Yonit Hochberg
22/09/2020, 13:45
Mr
Paul Frederik Depta
(DESY)
22/09/2020, 14:15
Cosmology & Astroparticle Physics
Dark matter (DM) as a thermal relic of the primordial plasma is increasingly pressured by direct and indirect searches, while the same production mechanism in a decoupled sector is much less constrained. We extend the standard treatment of the freeze-out process to such scenarios and perform precision calculations of the annihilation cross section required to match the observed DM abundance....
Oindrila Ghosh
(II. Institute for Theoretical Physics, University of Hamburg)
22/09/2020, 14:28
Cosmology & Astroparticle Physics
I will describe a new scheme for the detection of radio signals from the decay of axions and axion-like particles, called *axion gegenschein*, using next-generation facilities such as SKA. Ambient radiation arriving from astrophysical radio-bright objects drive stimulated decay in the Galactic halo creating a *countersource* with the dimensions and morphological features of each source in the...
Mrs
Ersilia Guarini
(Physics Department, University of Bari)
22/09/2020, 14:41
Cosmology & Astroparticle Physics
Axions can be produced in the Sun via the Primakoff process leading to conversions of thermal photons into axions in the flucutuating electric and magnetic fields generated by the charged particles in the stellar plasmas. Currently this flux is searched by the helioscope experiment CAST at CERN. A future generation helioscope experiment, called IAXO, is currently under investigation.
Seismic...
Mr
Stefan Stelzl
(TUM Munich)
22/09/2020, 14:54
Cosmology & Astroparticle Physics
We consider finite density effects in models with a metastable ground state. We find that sufficiently dense objects, such as neutron stars, can destabilise the metastable minimum allowing for classical formation of bubbles of a new vacuum. As we show, these bubbles are not necessarily confined to the dense region, but can escape to infinity. This leads to a phase transition in the universe...
Dr
Cem Eröncel
(DESY)
22/09/2020, 15:07
Cosmology & Astroparticle Physics
Axion-like-particle (ALP) is a well-motivated candidate for dark matter, and it is subject to extensive theoretical and experimental research in recent years. The ALP production mechanisms mostly studied in the literature are misalignment, thermal production in the plasma, and decay of cosmic strings. Recently, a new mechanism, axion fragmentation, has been proposed. It can arise if the axion...
Mr
Wolfram Ratzinger
(Johannes Gutenberg University Mainz)
22/09/2020, 15:20
Cosmology & Astroparticle Physics
Conventional approaches to probing axions and axion-like particles (ALPs) typically rely on a coupling to photons. However, if this coupling is extremely weak, ALPs become invisible and are effectively decoupled from the Standard Model. We show that such invisible axions, which are viable candidates for dark matter, can produce a stochastic gravitational wave background in the...
Yvette Welling
(DESY)
22/09/2020, 15:33
Cosmology & Astroparticle Physics
Axion inflation entails a coupling of the inflaton field to gauge fields through the Chern-Simons term. This results in a strong gauge field production during inflation, which backreacts on the inflaton equation of motion. We show that this strongly non-linear system generically experiences a resonant enhancement of the gauge field production, resulting in oscillatory features in the inflaton...
Mariam Tortola
22/09/2020, 16:15
Miguel Escudero
(TUM)
22/09/2020, 16:45
Cosmology & Astroparticle Physics
At present, cosmological observations set the most stringent bound on the neutrino mass scale. Within the standard cosmological model (ΛCDM), the Planck collaboration reports $\Sigma m_\nu < 0.12$ eV at 95% CL. This bound, taken at face value, excludes many neutrino mass models. However, unstable neutrinos, with lifetimes shorter than the age of the universe $\tau_\nu < t_U$, represent a...
Mr
Sven Baumholzer
(Johannes Gutenberg-Universitaet Mainz)
22/09/2020, 16:58
Cosmology & Astroparticle Physics
In the framework of the scotogenic model, which features radiative generation of neutrino
masses, we explore light dark matter scenario. Throughout the paper we chiefly focus on
keV-scale dark matter which can be produced either via freeze-in through the decays of the
new scalars, or from the decays of next-to-lightest fermionic particle in the spectrum, which
is produced through...
Mr
Petter Taule
(Technical University of Munich)
22/09/2020, 17:11
Cosmology & Astroparticle Physics
Current and near future surveys are expected to map out the large-scale structure of the Universe at unprecedented precision. In order to extract information from observational data, a solid theoretical understanding is required, and in recent years considerable efforts has been dedicated to model the weakly non-linear regime using perturbative methods. In this talk, I will describe an...
Dr
Chandan Hati
(Technische Universität München, James-Franck-Straße 1, D-85748 Garching, Germany)
22/09/2020, 17:24
Cosmology & Astroparticle Physics
Neutron-antineutron ($n-\bar{n}$) oscillation violates baryon number by two units and an observable rate of such a process would strongly advocate physics beyond the Standard Model (BSM). Many prospective future experiments such as ESS and DUNE are planning to search for $n-\bar{n}$ oscillation improving on the current limits. In this talk, we will discuss the impact of the observation of...
Dr
Alexandra Dobrynina
(P. G. Demidov Yaroslavl State University & University of Hamburg)
22/09/2020, 17:37
Cosmology & Astroparticle Physics
An influence of a magnetic field on beta-processes is investigated under conditions of a core-collapse supernova. For realistic magnetic fields reachable in astrophysical objects we obtain simple analytical expressions for reaction rates of beta-processes as well as the energy and momentum transferred from neutrinos and antineutrinos to the matter. Based on the results of one-dimensional...
Mr
Pierluca Carenza
(Università degli Studi di Bari)
22/09/2020, 17:50
Cosmology & Astroparticle Physics
The cumulative emission of Axion-Like Particles (ALPs) from all past core-collapse supernovae (SNe) would lead to a diffuse flux with energies ${\mathcal O}(50)$ MeV. We use this to constrain ALPs featuring couplings to photons and to nucleons. ALPs coupled only to photons are produced in the SN core via the Primakoff process,and then converted into gamma rays in the Galactic magnetic field....
Mr
Henrique Rubira
(DESY)
22/09/2020, 18:03
Cosmology & Astroparticle Physics
LISA telescope will be specially interesting to probe the scenario of a first order phase transition happening close to the electroweak scale. Recently, it became evident that the main contribution to the GW spectra would come from the sound waves propagating through the plasma. Current estimates of the GW spectra are based on numerical simulations of a scalar field interacting with the plasma...
Lorenzo Tancredi
(CERN TH)
23/09/2020, 13:45
Mr
Alejo Nahuel Rossia
(DESY, HU Berlin)
23/09/2020, 14:15
Particle Phenomenology
The lack of evidence of New Physics coming from direct searches of resonances at the LHC calls for an increase in efforts to devise new observables that can indirectly probe New Physics. Additionally, the future FCC-hh will make available new processes, inaccessible so far due to their low number of events. Studying the high transverse momentum distribution of diboson production processes at...
Mr
Sebastian Bruggisser
(ITP Heidelberg)
23/09/2020, 14:30
Particle Phenomenology
I will discuss a global analysis of Run II top measurements at the LHC in terms of dimension-6 operators. A distinctive feature of the top sector is the large number of four-fermion operators. This potentially leads to a large number of degeneracies. I will show in detail how those degeneracies can be resolved and how quadratic terms lead to stable limits on each of the Wilson coefficients.
Mr
Maximilian Dichtl
(TUM)
23/09/2020, 14:45
Particle Phenomenology
We present collider probes of the GRSMEFT, the most general effective field theory of gravity coupled to the SM of particle physics. In particular, we focus on graviton production in association with a jet, for which we derive the leading new-physics scattering amplitude, the expected cross section, and compare with missing energy searches at the LHC in order to bound the size of the relevant...
Ulserik Moldanazarova
(University of Liverpool)
23/09/2020, 15:00
Particle Phenomenology
In this talk we will discus the flavour violating four-fermion interactions and dipole interaction in models with extra heavy particles whose masses are
equal to or above the electro-weak scale.
We use the Becchi-Rouet-Stora-Tyutin symmetry to constrain tree-level couplings to construct perturbatively unitary theories, for which we calculate one-loop corrections.
We focus on the gauge...
Ms
Bianka Mecaj
(Johannes Gutenberg University)
23/09/2020, 15:15
Particle Phenomenology
Soft functions enter in factorization theorems in soft collinear effective field theory (SCET) and they capture the large distance effects of a process. They are defined as matrix elements of soft fields dressed by Wilson lines. While at leading order in power counting they are described by emissions of soft gauge bosons at sub-leading order one needs to consider emissions of soft fermions...
Dr
Wojciech Kotlarski
(TU - Dresden)
23/09/2020, 15:30
Particle Phenomenology
We present FlexibleDecay - a tool to calculate decays of scalars in arbitrary BSM models.
BSM effects are taken into account at the leading order - meaning that for loop induced decays all one-loop BSM contributions are automatically included.
In case of scalar and pseudoscalar Higgs boson decays the known higher order SM QED, QCD and EW effects are taken into account where possible....
Stefania Gori
(UCSC)
23/09/2020, 16:15
Kåre Fridell
(Technical University of Munich)
23/09/2020, 16:45
Particle Phenomenology
We investigate the possibility to probe lepton number violating (LNV) operators in the rare kaon decay $K\to\pi\nu\nu$. Performing the analysis in the Standard Model effective field theory with only light active Majorana neutrinos, we determine the current limits on the corresponding LNV physics scale from the past E949 experiment at BNL as well as the currently operating experiments NA62 at...
Mr
Rigo Bause
(TU Dortmund)
23/09/2020, 17:00
Particle Phenomenology
Rare $|\Delta c|=|\Delta u|=1$ processes are unique probes of flavour physics in the Standard Model (SM) and beyond and provide an excellent opportunity to analyse CP-violation and search for new physics (NP) due to their strong GIM-suppression in the SM.
Furthermore, a variety of null test observables is available for decays, such as $D\to \pi \ell^+ \ell^-$, $\ell = e,\,\mu$, and provide...
Mr
Marvin Schnubel
(Johannes Gutenberg-University Mainz)
23/09/2020, 17:15
Particle Phenomenology
Axionlike Particles (ALPs) appear in many well-motivated extensions of the Standard Model. Their lepton-flavor violating couplings can be probed in exotic muon and tau decays. When ALPs are produced resonantly, the sensitivity of three-body decays such as $\mu\to3e$ and $\tau\to3\mu$ exceeds that of radiative decays like $\mu\to e\gamma$ and $\tau\to\mu\gamma$ by multiple orders of magnitude....
Gonzalo Alonso Álvarez
(Heidelberg University)
23/09/2020, 17:30
Particle Phenomenology
The low-energy phenomenology of the QCD axion is usually studied in a model-independent way using an effective Lagrangian. However, one-loop processes that exhibit logarithmic divergencies are sensitive to the high-energy completion of each specific model. This is extremely important for some axion searches, like the ones conducted at Kaon facilities such as NA62 that aim to look for the rare...
Quentin Bonnefoy
(DESY)
23/09/2020, 17:45
Particle Phenomenology
I will revisit EFT couplings between an axion and massive gauge bosons. It is known that massive vectors allow for more freedom than massless ones when building an EFT, thanks to the existence of the non-linear realization of (gauge) symmetries. It is also known that such a non-linear realization must sometimes be used even to describe physics at energy scales above the electroweak vev, due to...
Ms
Clara Hormigos-Feliu
(TU Dortmund)
23/09/2020, 18:00
Particle Phenomenology
Standard Model extensions inspired by asymptotic safety generally contain vector-like fermions and singlet matrix scalar fields. Here we study several models where three generations of colorless vector-like fermions allow for portal Yukawa interactions
with leptons, leading to rich phenomenological implications. A novel feature is that the enlarged scalar sector, which also contains a Higgs...
Mr
Christoph Dlapa
(Max Planck Institute for Physics)
24/09/2020, 13:45
Strings & Mathematical Physics
Differential equations are a powerful tool for computing Feynman integrals. Their solution is straightforward if one can find a transformation to a certain ‘canonical’ form, where the answer is manifestly given in terms of iterated integrals, such as multiple polylogarithms. An algorithmic way to construct the necessary transformation is therefore highly desired, and recent years have seen...
Niklas Henke
(DESY)
24/09/2020, 14:05
Strings & Mathematical Physics
Using the symbol bootstrap, loop amplitudes of planar $\mathcal{N}=4$ SYM theory can be obtained from their alphabet, the list of their singularities. The elements of this alphabet, the letters, coincide with the variables of certain cluster algebras. However, at eight and more particles these cluster algebras become infinite, whereas it is believed that the amplitudes only have finitely many...
Mr
Christoph Nega
(Bethe Center for Theoretical Physics)
24/09/2020, 14:25
Strings & Mathematical Physics
Using the Gelfand-Kapranov-Zelevinsk\u{\i} system for the primitive cohomology
of an infinite series of complete intersection Calabi-Yau manifolds, whose dimension is the loop
order minus one, we completely clarify the analytic structure of all banana amplitudes with arbitrary
masses. In particular, we find that the leading logarithmic structure in the high energy regime, which ...
Mr
Anders Schreiber
(Brown University)
24/09/2020, 14:45
Strings & Mathematical Physics
A key challenge in the study of scattering amplitudes of $\mathcal{N}=4$ super-Yang-Mills theory is to understand their analytic structure. Symbols, a central tool in this topic, are known to contain particular cluster coordinates of $Gr(4,n)$ together with certain algebraic functions of cluster coordinates. In my talk, I will present an algorithm for computing symbol alphabets by solving...
Mr
Julian Miczajka
(Humboldt-Universität zu Berlin)
24/09/2020, 15:30
Strings & Mathematical Physics
Much of the calculational progress in $\mathcal{N}=4$ Super-Yang-Mills theory has been due to its integrability in the planar limit, which presents itself in form of an infinite-dimensional symmetry of Yangian-type. Recently it has been found that certain classes of ubiquituous massive Feynman diagrams feature a similar dual-conformal Yangian symmetry. I report on this progress and show how...
Dr
Markus Dierigl
(UPenn)
24/09/2020, 15:50
Strings & Mathematical Physics
In this talk I will summarize recent results on the fate of center 1-form symmetries in six and eight dimensions. In particular, I will discuss their interplay between other gauged higher-form symmetries causing obstructions to the gauging of the discrete center 1-form symmetries, which would result in non-simply connected non-Abelian gauge groups. In this way we can find previously unknown...
Dr
Daniel Kläwer
(Mainz University)
24/09/2020, 16:10
Strings & Mathematical Physics
We revisit infinite distance limits in the Kähler moduli space of F-theory compactifications to 4D with $\mathcal{N}=1$ supersymmetry. At the classical level, it is known that the existence of certain such limits imposes the structure of a rational or genus-one fibration on the three-dimensional base. As the fiber volume vanishes in the limit, wrapping the D3 brane on it gives rise to an...
Mrs
Nicole Righi
(DESY)
24/09/2020, 16:30
Strings & Mathematical Physics
I will present a mechanism for realising hybrid inflation using two axion fields with a purely non-perturbatively generated scalar potential. I will show that such model generates observationally viable slow-roll inflation for a wide range of initial conditions while accommodating certain Swampland conjectures. I will focus mainly on two possible avenues to embed harmonic hybrid inflation in...
Dr
Paul-Konstantin Oehlmann
(Uppsala University)
24/09/2020, 16:50
Strings & Mathematical Physics
In this work we consider pairs of elliptic Calabi-Yau threefolds, related by mirror symmetry that factorizes between fiber and base.
Extending work of Berglund and Mayr, this allows us to deduce the mirror dual base and fibration structures which we use to build up a dictionary between two different F-theory SUGRA theories:
The mirror acts as a quotient on the base while local gauge group...
Dr
Ignacio A. Reyes
(Max Planck Institute, Potsdam)
24/09/2020, 17:10
Strings & Mathematical Physics
Recent progress in our understanding of the black hole information paradox has lead to a new prescription for calculating entanglement entropies, which involves special subsystems in regions where gravity is dynamical, called *quantum extremal islands*. We present a simple holographic framework where the emergence of these islands can be understood in terms of the standard Ryu-Takayanagi...
Daniel Figueroa
25/09/2020, 13:30
Mr
Peera Simakachorn
(UHH and DESY)
25/09/2020, 14:00
Cosmology & Astroparticle Physics
A stochastic gravitational-wave (GW) background from cosmic strings spans a broad range of frequencies. By measuring the slope of its spectrum with future GW observatories, we can infer the equation of state of the universe much earlier than the onset of Big-Bang Nucleosynthesis (BBN). In this work, we consider a variety of cosmological scenarios beyond the standard hot-Big-Bang cosmology and...
Mr
Felix Giese
(DESY/Hamburg U.)
25/09/2020, 14:12
Cosmology & Astroparticle Physics
We study the energy budget of a first-order cosmological phase transition, which is an important factor in the prediction of the resulting gravitational wave spectrum. Formerly, this analysis was based mostly on simplified models as for example the bag equation of state. Here, we present a model-independent approach that is exact up to the temperature dependence of the speed of sound in the...
Mr
Juan S. Cruz
(Technical University Munich)
25/09/2020, 14:24
Cosmology & Astroparticle Physics
We study false vacuum decay for a gauged complex scalar field in a polynomial potential with nearly degenerate minima. Radiative corrections to the profile of the nucleated bubble as well as the full decay rate are computed in the planar thin-wall approximation using the effective action. This allows to account for the inhomogeneity of the bounce background and the radiative corrections in a...
Dr
Aleksandr Chatrchyan
(Heidelberg University, Institute for theoretical physics)
25/09/2020, 14:36
Cosmology & Astroparticle Physics
Axion-like particles (ALPs) play an important role in cosmology and, among others, are well motivated dark matter candidates. In the presence of a monodromy the discrete shift symmetry of ALPs can be broken, and this talk is devoted to the rich nonlinear dynamics that becomes available in such systems. We consider coherent oscillations of the field, which trigger the resonant amplification of...
Ricardo Landim
(Techinical University of Munich)
25/09/2020, 14:48
Cosmology & Astroparticle Physics
Extra dimensions (ED) have been used as attempts to explain several phenomena in particle physics, such as the hierarchy and flavor problems. The interaction between new mediators in the bulk (vector, scalar of fermion fields) and the Standard Model (SM) particles can be naturally suppressed if one employs a single, flat ED. In this setup, the SM fields are localized in a finite width ‘fat’...
Stefan Vogl
25/09/2020, 15:15
Dr
Christoph Borschensky
(Eberhard Karls Universität Tübingen)
25/09/2020, 15:45
Particle Phenomenology
In my talk, I will present a calculation of the next-to-leading order QCD corrections for the scattering of Dark Matter particles off nucleons in the framework of simplified models with $s$- and $t$-channel mediators. These results are matched to the Wilson coefficients and operators of an effective field theory that is generally used for the presentation of experimental results on...
Ms
Ghazal Ghafari
(Bonn University)
25/09/2020, 16:00
Particle Phenomenology
We postulate the WIMP neutralino Dark Matter's interaction with ordinary matter as scattering from the direct detection experiments' nucleon target. Recently, one of the most sensitive direct detection experiments XENON1T submitted an upper bound on the WIMP-Nucleon Spin-Independent elastic cross-section $ \sigma_{SI} $ at $ 4.1 \times 10^{-47} GeV^2 $ for a mass of $ 30 \frac{GeV}{c^2} $. We...
Dr
Elisa Todarello
(KIT)
25/09/2020, 16:15
Particle Phenomenology
Axion--photon interactions can lead to an enhancement of the electromagnetic field by parametric resonance in the presence of a cold axion background, for modes with a frequency close to half the axion mass. In this paper, we study the role of the axion momentum dispersion as well as the effects of a background gravitational potential, which can detune the resonance due to gravitational...
Mr
Maximilian Ruhdorfer
(Technical University of Munich)
25/09/2020, 16:30
Particle Phenomenology
We examine the contribution of small instantons to the axion mass in various UV completions of QCD. We show that the reason behind the potential dominance of such contributions is the non-trivial embedding of QCD into the UV theory. The effects from instantons in the partially broken gauge group appear as “fractional instanton” corrections in the effective theory. These will exhibit unusual...
Dr
Markus B. Fröb
(Universität Leipzig)
25/09/2020, 17:00
Strings & Mathematical Physics
I present a formula for the coupling-constant derivative of the coefficients of the operator product expansion (Wilson OPE coefficients) in an arbitrary curved space, as the natural extension of the quantum action principle. Expanding the coefficients themselves in powers of the coupling constants, this formula allows to compute them recursively to arbitrary order. As input, only the OPE...
Domenico Bonocore
(University of Münster)
25/09/2020, 17:20
Strings & Mathematical Physics
The worldline representation of the relativistic spinning particles has been known for a long time. Much of the studies focused on the calculation of effective actions, with less attention to open propagators. In 0811.2067 the formalism has been applied to asymptotic states dressed by soft radiation at next-to-leading power (NLP) in the soft expansion. This led to the definition of the...
Mr
Joren Brunekreef
(Radboud University)
25/09/2020, 17:40
Strings & Mathematical Physics
Causal Dynamical Triangulation (CDT) is a non-perturbative theory of quantum gravity. It is based on a lattice discretization of general relativity, where the background metric should emerge dynamically. This makes it difficult to construct suitable observables in the model. A recent addition to the list of available CDT observables is the Quantum Ricci Curvature (QRC), which allows one to...
Gizem Sengor
(CEICO at the Institute of Physics of the Czech Academy of Sciences)
25/09/2020, 18:00
Strings & Mathematical Physics
In this talk we will focus on free scalar fields of various mass on D-dimensional de sitter, define late time boundary states from their late time behavior, discuss how they are classified in terms of irreducible representations of the symmetry group of de Sitter SO(1,D) by considering their inner products and say a few words about their correlators.