H2020Individual fellowship2018–2021

InflaBoot · Bootstrapping Inflationary Cosmology

Horizon 2020 — Marie Skłodowska-Curie Actions

Duration
2018-10-01 → 2021-09-30
EU contribution
€240,530
Participants
2
Scheme
MSCA-IF

Lines connect the coordinator with its partners.

Results in brief

Bootstrapping Inflationary Cosmology

"Cosmology is the source, but also the adjudicator, of some of the biggest questions in physics. There is growing evidence that the very early universe underwent a period of rapid, approximately de Sitter (dS), inflationary expansion -- providing an elegant explanation for the primordial density fluctuations inferred from observations of the cosmic microwave background and the large-scale structure of the universe. Since the energy scale of inflation could be as high as 10^14 Gev, far beyond the reach of our terrestrial experiments, this would make inflation the highest energy observable natural process. We are therefore presented with a remarkable opportunity to probe the laws of physics at these scales, which thus far have remained rather elusive. In anticipation of increasingly precise observations it is imperative that we understand how to extract information about the laws of physics at such scales. While in recent years there have been significant theoretical advances in our understanding of cosmological correlation functions, we still find it challenging to isolate fundamental physics from them. In particular, we don’t yet have a firm grasp of the rules that govern cosmological correlators, so that, naively, it would appear that anything goes. At the same time, the last few decades has seen significant advances in our understanding of gravitational observables. In particular, the striking notion that Quantum Gravity is “holographic” in nature -- in studying Quantum Gravity, we are led to consider holographic theories for the boundary observables at infinity. The most precise formulation of such a duality is the AdS/CFT correspondence, where boundary observables of Quantum Gravity in asymptotically anti-de Sitter (AdS) space are given by correlation functions of a Conformal Field Theory (CFT) in flat space-time. In this setting, the rules that govern gravitational observables in anti-de Sitter space are given by those of consistent CFTs, for which various powerful techniques have been developed in last decade within the framework of the “Conformal Bootstrap”. By extending this understanding of observables in AdS space to dS, which are related by analytic continuation, this would provide key insights into understanding the ""rules of the game"" for cosmological correlators. This is the overall objective of the project. In particular, to extend Conformal Bootstrap techniques and results that so far have been tailored to physics in anti-de Sitter to physics in de Sitter space."

Data: CORDIS, © European Union

Project objective

Cosmic inflation is one of the most promising explanations for the origin of the structure in the observed universe. However, while quantum-mechanical fluctuations during an early epoch of inflationary expansion provides a remarkably good description of the data, establishing the precise field content during inflation is a fundamental challenge for primordial cosmology. Since it is almost certain that the inflationary era involved physics beyond the Standard Model, this is also an incredible opportunity to learn about physics at the highest energy scales from current and future cosmological observations.On the theoretical side, it is important to classify the signatures of new degrees of freedom in primordial correlation functions to compare with observations. However, progress has been hindered due to the lack of tools to go beyond the simplest of cases. I propose a research and training programme to develop new systematic tools at the interface between scattering methods in de Sitter (dS) space, and, via holography, the conformal bootstrap in the dual CFT picture, to carve out the non-Gaussianities associated to: (1) Regge trajectories of higher-spin fields predicted by string theory/other UV complete theories of gravity (2) partially massless higher-spin fields, both at tree and 1-loop level. This proposal combines my expertise on higher-spin theories, scattering methods on anti-dS and holography with extensive training on various aspects of inflation and CMB physics from world-leading experts at IAS Princeton. The project will be completed at ULB, whose complementary expertise on higher-spins and holography will provide fertile ground to transfer my knowledge gained from the outgoing phase and continue the directions generated by the project. The importance of the project outcomes to cosmology and high-energy physics, as well as the experience gained, will facilitate me in obtaining a junior researcher position in Europe – the natural next step in my career.

Original text from CORDIS.

Participants

  • UNIVERSITE LIBRE DE BRUXELLES · Bruxelles / BrusselCoordinatorBelgium
  • INSTITUTE FOR ADVANCED STUDY - LOUIS BAMBERGER AND MRS FELIX FULD FOUNDATION CORPORATION · PRINCETONUnited States

Links

Data: CORDIS, © European Union