Conveners
Parallel: Cosmology I
- Daniel Chung (Unknown)
Parallel: Dark Matter I
- Manfred Lindner (Max-Planck-Institut fuer Kernphysik, Heidelberg, Germany)
Parallel: Particle I
- Stuart Raby (The Ohio State University)
Parallel: Cosmology II
- Susha Louise Parameswaran (University of Liverpool)
Parallel: Dark Matter II
- Henry Sobel
Parallel: Particle II
- Yu-Dai Tsai (University of California, Irvine)
Parallel: Dark Matter III
- Dave Casper (University of California Irvine (US))
Parallel: Cosmology III
- Julian Heeck
Parallel: Particle III
- Ryuichiro Kitano
Parallel: Dark matter IV
- Brian Shuve (Harvey Mudd College)
Parallel: Particle IV
- Daniel Stolarski (Carleton University)
Parallel: Strings/formal I
- Saul Ramos-Sanchez (UNAM, Mexico)
Parallel: Dark Matter V
- Sebastian Trojanowski
Parallel: Particle V
- Lisa Everett
Parallel: Strings/formal II
- Daniel Harlow (MIT)
Parallel: Particle VI
- Yael Shadmi
Parallel: Cosmology IV
- Graciela Beatriz Gelmini (University of California Los Angeles (US))
Parallel: Dark Matter VI
- Ofri Telem (UC Berkeley)
Parallel: Dark Matter VII
- Xiao-Gang He
Parallel: Strings/formal III
- Christopher Verhaaren (Brigham Young University)
Parallel: Particle VII
- Ferruccio Feruglio
Parallel: Dark Matter VIII
- Delilah Gates (Princeton)
Parallel: Particle VIII
- Shufang Su (University of Arizona)
Parallel: Strings/formal IV
- Hans Peter Nilles (Institut fuer Theoretische Physik)
-
Saarik Kalia (University of Minnesota)26/06/2023, 14:20DM
Ultralight bosonic particles, including axionlike particles and kinetically mixed dark photons, can be promising dark matter candidates. It was recently shown that the Earth can act as a transducer for ultralight dark matter detection, by converting the dark matter into an oscillating monochromatic magnetic field signal across the Earth's surface. This occurs because the ground and ionosphere...
Go to contribution page -
Philipp Klose (Universitรคt Bern)26/06/2023, 14:20Cosmology
We revisit the framework of axion-like inflation, considering a warm inflation scenario in which the inflaton couples to the topological charge density of non-Abelian gauge bosons whose self-interactions result in a rapidly thermalizing heat bath. Including both dispersive (mass) and absorptive (friction) effects, we find that the system remains in a weak regime of warm inflation (thermal...
Go to contribution page -
shaikh saad (University of Basel)26/06/2023, 14:20Particle
Motivated by the direct discovery of gravitational waves (GWs) from black holes and neutron stars, there is a growing interest in investigating GWs from other sources. Among them, GWs from cosmic strings are particularly fascinating since they naturally appear in a large class of grand unified theories (GUTs). Remarkably, a series of pulsar-timing arrays (PTAs) might have already observed GWs...
Go to contribution page -
Dr Takahiro Terada (Institute for Basic Science)26/06/2023, 14:40Cosmology
Inflationary models, especially those with plateau-type potentials, are consistent with the cosmological data, but inflation itself does not resolve the initial singularity. This singularity is resolved, for example, by the idea of the quantum creation of the Universe from nothing such as the tunneling and no-boundary proposals. The simplest one predicts a closed Universe. Motivated by these...
Go to contribution page -
Kevin Hinze26/06/2023, 14:40Particle
What is the minimal viable renormalizable $SU(5)$ GUT with representations no higher than adjoints? In this talk I discuss a $SU(5)$ model in which vectorlike fermions $5_F+\overline{5}_F$ as well as two copies of $15_H$ Higgs fields are introduced in order to accommodate for correct charged fermion and neutrino masses and to reproduce the matter-antimatter asymmetry of the universe. The...
Go to contribution page -
Jacques Pienaar (The University of Chicago)26/06/2023, 14:40DM
The current best limits on properties of potential particle physics candidates for dark matter are set by direct dark matter detectors using high purity liquid xenon. XENONnT, with 5.9 tonnes of instrumented liquid xenon, was commissioned in the middle of 2021, and completed its first science run in 2022. This talk will present the results of the first science run of XENONnT.
Go to contribution page -
Yitian Sun26/06/2023, 15:20DM
Axion dark matter produces echo images of bright radio sources due to stimulated decay. These echo images take the form of a faint radio line centered at half the axion mass with a width determined by the dark matter velocity dispersion. Due to the kinematics of the decay, the echo image can either be antipodal to the incoming source of stimulating radiation (gegenschein) or can be along the...
Go to contribution page -
The CUORE Collaboration26/06/2023, 15:20Particle
The Cryogenic Underground Observatory for Rare Events (CUORE) is the first bolometric experiment searching for $0\nu\beta\beta$ decay that has been able to reach the one-tonne mass scale. The detector, located at the LNGS in Italy, consists of an array of 988 TeO$_2$ crystals arranged in a compact cylindrical structure of 19 towers. CUORE began its first physics data run in 2017 at a base...
Go to contribution page -
George Fanaras26/06/2023, 15:20Cosmology
In light of the recent swampland conjectures, we explore quantum cosmology and eternal inflation beyond the slow roll regime. We consider a model of a closed universe with a scalar field $\phi$ in the framework of tunneling approach to quantum cosmology. The scalar field potential is assumed to have a maximum at $\phi=0$ and can be approximated in its vicinity as $V(\phi)\approx...
Go to contribution page -
Prof. Lilia Anguelova (INRNE, Bulgarian Academy of Sciences)26/06/2023, 15:40Cosmology
We derive consistency conditions for sustained slow roll and rapid turn inflation in two-field cosmological models with oriented scalar field space, which imply that inflationary models with field-space trajectories of this type are non-generic. In particular, we show that third order adiabatic slow roll, together with large and slowly varying turn rate, requires the scalar potential of the...
Go to contribution page -
Prof. Fa Peng Huang (Sun Yat-sen University)26/06/2023, 15:40DM
We study the gravitational wave signals of ultralight axion dark matter around Kerr black hole by LISA in synergy with SKA.
Go to contribution page -
Janina Hakenmรผller (Duke University)26/06/2023, 15:40Particle
In coherent elastic neutrino nucleus scattering (CE$\nu$NS), the neutrino interacts with the nucleus as a whole. This leads to a tiny recoil that can be registered with suitable detector technologies. The detection is highly challenging and requires a neutrino source within the coherent energy regime such as a nuclear power plant, a low enough energy threshold of the detectors and an excellent...
Go to contribution page -
Marianne Moore27/06/2023, 14:20Particle
The sexaquark, a hypothesized six-quark bound state, has garnered interest as a potential dark matter candidate. At the same time, there are many arguments in the literature that place severe limitations on this possibility. Assuming it exists and is stable, I will advance a compelling case for the limited viability of the sexaquark as a dark matter candidate by presenting the first...
Go to contribution page -
Lu Yin (APCTP)27/06/2023, 14:20Cosmology
Exciting clues to isotropic cosmic birefringence have recently been detected in the $EB$ cross-power spectra of the polarization data of the cosmic microwave background (CMB). Early Dark Energy (EDE) models with a pseudoscalar field coupled to photons via a Chern-Simons term can be used to explain this phenomenon, and can also potentially be used to simultaneously resolve the $H_0$ tension. In...
Go to contribution page -
Omar Medina (IFIC (CSIC-Universitat de Valรจncia))27/06/2023, 14:20Particle
We present a model that explains the origin of the neutrino mass ordering through the spontaneous breaking of a discrete flavor symmetry. Our model addresses the hierarchy between neutrino masses by combining the seesaw and scotogenic mechanisms, both emerging naturally from an $A_4$ discrete symmetry broken at the electroweak scale. The model incorporates a scalar dark matter particle...
Go to contribution page -
Marcell Howard27/06/2023, 14:40Cosmology
Stochastic gravitational wave backgrounds (SGWBs) are the conglomeration of unresolved gravitational wave signals from the early universe and from astrophysical sources, which make them a promising tool for cosmologists. Because gravitons decouple from the cosmic plasma early on, one can consider interactions between gravitons and any particle species that were present in the very early...
Go to contribution page -
Prof. Hsiang-nan Li (Academia Sinica)27/06/2023, 14:40Particle
We demonstrate that the Higgs boson mass can be extracted from the dispersion relation obeyed by the correlation function of two b-quark scalar currents. The solution to the dispersion relation with the input from the perturbative evaluation of the correlation function up to next-to-leading order in QCD and with the $b$ quark mass $m_b=4.43$ GeV demands a specific Higgs mass $115^{+13}_{-9}$...
Go to contribution page -
Orion Ning27/06/2023, 14:40DM
The Hitomi X-ray satellite mission carried unique high-resolution spectrometers that were set to revolutionize the search for sterile neutrino dark matter (DM) by looking for narrow X-ray lines arising from DM decays. Unfortunately, the satellite was lost shortly after launch, and to-date the only analysis using Hitomi for DM decay during its brief, one-month long live time was for data taken...
Go to contribution page -
108. Affleck-Dine leptogenesis with one loop neutrino masses and a solution to the strong CP problemNobuchika Okada27/06/2023, 15:00Cosmology
We discuss a unified model that solves four major problems of the standard model i.e. neutrino masses the origin of matter the strong CP problem and dark matter by using the framework of the Affleck-Dine (AD) mechanism. The AD field is responsible for inflation the origin of matter and neutrino masses which arise at the one-loop level. Neutrino masses are therefore intimately...
Go to contribution page -
Xiaobin Lu27/06/2023, 15:00Particle
PROSPECT, the Precision Reactor Oscillation and SPECTrum Experiment, is a short-baseline reactor-based neutrino experiment aiming to make a precision measurement of reactor antineutrino energy spectra and model-independently search for eV-scale sterile neutrinos. The experiment collected over 50,000 neutrino interactions over the course of five reactor-on cycles at the High Flux Isotope...
Go to contribution page -
Satoshi Shirai (Kavli IPMU)27/06/2023, 15:00DM
An electroweak-charged dark matter Model a well-motivated dark matter candidate. The Wino, Higgsino and 5plet fermions are typical examples.
Go to contribution page
In these models, the charged partner becomes metastable.
Disappearing charged tracks and soft objects produced by the charged partner are important for the test of this model in collider experiments.
The signals strongly depend on the lifetime and... -
Mehrdad Phoroutan-Mehr (University of California, Riverside (UCR))27/06/2023, 15:40Formal/strings
The existence of supermassive black holes at the center of galaxies redistributes the dark matter density profile in the region of influence and creates a higher density region so-called density spike. In the self-interaction dark matter scenario, the velocity dispersion in the spike region scales with a power law of r^โ1/2, and the density spike scales with a power law of r^โ(3+a)/4, where...
Go to contribution page -
GEORGE WOJCIK27/06/2023, 15:40Particle
In this talk I discuss recent work on model building for the anomalous muon magnetic moment with ``portal matter'' vector-like fermions charged under both SM hypercharge and a hidden Abelian gauge group U(1)D which can induce kinetic mixing at one loop. The portal matter fields are a well-motivated extension of simplified dark matter models in which the dark matter candidate interacts with...
Go to contribution page -
So Chigusa27/06/2023, 15:40DM
Axions and dark photons are well-motivated dark matter candidates but much of their parameter space remains unexplored. We demonstrate that magnetometry with nitrogen-vacancy centers can cover a broad parameter space with masses over several orders of magnitude. Its unique advantages include a wide dynamic range and the ability to perform measurements without magnetic shielding enhancing its...
Go to contribution page -
Marco Palmiotto (Institut de physique des deux infinis Lyon, Universitรฉ Claude Bernard Lyon 1)27/06/2023, 16:00DM
Go to contribution pageDarkPACKis a software that automatically generates a numerical library
of scattering amplitudes from the Lagrangian density of the model, to
compute dark matter observables such as relic density. It relies on
MARTYandSuperIso relicand is written inC++. In the current
version,DarkPACKcan easily generate all the squared
amplitudes of 2 NP particles into 2 Standard Model... -
Teerthal Patel (Arizona State University)27/06/2023, 16:00Formal/strings
The โelectroweak dumbbellโ consists of a magnetic monopole and an antimonopole of the standard electroweak model connected by a string made of Z-magnetic field. The dumbbells formed during the epoch of electroweak symmetry breaking in the early Universe undergo annihilation, and leave behind cosmological relic magnetic fields. Electroweak dumbbells may also be produced in scattering...
Go to contribution page -
Sergio Sevillano27/06/2023, 16:00Particle
The ability to represent perturbative expansions of interacting quantum field theories in terms of simple diagrammatic rules has revolutionized calculations in particle physics. However in the case of extended theories of gravity deriving this set of rules requires linearization of gravity perturbation of the scalar fields and multiple field redefinitions making this process very...
Go to contribution page -
Yo Toda27/06/2023, 16:20DM
We investigate the model where electrons and dark matter interact with dark energy through the rolling of a scalar field which comes from extra dimensional theories such as the braneworld theory and Brans-Dicke theory. In this model dark energy couples to dark matter and electrons which leads to larger values of the mass energies of dark matter and electrons in the early universe. We also...
Go to contribution page -
YI LIU (university of Southampton)27/06/2023, 16:20Particle
We study the possibility of measuring neutrino Yukawa couplings in the Next-to-Minimal Supersymmetric Standard Model with right-handed neutrinos (NMSSMr) when the lightest right-handed sneutrino is the Dark Matter (DM) candidate by exploiting a `dijet + dilepton + Missing Transverse Energy' (MET or $\slashed{E}_T$) signature. We show that this extended model of SUSY offers a much lighter...
Go to contribution page -
Juan Carlos Vasquez (Amherst College)27/06/2023, 16:20Formal/strings
Under certain assumptions and independent of the instantons, we show that the
Go to contribution page
logarithm expansion of dimensional regularization in quantum field theory needs a
nonperturbative completion to have a renormalization-group flow valid at all ener-
gies. Then, we show that such nonperturbative completion has the analytic proper-
ties of the renormalons, which we find with no reference to... -
Jacob Spisak (University of California, San Diego)27/06/2023, 16:40DM
Very light pseudoscalar fields, often referred to as axions, are compelling dark matter candidates and can potentially be detected through their coupling to the electromagnetic field. Recently a novel detection technique using the cosmic microwave background (CMB) was proposed, which relies on the fact that the axion field oscillates at a frequency equal to its mass in appropriate units,...
Go to contribution page -
Dr Supriya Senapati (University of Massachusetts Amherst)27/06/2023, 16:40Particle
Left-Right (LR) theories are one of the successful beyond Standard Model (SM) frameworks that explain the origin of small neutrino masses and low-energy weak parity violation. However, the conventional LR theory faces a challenge due to the presence of flavor changing neutral currents (FCNCs). To address this, we have studied an Alternative LR model (ALRM), which avoids FCNC constraints. Our...
Go to contribution page -
Tatsuya Daniel (Brown University)27/06/2023, 16:40
I will discuss ongoing work in studying how the combination of two modified gravity theories that are well motivated from string theory, Dynamical Chern-Simons (dCS) and Einstein-dilaton-Gauss-Bonnet (EdGB) gravity, will affect the gravitational waveforms emitted from a binary neutron star system, as well as observed neutron star relations such as the mass-radius relation and universal...
Go to contribution page -
Daniel Stolarski (Carleton University)28/06/2023, 14:20DM
I will describe a unified mechanism for generating a baryon and dark matter asymmetry in models with multiple hidden sectors that are Standard Model-like but with varying Higgs mass parameters. These models have a unique cosmology with the different sectors reheated asymmetrically to relatively low temperature. A hidden sector with positive Higgs mass squared can accommodate dark matter with...
Go to contribution page -
Zach Bogorad28/06/2023, 14:20Particle
I will present a new constraint on long-range interactions between dark matter and the Standard Model, based on the effects of dynamical friction in ultrafaint dwarf galaxies (UFDs). Parsec-scale interactions between dark matter and the Standard Model are currently poorly constrained. However, such long-range forces can lead to a gradual transfer of kinetic energy from stars to the dark matter...
Go to contribution page -
Yoshiki Kanazawa (University of Tokyo)28/06/2023, 14:20Formal/strings
It is expected that any global symmetry is explicitly violated by gravity. In QCD axion models the effective axion potential obtains other terms than QCD contributions due to gravitational violation of the global U(1) Peccei-Quinn (PQ) symmetry and the minimum of the potential is deviated from the CP-conserving points. In general the deviation is large enough to invalidate the PQ solution...
Go to contribution page -
Yohei Ema28/06/2023, 14:40Particle
There are many New Physics scenarios that may affect the current discrepancy between the measurement and the prediction of the muon anomalous magnetic moment. One such possibility is a long-range force created by ordinary atoms acting on the muon spin. If the muon $g-2$ discrepancy is attributed to such a force, it would imply a tiny, $\mathcal{O}(10^{-13})\,\mathrm{eV}$ spin energy splitting...
Go to contribution page -
Yahya Almumin28/06/2023, 14:40Formal/strings
Complex scalars in U(1)-symmetric potentials can form stable Q-balls, non-topological solitons that correspond to spherical bound-state solutions. If the U(1) charge of the Q-ball is large enough, it can support a tower of unstable radial excitations with increasing energy. Previous analyses of these radial excitations were confined to fixed parameters, leading to excited states with different...
Go to contribution page -
Hao Chen28/06/2023, 14:40DM
LUX-ZEPLIN (LZ) is located at Sanford Underground Research Facility (SURF) in Lead, South Dakota. It uses a dual-phase xenon time projection chamber to search for Weakly Interacting Massive Particles (WIMP) and other new physics beyond the Standard Model. LZ completed its first science run in 2022. With its low background and large mass (7 tonne) of liquid xenon, LZ has set the most stringent...
Go to contribution page -
Xucheng Gan28/06/2023, 15:00Particle
The portal connecting the invisible and visible sectors is one of the most natural explanations of the dark world. However, the early-time dark matter production via the portal faces extremely stringent late-time constraints. To solve such tension, we construct the scalar-controlled kinetic mixing varying with the ultralight CP-even scalar's cosmological evolution. To realize this and...
Go to contribution page -
Alex Stewart28/06/2023, 15:00Formal/strings
Cachazo, He, and Yuan (CHY) demonstrated an alternative approach for computing the tree-level S-matrix of pure Yang-Mills theories in arbitrary spacetime dimensions on shell, as a contour integral encircling solutions of the so-called "scattering equations" in their paper "Scattering of Massless Particles in Arbitrary Dimensions." Later, Dolan and Goddard analyzed the scattering equations and...
Go to contribution page -
Brian Shuve (Harvey Mudd College)28/06/2023, 15:00DM
Many scenarios of physics beyond the Standard Model predict new
Go to contribution page
particles with masses well below the electroweak scale. Low-energy, high
luminosity colliders such as BABAR are ideally suited to discover these
particles. We present several recent searches for low-mass dark sector
particles at BABAR, self-interacting dark matter, axion like particles,
and dark sector particles produced in B... -
Brooks Thomas28/06/2023, 15:40Particle
Cosmic stasis is a phenomenon in which the abundances of multiple cosmological energy components โ components such as matter, radiation, or vacuum energy โ remain effectively constant despite the expansion of the universe. One mechanism which can give rise to an extended period of cosmic stasis is the evaporation of a population of primordial black holes (PBHs). In this talk, I review how PBH...
Go to contribution page -
Claudio Savarese (Princeton University)28/06/2023, 15:40DM
Among the numerous technologies developed in the field of Dark Matter direct detection, noble element dual-phase time projection chambers (TPC) have proved to be an outstanding solution, scalable to extremely high target masses without dramatic increases in read-out complexity. The DarkSide programme pioneered the use of liquid argon as a DM scattering target in such detectors and is now...
Go to contribution page -
Helena Garcia Escudero (UCI)28/06/2023, 15:40Cosmology
We explore possible mechanisms of suppressing the production of keV scale sterile neutrinos, which is the target parameter space of several current/upcoming laboratory experiments such as KATRIN, HUNTER or MAGNETO-nu. These alternative scenarios include universes with a nontrivial cosmic lepton number, new neutrino interactions with light bosons, late-time neutrino mass generation, low...
Go to contribution page -
Jeffrey Kuntz (Max-Planck-Institute for Nuclear Physics)28/06/2023, 16:00Cosmology
It is well-known that renormalizable theories of quadratic gravity pose a risk to unitarity of the S-matrix due to the spin-2 ghost degrees of freedom that they inevitably propagate. However, in recent years, a few promising methods to guarantee unitarity in the presence of these ghosts have been proposed. In light of these recent developments, we consider a generic model of quadratic gravity...
Go to contribution page -
Dr Subhajit Ghosh (University of Notre Dame)28/06/2023, 16:00DM
We study the cosmological signatures of a completely secluded dark sector consisting of axion-like particles (ALPs) with anomalous coupling to a dark Abelian gauge boson. The lighter ALP starts rolling during matter domination and produces dark photons through tachyonic instabilities. The resulting exponential growth in dark photon quanta sources tensor and scalar perturbations which are...
Go to contribution page -
Dr Fazlollah Hajkarim (University of Oklahoma)28/06/2023, 16:00Particle
The impact of axion-like particles on the light polarization around the horizon of supermassive black hole (SMBH) is discussed in the light of the latest polarization measurement of the Event Horizon Telescope (EHT). We investigate different sources of the polarization due to axion interaction with photons and the magnetic field of SMBH. These can modify the linear and circular polarization...
Go to contribution page -
Daneng Yang28/06/2023, 16:20DM
We propose a parametric model for studying self-interacting dark matter (SIDM) halos. The model uses an analytical density profile, calibrated using a controlled N-body SIDM simulation that covers the entire gravothermal evolution, including core-forming and -collapsing phases. By normalizing the calibrated density profile, we obtain a universal description for SIDM halos at any evolution...
Go to contribution page -
Dr Keisuke Inomata (University of Chicago, KICP)28/06/2023, 16:20DM
Rotations of axion fields in the early universe can produce dark matter and matter-antimatter asymmetry of the universe.
Go to contribution page
In a class of models, the equation of state of the rotations rapidly changes from a non-relativistic matter-like one to a kination-like one.
We point out that the rapid change can produce an observable amount of gravitational waves through the Poltergeist mechanism. -
Matthew Sullivan (Brookhaven National Laboratory)28/06/2023, 16:20Particle
The Standard Model effective field theory (SMEFT) is a standard tool for parametrizing the effects of new physics. The ordiinary approach to SMEFT is to use the truncation at dimension-6, which would typically be the leading contribution beyond the Standard Model. We perform the matching to dimension-8 in the two-Higgs-doublet model (2HDM) and critically examine the dimension-6 and dimension-8...
Go to contribution page -
Tyler Smith (University of California, Irvine)28/06/2023, 16:40
In the ever-expanding landscape of BSM model building, the ubiquitous presence of new vector bosons has led to new frontiers in probing the depths of fundamental physics. While it is widely acknowledged that non-conserved currents of these vector bosons can lead to (energy/vector mass)^2 enhancements, we diverge from standard literature and consider the realm of conserved currents. We...
Go to contribution page -
Michael A. Fedderke (Johns Hopkins University)28/06/2023, 16:40DM
In this talk, I will present a novel technique to search for axions with a CP-violating monopole coupling $\tilde{g}_{Q}$ to bulk SM charges $Q \in \{B,L,B-L\}$. Gradients in the static axion field configurations sourced by matter induce achromatic circular photon birefringence via the axion-photon coupling $g_{\phi \gamma}$. Circularly polarized light fed into an optical or (open)...
Go to contribution page -
Huangyu Xiao (Fermilab)28/06/2023, 16:40Cosmology
Axion-like dark matter whose symmetry breaking occurs after the end of inflation predicts enhanced primordial density fluctuations at small scales. This leads to dense axion minihalos (or miniclusters) forming early in the history of the Universe.
Go to contribution page
Condensation of axions in the minihalos leads to the formation and subsequent growth of axion stars at the cores of these halos. If, like the... -
Dr Andrey Shkerin (University of Minnesota)29/06/2023, 14:20DM
Dark matter particles can form halos gravitationally bound to massive astrophysical objects. The Earth could have such a halo where depending on the particle mass, the halo either extends beyond the surface or is confined to the Earthโs interior. We consider the possibility that if dark matter particles are coupled to neutrinos, then neutrino oscillations can be used to probe the Earthโs dark...
Go to contribution page -
Prof. Evgueni Goudzovski (University of Birmingham)29/06/2023, 14:20Particle
Rare kaon decays are among the most sensitive probes of both heavy and light new physics beyond the Standard Model description thanks to high precision of the Standard Model predictions, availability of very large datasets, and the relatively simple decay topologies. The NA62 experiment at CERN has reported the first observation of the ultra-rare $K^+\to\pi^+\nu\bar\nu$ decay, and is...
Go to contribution page -
Eleanor Hall29/06/2023, 14:20Formal/strings
Abstract: Gravitational waves from cosmological phase transitions offer the chance to probe the very first second of the universeโs history and are one of our most promising signal channels of BSM physics. With space-based detectors such as LISA on the horizon, we urgently need reliable tools for predicting GW signals in strongly-coupled theories. In this talk, I discuss our recent proposal...
Go to contribution page -
Andrzej Hryczuk29/06/2023, 14:40DM
In this talk I will discuss some of the recent progress in understanding the impact of non-equilibrium effects on dark matter (DM) production. First I will present a framework for performing calculations beyond kinetic equilibrium and exemplify its importance on several classes of DM models. Then I will discuss the latest results regarding impact of processes distorting the momentum...
Go to contribution page -
Chen-Te Ma29/06/2023, 14:40Formal/strings
The gauge formulation of Einstein gravity in AdS$_3$ background leads to a boundary theory that breaks modular symmetry and loses the covariant form. We examine the Weyl anomaly for the cylinder and torus manifolds. The divergent term is the same as the Liouville theory when transforming from the cylinder to the sphere. The general Weyl transformation on the torus also reproduces the Liouville...
Go to contribution page -
Julian Bollig (Albert-Ludwigs-Universitรคt Freiburg)29/06/2023, 14:40DM
Indirect detection is one of the most powerful methods to search for annihilating dark matter (DM) covering a broad range of masses and interactions. Recently, non-perturbative effects have been shown to significantly alter model observables. In this work, we investigate the impact of non-perturbative effects in the indirect detection of DM. For this purpose we utilize a minimal model...
Go to contribution page -
Dr Savan Kharel29/06/2023, 15:20Formal/strings
I will focus on the computation of graviton function in (Anti)-de Sitter space, specifically concentrating on gravitons with all positive external helicity. To tackle this problem, I will introduce a generalized recursion method inspired by the BCFW (Britto-Cachazo-Feng-Witten) technique. This method involves a deforming of the external momentum of the graviton function by complexifying it and...
Go to contribution page -
Dr Javier Acevedo (SLAC)29/06/2023, 15:20DM
The minimum testable dark matter (DM) mass for almost all DM signatures in celestial bodies is determined by the rate at which DM evaporates. DM evaporation has previously been calculated assuming a competition between the gravitational potential of the object, and thermal kicks from the celestial-body matter. I will point out a new effect, where mediators with a range larger than the...
Go to contribution page -
Dr Xiang-Gan Liu (University of California - Irvine)29/06/2023, 15:20Formal/strings
The Kahler potentials of modular symmetry models receive unsuppressed contributions which may be controlled by a flavor symmetry, where the combination of the two symmetry types is referred to as eclectic flavor symmetry. After briefly reviewing the consistency conditions of eclectic flavor symmetry models, including those with generalised (g)CP, we perform a comprehensive bottom-up study of...
Go to contribution page -
Sarunas Verner (University of Florida)29/06/2023, 15:40DM
In this presentation, I discuss the production of a spectator scalar dark matter field that directly couples to the inflaton. Conventional scenarios of purely gravitationally produced dark matter with masses below the Hubble parameter at the end of inflation are in tension with Cosmic Microwave Background (CMB) constraints on the isocurvature power spectrum. We explore a more general scenario...
Go to contribution page -
Max Fieg29/06/2023, 15:40Particle
Neutral particles are notoriously difficult to observe through electromagnetic
Go to contribution page
interactions. As a result, they naturally elude detection in most collider detectors. In this talk, I will point out that neutral particles that interact through a
dipole interaction can nevertheless be detected in far-forward detectors
designed to search for long-lived particles (LLPs). In contrast to previous... -
Victor Knapp Perez (UCI)29/06/2023, 15:40Formal/strings
Modular flavor symmetries have gained significant attention as a promising method for predicting lepton mixing parameters. However, in a bottom-up approach, the lack of precise control over the parameters in the kinetic terms limits their predictability . To address this, we propose deriving the Yukawa couplings from an underlying geometry, specifically magnetized tori.
In this talk, we...
Go to contribution page -
Alec HewittParticle
Heavy Neutral Leptons (HNLs) are among the leading examples of long-lived particles. For masses in the MeV to GeV range, HNLs are light enough to be produced at many collider and accelerator facilities, but also heavy enough to decay to visible particles on length scales that can be observed in particle detectors. We discuss the FORESEE simulation package to include the production and decay...
Go to contribution page