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PIKIMO 18, University of Kentucky, 19 April 2025
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America/New_York
153 (Chemistry Physics (CP) Building )
153
Chemistry Physics (CP) Building
506 Library Drive, Lexington KY 40506
(CP 153 faces the blocked-off continuation of Rose St.)
Susan Gardner
(University of Kentucky),
Richard Hill
(University of Kentucky)
Description
The Department of Physics and Astronomy at the University of Kentucky is pleased to host PIKIMO 18, April 19, 2025.
PIKIMO ("Phenomenology in Indiana, Kentucky, Illinois, Michigan, and Ohio") is a series of informal pheno meetings, geared towards graduate students and young postdocs. Its goal is to connect researchers at "local" institutions in the midwest (roughly at driving distance from each other). The meetings usually happen on a Saturday during the fall and spring terms and feature short presentations, one or two longer talks by invited keynote speakers, and ample time of discussion during lunch and coffee breaks.
Invited speakers: Gordan Krnjaic (Fermilab / U. Chicago) and Tim Kovachy (Northwestern U.)
Registration
PIKIMO 18 Spring 2025
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08:30
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09:30
Breakfast 1h
A continental breakfast (coffee, donuts) will be set up in the hallway outside CP153
--- this faces the blocked-off continuation of Rose St. -
09:30
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10:30
Morning keynote: Gordan Krnjaic (Fermilab / U. Chicago)Convener: Richard Hill (University of Kentucky)
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09:30
Observable CMB B-modes from Cosmological Phase Transitions 1hSpeaker: Gordan Krnjaic (Fermilab)
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09:30
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10:30
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12:00
Morning contributed talks (chairperson R. Hill)
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10:30
Enhancing Solar Neutrino Sensitivity with Neutron Tagging 30m
Solar neutrinos provide crucial insights into the Sun’s fusion processes and neutrino oscillations in matter. However, detecting them requires effective suppression of backgrounds. One of these is spallation backgrounds—beta decays of unstable isotopes produced by cosmic-ray muons— which pose a major challenge above 6 MeV. We show that neutron tagging, made possible by the recent addition of dissolved gadolinium, provides a powerful new method to identify and reject these backgrounds. This technique is particularly relevant for future shallower detectors like Hyper-Kamiokande and JUNO.
Speaker: Obada Nairat (The Ohio State University) -
11:00
Non-Gaussianity from explicit $U(1)$-breaking interactions 30m
We investigate primordial non-Gaussianity (NG) that arises from explicit $U(1)$ symmetry-breaking interactions during inflation, focusing on a nearly massless axial component of a complex scalar field $P$. We compute the resulting NG parameter $f_{\mathrm{NL}}$, allowing the axial field to act as either a curvaton or cold dark matter (CDM). We consider two scenarios in which the interaction emerges from an explicit $U(1)$ symmetry-breaking potential and from explicit $U(1)$ symmetry-breaking kinetic mixing. We also explore the role of a heavy radial field in generating oscillating correlation signals, noting that such signals can dominate the shape of the mixed adiabatic-isocurvature bispectrum. In certain cases, an oscillatory isocurvature bispectrum signal may be observable in the future, aiding in distinguishing between certain types of the $U(1)$-breaking self-interactions of the axial field.
Speaker: Taegyu Lee (Indiana University) -
11:30
Constraining Cosmological Phase Transitions through Curvature Perturbations 30m
Cosmological first order phase transitions proceed via the random nucleation and expansion of bubbles throughout space. This inherently stochastic process leads to statistical fluctuations across causally disconnected patches from which super-horizon curvature perturbations emerge. I will discuss how such phase transitions generate scalar perturbations that follow a universal power-law scaling in the phase transition parameters. By numerically modelling the resulting curvature perturbation, we can set constraints on the phase transition parameters in light of cosmological data such as CMB, Lyman-alpha, and the observation of dynamical heating in ultra-faint dwarf galaxies. This gives us a handle on constraining cosmological phase transitions even if they occur in a dark sector that interacts with us only gravitationally.
Speaker: Daven Wei Ren Ho
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10:30
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12:00
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13:30
Lunch 1h 30m
Box lunches from Panera (and beverages) will be provided to registered participants (as of 4/14/25); they will be made available in the hallway outside of CP 153 where breakfast was served.
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13:30
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14:30
Afternoon keynote: Timothy Kovachy (Northwestern University)Convener: Susan Gardner (University of Kentucky)
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13:30
New Tools for Dark Matter and Gravitational Wave Detection: Cryogenic Optical Resonators and Long-Baseline Atom Interferometers 1h
Abstract: The search for dark matter and for new sources of gravitational waves offers potentially revolutionary opportunities to learn about the fundamental properties of the Universe. Strong astrophysical evidence indicates that dark matter makes up most of the matter in the Universe, yet its nature remains a great mystery. The detection of gravitational waves in currently unexplored frequency ranges could provide unique insights into astrophysics and cosmology. In this talk, I will discuss two emerging techniques for probing dark matter and gravitational waves. The first method involves precise optical comparisons of the lengths of cryogenic, vibration-isolated optical resonators. I will discuss the results from the first dark matter search using this approach, as well as prospects for using this method for high-frequency gravitational wave detection. The second method, long-baseline atom interferometry, involves the coherent splitting of the wavefunctions of atoms over large distances and the subsequent observation of interference of the recombined wave packets. I will introduce MAGIS-100—a 100-meter-tall atom interferometer currently under construction at Fermilab—and describe experimental demonstrations of a new approach to atom interferometry that paves the way for long-baseline atom interferometers to reach their full scientific potential.
Speaker: Timothy Kovachy
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13:30
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14:30
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17:30
Afternoon contributed talks (chairperson S. Gardner)
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14:30
New Physics from Light Scalars in Rare Kaon Decay 30m
We introduce and investigate the effects of a light scalar interacting with the
short-lived kaon and the KS → μ+μ− decay. We use the results of searches performed at
kaon factories as well as the Standard Model predictions for this decay to constrain the
couplings of a ϕ particle with a mass mϕ of the order of MeV. In addition to this we find
the allowed parameter space for further CP violating effects in this decay mode as well as
to one loop order. We also examine the time evolution of the kaon beams with the full
mixing considered and the effect of its lifetime on extractable experimental parameters.Speaker: Rahul Pradeep (University of Cincinnati) -
15:00
The Z \alpha^2 order radiative correction to nuclear beta decays 30m
Superallowed nuclear beta decays offer one of the most precise ways of extracting the CKM matrix |V_ud|, which is an important parameter in the Standard Model. QED radiative corrections play an important role in the precision computation of nuclear beta decays, which can be expressed in a series of Z \alpha and \alpha. Given the current experimental uncertainty, the order Z \alpha^2 correction should be taken into account. In this talk, I show how the virtual contribution to the Z \alpha^2 correction can be computed using factorization in the limit of small electron mass. I demonstrate the formalism by reproducing Sirlin's g function at one loop order, and discuss the inclusion of real photons and finite electron mass for the Z \alpha^2 correction.
Speaker: Zehua Cao -
15:30
Electron EDM and Γ(μ → eγ) in the 2HDM 30m
We present the first complete two-loop calculation of the electric dipole moment of the electron, as well as the rates of the lepton-flavor violating decays μ→e+γ and τ→e/μ+γ, in the unconstrained two-Higgs doublet model. We include the most general Yukawa interactions of the Higgs doublets with the Standard Model fermions up to quadratic order, and allow for generic phases in the Higgs potential. A python implementation of our results is provided via a public git repository.
Speaker: Daniil Volkov (University of Cinccinati) -
16:00
The Fermi Function, Factorization and the Neutron’s Lifetime 30m
The neutron lifetime is a precision observable of the Standard Model probing the CKM matrix element $|V_{ud}|$ and beyond the Standard Model physics. For nuclear beta decay, in the region of small electron velocity or the limit of large nuclear charge $Z$, a Fermi function is used to account for enhanced perturbative effects. In this talk, I will present the derivation of the quantum field theoretic analog of the Fermi function valid for neutron beta decay in which neither of the aforementioned limits apply. This QFT analog is related to renormalization group effects of objects occurring in the context of a factorization formula valid in the limit of small electron mass. I will introduce this factorization formula and present results through two-loop order. The main phenomenological results are two-loop input to the long-distance corrections to neutron beta decay and an accompanying calculation of $|V_{ud}|$.
Speaker: Peter Vander Griend -
16:30
BREAK 10m
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16:40
Primordial black holes and induced gravitational waves from an underdamped axion-like curvaton 25m
We explore the generation of primordial black holes (PBHs) and second-order induced gravitational waves (GWs) arising from underdamped isocurvature fluctuations of an axion-like curvaton field. During inflation, the radial component of the curvaton undergoes underdamped evolution, leading to a resonant amplification of the curvaton's quantum fluctuations. This mechanism imprints scale-dependent oscillations and localized bumps in the blue-tilted isocurvature power spectrum. In large regions of parameter space, these enhancements can exceed three orders of magnitude. While standard quadratic curvaton models fail to produce dark matter-like PBHs from Gaussian fluctuations, we show that the dynamically induced non-adiabatic features in our scenario can successfully overcome this limitation. As a result, both PBHs and a detectable stochastic GW background are generated, with distinctive oscillatory signatures in the GW spectrum offering a new observational avenue.
Speaker: Dr Sai Chaitanya Tadepalli (Dept of Physics, Indiana University, Bloomington) -
17:05
Direct detection of ultralight dark matter with charged lepton flavor violation 25m
I will discuss a class of ultralight dark matter models with charged-lepton-flavor violating couplings that can induce potentially observable time-dependent signals at the intensity frontier. I will highlight the sensitivity of current/future experiments and outline possible UV completions.
Speaker: Tony Menzo
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14:30
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08:30
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09:30
