Kaluza-Klein axions appear in theories with extra dimensions as higher mass, significantly shorter lifetime, excitations of the Peccei-Quinn axion. When produced in the Sun, they would remain gravitationally trapped in the solar system, and their decay to a pair of photons could provide an explanation of the solar corona heating problem. A low-density detector would discriminate such a signal from the background, by identifying the separation of the interaction point of the two photons. The NEWS-G collaboration uses large volume spherical proportional counters, gas-filled metallic spheres with a spherical anode in their centre. After observation of a single axionlike event in a 42 day long run with the SEDINE detector, a 90% C.L. upper limit of is set on the axion-photon coupling for the benchmark of a Kaluza-Klein axion density on Earth of and two extra dimensions of size .
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"value": "Kaluza-Klein axions appear in theories with extra dimensions as higher mass, significantly shorter lifetime, excitations of the Peccei-Quinn axion. When produced in the Sun, they would remain gravitationally trapped in the solar system, and their decay to a pair of photons could provide an explanation of the solar corona heating problem. A low-density detector would discriminate such a signal from the background, by identifying the separation of the interaction point of the two photons. The NEWS-G collaboration uses large volume spherical proportional counters, gas-filled metallic spheres with a spherical anode in their centre. After observation of a single axionlike event in a 42 day long run with the SEDINE detector, a 90% C.L. upper limit of <math><mrow><msub><mrow><mi>g</mi></mrow><mrow><mi>a</mi><mi>\u03b3</mi><mi>\u03b3</mi></mrow></msub><mo><</mo><mn>8.99</mn><mo>\u00d7</mo><msup><mrow><mn>10</mn></mrow><mrow><mo>\u2212</mo><mn>13</mn></mrow></msup><mtext> </mtext><mtext> </mtext><msup><mrow><mi>GeV</mi></mrow><mrow><mo>\u2212</mo><mn>1</mn></mrow></msup></mrow></math> is set on the axion-photon coupling for the benchmark of a Kaluza-Klein axion density on Earth of <math><mrow><msub><mrow><mi>n</mi></mrow><mrow><mi>a</mi></mrow></msub><mo>=</mo><mn>4.07</mn><mo>\u00d7</mo><msup><mrow><mn>10</mn></mrow><mrow><mn>13</mn></mrow></msup><mtext> </mtext><mtext> </mtext><msup><mrow><mi>m</mi></mrow><mrow><mo>\u2212</mo><mn>3</mn></mrow></msup></mrow></math> and two extra dimensions of size <math><mrow><mi>R</mi><mo>=</mo><mn>1</mn><mtext> </mtext><mtext> </mtext><msup><mrow><mi>eV</mi></mrow><mrow><mo>\u2212</mo><mn>1</mn></mrow></msup></mrow></math>."
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