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- W4381094251 abstract "Abstract We propose the first Se arch for D ark S ector at the Brazilian Synchrotron Light Laboratory, site of Sirius, a fourth-generation storage ring. We show that UVX, Sirius predecessor, can be a promising dark sector detector, SeDS , with unprecedented sensitivity. The search is based on a $$1-3$$ <mml:math xmlns:mml=http://www.w3.org/1998/Math/MathML> <mml:mrow> <mml:mn>1</mml:mn> <mml:mo>-</mml:mo> <mml:mn>3</mml:mn> </mml:mrow> </mml:math> GeV positron beam impinging on a thick target leading the $$e^+ e^- rightarrow gamma A'$$ <mml:math xmlns:mml=http://www.w3.org/1998/Math/MathML> <mml:mrow> <mml:msup> <mml:mi>e</mml:mi> <mml:mo>+</mml:mo> </mml:msup> <mml:msup> <mml:mi>e</mml:mi> <mml:mo>-</mml:mo> </mml:msup> <mml:mo>→</mml:mo> <mml:mi>γ</mml:mi> <mml:msup> <mml:mi>A</mml:mi> <mml:mo>′</mml:mo> </mml:msup> </mml:mrow> </mml:math> reaction, followed by a missing mass spectrum event reconstruction. We show that SeDS has the potential to probe dark photons with masses up to 55 MeV and kinetic coupling down to $$epsilon ^2 sim 10^{-12}$$ <mml:math xmlns:mml=http://www.w3.org/1998/Math/MathML> <mml:mrow> <mml:msup> <mml:mi>ϵ</mml:mi> <mml:mn>2</mml:mn> </mml:msup> <mml:mo>∼</mml:mo> <mml:msup> <mml:mn>10</mml:mn> <mml:mrow> <mml:mo>-</mml:mo> <mml:mn>12</mml:mn> </mml:mrow> </mml:msup> </mml:mrow> </mml:math> . Therefore, such experiment would constitute the best dark photon probe worldwide in the $$10{-}55$$ <mml:math xmlns:mml=http://www.w3.org/1998/Math/MathML> <mml:mrow> <mml:mn>10</mml:mn> <mml:mo>-</mml:mo> <mml:mn>55</mml:mn> </mml:mrow> </mml:math> MeV mass range, being able to probe an unexplored region of parameter space." @default.
- W4381094251 created "2023-06-18" @default.
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- W4381094251 date "2023-06-17" @default.
- W4381094251 modified "2023-10-07" @default.
- W4381094251 title "Search for dark sector by repurposing the UVX Brazilian synchrotron" @default.
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- W4381094251 doi "https://doi.org/10.1140/epjc/s10052-023-11603-x" @default.
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