## Fluid-Gravity correspondence and its application to Quark Gluon Plasma

##### Michael Lublinsky

One of the most intriguing and fundamental questions is a formation of Quark Ggluon Plasma (QGP). Experimentally, QGP is created in the heavy ion collisions. A quest for QGP is the driving force behind two major experimental programs, one at the Relativistic Heavy Ion Collider (RHIC) and another one at the LHC.

Among most striking recent discoveries is the observation made at the RHIC that QGP produced there at temperatures about twice the QCD critical temperature is in fact strongly coupled. The  RHIC data  indicate that QGP at not too high temperatures behaves like a nearly perfect fluid with relativistic hydrodynamics being an appropriate description of the observed phenomena. Remarkably, gauge theories at strong coupling can be studied using the AdS/CFT duality: from the string theory point of view, QGP is holographically dual to weakly coupled string theory in the 5-dimensional  Anti-de-Sitter (AdS) Black Hole background metric.  Many interesting phenomena relevant for heavy ion collisions can be learn from the (super) gravity approximation to the string theory. In particular by studying gravitons absorption into the AdS Black Hole within Einsteins general relativity, one can learn a great deal about dissipative processes taking place in QGP.

## Quantum Chromo-Dynamics at high energies

##### Michael Lublinsky

We have entered the fascinating era of the Large Hadron Collider: the initial proton and heavy
ion collisions are already underway. Heavy ion collisions provide the unique possibility of
creating and studying a new state of matter, known as quark gluon plasma, at energy densities
and temperatures similar to those of the early Universe at $$10^{-5}$$ seconds after the Big Bang.
The microscopic theory describing the structure of protons and nuclei is the theory of strong
interactions, know as Quantum ChromoDynamics (QCD). Even though the fundamental theory
is known, it is extremely dicult to deduce from the QCD results of collision processes. This is
due to the high level of complexity of the theory involving mutual interactions between gluons,
the "photons" of strong interactions. When probed at very high energies, heavy nuclei, and
even protons, appear as very dense clouds of gluons. The main objective of this proposal is to
develop the theory of high energy collisions of dense gluonic objects, using rst principle QCD
calculation and apply it to experimental data on heavy ion collisions at the LHC.

## Methods to measure quark polarizations at the LHC

##### Yevgeny Kats
 While it's easy for the LHC detectors to reconstruct the momentum of an energetic quark by measuring the jet it produces, there is no straightforward way to determine the quark's polarization. We have pointed out that it is actually possible. For the bottom and charm quarks, which are heavy relative to the QCD scale, the polarization is expected to be largely preserved when they hadronize into the Λb and Λc baryons, respectively. With collaborators from the CMS experiment, we analyzed how such measurements can be done using various decays of these baryons. The most interesting application would be characterization of new physics processes producing bottom or charm quarks. While new physics is yet to be discovered, we motivated a set of Standard Model analyses for ATLAS, CMS, LHCb, BaBar and Belle that would help calibrate the polarization measurements. Further reading: Heavy baryons as polarimeters at colliders, M. Galanti, A. Giammanco, Y. Grossman, Y. Kats, E. Stamou, J. Zupan, JHEP 1511, 067 (2015) [pdf] Measuring c-quark polarization in W+c samples at ATLAS and CMS, Y. Kats, JHEP 1611, 011 (2016) [pdf] An example top-antitop event that can be used for measuring the polarization of c quarks produced in W boson decays.

For the strange quark, the heavy-quark approximation cannot be used. However, it is known from experiments at LEP that Λ baryons in fact preserve much of the strange-quark polarization. We argued that this allows measuring the polarization of strange quarks at the LHC. Furthermore, there are reasons to believe that up and down quarks hadronizing into a Λ may also be transferring some of their polarization. This may open the way for measuring their polarization as well. We motivated studies in top-quark samples in ATLAS and CMS that would provide additional information about the polarization transfer from the strange, up and down quarks to the Λ.

Further reading: Measuring polarization of light quarks at ATLAS and CMS, Y. Kats, Phys. Rev. D 92, 071503(R) (2015) [pdf]

Several additional interesting projects on these topics are underway or planned for the near future.

For more highlights see: https://physics.bgu.ac.il/~katsye

## Interplay between measurements in particle colliders and theories beyond the Standard Model

##### Yevgeny Kats

The most powerful particle physics experiment ever built, the Large Hadron Collider (LHC) at CERN, holds great promise. In 2012, it discovered the Higgs boson, and the significantly higher energy and collision rate that it provides today may allow discovering new types of particles, some of which could explain the various open questions in fundamental physics (the origin of the electroweak scale, dark matter, the matter-antimatter asymmetry in the Universe, and others).

While waiting for discoveries, the results of measurements and new-physics searches from the LHC can be re-used for examining the viability of new physics scenarios other than those for which they were originally designed. Determining the status of those scenarios involves simulating the relevant physical process, the resulting signatures in the detectors, and the analysis done in the experimental studies. As a welcome by-product, we identify general gaps in the experimental coverage of potential new physics signatures.

 In one such project, our goal was to clarify the experimental status of supersymmetry as a natural explanation for the electroweak symmetry breaking scale. Besides requiring the existence of a light superpartner (as at least the higgsino is expected to be light), and a gluino within the kinematic range of the 8 TeV LHC, we have kept our analysis quite general, allowing for arbitrary departures from any minimal model of supersymmetry. We were able to argue that gluino decays always give rise to either a significant amount of missing energy and/or frequently produce top quarks and/or large jet multiplicity, to the extent that they are covered by a certain class of LHC searches in each case. We have found that gluinos are almost always excluded up to masses above 1 TeV. We have also identified several classes of scenarios in which the limits were weaker, and proposed strategies for addressing these gaps. Further reading: Toward Full LHC Coverage of Natural Supersymmetry, J. A. Evans, Y. Kats, D. Shih, M. J. Strassler, JHEP 1407, 101 (2014) [pdf] In an earlier work, motivated by the lack of any signals in supersymmetry searches based on missing energy, we have addressed the status of more general models of supersymmetry, those that do not assume R-parity. As a compromise between minimizing the fine-tuning of the electroweak symmetry breaking scale, and the apparent absence of significant production of colored superpartners, we considered scenarios in which the only light colored superpartners are the third-generation squarks (and in particular, one of the stops). We constructed a set of simplified models that span the parameter space of the R-parity violating couplings and the mediators through which the stop may decay. We derived limits on these models using a complete set of potentially relevant recent LHC searches. We then looked into the least constrained scenarios in more detail and suggested several ideas for search methods that may allow addressing many of them. Further reading: LHC Coverage of RPV MSSM with Light Stops, J. A. Evans and Y. Kats, JHEP 1304, 028 (2013) [pdf] Currently we are analyzing certain novel LHC signatures predicted by the Clockwork Theory. Stay tuned! One of the LHC searches motivated by our models [CMS collaboration, Phys. Lett. B 739 (2014) 229]

Apart from providing feedback to the experimental community, this type of studies make us prepared to interpret any hints of new particles that the LHC might report in the future. One hint, near the mass of 750 GeV, was reported at the end of 2015. The hint has disappeared since then, by it made us think about various theoretical ideas that may still turn out useful in other contexts.

• Interpreting a 750 GeV Diphoton Resonance, R. S. Gupta, S. Jaeger, Y. Kats, G. Perez, E. Stamou, JHEP 1607, 145 (2016) [pdf]
• Resonances from QCD bound states and the 750 GeV diphoton excess, Y. Kats and M. J. Strassler, JHEP 1605, 092 (2016) [pdf]
• Colorful twisted top partners and partnerium at the LHC, Y. Kats, M. McCullough, G. Perez, Y. Soreq, J. Thaler, JHEP 1706, 126 (2017) [pdf]

## Vacuum Energy and Child Universes

##### Eduardo Guendelman

In particle physics, spontaneous breaking of scale invariance (SSB of SI) is applied to mechanisms for confinement of quarks and gluons, while in gravity and cosmology it relates to the acceleration of the present universe, quintessence scenarios and inflation of early universe. In gravity and cosmology, SSB of SI is nicely implemented in the context of the Two Measures Theory, which I have developed with Alex Kaganovich. This model addresses all the cosmological questions mentioned before and also provides an interesting solution to the 5th force problem that most quintessence scenarios suffer. I have also been studying the possibility of creating a universe in the laboratory starting from a bubble of false vacuum (see figure).

In particular, with Jacob Portnoy, I have considered the creation of a universe from a stable particle like configuration and with Idan Shilon, I study the gravitational trapping of particles by these stabilized particle like configurations.

## Determining the nature of dark energy

##### Ram Brustein

The accelerated expansion of our universe, and consequently that it apparently contains a substantial amount of dark energy are still unexplained. Interpreting and understanding the accelerating universe is arguably one of the major scientific challenges of our times. The challenge can be approached on several levels, from the most practical level: how to interpret the data, through an intermediate level: phenomenological models that can be embedded into theories of fundamental physics, to the most profound level: the cosmological constant problem.