activity
20162026
most citedThe Structure of the Oscillon: The Dynamics of Attractive Self-Interaction

40 citations · 136 across the 12 of their papers we have counts for

collaborators

13 papers

hep-ph2026

Technically Natural Baryogenesis with the QCD Axion

Pouya Asadi, David Cyncynates, Stefania Gori

The strong CP problem, dark matter, and the observed baryon abundance may all be connected dynamically through the QCD axion, though whether this connection is realized in Nature d…

hep-ph2026

Axiverse Lampposts

Masha Baryakhtar, David Cyncynates, Ella Henry

The string axiverse predicts a unique connection between the high scales approachable only through theory and the low energies within reach of experimental verification: a multitud…

hep-ph2025

Axiverse Baryogenesis

Pouya Asadi, David Cyncynates, Stefania Gori

The QCD axion may offer a unified origin for the baryon asymmetry and dark matter through axiogenesis. However, in the minimal QCD axion scenario, axiogenesis either underproduces…

hep-ph2024

Scalar relics from the hot Big Bang

David Cyncynates, Olivier Simon

In this Letter, we motivate the fact that couplings between a scalar field and the Standard Model with strengths relative to gravity yield the total…

hep-ph2024★ 16 cited

Experimental targets for dark photon dark matter

David Cyncynates, Zachary J. Weiner

Ultralight dark photon dark matter features distinctive cosmological and astrophysical signatures and is also supported by a burgeoning direct-detection program searching for its k…

hep-ph2024

Minimal targets for dilaton direct detection

David Cyncynates, Olivier Simon

Fifth force and equivalence principle tests search for new interactions by precisely measuring forces between macroscopic collections of atoms and molecules and their properties un…

hep-ph2023★ 17 cited

Detectable and defect-free dark photon dark matter

David Cyncynates, Zachary J. Weiner

Ultralight dark photons are compelling dark matter candidates, but their allowed kinetic mixing with the Standard Model photon is severely constrained by requiring that the dark ph…

hep-ph2023

Heavy QCD axion dark matter from avoided level crossing

David Cyncynates, Jedidiah O. Thompson

The QCD axion offers a natural resolution to the strong CP problem and provides a compelling dark matter candidate. If the QCD axion constitutes all the dark matter, the simplest m…

hep-ph2022★ 18 cited

Nonperturbative structure in coupled axion sectors and implications for direct detection

David Cyncynates, Olivier Simon, Jedidiah O. Thompson +1

Pairs of misalignment-produced axions with nearby masses can experience a nonlinear resonance that leads to enhanced direct and astrophysical signatures of axion dark matter. In mu…

hep-ph2021★ 35 cited

Friendship in the Axiverse: Late-time direct and astrophysical signatures of early-time nonlinear axion dynamics

David Cyncynates, Tudor Giurgica-Tiron, Olivier Simon +1

A generic low-energy prediction of string theory is the existence of a large collection of axions, commonly known as a string axiverse. Axions also have a natural cosmological prod…

hep-ph2021★ 40 cited

The Structure of the Oscillon: The Dynamics of Attractive Self-Interaction

David Cyncynates, Tudor Giurgica-Tiron

Real scalar fields with attractive self-interaction may form self-bound states, called oscillons. These dense objects are ubiquitous in leading theories of dark matter and inflatio…

astro-ph.GA2017

Could 1I/'Oumuamua be macroscopic dark matter?

David Cyncynates, Emanuela Dimastrogiovanni, Saurabh Kumar +2

1I/'Oumuamua, formerly known as A/2017 U1, is a sizable body currently passing through the solar system. It is generally considered to be a rocky asteroid-like object that came fro…

astro-ph.CO2016★ 10 cited

Reconsidering seismological constraints on the available parameter space of macroscopic dark matter

David Cyncynates, Joshua Chiel, Jagjit Sidhu +1

Using lunar seismological data, constraints have been proposed on the available parameter space of macroscopic dark matter (macros). We show that actual limits are considerably wea…