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			<titleStmt><title level='a'>A measurement of the K+ → π+μ+μ− decay</title></titleStmt>
			<publicationStmt>
				<publisher></publisher>
				<date>11/01/2022</date>
			</publicationStmt>
			<sourceDesc>
				<bibl> 
					<idno type="par_id">10447112</idno>
					<idno type="doi">10.1007/JHEP11(2022)011</idno>
					<title level='j'>Journal of High Energy Physics</title>
<idno>1029-8479</idno>
<biblScope unit="volume">2022</biblScope>
<biblScope unit="issue">11</biblScope>					

					<author>E. Cortina Gil</author><author>A. Kleimenova</author><author>E. Minucci</author><author>S. Padolski</author><author>P. Petrov</author><author>A. Shaikhiev</author><author>R. Volpe</author><author>T. Numao</author><author>Y. Petrov</author><author>B. Velghe</author><author>V. W. Wong</author><author>D. Bryman</author><author>J. Fu</author><author>T. Husek</author><author>J. Jerhot</author><author>K. Kampf</author><author>M. Zamkovsky</author><author>R. Aliberti</author><author>G. Khoriauli</author><author>J. Kunze</author><author>D. Lomidze</author><author>L. Peruzzo</author><author>M. Vormstein</author><author>R. Wanke</author><author>P. Dalpiaz</author><author>M. Fiorini</author><author>I. Neri</author><author>A. Norton</author><author>F. Petrucci</author><author>H. Wahl</author><author>A. Cotta Ramusino</author><author>A. Gianoli</author><author>E. Iacopini</author><author>G. Latino</author><author>M. Lenti</author><author>A. Parenti</author><author>A. Bizzeti</author><author>F. Bucci</author><author>A. Antonelli</author><author>G. Georgiev</author><author>V. Kozhuharov</author><author>G. Lanfranchi</author><author>S. Martellotti</author><author>M. Moulson</author><author>T. Spadaro</author><author>G. Tinti</author><author>F. Ambrosino</author><author>T. Capussela</author><author>M. Corvino</author><author>D. Di Filippo</author><author>R. Fiorenza</author><author>P. Massarotti</author><author>M. Mirra</author><author>M. Napolitano</author><author>G. Saracino</author><author>G. Anzivino</author><author>F. Brizioli</author><author>E. Imbergamo</author><author>R. Lollini</author><author>R. Piandani</author><author>C. Santoni</author><author>M. Barbanera</author><author>P. Cenci</author><author>B. Checcucci</author><author>P. Lubrano</author><author>M. Lupi</author><author>M. Pepe</author><author>M. Piccini</author><author>F. Costantini</author><author>L. Di Lella</author><author>N. Doble</author><author>M. Giorgi</author><author>S. Giudici</author><author>G. Lamanna</author><author>E. Lari</author><author>E. Pedreschi</author><author>M. Sozzi</author><author>C. Cerri</author><author>R. Fantechi</author><author>L. Pontisso</author><author>F. Spinella</author><author>I. Mannelli</author><author>G. D’Agostini</author><author>M. Raggi</author><author>A. Biagioni</author><author>P. Cretaro</author><author>O. Frezza</author><author>E. Leonardi</author><author>A. Lonardo</author><author>M. Turisini</author><author>P. Valente</author><author>P. Vicini</author><author>R. Ammendola</author><author>V. Bonaiuto</author><author>A. Fucci</author><author>A. Salamon</author><author>F. Sargeni</author><author>R. Arcidiacono</author><author>B. Bloch-Devaux</author><author>M. Boretto</author><author>E. Menichetti</author><author>E. Migliore</author><author>D. Soldi</author><author>C. Biino</author><author>A. Filippi</author><author>F. Marchetto</author><author>J. Engelfried</author><author>N. Estrada-Tristan</author><author>A. M. Bragadireanu</author><author>S. A. Ghinescu</author><author>O. E. Hutanu</author><author>A. Baeva</author><author>D. Baigarashev</author><author>D. Emelyanov</author><author>T. Enik</author><author>V. Falaleev</author><author>V. Kekelidze</author><author>A. Korotkova</author><author>L. Litov</author><author>D. Madigozhin</author><author>M. Misheva</author><author>N. Molokanova</author><author>S. Movchan</author><author>I. Polenkevich</author><author>Yu. Potrebenikov</author><author>S. Shkarovskiy</author><author>A. Zinchenko</author><author>S. Fedotov</author><author>E. Gushchin</author><author>A. Khotyantsev</author><author>Y. Kudenko</author><author>V. Kurochka</author><author>M. Medvedeva</author><author>A. Mefodev</author><author>S. Kholodenko</author><author>V. Kurshetsov</author><author>V. Obraztsov</author><author>A. Ostankov</author><author>V. Semenov</author><author>V. Sugonyaev</author><author>O. Yushchenko</author><author>L. Bician</author><author>T. Blazek</author><author>V. Cerny</author><author>Z. Kucerova</author><author>J. Bernhard</author><author>A. Ceccucci</author><author>H. Danielsson</author><author>N. De Simone</author><author>F. Duval</author><author>B. Döbrich</author><author>L. Federici</author><author>E. Gamberini</author><author>L. Gatignon</author><author>R. Guida</author><author>F. Hahn</author><author>E. B. Holzer</author><author>B. Jenninger</author><author>M. Koval</author><author>P. Laycock</author><author>G. Lehmann Miotto</author><author>P. Lichard</author><author>A. Mapelli</author><author>R. Marchevski</author><author>K. Massri</author><author>M. Noy</author><author>V. Palladino</author><author>M. Perrin-Terrin</author><author>J. Pinzino</author><author>V. Ryjov</author><author>S. Schuchmann</author><author>S. Venditti</author><author>T. Bache</author><author>M. B. Brunetti</author><author>V. Duk</author><author>V. Fascianelli</author><author>J. R. Fry</author><author>F. Gonnella</author><author>E. Goudzovski</author><author>J. Henshaw</author><author>L. Iacobuzio</author><author>C. Lazzeroni</author><author>N. Lurkin</author><author>F. Newson</author><author>C. Parkinson</author><author>A. Romano</author><author>A. Sergi</author><author>A. Sturgess</author><author>J. Swallow</author><author>A. Tomczak</author><author>H. Heath</author><author>R. Page</author><author>S. Trilov</author><author>B. Angelucci</author><author>D. Britton</author><author>C. Graham</author><author>D. Protopopescu</author><author>J. Carmignani</author><author>J. B. Dainton</author><author>R. W. Jones</author><author>G. Ruggiero</author><author>L. Fulton</author><author>D. Hutchcroft</author><author>E. Maurice</author><author>B. Wrona</author><author>A. Conovaloff</author><author>P. Cooper</author><author>D. Coward</author><author>P. Rubin</author>
				</bibl>
			</sourceDesc>
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		<profileDesc>
			<abstract><ab><![CDATA[A              bstract                                      A sample of 2              .              8 × 10              4              K              +              →              π              +              μ              +              μ                              −                            candidates with negligible background was collected by the NA62 experiment at the CERN SPS in 2017–2018. The model-independent branching fraction is measured to be (9              .              15 ± 0              .              08) × 10                              −                8                            , a factor three more precise than previous measurements. The decay form factor is presented as a function of the squared dimuon mass. A measurement of the form factor parameters and their uncertainties is performed using a description based on Chiral Perturbation Theory at                                                $$ \mathcal{O} $$                                      O                                                              (              p              6              ).]]></ab></abstract>
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<div xmlns="http://www.tei-c.org/ns/1.0"><head>Introduction</head><p>The flavour-changing neutral current decays K &#177; &#8594; &#960; &#177; &#8467; + &#8467; -(denoted K &#960;&#8467;&#8467; ), with &#8467; = e, &#181; have been the focus of extensive theoretical work <ref type="bibr">[1]</ref><ref type="bibr">[2]</ref><ref type="bibr">[3]</ref><ref type="bibr">[4]</ref>. Dominant contributions to the K &#960;&#8467;&#8467; decays are mediated by virtual photon exchange K &#177; &#8594; &#960; &#177; &#947; * &#8594; &#960; &#177; &#8467; + &#8467; -and involve long-distance hadronic effects described by a vector interaction form factor.</p><p>Studies of the K &#960;ee and K &#960;&#181;&#181; decay form factors contribute to experimental tests of lepton flavour universality <ref type="bibr">[5,</ref><ref type="bibr">6]</ref>. The first lattice QCD calculation of the form factor value at a specific lepton pair mass (lying outside the K &#960;&#181;&#181; kinematic region) using physical lightquark masses is presented in <ref type="bibr">[7]</ref>. Future methodology optimizations together with advances in computing technology are expected to provide competitive lattice QCD predictions of the form factor.</p><p>The E787 collaboration at the Brookhaven National Laboratory reported the first observation of the K &#960;&#181;&#181; decay in 1997 <ref type="bibr">[8]</ref>, which was followed by the E865 <ref type="bibr">[9]</ref> and Hy-perCP <ref type="bibr">[10]</ref> measurements. The E865 result established the vector nature of the decay form factor, while HyperCP studied both K + &#960;&#181;&#181; and K - &#960;&#181;&#181; decays and measured the CP violating -1 -</p></div>
<div xmlns="http://www.tei-c.org/ns/1.0"><head>JHEP11(2022)011</head><p>decay rate asymmetry, found to be compatible with zero. The most precise study <ref type="bibr">[11]</ref> of K &#960;&#181;&#181; was performed by the NA48/2 collaboration at the CERN SPS. The K &#960;ee decay was first observed at the CERN PS by the Geneva-Saclay collaboration in 1975 <ref type="bibr">[12]</ref>, and subsequently measured by the E777 <ref type="bibr">[13]</ref>, E865 <ref type="bibr">[14]</ref> and NA48/2 <ref type="bibr">[15]</ref> experiments. A summary of form factor measurements can be found in <ref type="bibr">[16]</ref>. Improved measurements of the K &#960;&#181;&#181; model-independent branching fraction and form factor parameters, based on the dataset collected in 2017-2018 by the NA62 experiment at the CERN SPS, are presented in the following. The forward-backward asymmetry of the decay with respect to angle &#952; K&#181; between the K + and the &#181; -three-momenta in the &#181; + &#181; - rest frame, is also measured.</p></div>
<div xmlns="http://www.tei-c.org/ns/1.0"><head n="1">Beam, detector and data sample</head><p>The layout of the NA62 beamline and detector <ref type="bibr">[17]</ref> is shown schematically in figure <ref type="figure">1</ref>. An unseparated secondary beam of &#960; + (70%), protons (23%) and K + (6%) is created by directing 400 GeV/c protons extracted from the CERN SPS onto a beryllium target in spills of 3 s effective duration. The target position defines the origin of the NA62 reference system: the beam travels along the Z axis in the positive direction (downstream), the Y axis points vertically up, and the X axis is horizontal and directed to form a right-handed coordinate system. The central beam momentum is 75 GeV/c, with a momentum spread of 1% (rms).</p><p>Beam kaons are tagged with a time resolution of 70 ps by a differential Cherenkov counter (KTAG), which uses nitrogen gas at 1.75 bar pressure contained in a 5 m long vessel as radiator. Beam particle positions, momenta and times (to better than 100 ps resolution) are measured by a silicon pixel spectrometer consisting of three stations (GTK1,2,3) and four dipole magnets. A toroidal muon sweeper, called scraper (SCR), is installed between GTK1 and GTK2. A 1.2 m thick steel collimator (COL) with a 76&#215;40 mm 2 central aperture and 1.7 &#215; 1.8 m 2 outer dimensions is placed upstream of GTK3 to absorb hadrons from upstream K + decays; a variable aperture collimator of 0.15 &#215; 0.15 m 2 outer dimensions was used up to early 2018. Inelastic interactions of beam particles in GTK3 are detected by an array of scintillator hodoscopes (CHANTI). A dipole magnet (TRIM5) providing a 90 MeV/c horizontal momentum kick is located in front of GTK3. The beam is delivered into a vacuum tank evacuated to a pressure of 10 -6 mbar, which contains a 75 m long fiducial volume (FV) starting 2.6 m downstream of GTK3. The beam angular spread at the FV entrance is 0.11 mrad (rms) in both horizontal and vertical planes. Downstream of the FV, undecayed beam particles continue their path in vacuum.</p><p>Three-momenta of charged particles produced in K + decays are measured by a magnetic spectrometer (STRAW) located in the vacuum tank downstream of the FV. The spectrometer consists of four tracking chambers made of straw tubes, and a large aperture dipole magnet (M), located between the second and third chamber, that provides a horizontal momentum kick of 270 MeV/c. The momentum resolution is &#963; p /p = (0.30 &#8853; 0.005 &#8226; p)%, with the momentum p expressed in GeV/c.</p><p>-2 -</p></div>
<div xmlns="http://www.tei-c.org/ns/1.0"><head>JHEP11(2022)011</head><p>2&#181;MT line selects the K &#960;&#181;&#181; signal decays. The low-level hardware (L0) trigger <ref type="bibr">[19]</ref> for both lines is based on RICH signal multiplicity and coincidence of signals in two opposite CHOD quadrants. The 2&#181;MT line additionally involves a requirement of signal coincidence in two outer MUV3 tiles. The high-level software (L1) trigger requires K + identification by KTAG, and reconstruction of a negatively charged STRAW track for both MT and 2&#181;MT trigger lines. A detailed description of the NA62 trigger system and its performance is given in <ref type="bibr">[20]</ref>.</p><p>Monte Carlo (MC) simulations of particle interactions with the detector and its response are performed using a software package based on the Geant4 toolkit <ref type="bibr">[21]</ref>. In addition, the accidental activity is simulated, and the response of both trigger lines is emulated.</p></div>
<div xmlns="http://www.tei-c.org/ns/1.0"><head n="2">Event selection</head><p>Kinematic similarities of the signal (K &#960;&#181;&#181; ) and normalization (K 3&#960; ) decays allow for substantial overlap between the signal and normalization event selections, which results in first-order cancellation of most detector and trigger inefficiencies, thus reducing the systematic uncertainties in the measurement.</p><p>The following selection criteria are common to the K &#960;&#181;&#181; and K 3&#960; event selections.</p><p>&#8226; Each STRAW track is assigned a time computed as a weighted average of the associated CHOD hodoscope signals. The weights are obtained from the time resolutions of the CHOD hodoscopes. Triplets of STRAW tracks compatible with a common origin in the FV are combined into three-track vertices. Vertex time is defined as the weighted average of the times of CHOD signals associated with the vertex tracks.</p><p>&#8226; Exactly one three-track vertex with the following properties is required to be present: total charge q = 1, time within 6 ns of the trigger time, Z position between 110 m and 180 m from the target, total momentum compatible with the mean beam momentum within 2.5 GeV/c, total transverse momentum with respect to the beam axis below 30 MeV/c, and vertex distance from the beam axis below 5 cm. The beam axis and momentum are monitored throughout the data taking with fully reconstructed K 3&#960; decays. Only the three tracks forming the chosen vertex are considered in the following.</p><p>&#8226; All track times must be within 12 ns of the vertex time, and the vertex time is required to be within 6 ns of a KTAG kaon signal.</p><p>&#8226; The tracks must be within the geometrical acceptance of all STRAW chambers, and extrapolate to lie within the CHOD, LKr, and MUV3 acceptances.</p><p>&#8226; The track momenta should exceed 10 GeV/c to ensure track reconstruction efficiency above 90%. The angles between each track and the beam axis must be smaller than 9 mrad to reduce background to the K &#960;&#181;&#181; sample from K 3&#960; decays followed by &#960; &#177; &#8594; &#181; &#177; &#957; decays.</p><p>&#8226; The spatial separation between each pair of vertex tracks must be at least 15 mm in the plane of the first STRAW chamber and 200 mm in the LKr front plane to suppress photon conversions and the overlap of energy deposits.</p><p>The following particle identification criteria are employed.</p><p>&#8226; A track is identified as a charged pion if it has no spatially associated MUV3 signals within 10 ns of the vertex time, and the ratio of the associated LKr cluster energy to the track momentum is E/p &lt; 0.9.</p><p>&#8226; A track with E/p &lt; 0.2 is identified as a muon if it has a spatially associated MUV3 signal in an outer tile within 6 ns of both the vertex and the trigger times.</p><p>The following criteria are specific to the K &#960;&#181;&#181; event selection.</p><p>&#8226; Only vertices with tracks identified as &#960; + &#181; + &#181; -are considered.</p><p>&#8226; To reduce the background from K 3&#960; decays occurring upstream of the FV, the track identified as a &#960; + is extrapolated backward to the COL plane, taking into account the TRIM5 magnetic field. The extrapolated position is required to lie outside a rectangle defined by |X| &lt; 40 mm and |Y | &lt; 25 mm.</p><p>&#8226; Further K 3&#960; background suppression is achieved by requiring the momenta of both muon tracks to be below 45 GeV/c.</p><p>&#8226; The invariant mass m(&#960;&#181;&#181;) of the three selected tracks is reconstructed with a 1.1 MeV/c 2 resolution and must be within 8 MeV/c 2 of the nominal K + mass m K <ref type="bibr">[22]</ref>.</p><p>The following criteria are specific to the K 3&#960; event selection.</p><p>&#8226; In order to minimize differences between the signal and normalization selections, only one positive track, chosen at random, is required to be identified as a &#960; + .</p><p>&#8226; The identified &#960; + track extrapolated to the COL plane must satisfy the same requirements as the &#960; + in the K &#960;&#181;&#181; selection.</p><p>&#8226; The invariant mass m(3&#960;) of the three selected tracks is reconstructed with a 0.8 MeV/c 2 resolution and must be within 8 MeV/c 2 of m K .</p><p>For both selections, simulated events are required to be accepted by a set of software algorithms emulating the conditions employed in the online trigger system.</p></div>
<div xmlns="http://www.tei-c.org/ns/1.0"><head n="3">Signal and normalization samples</head><p>The reconstructed mass spectra of the data and simulated events passing the signal and normalization event selections are shown in figure <ref type="figure">2</ref>. The selected K 3&#960; data sample, contaminated by background decays to a negligible level of 10 -6 , is used together with the simulated K 3&#960; events with inner bremsstrahlung included <ref type="bibr">[23]</ref>, to obtain the effective number of kaon decays in the FV where the index i runs over data taking periods defined by constant trigger downscaling factors, N i 3&#960; are the numbers of K 3&#960; events selected with the MT trigger with downscaling factor D i MT , D i 2&#181;MT are the downscaling factors of the 2&#181;MT trigger, and A 3&#960; = (6.58 &#177; 0.16)% and B 3&#960; = (5.583 &#177; 0.024)% are the acceptance (obtained from simulation) and the branching fraction <ref type="bibr">[22]</ref> of the K 3&#960; decay, respectively. The statistical errors in A 3&#960; and N K are negligible, while the systematic uncertainties are dominated by the accuracy of the CHOD detector efficiency in the simulation. The external error on N K stems from the uncertainty on the K 3&#960; branching fraction.</p><p>The m(&#960;&#181;&#181;) signal region contains 27679 data events with a background contamination of about 8 events, estimated from simulation.</p></div>
<div xmlns="http://www.tei-c.org/ns/1.0"><head n="4">Interpretation of the data</head></div>
<div xmlns="http://www.tei-c.org/ns/1.0"><head n="4.1">Decay width and form factor parameterization</head><p>The one-photon-inclusive K &#960;&#181;&#181; differential decay width expressed in terms of the normal-</p><p>where</p><p>is the form factor of the K + &#8594; &#960; + &#181; + &#181; - transition, and g(z) is a function describing the decay kinematics <ref type="bibr">[3]</ref> and including nextto-leading order electromagnetic effects in terms of radiative corrections. While the &#181; + &#181; - interactions are fully taken into account by virtual and bremsstrahlung corrections for the lepton and meson contributions, discussed in <ref type="bibr">[4]</ref> and extended beyond the soft-photon approximation, the semi-classical Coulomb corrections, summarized for example in <ref type="bibr">[25]</ref>, are applied to the &#960; + &#181; + and &#960; + &#181; -pairs. These last corrections have opposite sign and the same average magnitude; their combined effect on the results of the present analysis is found to be negligible. The hard-photon 4-body (K + &#8594; &#960; + &#181; + &#181; -&#947;) part of the phase-space is separated from the soft-photon 3-body (K + &#8594; &#960; + &#181; + &#181; -) part by the condition (P &#960; + P &#947; ) 2 -m 2 &#960; &gt; 100 MeV 2 , where P &#960; and P &#947; are 4-momenta of the &#960; + and &#947;, respectively. The cutoff value is optimized with respect to the experimental resolution. The resulting ratio of the 4-body to 3-body integrated decay widths is (1.64 &#177; 0.02)%, where the uncertainty comes mainly from the accuracy of the theoretical description d&#915; 4-body (z)/dz of the 4-body decay <ref type="bibr">[24]</ref>. In the present analysis, the 4-body decay width, depending non-trivially on the form factor, is approximated by a unique function displayed in figure <ref type="figure">3</ref>-left. Effects of this approximation are treated as systematic uncertainties.</p><p>The Chiral Perturbation Theory parameterization of W (z) at O(p 6 ), introduced in <ref type="bibr">[2]</ref>, is used in the present paper:</p><p>where a + and b + are real parameters, and W &#960;&#960; (z) is a complex function describing the contribution from a two-pion loop. The term W &#960;&#960; (z) depends on additional real parameters &#945; + and &#946; + ; the values &#945; + = (-20.40 &#177; 0.18) &#215; 10 -8 and &#946; + = (-2.05 &#177; 0.06) &#215; 10 -8 <ref type="bibr">[26]</ref> are used.</p></div>
<div xmlns="http://www.tei-c.org/ns/1.0"><head n="4.2">Measurement of the model-independent branching fraction and form factor</head><p>The selected K &#960;&#181;&#181; signal sample with negligible background contamination is distributed in 50 equipopulated bins in z with widths ranging from 0.004 for z &#8776; 0.25 to 0.066 for the last bin. The resolution in z increases linearly from zero to 0.0035 within the allowed kinematic range, and is always several times smaller than the corresponding bin width. The reconstructed differential decay width, shown in figure <ref type="figure">3</ref>-left, is given by d&#915;(z)</p><p>where for each bin i: N &#960;&#181;&#181;,i is the number of K &#960;&#181;&#181; signal candidates, &#8710;z i is the bin width, A &#960;&#181;&#181;,i is the signal selection acceptance of the K &#960;&#181;&#181; decay (obtained from simulation, and equal to zero at both kinematic bounds of z while reaching the maximum of 12.5% around z = 0.2, see also figure <ref type="figure">4</ref>-left), N K is the effective number of kaon decays in the FV collected by the 2&#181;MT trigger (eq. (3.1)), is the reduced Planck constant, and &#964; K = (1.238 &#177; 0.002) &#215; 10 -8 s is the mean charged kaon lifetime <ref type="bibr">[22]</ref>. The model-independent K &#960;&#181;&#181; branching fraction  is obtained from the reconstructed binned differential decay width (eq. ( <ref type="formula">4</ref>.3), figure <ref type="figure">3-left</ref>) by integrating the spectrum over z and multiplying by &#964; K / .</p><p>The K &#960;&#181;&#181; data sample is also used to extract the |W (z)| 2 form factor (figure <ref type="figure">3-right</ref>). The values of the |W (z)| 2 function are reconstructed from the differential decay spectrum (figure <ref type="figure">3</ref>-left) under the assumption that |W (z)| 2 is linear in each bin of z. This assumption defines the horizontal positions of the data points in figure <ref type="figure">3</ref>-right, which are different from the positions in figure <ref type="figure">3</ref>-left.</p><p>The form factor parameters a + and b + best describing the data are determined by a &#967; 2 fit of the data points shown in figure <ref type="figure">3</ref>. Fits of d&#915;(z)/dz and |W (z)| 2 give identical results. The theoretically-preferred <ref type="bibr">[16]</ref> negative solution with both a + and b + negative and &#967; 2 /ndf = 45.1/48 (p-value = 0.59) is a + = -0.575 &#177; 0.012 stat , b + = -0.722 &#177; 0.040 stat , with correlation &#961;(a + , b + ) = -0.972.</p><p>A second &#967; 2 (a + , b + ) minimum is found, corresponding to the positive solution: &#967; 2 /ndf = 56.4/48 (p-value = 0.19), a + = 0.373&#177;0.012 stat , b + = 2.017&#177;0.040 stat , &#961;(a + , b + ) = -0.973. Only the negative solution is considered in the following.</p></div>
<div xmlns="http://www.tei-c.org/ns/1.0"><head n="4.3">Forward-backward asymmetry measurement</head><p>The forward-backward asymmetry A FB of the K &#960;&#181;&#181; decay is defined in terms of the angle &#952; K&#181; between the K + and the &#181; -three-momenta in the &#181; + &#181; -rest frame, as</p><p>where the numbers of events N are obtained after correction for the non-uniform acceptance in the (cos &#952; K&#181; , z) plane (figure <ref type="figure">4</ref>-left). The resulting cos &#952; K&#181; spectrum of the data events and the distribution expected from the Standard Model (SM) are displayed in figure <ref type="figure">4</ref>-right.</p><p>The asymmetry is measured to be</p><p>and shows no significant dependence on z. The statistical precision is at the level of the upper limits on A FB predicted by the Minimal Supersymmetric Standard Model <ref type="bibr">[28]</ref> and by the calculation of the two-photon intermediate state</p></div>
<div xmlns="http://www.tei-c.org/ns/1.0"><head n="5">Systematic and external uncertainties</head><p>The individual contributions to the total uncertainties are discussed in the following and listed in table <ref type="table">1</ref>.</p></div>
<div xmlns="http://www.tei-c.org/ns/1.0"><head n="5.1">Trigger efficiency</head><p>The trigger behaviour is emulated with a set of software algorithms applied to simulated events. The algorithms are tuned and validated on K 3&#960; events. The L0 RICH, L0 CHOD, L0 MUV3 and L1 KTAG trigger efficiencies (equal to 99.8%, 98.2%, 98.9% and 99.8%, respectively) are found to be independent of the decay kinematics. Data and simulation efficiencies agree within 0.3%. The L1 STRAW trigger efficiency is 94.7% and varies as a function of decay kinematics within O(1%). Data and simulation efficiencies agree within 0.5%. The similarity of the MT and 2&#181;MT trigger lines results in substantial cancellation of trigger-related systematic effects. The residual systematic uncertainties are estimated by either disabling the software trigger emulators in simulation (in the case of the L0 RICH and L0 CHOD conditions), or replacing them with simplified emulators (L0 MUV3, L1 KTAG, L1 STRAW).</p><p>-9 -JHEP11(2022)011</p></div>
<div xmlns="http://www.tei-c.org/ns/1.0"><head n="5.2">Reconstruction and particle identification</head><p>The similarity of the signal and normalization selections allows for significant cancellation of most systematic effects coming from reconstruction and particle identification efficiencies.</p><p>Systematic uncertainties arising from differences between event reconstruction efficiencies in data and simulation are dominated by the three-track event reconstruction in the STRAW spectrometer. A dedicated K 3&#960; event selection, relying on a reconstructed kaon track in the GTK and two pion tracks in the STRAW, is used to measure the efficiency of reconstructing the third pion track. The average measured efficiency is 84% and depends on the decay kinematics. The observed differences of up to 2% between the efficiencies in data and simulation are considered in evaluating the systematic effects resulting from the STRAW track reconstruction efficiency.</p><p>The CHOD and MUV3 reconstruction efficiencies are above 99%, with no more than 0.6% difference between data and simulation.</p><p>The differences between data and simulation in the hadronic shower development and energy reconstruction in the LKr are another source of systematic uncertainty. No significant difference is observed in the efficiency of the muon identification. The efficiency of the pion identification measured on data is 99%. The agreement between data and simulation varies with pion momentum within 1%. Residual effects due to different K &#960;&#181;&#181; and K 3&#960; pion kinematics are treated as systematic uncertainties.</p></div>
<div xmlns="http://www.tei-c.org/ns/1.0"><head n="5.3">Beam and accidental activity simulation</head><p>Systematic uncertainties stemming from the quality of the simulation of the beam momentum spectrum and intensity profile, and from the accuracy of the simulation of the halo muons accompanying the beam, are combined into a single systematic uncertainty. The selected normalization sample of K 3&#960; events is used for the beam momentum and intensity studies. The halo muons are selected from out-of-time STRAW tracks that have associated signals in MUV3 and are not compatible with originating from decays in the FV.</p></div>
<div xmlns="http://www.tei-c.org/ns/1.0"><head n="5.4">Background</head><p>The number of background events is estimated using simulation to be 7.8 &#177; 5.6, where the error comes from the limited statistics of simulated background decays. The background arises mainly from the K 3&#960; contribution with two &#960; &#177; &#8594; &#181; &#177; &#957; decays in flight. More details on the methods employed in the K 3&#960; background estimation can be found in <ref type="bibr">[30]</ref>.</p><p>Systematic uncertainties from the background contamination are estimated conservatively as differences between the results obtained with background neglected and background subtracted.</p></div>
<div xmlns="http://www.tei-c.org/ns/1.0"><head n="5.5">External uncertainties</head><p>External uncertainties in the measured quantities originate from the K 3&#960; branching fraction <ref type="bibr">[22]</ref>, from the accuracy of the radiative corrections to the K &#960;&#181;&#181; decay, including the numerical approximation of d&#915; 4-body /dz, and from the pion loop term parameters &#945; + and &#946; + <ref type="bibr">[26]</ref>.</p><p>- </p></div>
<div xmlns="http://www.tei-c.org/ns/1.0"><head n="6">Comparison with earlier measurements</head><p>A comparison of the present results with those from previous measurements by E787, E865, HyperCP and NA48/2 is shown in figure <ref type="figure">5</ref>, table 2, and table <ref type="table">3</ref>. Note that the NA48/2 measurement <ref type="bibr">[11]</ref>, until now the most precise, used a different K 3&#960; branching fraction <ref type="bibr">[31]</ref>, and did not simulate the inner bremsstrahlung radiation of K 3&#960; decays. Implementing these conditions in the NA62 analysis has minor impact on the results, which would change by &#948;a + = -0.001, &#948;b + = -0.002, and &#948;B &#960;&#181;&#181; = +0.03 &#215; 10 -8 .</p><p>Furthermore, the analysis by NA48/2 did not simulate inclusive radiative corrections and the 4-body radiative decay K + &#8594; &#960; + &#181; + &#181; -&#947; in the K &#960;&#181;&#181; sample, but implemented only the soft-photon Coulomb corrections for all pairs of the K &#960;&#181;&#181; decay products. Adopting this approach changes the NA62 results by &#948;a + = -0.006, &#948;b + = +0.034, and &#948;B &#960;&#181;&#181; = -0.06 &#215; 10 -8 , where the 0.7% relative change in the branching fraction comes from the increase of the signal acceptance measured with the 3-body simulated K &#960;&#181;&#181; sample including Coulomb corrections.</p><p>In addition, previous experiments employed values of &#945; + = -20.6 &#215; 10 -8 and &#946; + = -2.8 &#215; 10 -8 , taken from <ref type="bibr">[2]</ref>. Using these values instead of the revised ones (&#945; + = -20.40 &#215; 10 -8 , &#946; + = -2.05 &#215; 10 -8 <ref type="bibr">[26]</ref>), the NA62 results would change<ref type="foot">foot_0</ref> by &#948;a + = -0.011, &#948;b + = +0.026.</p></div>
<div xmlns="http://www.tei-c.org/ns/1.0"><head n="7">Summary</head><p>A sample of 27679 K &#960;&#181;&#181; candidates with negligible background contamination was collected by the NA62 experiment in 2017-2018. The size of the K &#960;&#181;&#181; data sample is the main factor limiting the precision of the present analysis.</p></div><note xmlns="http://www.tei-c.org/ns/1.0" place="foot" n="1" xml:id="foot_0"><p>The measured slopes are &#948;a+/&#948;&#945;+ = +0.004 &#215; 10 8 , &#948;b+/&#948;&#945;+ = -0.029 &#215; 10 8 , &#948;a+/&#948;&#946;+ = +0.013 &#215; 10 8 , and &#948;b+/&#948;&#946;+ = -0.027 &#215; 10 8 .</p></note>
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