Neutron scattering and extra interactions Guillaume Pignol Valery


















- Slides: 18
Neutron scattering and extra interactions. Guillaume Pignol Valery Nesvizhevsky Konstantin Protasov Rencontres des particules 2008 LAPTH Guillaume Pignol (LPSC) Neutrons and extra interactions 23/01/2008 1
The institute Laue-Langevin in Grenoble Mountain European Synchrotron The ILL : § Nuclear core 53 MW § The most intense neutron source in the world Guillaume Pignol (LPSC) Neutrons and extra interactions 23/01/2008 2
Optical and Ultra Cold Neutrons (UCN) Optical neutrons § wavelength >2 Å § interaction with bulk matter described by a mean potential (Fermi potential) ~ 100 ne. V 0. 025 e. V 100 ne. V production n Thermal neutrons Ultra Cold Neutrons Guillaume Pignol (LPSC) Optical neutrons 10 Me. V matter Ultra Cold Neutrons § energy < Fermi potential § total reflection at surfaces Can be stored in bottles E velocity < 7 m/s Neutrons and extra interactions 23/01/2008 3
Slow neutrons and fundamental interactions Free neutrons feel all interactions very weakely § Weak interaction β decay: 886 s § Strong interaction Fermi potentials ~100 ne. V § Electromagnetism No electric charge B = 1 T induce Zeeman split of ~100 ne. V § Gravity 1 m fall: neutron increases its energy by ~100 ne. V Neutrons can be very sensitive to new interactions! Guillaume Pignol (LPSC) Neutrons and extra interactions 23/01/2008 4
Extra short range interaction We assume a new interaction between neutron and nucleus with A nucleons Mediated by a new light boson of mass M High Energy Physics Guillaume Pignol (LPSC) Neutrons and extra interactions Modification of gravity 23/01/2008 5
Extra short range interaction If a new boson gets its mass by a «Higgs mechanism» at the Electroweak scale: If the new boson travels in large flat extra dimensions (ADD) the coupling is suppressed. High Energy Physics Guillaume Pignol (LPSC) Neutrons and extra interactions Modification of gravity 23/01/2008 6
Slow neutron scattering with extra interaction Slow neutron Atom E < 1 e. V Coherent scattering length (Fermi) § Isotropic § Energy independant § Scales as ~ A 1/3 Guillaume Pignol (LPSC) § Not isotropic § Energy dependant § Scales as ~ A Neutrons and extra interactions 23/01/2008 7
1 Simple nuclear model We aim to exclude a contribution ~A in the set of measured scattering lengths Random potential model Peskhin, Ringo, Am. J. Phys. 39 (1971) § Square well potential for nuclear interaction § Radius R x A 1/3 § Random depth. Guillaume Pignol (LPSC) Neutrons and extra interactions 23/01/2008 8
1 Simple nuclear model + extra interaction We repeated the analysis with an extra force included Random potential model Guillaume Pignol (LPSC) Additional parameter Neutrons and extra interactions 23/01/2008 9
2 Comparing forward and backward scattering Slow neutron Atom Interference measurement Bragg diffraction measurement § Measurements using interference method sensitive to the forward scattering amplitude one actually measures § Measurements using Bragg-diffraction method sensitive to q = 10 nm-1 scattering amplitude one actually measures The two methods for measuring the scattering lengths do not bear the same sensitivity to extra force Guillaume Pignol (LPSC) Neutrons and extra interactions 23/01/2008 10
2 Comparing forward and backward scattering No difference is observed for the nuclei for which both measures exist Guillaume Pignol (LPSC) Neutrons and extra interactions 23/01/2008 11
3 Comparing forward scattering and total X-section Slow neutron Atom § Measurements using optical method sensitive to the forward scattering amplitude one actually measures § Measurements using transmission method sensitive to the total cross-section at 1 e. V one actually measures This idea first appeared in Leeb and Schmiedmayer, PRL 68 (1992) Guillaume Pignol (LPSC) Neutrons and extra interactions 23/01/2008 12
3 Comparing forward scattering and total X-section Very precise measurements exist for both methods, on lead and bismuth nuclei. No deviation is observed There is a hidden difficulty: for scattering at 1 e. V, electromagnetic effects have to be taken into account. Guillaume Pignol (LPSC) Neutrons and extra interactions 23/01/2008 13
Measuring asymmetry of scattering Diluted noble gaz Possible dedicated experiment § Forward/Backward asymmetry of scattering at noble gaz as a probe of new interactions § Can detect asymmetry of 10 -3 Must take into account Doppler thermal effect § Guillaume Pignol (LPSC) Neutrons and extra interactions 23/01/2008 14
Conclusions § Neutron constraints on extra interactions are several orders of magnitude better than those usually cited in the range 1 pm 5 nm. § We provided several independant strategies: neutron constraints are reliable. § Dedicated experiment (asymmetry of scattering) can easily improve the constraints by one order of magnitude. For the detailed analysis, see hep-ph/0711. 2298 (accepted in Phys Rev D) Guillaume Pignol (LPSC) Neutrons and extra interactions 23/01/2008 15
Quantum reflection of UCN Measured reflectivity agrees with Q. M. simplest calculation (Koester 1986 as an example) Ultra Cold Neutrons § velocity < 7 m/s § wavelength > 50 nm § Elastic reflection 99. 99 % § 10 -4 inelastic reflection at phonons § 10 -5 inelastic reflection at surface nanoparticles § 10 -5 absorption Guillaume Pignol (LPSC) Neutrons and extra interactions 23/01/2008 16
Sensitivity to extra short range interactions neu tron MIRROR New light boson of mass M New interaction between the neutron and the mirror with range monopole-monopole coupling spin-independant Modification of the spectrum Guillaume Pignol (LPSC) Neutrons and extra interactions 23/01/2008 17
Spin dependant extra short range interactions neu tron MIRROR New light boson of mass M New interaction between the neutron and the mirror with range monopole-dipole coupling Spin-dependent Different spectrum for spin up and spin down neutrons Guillaume Pignol (LPSC) Neutrons and extra interactions 23/01/2008 18


















