Larmor Power Limit for Cyclotron Radiation of Relativistic Particles in a Waveguide
Cyclotron radiation emission spectroscopy (CRES) is a modern technique for high-precision energy spectroscopy, in which the energy of a charged particle in a magnetic field is measured via the frequency of the emitted cyclotron radiation. The He6-CRES collaboration aims to use CRES to probe beyond t...
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| creator | Buzinsky, N Taylor, R J Byron, W DeGraw, W Dodson, B Fertl, M García, A Goodson, A P Graner, B Harrington, H Hayen, L Malavasi, L McClain, D Melconian, D Müller, P Novitski, E Oblath, N S Robertson, R G H Rybka, G Savard, G Smith, E Stancil, D D Storm, D W Swanson, H E Tedeschi, J R VanDevender, B A Wietfeldt, F E Young, A R |
| description | Cyclotron radiation emission spectroscopy (CRES) is a modern technique for high-precision energy spectroscopy, in which the energy of a charged particle in a magnetic field is measured via the frequency of the emitted cyclotron radiation. The He6-CRES collaboration aims to use CRES to probe beyond the standard model physics at the TeV scale by performing high-resolution and low-background beta-decay spectroscopy of \({}^6\textrm{He}\) and \({}^{19}\textrm{Ne}\). Having demonstrated the first observation of individual, high-energy (0.1 -- 2.5 MeV) positrons and electrons via their cyclotron radiation, the experiment provides a novel window into the radiation of relativistic charged particles in a waveguide via the time-derivative (slope) of the cyclotron radiation frequency, \(\mathrm{d}f_\textrm{c}/\mathrm{d}t\). We show that analytic predictions for the total cyclotron radiation power emitted by a charged particle in circular and rectangular waveguides are approximately consistent with the Larmor formula, each scaling with the Lorentz factor of the underlying \(e^\pm\) as \(\gamma^4\). This hypothesis is corroborated with experimental CRES slope data. |
| doi_str_mv | 10.48550/arxiv.2405.06847 |
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The He6-CRES collaboration aims to use CRES to probe beyond the standard model physics at the TeV scale by performing high-resolution and low-background beta-decay spectroscopy of \({}^6\textrm{He}\) and \({}^{19}\textrm{Ne}\). Having demonstrated the first observation of individual, high-energy (0.1 -- 2.5 MeV) positrons and electrons via their cyclotron radiation, the experiment provides a novel window into the radiation of relativistic charged particles in a waveguide via the time-derivative (slope) of the cyclotron radiation frequency, \(\mathrm{d}f_\textrm{c}/\mathrm{d}t\). We show that analytic predictions for the total cyclotron radiation power emitted by a charged particle in circular and rectangular waveguides are approximately consistent with the Larmor formula, each scaling with the Lorentz factor of the underlying \(e^\pm\) as \(\gamma^4\). This hypothesis is corroborated with experimental CRES slope data.</description><identifier>EISSN: 2331-8422</identifier><identifier>DOI: 10.48550/arxiv.2405.06847</identifier><language>eng</language><publisher>Ithaca: Cornell University Library, arXiv.org</publisher><subject>Beta decay ; Charged particles ; Cyclotron radiation ; Cyclotrons ; Lorentz factor ; Particle physics ; Physics - Nuclear Experiment ; Positrons ; Radiation ; Rectangular waveguides ; Relativistic effects ; Relativistic particles ; Spectrum analysis</subject><ispartof>arXiv.org, 2024-12</ispartof><rights>2024. This work is published under http://arxiv.org/licenses/nonexclusive-distrib/1.0/ (the “License”). 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The He6-CRES collaboration aims to use CRES to probe beyond the standard model physics at the TeV scale by performing high-resolution and low-background beta-decay spectroscopy of \({}^6\textrm{He}\) and \({}^{19}\textrm{Ne}\). Having demonstrated the first observation of individual, high-energy (0.1 -- 2.5 MeV) positrons and electrons via their cyclotron radiation, the experiment provides a novel window into the radiation of relativistic charged particles in a waveguide via the time-derivative (slope) of the cyclotron radiation frequency, \(\mathrm{d}f_\textrm{c}/\mathrm{d}t\). We show that analytic predictions for the total cyclotron radiation power emitted by a charged particle in circular and rectangular waveguides are approximately consistent with the Larmor formula, each scaling with the Lorentz factor of the underlying \(e^\pm\) as \(\gamma^4\). 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| subjects | Beta decay Charged particles Cyclotron radiation Cyclotrons Lorentz factor Particle physics Physics - Nuclear Experiment Positrons Radiation Rectangular waveguides Relativistic effects Relativistic particles Spectrum analysis |
| title | Larmor Power Limit for Cyclotron Radiation of Relativistic Particles in a Waveguide |
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