumiller and Kentaro Tanabe, Large D gravity and low D strings hep-th/1303.1995
  • TUW-13-05 Steineder, Stricker, Vuorinen, Probing the pattern of holographic thermalization with photons hep-ph/1304.3404
  • TUW-13-06 Arjun Bagchi, Stephane Detournay and Daniel Grumiller, Joan Simon, Cosmic evolution from phase transition of 3-dimensional flat space hep-th/1305.2919
  • TUW-13-07 R. Andringa, E. Bergshoeff, J. Rosseel and E. Sezgin, Newton-Cartan Supergravity hep-th/1305.6737
  • TUW-13-08 S. Stricker, Holographic thermalization in N=4 Super Yang-Mills theory at finite coupling hep-th/1307.2736
  • TUW-13-09 H. Afshar, A. Bagchi, R. Fareghbal, D. Grumiller and J. Rosseel, Higher spin theory in 3-dimensional flat space, hep-th/1307.4768
  • TUW-13-10 H. R. Afshar, Flat/AdS boundary conditions in three dimensional conformal gravity, hep-th/1307.4855
  • TUW-13-12 K. Hori and J. Knapp, Linear Sigma Models With Strongly Coupled Phases - One Parameter Models, hep-th/1308.xxxx
  • TUW-13-13 R. Baier, S. Stricker, O. Taanila, Critical scalar field collpase in AdS3: an analytic approach, hep-th/1309.xxxx
  • TUW-13-14 D. Parganlija, P. Kovacs, Gy. Wolf, F. Giacosa and D. Rischke, Eta, Eta' and eLSM, hep-ph/1301.3478
  • TUW-13-15 D. Grumiller, M. Irakleidou, I. Lovrekovic and R. McNees, Conformal gravity holography in four dimensions, hep-th/1310.0819
  • TUW-13-17 D. Arnaudov, R.C. Rashkov and T. Vetsov, On the algebraic curves for circular and folded strings in AdS5 x S5, hep-th/1311.6114
  • TUW-13-18 Daniel Grumiller, Mauricio Leston and Dmitri Vassilevich, Anti-de Sitter holography for gravity and higher spin theories in two dimensions, hep-th/1311.7413


2012

  • TUW-12-01 M. Gary, D. Grumiller and R. Rashkov, Towards non-AdS holography in 3-dimensional higher spin gravity hep-th/1201.0013
  • TUW-12-02 P. Anastasopoulos, I. Antoniadis, K. Benakli, M.D.Goodsel and A. Vichi, One-loop adjoint masses for branes at non-supersymmetric angles hep-th/1201.2663
  • TUW-12-03 A. Ipp, J. Evers, C. H. Keitel, K. Z. Hatsagortsyan, Streaking at high energies with electrons and positrons hep-ph/1202.0180
  • TUW-12-04 A.P. Braun, A. Collinucci and R. Valandro, Algebraic description of G-flux in F-theory: new techniques for F-theory phenomenology hep-th/1202.5029
  • TUW-12-05 H. Steinacker, Gravity and compactified branes in matrix models hep-th/1202.6306
  • TUW-12-06 Gabriela-Raluca Mocanu and Daniel Grumiller Self-organized criticality in boson clouds around black holes astro-ph/1203.4681
  • TUW-12-07 Victor Batyrev and Maximilian Kreuzer Conifold degenerations of Fano 3-folds as hypersurfaces in toric varieties math.AG/1203.6058
  • TUW-12-08 Harald Skarke How to Classify Reflexive Gorenstein Cones hep-th/1204.1181
  • TUW-12-09 Niklas Johansson, Ali Naseh and Thomas Zojer Holographic two-point functions for 4d log-gravity hep-th/1205.5804
  • TUW-12-10 A.P. Braun, J.Knapp, E.Scheidegger, H.Skarke and N.-O. Walliser PALP: a User Manual math.AG/1205.4147
  • TUW-12-11 D.Arnaudov, R.C.Rashkov On semiclassical four-point correlators in AdS5 x S5 hep-th/1206.2613
  • TUW-12-12 A. Ipp, P. Somkuti Yoctosecond metrology through HBT correlations from a quark-gluon plasma hep-th/1207.0197
  • TUW-12-13 R. Baier, S. Stricker, O. Taanila, A. Vuorinen Production of Prompt Photons: Holographic Duality and Thermalization hep-ph/1207.1116
  • TUW-12-14 R. Baier, S. Stricker, O. Taanila, A. Vuorinen Holographic dilepton production in a thermalizing plasma hep-ph/1205.2998
  • TUW-12-15 A. Rebhan, D. Steineder Probing Two Holographic Models of Strongly Coupled Anisotropic Plasma hep-th/1205.4684
  • TUW-12-16 M. Attems, A. Rebhan, M. Strickland Instabilities of an anisotropically expanding non-Abelian plasma: 3D+3V discretized hard-loop simulations hep-ph/1207.5795
  • TUW-12-17 P. Candelas, A. Constantin, H. Skarke An Abundance of K3 Fibrations from Polyhedra with Interchangeable Parts hep-th/1207.4792
  • TUW-12-18 A. Gynther, A. Rebhan, D. Steineder Thermodynamics and phase diagram of anisotropic Chern-Simons deformed gauge theories hep-th/1207.6283
  • TUW-12-19 Michal Michalcik, Radoslav C. Rashkov, "On finite size corrections to the dispersion relations of giant magnon and single spike on γ-deformed T^{1,1}" hep-th/1208.0698
  • TUW-12-20 Arjun Bagchi, Stephane Detournay and Daniel Grumiller Flat-Space Chiral Gravity hep-th/1208.1658
  • TUW-12-21 Stanley Deser, Sabine Ertl and Daniel Grumiller Canonical bifurcation in higher derivative, higher spin, theories hep-th/1208.0339
  • TUW-12-22 H. Afshar, M. Gary, D. Grumiller, R. Rashkov and M. Riegler Non-AdS holography in 3-dimensional higher spin gravity - General recipe and example hep-th/1209.2860
  • TUW-12-23 D. Steineder, S. A. Stricker and A. Vuorinen Thermalization at intermediate coupling hep-ph/1209.0291
  • TUW-12-24 M. Gary A Holographic Holographic Bound and the Black Hole S-Matrix hep-th/1209.3040
  • TUW-12-25 M. Bertin, S. Ertl, P. Ghorbani, D. Grumiller, N. Johansson and D. Vassilevich Lobachevsky holography in conformal Chern-Simons gravity hep-th/1212.3335
  • TUW-12-26 J. Aparicio, D. Grumiller, E. Lopez, I. Papadimitriou and S. Stricker Bootstrapping gravity solutions hep-th/1212.3609
  • TUW-12-27 Harald Skarke Why is the Legendre Transformation Involutive? math-ph/1209.6193
  • TUW-12-28 K. Chelabi, M. Schweda and S. Kouadik Translation-Invariant Renormalizable Noncommutative Chern-Simons Theory hep-th/1207.4591
  • TUW-12-29 D. N. Blaschke, T. Garschall, F. Gieres, F. Heindl, M. Schweda and M. Wohlgenannt On the Renormalization of Non-Commutative Field Theories hep-th/1207.5494
  • TUW-12-30 D. Grumiller, R. McNees and S. Zonetti, Black holes in the conical ensemble, gr-qc/1210.6904
  • TUW-12-31 A. Ipp, Unstable dynamics of Yang-Mills fields at early times of heavy ion collisions, hep-th/1210.5150
  • TUW-12-32 P. Anastasopoulos, M. Cvetic, R. Richter, P. Vaudrevange Discrete symmetries in semi-realistic orientifold compactifications, hep-th/1210.xxxx
  • TUW-12-33 P. Anastasopoulos, M. Goodsell, R. Richter, Excited twist correlators in open string models, hep-th/1211.xxxx
  • TUW-12-34 H. Afshar, M. Gary, D. Grumiller, R. Rashkov and M. Riegler, Semi-classical unitarity in 3-dimensional higher-spin gravity for non-principal embeddings, hep-th/1211.4454
  • TUW-12-35 H. Afshar, H. Firouzjahi and S. Parvizi, dS solutions with co-dimension two branes in six dimensions, hep-th/1212.xxxx
  • TUW-12-37 D. Parganlija, P. Kovacs, Gy. Wolf, F. Giacosa and D. Rischke, Meson vacuum phenomenology in a three-flavor linear sigma model with (axial-)vector mesons, hep-ph/1208.0585
  • TUW-12-38 D. Parganlija, P. Kovacs, Gy. Wolf, F. Giacosa and D. Rischke, Phenomenology of Axial-Vector Mesons from an Extended Linear Sigma Model, hep-ph/1208.2054
  • TUW-12-39 D. Parganlija, P. Kovacs, Gy. Wolf, F. Giacosa and D. Rischke, Scalar mesons in a linear sigma model with (axial-)vector mesons, hep-ph/1208.5611
  • TUW-12-40 F. Giacosa, D. Parganlija, P. Kovacs and Gy. Wolf, Phenomenology of light mesons within a chiral approach, hep-ph/1208.6202


2011

  • TUW-11-01 R. S. Garavuso, L. Katzarkov, M. Kreuzer and A. Noll, Super Landau-Ginzburg mirrors and algebraic cycles hep-th/1101.1368
  • TUW-11-02 J. Knapp, M. Kreuzer, C. Mayrhofer and N.-O. Walliser, Toric Construction of Global F-Theory GUTs, JHEP03(2011)138, hep-th/1101.4908
  • TUW-11-03 J. Knapp and M. Kreuzer, Toric Methods in F-theory Model Building hep-th/1103.3358
  • TUW-11-04 A. Ipp, Yoctosecond photon pulse generation in heavy ion collisions hep-ph/1102.0420
  • TUW-11-05 S. Carloni, D. Grumiller and F. Preis, Solar system constraints on Rindler acceleration astro-ph/1103.0274
  • TUW-11-06 M. Bertin, D. Grumiller, D. Vassilevich and T. Zojer, Generalised massive gravity one-loop partition function and AdS/(L)CFT hep-th/1103.5468
  • TUW-11-07 H. Afshar, B. Cvetkovic, S. Ertl, D. Grumiller and N. Johansson, Holograms of Conformal Chern-Simons Gravity hep-th/1106.6299
  • TUW-11-08 D. Arnaudov, R.C. Rashkov, and T. Vetsov, Three- and four-point correlators of operators dual to folded string solutions in AdS_5 x S^5 hep-th/1103.6145
  • TUW-11-09 P. Anastasopoulos, I. Antoniadis, K. Benakli, M.D.Goodsel and A. Vichi, One-loop adjoint masses for non-supersymmetric intersecting branes hep-th/1105.0591
  • TUW-11-10 D. Arnaudov and R.C. Rashkov, Quadratic corrections to three-point functions hep-th/1106.0859
  • TUW-11-11 D. Arnaudov and R.C. Rashkov, Three-point correlators: examples from Lunin-Maldacena background hep-th/1106.4298
  • TUW-11-12 A. P. Braun and N.-O. Walliser, A new offspring of PALP hep-th/1106.4529
  • TUW-11-13 A. Rebhan and D. Steineder, Electromagnetic signatures of a strongly coupled anisotropic plasma hep-th/1106.3539
  • TUW-11-14 M. Cicoli, M. Kreuzer and Christoph Mayrhofer, Toric K3-Fibred Calabi-Yau Manifolds with del Pezzo Divisors for String Compactifications hep-th/1107.0383
  • TUW-11-16 C.-M. Chen, S. Hu, T. Li, D.V. Nanopoulos, Type IIB Supersymmetric Flux vacua hep-th/1107.3465
  • TUW-11-17 K. Z. Hatsagortsyan, A. Ipp, J. Evers, A. Di Piazza, and C. H. Keitel, Ultra-strong laser pulses: streak-camera for gamma-rays via pair production and quantum radiative reaction physics.ins-det/1107.4036
  • TUW-11-18 D. Burke and R. Wimmer, Quantum energies and tensorial central charges of confined monopoles hep-th/1107.3568
  • TUW-11-19 A.P. Braun, A. Collinucci and R. Valandro, G-Flux in F-theory and algebraic cycles hep-th/1107.5337
  • TUW-11-20 A.P. Braun, N. Johansson, M. Larfors and N.-O. Walliser, Restrictions on infinite sequences of type IIB vacua hep-th/1108.1394
  • TUW-11-21 S. Carlip and D. Grumiller, Lower bound on the spectral dimension near a black hole gr-qc/1108.4686
  • TUW-11-22 H. Afshar, B. Cvetkovic, S. Ertl, D. Grumiller and N. Johansson, Conformal Chern-Simons holography - lock, stock and barrel hep-th/1110.5644
  • TUW-11-23 P. Anastasopoulos, M. Bianchi and R. Richter, Light stringy states hep-th/1110.5424
  • TUW-11-24 P. Anastasopoulos, M. Bianchi and R. Richter, On closed-string twist-field correlators and their open-string descendants hep-th/1110.5359
  • TUW-11-25 Michal Michalcik, Radoslav C. Rashkov, Maria Schimpf, Three-point correlators: Examples from Lunin-Maldacena background hep-th/1107.5795
  • TUW-11-26 D. Arnaudov and R.C. Rashkov, Subleading semiclassical four-poinr functions hep-th/1111.xxxx
  • TUW-11-27 F. Preis, A. Rebhan and A. Schmitt, Holographic baryonic matter in a background magnetic field hep-th/1109.6904
  • TUW-11-28 A. Rebhan and D. Steineder, Violation of the Holographic Viscosity Bound in a Strongly Coupled Anisotropic Plasma hep-th/1110.6825


2010

  • TUW-10-01 D.N. Blaschke, E. Kronberger, R.I.P. Sedmik and M. Wohlgenannt, Gauge Theories on Deformed Spaces math.AG/1106.4529
  • TUW-10-02 V.G. Filev and R.C. Rashkov, Magnetic Catalysis of Chiral Symmetry Breaking. A Holographic Prospective. hep-th/1010.0444
  • TUW-10-03 S. Ertl, D. Grumiller and N. Johansson, All stationary axi-symmetric local solutions of topologically massive gravity. hep-th/1006.3309
  • TUW-10-04 A. Gynther, K. Landsteiner, F. Pena-Benitez and A. Rebhan, Holographic Anomalous Conductivities and the Chiral Magnetic Effect hep-th/1005.2587
  • TUW-10-05 C. P. Herzog, S. A. Stricker and A. Vuorinen, Hyperfine splitting and the Zeeman effect in holographic heavy-light mesons hep-th/1005.3285
  • TUW-10-06 C.-M. Chen and Y.-C. Chung, Flipped SU(5) GUTs from E8 singularity in F-theory hep-th/1005.5728
  • TUW-10-07 C.-M. Chen , J. Knapp , M. Kreuzer and C. Mayrhofer, Global SO(10) F-theory GUTs hep-th/1005.5735
  • TUW-10-08 M. Schweda and M. Wohlgenannt, On NCQFT and dimensionless insertions hep-th/1005.5107
  • TUW-10-09 D. Arnaudov, H. Dimov and R.C. Rashkov, On the pulsating strings in $AdS_5\times T^{1,1}$ hep-th/1005.1539
  • TUW-10-10 Jean-Paul Blaizot, Andreas Ipp, Nicolás Wschebor, Calculation of the pressure of a hot scalar theory within the Non-Perturbative Renormalization Group hep-th/1007.0991
  • TUW-10-11 Matthias R. Gaberdiel, Daniel Grumiller and Dmitri Vassilevich, Graviton 1-loop partition function for 3-dimensional massive gravity hep-th/1007.5189
  • TUW-10-12 Andreas Ipp, Jörg Evers, Christoph H. Keitel, Karen Z. Hatsagortsyan, Streaking at high energies with electrons and positrons hep-th/1008.0355
  • TUW-10-13 Daniel Grumiller, Niklas Johansson and Thomas Zojer, Short-cut to new anomalies in gravity duals to logarithmic conformal field theories hep-th/1010.4449
  • TUW-10-14 Matteo Beccaria, Maximilian Kreuzer and Andrea Puhm, Counting charged massless states in the (0,2) heterotic CFT/geometry connection hep-th/1010.4564
  • TUW-10-16 P. Anastasopoulos, G. K. Leontaris, R. Richter, A. N. Schellekens, SU(5) D-brane realizations, Yukawa couplings and proton stability hep-th/1010.5188
  • TUW-10-17 Andreas Ipp, Anton Rebhan, Michael Strickland, Non-Abelian plasma instabilities: SU(3) vs. SU(2) hep-ph/1012.0298
  • TUW-10-18 M.E. Carrington and A. Rebhan, Perturbative and Nonperturbative Kolmogorov Turbulence in a Gluon Plasma hep-ph/1011.0393
  • TUW-10-20 D. Arnaudov and R.C. Rashkov, On semiclassical calclation of three-point functions in AdS_4 x CP^3 hep-th/1011.4669
  • TUW-10-21 F. Preis, A. Rebhan and A. Schmitt, Inverse magnetic catalysis in dense holographic matter hep-th/1012.4785


Previous years

2009, 2008, 2007, 2006, 2005, 2004, 2003, 2002, 2001, 2000, 1999, 1998, 1997, 1996

For published articles, talks, and poster presentations see Publications

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