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Topological defects creation at fast transition: Kibble mechanism and Zurek scenario

COSLAB and TOPDIF Grenoble connection. Yuriy M. Bunkov. C R T B T – C N R S, Grenoble, France. Topological defects creation at fast transition: Kibble mechanism and Zurek scenario Experiments with neutrons: Vortex creation in 3He+n reaction Dark matter search

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Topological defects creation at fast transition: Kibble mechanism and Zurek scenario

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  1. COSLAB and TOPDIF Grenoble connection Yuriy M. Bunkov C R T B T – C N R S, Grenoble, France • Topological defects creation at fast transition: • Kibble mechanism and Zurek scenario • Experiments with neutrons: • Vortex creation in 3He+n reaction • Dark matter search • Muons and electrons scintillation • A-B transition in 3He • Aurora de Venice versus Baked Alaska • Q-ball in 3He-B • Persistent induction signal

  2. Suprconducters, 4He, A eif E 1/4

  3. 4He experiment: Lancaster University Fast pressure release. P.C.Hendry, N.S Lawson, R.A.M. Lee, P.V.E. McClintock, C.H.D. Williams, Nature, 368, 315 (1994) P Solid Liquid Superfluid Solid P A Superfluid B Liquid + rotation Helsinki Grenoble 1mK T No conformation at better prepared experiments 3He experiments: Lancaster Grenoble and Helsinki fast cooling after a localise heating from 3He neutron nuclear reaction n + 3He = p + 3H + 764 keV T 2K D.I. Bradley, Yu.M.Bunkov, D.J.Cousins, M.P.Enrico,S.N.Fisher, M.R.Follows, A.M.Guénault, W.M.Hayes, G.R.Pickett, T.Sloan, Phys. Rev. Lett., v. 75. p. 1887, (1995) C. Bauerle, Yu.M.Bunkov, S.N.Fisher, H. Godfrin, G.R.Pickett, Nature, 382, 332 (1996) V.M.H. Ruutu, V.B.Eltsov, A.J.Gill, T.W.B. Kibble, M. Krusius, Yu.G. Makhlin, B. Placcais, G.E. Volovik, W. Xu, Nature , 382, 334, (1996)

  4. Yuriy M. Bunkov Henri Godfrin Eddy Collin Matty Krusius Shaun Fisher Derek J. Cousins Cristopher. Bäuerle Ann-Sophie Chen Clemens Winkelmann Johannes Elbs

  5. Superfluid 3He bolometry

  6. n + 3He = p + 3H + 764 keV

  7. scintillation Grenoble 1995

  8. scintillation Grenoble 1995 Theory: V.B. Eltsov, M. Krusius, G.E. Volovik Progress Low Temp Phys 2005

  9. scintillation Grenoble 1995 Grenoble 2004 Theory: V.B. Eltsov, M. Krusius, G.E. Volovik Progress Low Temp Phys 2005

  10. scintillation Grenoble 1995 Grenoble 2004 Grenoble 2005 Theory: V.B. Eltsov, M. Krusius, G.E. Volovik Progress Low Temp Phys 2005

  11. A Bolometric calibration by pulsed heating s1/√T

  12. In 3He + n reaction 9% +- 1% of energy going for scintillation H. Godfrin G. R. Pickett G.M.Seidel

  13. From the fit, the energy emitted into a solid angle of 4p steradians is 87 keV, or 24% of the total energy of the 364 keV electron. In contrast, for an alpha particle stopped in helium we found, upon correcting for reflectivity, that only 10% of the initial energy of the particle is emitted as uv radiation. Journal of Low Temperature Physics, Vol. 113,5/6, 1998

  14. scintillation Grenoble 1995 Grenoble 2004 Grenoble 2005 Theory: V.B. Eltsov, M. Krusius, G.E. Volovik Progress Low Temp Phys 2005

  15. • Detection of cosmic muons: good agreement experience/simulation if fUV(muons) ≈ 25 % Analysis and simulation LPSC (GEANT4)

  16. 266 10 keV coincidence 264 W(t) (mHz) 262 260 0 100 200 300 Wmes(Hz) temps (s) time (s) Time (s)

  17. Electron detection spectrum Analysis LPSC, d5, B=100 mT, W0=430 mHz S/B>5 cell A (without source) cell B (with source) • • resolution of low energy emission spectrum of 57Co • • Comparison to 14 keV peak with bolometric calibration • Energy deficit of fUV(e-,14keV)≈265% • UV Scintillation

  18. Ultra Low Temperature Instrumentation for Measurements in Astrophysics The idea : Use the Bose –Einstein condensed coherent quantum state of superfluid 3He at a limit of extremely low temperatures as a sensitive medium for the direct bolometric search of non-baryonic Dark Matter First suggestion G.R.Pickett in Proc. «Second european worshop on neutrinos and dark matters detectors», ed by L.Gonzales-Mestres and D.Perret-Gallix, Frontiers, 1988, p. 377. Yu.Bunkov, S.Fisher, H.Godfrin, A.Guenault, G.Pickett. in Proc. « International Workshop Superconductivity and Particles Detection (Toledo, 1994)», ed. by T.Girard, A.Morales and G.Waysand. World Scientific,p. 21-26.

  19. Bose – Einstein condensed coherent quantum state with rear gas of collective excitations. At about 100 mK at 0.1 cm3 remains only 10 keV from the level of absolute zero of temperature. Temperature is the density of quasiparticles, that measured directly by damping of mikro vibrating wire. The deposited energy is intimately associated with the 3He nuclear. There is no isolated nuclear thermal bath, separated from electronic and phononic subsystems!

  20. CandidatesWhat is the dark matter made of ? The non-baryonic candidate zoo Gianfranco Bertonea, Dan Hooperb, Joseph Silkb, Physics Reports 405 (2005) 279–390 Standard Model neutrinos < 0.07 Sterile neutrinos (without Standard Model weak interactions) Axions Introduced in an attempt to solve the problem of CP violation in particle physics Supersymmetric candidates Neutralinos WIMP Sneutrinos (superpartners of the Standard Model neutrinos in supersymmetric models) Gravitinos (superpartners of the graviton in supersymmetric models.) Axinos (superpartner of the axion,) Light scalar dark matter (fermionic dark matter candidates) Dark matter from little Higgs models Kaluza–Klein excitations of Standard Model fields which appear in models of universal extra dimensions Superheavy dark matter called Wimpzillas, Q-balls, mirror particles, CHArged Massive Particles (CHAMPs), self interacting dark matter, D-matter, cryptons, superweakly interacting dark matter, brane world dark matter, heavy fourth generation neutrinos, etc.

  21. Spin dependent interaction 100g 3He detector For spin dependent interaction 100g 3He = 30 kg Ge

  22. scintillation Grenoble 1995 Grenoble 2004 Grenoble 2005 Theory: V.B. Eltsov, M. Krusius, G.E. Volovik Progress Low Temp Phys 2005

  23. Solid P A Superfluid B Liquid Helsinki + rotation Grenoble 1mK T Meyer, Sloan, JLTP 1998 3H- 1 mm p 10 mm 70 mm D(0bar) = 21 cm2/s; R=27mm D(19bar) = 0.94 cm2/s; R=12mm

  24. Suprconducters, 4He, A eif ik E Aik eif 3He, Universe Aik Bunkov and Timofeevskaya modification of Kibble-Zurek theory PRL 1998 Transition triggered by radiation (Osheroff) “Baked Alaska” due to Leggett does not work Volovik suggestion, LT, Praga, 1996 3He-A Inflation of B phase in the space of A phase

  25. A – B transition Solid P A Superfluid B Liquid T 18 D manifold B

  26. A – B transition Solid P A Superfluid B Liquid T

  27. The end

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