Clemente Smarra

ORCID: 0000-0002-0817-2830
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About
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Research Areas
  • Dark Matter and Cosmic Phenomena
  • Cosmology and Gravitation Theories
  • Particle physics theoretical and experimental studies
  • Pulsars and Gravitational Waves Research
  • Quantum Chromodynamics and Particle Interactions
  • Quantum Electrodynamics and Casimir Effect
  • Radio Astronomy Observations and Technology
  • Geophysics and Gravity Measurements
  • Scientific Research and Discoveries
  • Galaxies: Formation, Evolution, Phenomena

Istituto Nazionale di Fisica Nucleare, Sezione di Trieste
2023-2025

Scuola Internazionale Superiore di Studi Avanzati
2023-2025

University of Trieste
2024

Institute for Fundamental Physics of the Universe
2023-2024

Pulsar Timing Array experiments probe the presence of possible scalar or pseudoscalar ultralight dark matter particles through decade-long timing an ensemble galactic millisecond radio pulsars. With second data release European Array, we focus on most robust scenario, in which interacts only gravitationally with ordinary baryonic matter. Our results show that masses 10^{-24.0} eV≲m≲10^{-23.3} eV cannot constitute 100% measured local density, but can have at density ρ≲0.3 GeV/cm^{3}.

10.1103/physrevlett.131.171001 article EN Physical Review Letters 2023-10-25

Abstract A coherently oscillating ultra-light axion can behave as dark matter. In particular, its pressure perturbations source an scalar metric perturbation, with a characteristic oscillation frequency which is twice the Compton frequency. candidate in mass range 10 (-24,-21) eV provide signal tested by current and future Pulsar Timing Array (PTA) programs. Involving highly nonlinear environment, such analysis demands relativistic treatment. Here, we rigorous derivation of effect assuming...

10.1088/1475-7516/2024/02/014 article EN Journal of Cosmology and Astroparticle Physics 2024-02-01

Millisecond pulsars are extremely precise celestial clocks: as they rotate, the beamed radio waves emitted along axis of their magnetic field can be detected with telescopes, which allows for tracking subtle changes in pulsars' rotation periods. A possible effect on period a pulsar is given by potential coupling to dark matter, cases where it modeled an "ultralight" scalar field. In this paper, we consider universal conformal matter gravity, turn mediates effective between and matter. If...

10.1103/physrevd.110.043033 article EN Physical review. D/Physical review. D. 2024-08-26

Millisecond pulsars are extremely stable natural timekeepers. Pulsar Timing Array experiments, tracking subtle changes in the pulsars' rotation periods, can shed light on presence of ultralight particles our Galaxy. In this conference paper, we start by reviewing most conservative scenario, which interact only gravitationally. setting, show that Arrays able to constrain fields up a few tenths observed dark matter abundance. Then, consider conformally coupled candidates, demonstrating...

10.22323/1.474.0015 preprint EN cc-by-nc-nd 2025-01-29

In the presence of a magnetic field, axions can convert into photons and vice versa. The phenomenology conversion is captured by system two coupled Klein-Gordon equations, which, assuming that axion relativistic, usually recast pair first-order Schrödinger-like equations. such limit, focusing on constant field plasma frequency, equations admit an exact analytic solution. relativistic limit significantly simplifies calculations and, therefore, it widely used in phenomenological applications....

10.1103/physrevd.111.063021 article EN cc-by Physical review. D/Physical review. D. 2025-03-10

A pseudo Nambu-Goldstone boson (PNGB) coupled to a confining gauge group via an anomalous term is characterised, during the phase transition, by temperature dependent mass $m^2(T) \propto T^{-n}$. For $n>2$, non-relativistic population of such particles dominating cosmological energy density would act as dark (DE), accelerating expansion. We study possibility that PNGB $\varphi_b$ hidden presently undergoing confinement could realise this scenario. To obtain observed amount DE, number must...

10.48550/arxiv.2405.00090 preprint EN arXiv (Cornell University) 2024-04-30

A bstract local flavour symmetry acting on the quarks of Standard Model can automatically give rise to an accidental global U(1) which remains preserved from sources explicit breaking up a large operator dimension, while it gets spontaneously broken together with symmetry. Such non-fundamental symmetries are often endowed mixed QCD anomaly, so that strong CP problem is solved via axion mechanism. We illustrate general features required realise this scenario, and we discuss simple...

10.1007/jhep02(2023)201 article EN cc-by Journal of High Energy Physics 2023-02-20

In the presence of a magnetic field, axions can convert into photons and viceversa. The phenomenology conversion is captured by system two coupled Klein-Gordon equations, which, assuming that axion relativistic, usually recast pair first order Schr\"odinger-like equations. such limit, focusing on constant field plasma frequency, equations admit an exact analytic solution. relativistic limit significantly simplifies calculations; therefore, it widely used in phenomenological applications....

10.48550/arxiv.2410.02662 preprint EN arXiv (Cornell University) 2024-10-03

A coherently oscillating ultra-light axion can behave as dark matter. In particular, its pressure perturbations source an scalar metric perturbation, with a characteristic oscillation frequency which is twice the Compton frequency. candidate in mass range $10^{(-24,-21)}{\rm eV}$ provide signal tested by current and future Pulsar Timing Array (PTA) programs. Involving highly nonlinear environment, such analysis demands relativistic treatment. Here, we rigorous derivation of effect assuming...

10.48550/arxiv.2311.00234 preprint EN other-oa arXiv (Cornell University) 2023-01-01

A local flavour symmetry acting on the quarks of Standard Model can automatically give rise to an accidental global $U(1)$ which remains preserved from sources explicit breaking up a large operator dimension, while it gets spontaneously broken together with symmetry. Such non-fundamental symmetries are often endowed mixed QCD anomaly, so that strong CP problem is solved via axion mechanism. We illustrate general features required realise this scenario, and we discuss simple construction...

10.48550/arxiv.2211.05796 preprint EN cc-by arXiv (Cornell University) 2022-01-01
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