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The Cosmology Seminars are scheduled on **Wednesdays from 2:00pm-3:00pm. **

** Seminars may be attended in person | Goldwater Building 5th Floor | Conference room 505**

Date | Speaker | Institution | Faculty Host | Title | Abstract |
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9/7/2022 | George Zahariade | Inst HEP (IFAE) | Tanmay Vachaspati | Quantum formation of topological defects | In this blackboard talk I will describe recent work (in collaboration with M. Mukhopadhyay, O. Pujolas and T. Vachaspati) about the quantum formation of kinks and antikinks during a quantum phase transition in 1+1 dimensions. I will evaluate the number density of kinks as a function of time and show that it scales as t^{-1/2} in the late time limit (and independently of the details of the phase transition). This decay can be interpreted in terms of ballistic annihilation of kink-antikink pairs. Finally I will discuss the extension of the model to the case of asymmetric initial conditions. |

9/21/2022 | Lars Aalsma | Arizona State University | Cynthia Keeler | Entropic Aspects of De Sitter Quantum Gravity in Two Dimensions | In recent years, the (non-)existence of metastable de Sitter vacua in quantum gravity has been a subject of intense debate. Nonetheless, there is one aspect of de Sitter quantum gravity that has been widely accepted: the cosmological horizon carries an entropy proportional to its area. In an explicit two-dimensional setting, I will explain how this can lead to an information paradox, its resolution, and the consequences for the validity of semi-classical EFT. |

9/28/2022 | Dan Stolarski | Carleton via UCSD | Matt Baumgart | A chiral SU(5) theory with three generations | I will present a study of an interesting strongly coupled chiral quantum field theory. This theory has the same particle content as the simplest grand unified theory of the Standard Model. I will employ tools such as 't Hooft anomaly matching and softly broken supersymmetry to analyze the non-perturbative dynamics of the theory. I will also speculate on the more general lessons of my analysis. |

10/12/2022 | Pouya Asadi | Oregon University | Matt Baumgart | Thermal Squeezeout of Dark Matter | There has been substantial effort on searching for thermal Dark Matter (DM) in the conventional mass window of GeV to tens of TeV without any positive results. This null result has motivated efforts to develop new dynamics in the dark sector that allow us go beyond the usual thermal DM mass window. In this talk, I introduce one such simple dynamic in a broad class of confining dark sectors. I will point out a potentially dramatic effect on the DM abundance during its deconfinement phase transition. I will also discuss the effect of long-living glueballs in such a sector. Potential signals of such a sector will be briefly presented too. |

10/19/2022 | NO SEMINAR SCHEDULED | ||||

10/26/2022 | Peter Koroteev | Berkeley | Andrei Belitski | From Instantons to Vortices via a Double-Scaling Limit. | I will review the connection between soluble many-body systems and supersymmetric gauge theories. I will then study the so-called Inosemtsev limit which involves certain double-scaling, and which will enable us to transition from the moduli space of instantons to the moduli space of vortices. |

11/2/2022 | Kanu Sinha | Arizona State University | Tanmay Vachaspati | Quantum fluctuation phenomena in nanoscale quantum systems | Quantum fluctuation phenomena are a fascinating and fundamental feature of quantum electrodynamics (QED), with implications spanning spontaneous emission of atoms, stability of colloidal suspensions such as milk, adhesive properties of gecko feet and, potentially, the density perturbations in the cosmic microwave background. When considering particle-surface interactions at nanoscales, such fluctuation-induced interactions become an imperative element of consideration in understanding and designing nanoscale quantum systems. In this talk, I will introduce an open quantum systems approach to engineer fluctuation phenomena at nanoscales -- Casimir-Polder forces, dissipation and decoherence -- particularly focusing on fluctuation-induced decoherence of levitated nanoparticles. Our results illustra |

11/9/2022 | Kurt Hinterbichler | Case Western | Claire Zukowski | Symmetries and anomalies at the IR fixed point of gravity | I will discuss symmetries that arise at the infrared fixed point of the RG flow of Einstein gravity, including conformal vs. scale invariance in various dimensions, as well as 1-form generalized global symmetries and new anomalies that arise among them. |

11/30/2022 | Francis -Cyr-Racine | New Mexico University | Matt Baumgart | Scaling Invariance and the Origins of Cosmological Constraints | Since they naturally live in angular and redshift space, astronomical observations have a built-in invariance under rescaling all length scales in the problem. Breaking this invariance requires the use of anchors, such as known distances or energy scales, that can set the absolute scale of the problem. These anchors are fundamental to our knowledge of cosmological distances throughout the Universe, and provide the backbone on which much of our knowledge of cosmology rests. These pillars have recently come under renewed scrutiny due to apparently discrepant measurements of the Hubble constant, a very important cosmological quantity which sets the size and age of the observable Universe. Here, we carefully examine the key anchors underpinning observations of the cosmic microwave background and baryon acoustic oscillations, finding ways to detach these measurements from their traditional anchors and fully restore their intrinsic scaling invariance. Not only can this help to understand the possible cause of the Hubble constant discrepancy, but it also sheds new light on the origins of cosmological constraints on new physics beyond the Standard Model. This in turn provides us with a general toolbox to design novel cosmological models that are automatically compatible with observations. |

12/07/2022 |

Date | Speaker | Institution | Host | Title | Abstract | |
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01/19/2022 | Natalia Pinzani-Fokeeva | MIT | Enstrophy and black hole supertranslations | Enstrophy is an approximately conserved quantity in 2+1 dimensional nonrelativistic fluids that implies an inverse energy cascade in turbulent flows. In this talk, I will present an algorithm on how to construct an enstrophy current for generic fluid flows (relativistic and non). In addition, I will show how a subset of certain horizon symmetries of 3+1 dimensional AdS black holes also lead to enstrophy conservation in the dual holographic fluid theory. | ||

02/02/2022 | David Dunsky | UC Berkeley | Gravitational Wave Gastronomy | The symmetry breaking of grand unified gauge groups in the early universe often leaves behind relic topological defects such as cosmic strings, domain walls, or monopoles. For some symmetry breaking chains, hybrid defects can form where cosmic strings attach to domain walls or monopoles attach to strings. In general, such hybrid defects are unstable and can leave behind unique gravitational wave fingerprints. In this talk, I will discuss the gravitational wave spectrum from 1) the destruction of a cosmic string network by the nucleation of monopoles which cut up and `eat’ the strings, 2) the collapse and decay of a monopole-string network by strings that ‘eat’ the monopoles, 3) the destruction of a domain wall network by the nucleation of string-bounded holes on the wall that expand and `eat’ the wall, and 4) the collapse and decay of a string-bounded wall network by walls that `eat’ the strings. We call the gravitational wave signals produced from the `eating’ of one topological defect by another “gravitational wave gastronomy”. We find that the gravitational wave gastronomy signals considered yield unique spectra that can be used to narrow down the SO(10) symmetry breaking chain to the Standard Model and the scales of symmetry breaking associated with the consumed topological defects. | ||

02/16/2022 | Jacob Litterer | Tufts University | Bound on Squeezed State Gravitational Wave Fluctuations from LIGO | Gravitational wave observations at LIGO are in good agreement with classical predictions, with a residual that does not exhibit any unexplained correlations. In the context of general relativity as an effective quantum theory, gravitational waves have been thought to be in the most classical coherent state, in which quantum fluctuations are far too small to see at LIGO. However, it is plausible to suppose that gravitational waves may be produced in a more interesting squeezed state, in which quantum fluctuations can be exponentially enhanced by the squeezing parameter as pointed out in recent work. Computing space and time correlations of a class of squeezed states and taking into account the detector response, a simple comparison to LIGO data puts a bound on the squeezing parameter | ||

03/02/2022 | David Cyncynates | Stanford University | Friendship in the Axiverse | The Axiverse is a scenario in which axion-like particles are distributed over many orders of magnitude in mass and interact with one another through a joint potential. In this talk, I will show how non-linearities in this potential lead to a new type of resonant energy transfer between "friendly" axions with nearby masses. This resonance generically transfers energy from axions with larger decay constants to those with smaller decay constants, leading to a multitude of signatures. These include enhanced direct detection prospects for a resonant pair comprising even a small subcomponent of dark matter, and boosted small-scale structure if the pair is the majority of DM. Near-future iterations of experiments such as ADMX and DM Radio will be sensitive to this scenario, as will astrophysical probes of DM substructure. | ||

3/16/2022 - @ 4PM | Yuta Michimura | University of Tokyo | DANCE: Dark matter Axion search with riNg Cavity Experiment | Axion and axion-like particles are leading candidates for ultralight dark matter, and there have been enormous efforts to search for their signatures through a variety of experiments and astrophysical observations. Axion may cause a polarization rotation of light through the parity-violating interaction with photons. Recently, we have proposed to search for axion dark matter by enhancing the polarization rotation effect using a bow-tie optical ring cavity [PRL 121, 161301 (2018)]. We have shown that this Dark matter Axion search with riNg Cavity Experiment (DANCE) can improve the sensitivity to axion-photon coupling for axion mass m_a<10^{-10} eV by up to several orders of magnitude, compared with the current best limits. Currently, a prototype experiment DANCE Act-1 is underway at Tokyo to demonstrate the feasibility of the method. In this talk, I will present the principle of DANCE and the status of DANCE Act-1, including some of the preliminary results from the first 12-day run in May 2021. | ||

3/30/2022 | Glennys Farrar | New York University | Sexaquarks can be the Dark Matter: abundance, direct detection constraints, laboratory searches and neutron stars | It is possible that a neutral dibaryon composed of uuddss is sufficiently deeply bound that its mass is less than ~ 2.05 GeV, in which case it is effectively stable. Such a particle is designated S or sexaquark, to avoid confusion with hexaquarks which are generically short-lived. As will be explained, such a particle would not have been detected in experiments to date. Constraints on its mass and cross sections will be quickly reviewed and it will be shown that it is an excellent Dark Matter candidate. Undetected S Sbar production can also naturally explain the discrepancy between the measured cross section for e+e- -> hadrons, and lattice QCD and g-2 experimental determinations. | ||

4/06/2022 | Bryce Cyr | McGill University | Direct collapse black holes from superconducting cosmic strings | The observation of supermassive black holes in high redshift quasars presents a tantalizing mystery in astrophysics and cosmology, as they are difficult to explain within the standard LCDM paradigm. I will briefly review these challenges, and introduce a possible resolution through the monolithic collapse of a primordial gas cloud. I will present the astrophysical conditions necessary to achieve such a collapse, and show how a gas cloud surrounding a superconducting cosmic string is an ideal environment to satisfy these conditions. Finally, I will discuss the nuances of combining other constraints on superconducting strings with this idea, as well as introduce ongoing work to predict the number density of these string-seeded black holes. | ||

4/13/2022 | Tucker Manton | Arizona State University | Selected studies in the double copy: non-singular black holes, fluid/gravity duality, and external sources | The double copy is a procedure that relates gravity to simpler gauge and scalar field theories. Double copy structure was first discovered in the context of scattering amplitudes, and has since been realized at the level of classical fields and curvatures. In this defense, I focus on mappings between fields (the Kerr-Schild double copy) and curvatures (the Weyl double copy). First, I build the connection between non-singular black holes and non-singular gauge theories. Here, we find a subtlety between gravitational horizons and the gauge field strength. I will then study a perturbative double copy in the context of the fluid/gravity duality, where the associated gauge quantities have elegant interpretations in terms of certain classes of Navier-Stokes solutions. Finally, I will present a new formula that provides a consistent treatment of external sources in the Weyl double copy. After illustrating its consistency with the Kerr-Schild double copy, I apply the sourced Weyl double copy to the most general Petrov type D electro-vac spacetime before discussing various limits of the general solution. | ||

4/27/2022 | David Hosking | University of Oxford | Decay of primordial magnetic fields via reconnection can explain cosmic-void observations | It has been suggested [see 1, 2, and references therein] that the weak magnetic field hosted by the intergalactic medium (IGM) in voids might be a relic from the early Universe. If so, the strength and coherence length of void fields could be “predicted” from reasonable assumptions about the properties that the primordial field had at its genesis, provided the evolution of the field in the intervening time were understood. Previously held theories [1, 2] based on magnetogenesis at the electroweak phase transition (EWPT) indicated that parity-invariant primordial fields would have decayed too quickly to be consistent with the observational constraints on void fields. Thus, the “relic-field” hypothesis appeared unlikely [3]. However, recent numerical developments have shown that these decay theories are flawed: they do not predict the “inverse transfer” of magnetic energy to larger scales that has been observed in simulations [4, 5]. In my talk, I present a theory of the decay based on the conservation of the “fluctuation level” of magnetic helicity [6], with dynamics controlled by the reconnection of magnetic-field lines [6, 7, 8]. I show that this theory explains the “inverse-transfer” phenomenon, and predicts a slower decay of primordial fields, thus restoring consistency between the relic-field hypothesis and the observational constraints. |

Date | Speaker | Institution | Host | Title | Abstract | |
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9/22/2021 | Andy Svesko | University College London | Semi-classical thermodynamics of quantum extremal surfaces in 2D gravity | Quantum extremal surfaces (QESs) play an important role in the study of the black hole information problem, and, in a sense, are semi-classical generalizations of black hole horizons. Their thermodynamics, however, have largely been unexplored because a proper interpretation requires a detailed understanding of the backreaction of quantum fields outside of a black hole. In this talk I will consider a massless quantum field theory outside of an eternal anti-de Sitter (AdS) black hole in two-dimensional (2D) dilaton gravity, where back reaction may be studied exactly | ||

10/6/2021 | Michael Zantedeschi | Ludwig-Maximilians-Universität | Primordial Black Holes from Confinement | In this talk I will present a novel mechanism for the formation of primordial black holes. Here, heavy quarks of a confining gauge theory produced by de Sitter fluctuations are pushed apart by inflation and get confined after horizon re-entry | ||

10/13/2021 | Suvrat Raju | Tata Institute of Fundamental Research | Holography of Information and Massive Islands | We will review recent results that suggest that, in any standard theory of quantum gravity, information available on the bulk of a Cauchy slice must also be available near the boundary of the slice. These ideas indicate how holography should be extended to four dimensional asymptotically flat spacetimes but they also shed light on the origins of AdS/CFT. We contrast this picture with the paradigm of islands and argue that islands are consistent only in theories of massive gravity. References: 1) "Holography from the Wheeler-DeWitt equation" https://arxiv.org/abs/2107.14802 2) "Inconsistency of Islands in Theories with Long-Range Gravity" https://arxiv.org/abs/2107.03390 3) "Lessons from the Information Paradox" (review) https://arxiv.org/abs/2012.05770 | ||

10/20/2021 | Anson Hook | University of Maryland | Black Hole Production of Monopoles in the Early Universe | In the early universe, evaporating black holes heat up the surrounding plasma and create a temperature profile around the black hole that can be more important than the black hole itself. As an example, we demonstrate how the hot plasma surrounding evaporating black holes can efficiently produce monopoles via the Kibble-Zurek mechanism. In the case where black holes reheat the universe, reheat temperatures above ∼ 700 GeV can already lead to monopoles overclosing the universe. | ||

11/10/2021 | William Terrano | Arizona State University | Learning about Cosmology from Nuclear Spins | The most sensitive measurements of the energy splitting between quantum states are made on highly-coherent nuclear spin states. I will discuss how studying these energy splittings can inform our knowledge of cosmology and particle physics, in particular of baryogenesis (through EDM measurements) and of dark matter properties. I will describe how these measurements work, what makes them so powerful and the prospects for significant improvements here in the Goldwater basement. | ||

12/1/2021 | Jose Juan Blanco-Pillado | Ikerbasque and UPV/EHU | Dynamics of Excited Solitons | Many solitonic configurations in field theory have localized bound states in their spectrum of linear perturbations. This opens up the possibility of having long lived excitations of these solitons that could affect their dynamics. In this talk we will describe in detail how these states appear in some field theory models of low dimensionality like kinks in 1+1 dimensions and vortices in 2+1 dimensions and study their dynamical properties through a series of numerical experiments. |

Date | Speaker | Institution | Host | Title | Abstract | |
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1/27/2021 @ 3PM MST | Kohei Kamada | The University of Tokyo, Tokyo | Dr. Tanmay Vachaspati | Constraints on the primordial hypermagnetic fields from the baryon isocurvature perturbations | Gamma-ray observations of blazars suggest the existence of the intergalactic magnetic fields and their origin is interest for both astro physicsts and cosmologists. Among several proposals, magnetogenesis in the early Universe is an interesting option since it might also be a probe for the physics beyond the Standard Model of particle physics. Recently, it has also been proven that the baryon asymmetry of the Universe can be also generated if the magnetic fields are produced before the electroweak symmetry breaking with helicity without imposing any new physics. However, baryon isocurvature perturbations are also generated at the scale of the magnetic field coherence length in the mean time, which is constrained by the inhomogeneous Big Bang Nucleosynthesis. Note that this is an inevitable consequence of the Standard Model of particle physics. In this talk, I give generic constraints of the hypermagnetic field properties generated before the electroweak symmetry breaking. Noting that the baryon isocurvature perturbations are generated even from non-helical magnetic fields, I show that with reasonable parameter sets for the Standard Model of particle physics and magnetic field evolution laws, the intergalactic magnetic fields suggested by the blazar observations are hardly explained solely by the hypermagnetic fields generated before the electroweak symmetry breaking. Helical hypermagnetic fields can still be the origin of the present baryon asymmetry of the Universe, but we need an additional magnetogenesis or an unknown magnetic field amplification mechanism. | |

2/3/2021 | Michael Dine | University of California at Santa Cruz | Dr. Vachaspati | Axion Cosmic Strings: Players in the Early Universe? | Axion cosmic strings have long been considered as a potential source of enhancement of axion dark matter production, and have been the subject of extensive simulations in recent years. But axion strings are rather peculiar entities. We explore some aspects of these objects, and suggest that they may not play a distinguished role in early universe cosmology | |

2/24/2021 | Gordon Baym | University of Illinois Urbana-Champaign | Dr. Igor Shovkovy / Dr. Vachaspati | The evolution of primordial neutrino helicities under gravitational and magnetic fields and implications for their detection | Primordial neutrinos decoupled in the early universe in helicity eigenstates. As I will discuss, two effects -- dependent on neutrinos having a non-zero mass -- can modify their helicities as they propagate through the cosmos. First, finite mass neutrinos have a magnetic moment and thus their spins, but not their momenta, precess in cosmic and galactic magnetic fields. The second is the propagation of neutrinos past cosmic matter density fluctuations, which bend their momenta, and bend their spins by a smaller amount. (The latter is a general relativistic effect.) Both effects turn a fraction of left-handed neutrinos into right-handed neutrinos, and right-handed antineutrinos into left-handed. If neutrino magnetic moments approach that suggested by the XENON1T experiment as a possible explanation of their excess of low energy electron events -- a value well beyond the moment predicted by the standard model -- helicities of relic Dirac (but not Majorana) neutrinos could be considerably randomized. I finally will discuss the implications of neutrino helicity rotation, as well as their Dirac vs. Majorana nature, on their detection rates via the Inverse Tritium Beta Decay reaction. | |

3/31/2021 | Cecilia Lunardini | Arizona State University | Dr. Carlos Cardona | Has IceCube observed neutrinos from the tidal disruption of stars? A concordance scenario. | when a star falls within a critical distance from a supermassive black hole, it is disrupted, and its debris are in part accreted by the black hole. The accretion in these Tidal Disruption Event (TDE) results in a flare, and, in extreme cases, it can generate a relativistic hadronic jet, where high energy neutrinos could be produced. Recently, IceCube has detected a neutrino in spatial- and time-coincidence with tidal disruption event AT2019dsg. I present a phenomenological concordance scenario for this TDE, that includes a relativistic jet with efficient neutrino production. The model is based on the observed radiation spectra from AT2019dsg, and is consistent with numerical simulations of TDEs. This scenario offers an interpretation of the IceCube observation, and suggests that X-ray bright TDEs might be promising neutrino sources | |

4/14/2021 | Mudit Jain | Rice University | Dr. Tanmay Vachaspati | CMB birefringence from ultralight axion string networks | Ultralight axions (ULA), whose masses can lie in a wide range of values and can be even smaller than 10^{-28} eV, are generically predicted in UV theories such as string theory. In the cosmological context, the early Universe may have gotten filled with a network of ultralight axion (ULA) cosmic strings which, depending upon the mass of the axion, can survive till very late times. If the ULA also couples to electromagnetism, and the network survives post recombination, then the interaction between the strings and the CMB photons induces a rotation of the polarization axis of the CMB photons (otherwise known as the birefringence effect). This effect is independent of the string tension, and only depends on the coupling between the ULA and the photon (which in turn is sensitive to UV physics). In this talk I will present an analytical formalism to calculate this birefringence effect on the CMB photons, due to such ULA string networks. I will then consider three different models for the string networks and highlight some of the key features in the associated angular power spectrum, also comparing the results against some future CMB experiments. | |

4/21/2021 | Tina Kahniashvili & Emma Clarke | Carnegie Mellon University | Gravitational Waves from Early-Universe Turbulence: LISA Prospects and nanoGrav Signal Evidence | We will discuss gravitational wave signals sourced by hydrodynamic and hydromagnetic turbulent sources that might have been present in the early universe at epochs such as the electroweak and quantum chromodynamic (QCD) phase transitions. We consider various models of primordial turbulence: purely hydrodynamical turbulence induced by fluid motions, magnetohydrodynamic (MHD) turbulence dominated either by kinetic or magnetic energy both with and without helicity. We will also address the generation of circularly polarized gravitational waves by parity violating turbulent sources. We will present our results of numerical modeling of the early-universe turbulence and resulting gravitational waves and we will review the signal detection prospects through space based laser interferometers such as Laser Interferometer Space Antenna (LISA) and Pulsar Timing Arrays (PTAs). In particular, we will discuss the potential of explaining the recent observational evidence by NANOGrav collaboration for a stochastic gravitational wave background in the nanohertz frequency range through hydro and hydromagnetic turbulence at the QCD energy scale. | ||

4/28/2021 | Manibrata Sen | UC Berkeley and Northwestern University | Dr.Cecilia Lunardini | What can we learn from the future observation of the diffuse supernova neutrino background? | The Universe is awash with tens-of-MeV neutrinos of all species coming from all past core-collapse supernovae, also known as the diffuse supernova neutrino background (DSNB). Detecting the DSNB would open up new avenues in multi-messenger astronomy. In particular, it offers the unique opportunity to probe properties of the cosmos using neutrinos, as opposed to photons. The Super-Kamiokande experiment, loaded with gadolinium, is expected to collect dozens of events from the DSNB in the next decade. Future detectors such as Hyper-Kamiokande and Theia will perform even better, collecting hundreds of events after a decade of data-taking. In this talk, I will discuss how a future detection of the DSNB can be used to inform various research topics in cosmology, astrophysics and particle physics, focusing on a few examples from each field. In particular, I will expand on how the DSNB can be used to infer measurements of the Hubble constant, as well as constrain various parameters of the cosmological star formation rate. On the particle physics side, the DSNB can be used to probe the neutrino lifetime and the possibility that neutrinos are pseudo-Dirac fermions. |

Date | Speaker | Institution | Host | Title | Abstract | ||
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9/9/2020 | Geoffrey Penington | Stanford University | Cynthia Keeler | Replica Wormholes and Quantum External Surfaces | Hawking famously argued, based on semiclassical calculations, that the radiation from evaporating black holes is always perfectly thermal and contains no information about the matter that fell in. Such a result is inconsistent with the unitarity of quantum mechanics. In this talk, I will argue that a more careful replica trick calculation shows that the gravitational path integral becomes dominated at late times by saddles containing spacetime wormholes. These wormholes cause the entropy to decrease after the Page time, consistent with unitarity, and allow information to escape from the interior of the black hole. In very simple toy models, we can evaluate the path integral exactly, and see the information emerge. In more realistic black holes, the full wormhole solutions cannot be found explicitly. However, their existence, and their most important consequences, can be derived by studying the location and properties of a non-trivial ‘quantum extremal surface’ in the original Hawking solution | ||

9/23/2020 | Tom Kephart | Vanderbilt Univ | Antichirp: Gravitational Waves from a Black Hole Orbiting in a Wormhole Geometry | After a brief review of black hole--black hole mergers, and some background on wormholes and their construction, we discuss the case of a black hole orbiting a wormhole and the gravitational waves emitted. Results are based on recent work in collaboration with James Dent, Bill Gabella and Kelly Holly-Bockelmann (arXiv:2007.09135). | |||

9/30/2020 | Ke Fang | Kavli Stanford | Dr. Lunardini | Multi-messenger Astrophysics: Probing Compact Objects with Cosmic Particles | The study of compact objects such as black holes and neutron stars is an important component of modern astrophysics. Recent detections of astrophysical neutrinos, gamma-rays, ultrahigh energy cosmic rays, and gravitational waves open up opportunities to study compact objects with multi-messengers. In this talk, we first review the latest progress in Astroparticle Physics, including some surprising puzzles revealed by new observations. We demonstrate that the key to Multi-messenger Astrophysics is to understand and establish the link between the messengers. We then illustrate how to reach this goal from both theoretical and observational perspectives. From the theoretical side, we show that high-energy particle propagation in the vicinity of compact objects may play an important role in connecting multi-wavelength observation and source physics. From the observational side, we investigate analysis frameworks aiming to exploit data across multiple wavelengths and messengers. | ||

10/14/2020 | Xavier Siemens | University of Wisconsin | Dr. Vachaspati | The NANOGrav search for nanohertz gravitational waves | Supermassive black hole binaries (SMBHBs), and possibly other sources, generate gravitational waves in the nanohertz part of the spectrum. For over a decade and a half the North American Nanohertz Observatory for Gravitational Waves (NANOGrav) has been using the Green Bank Telescope, the Arecibo Observatory, and, more recently, the Very Large Array to observe millisecond pulsars. Our goal is to directly detect nanohertz gravitational waves, which cause small correlated perturbations to the times of arrival of radio pulses from millisecond pulsars. We currently monitor almost 80 millesecond pulsars with sub-microsecond precision and weekly to monthly cadences. I will present an overview of NANOGrav Physics Frontiers Center activities and summarize the results of our most recent search for a stochastic background of gravitational-waves on the 12.5-yr dataset. | ||

10/28/2020 | Cecilia Lunardini | Arizona State University | Has IceCube observed neutrinos from the tidal disruption of stars? A concordance scenario. | When a star falls within a critical distance from a supermassive black hole, it is disrupted, and its debris are in part accreted by the black hole. The accretion in these Tidal Disruption Event (TDE) results in a flare, and, in extreme cases, it can generate a relativistic hadronic jet, where high energy neutrinos could be produced. Recently, IceCube has detected a neutrino in spatial- and time-coincidence with tidal disruption event AT2019dsg. I present a phenomenological concordance scenario for this TDE, that includes a relativistic jet with efficient neutrino production. The model is based on the observed radiation spectra from AT2019dsg, and is consistent with numerical simulations of TDEs. This scenario offers an interpretation of the IceCube observation, and suggests that X-ray bright TDEs might be promising neutrino sources | |||

11/4/2020 @ 5PM AZ MST | Sergey Ketov | Tokyo Metropolitan University and Kavli IPMU, Japan | Carlos Cardona | Starobinsky inflation, primordial black holes and induced gravitational waves from modified supergravity | Basic (Starobinsky) inflationary model is reviewed as the theoretical probe of a more fundamental theory of gravity. Modified supergravity is introduced as an example of such theory towards a deeper understanding of cosmological inflation and (possible) formation of primordial black holes in the early Universe. A specific model of both phenomena in modified supergravity is proposed and investigated in detail. Their observational predictions (including black hole masses, dark matter and induced gravitational waves) are derived and compared to the current and future astrophysical and cosmological observations. The seminar is designed for those who are interested in theoretical cosmology and astrophysics, theoretical high energy physics, gravitational theory and string theory. | ||

11/11/2020 | |||||||

12/2/2020 |

Date | Speaker | Institution | Host | Title | ||
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01/22/2020 | Daniele Steer | APC (Paris) | Dr. Vachaspati | Cosmology and tests of General Relativity with gravitational waves | ||

01/29/2020 | Thomas Bachlechner | UCSD | Dr. Vachaspati | Testing the electric Aharonov-Bohm effect: electromagnetic memory vs. boundary gauge invariance | ||

02/05/2020 | Peter Geltenbort | Institut Laue Langevin | Dr. Alarcon | Probing Early Universe Particle Physics with Neutrons | ||

02/13/2020 (Thursday @ 12PM) | Kathryn Zurek | CalTech | Dr.Keeler | Spacetime fluctuations in AdS/CFT | ||

02/19/2020 | Tanmay Vachaspati | ASU | COSMO | Dynamical quantum collapse and an experimental test | ||

02/26/2020 | Benjamin Basso | ENS (Paris) | Dr. Belitsky | Six-gluon scattering amplitude at the origin in planar N=4 SYM | ||

04/15/2020 | Dr. Xiao Fang | University of Arizona | Cecilia Lunardini | ONLINE ONLY | ||

04/22/2020 | Prof. Lam Hui | Columbia University | ONLINE ONLY |

Date | Speaker | Institution | Title | Host | |
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9/11/2019 | FALL 2019 Welcome Reception | ASU | Tanmay Vachaspati | ||

9/18/2019 | Henry Lamm | University of Maryland | Quantum Computers for Quantum Field Theory | Rich Lebed | |

9/25/2019 | Ryan Westernacher-Schneider | University of Arizona | Multimessenger Seismology of Core-Collapse Supernovae | Dr. Lunardini | |

10/1/2019 | Ubirajara van Kolck | Institut de Physique Nucleaire d'Orsay and University of Arizona | A New Leading Mechanism for Neutrinoless Double-Beta Decay | Matthew Baumgart | |

10/9/2019 | Yue Zhao | University of Utah | Searching for Dark Photon Dark Matter with Gravitational Wave Detectors | Matthew Baumgart | |

10/16/2019 | Thiago Fleury | Federal University of Rio Grande do Norte | Correlation Functions in N=4 SYM and Integrability | Andrei Belitsky | |

10/23/2019 | Heling Deng | Arizona State University | Primordial black holes from primordial bubbles | Tanmay Vachaspati | |

10/30/2019 | Sergej Moroz | Technical University of Munich | Confined phases of fermions coupled to Z2 gauge fields | Andrei Belitsky | |

11/6/2019 | Atsushi Naruko | Yukawa Institute for Theoretical Physics | Possible resolution of a spacetime singularity with field transformations | George Zahariade | |

11/13/2019 | Ira Z. Rothstein | Carnegie Mellon University | Effective field theory for quantum mechanical black holes | Matthew Baumgart | |

11/20/2019 | Jaime Besprosvany | UNAM | Heavy quarks within the electroweak multiplet | Tanmay Vachaspati | |

HOLIDAY - THANKSGIVING | |||||

12/4/2019 | Jun Nian | Leinweber Center for Theoretical Physics, University of Michigan | Microstate Counting of Asymptotically AdS (Near-)BPS Black Holes and Hawking Radiation | Cynthia Keeler | |

Date | Speaker | Institution | Title | Host | |
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1/30/2019 | George Zahariade | ASU | Classical-Quantum Correspondence and Backreaction | Dr. Vachaspati | |

2/6/2019 | Raisa Trubko | Harvard | Precision Tune-out Wavelength Measurement with Atom Interferometry | Dr. Lunardini | |

2/20/2019 | Christoph Keller | University of Arizona | Holographic Conformal Field Theories in Two Dimensions | Dr. Keeler | |

2/27/2019 | Maulik Parikh | ASU | Forever Never Lasts: The Unruh-de Sitter State and the End of Eternal Inflation | Dr. Wilczek | |

3/13/2019 | Yanou Cui | UC Riverside | Probing the early Universe with gravitational waves from cosmic strings | Dr. Vachaspati | |

3/20/2019 | Andrew Long | University of Michigan | Ultra-light dark photons from a network of cosmic strings | Dr. Vachaspati | |

3/27/2019 | Yuber Perez | Fermi Lab | Neutrinos in Dark Matter detection experiments: Standard Model and Beyond. | Dr. Lunardini | |

4/10/2019 | Andres Luna | UCLA | Black holes and the double copy. | Dr. Keeler | |

4/17/2019 | Lucien Heurtier | UofA | EeV scale dark-matter: production mechanism through the inflaton portal and experimental signatures using the ANITA collaboration | Dr. Baumgart | |

4/24/2019 | Eleni Kontou | University of York | Quantum strong energy inequality and the Hawking singularity theorem | Dr. Vachaspati | |

5/1/2019 | Timothy Tait | UC Irvine | An Early Phase of QCD Confinement and the Baryon Asymmetry of the Universe | Dr. Baumgart |