Impact of nuclear spallation process to the Big-Bang nucleosynthesis induced by long lived charged particle Kenichi Sugai (Saitama University) Collaborators.

Slides:



Advertisements
Similar presentations
1 The and -Z Exchange Corrections to Parity Violating Elastic Scattering 周海清 / 东南大学物理系 based on PRL99,262001(2007) in collaboration with C.W.Kao, S.N.Yang.
Advertisements

Phi-Psi, Feb.-Mar., 2006, S.Uehara1 Experimental studies of charmonia in two-photon collisions at Belle S.Uehara (KEK) for the Belle Collaboration e +
Anomalous Pion Production in High Energy Particle Collisions Alexander Bylinkin, Andrey Rostovtsev XV Moscow School of Physics XXXX ITEP Winter School.
Joe Sato (Saitama University ) Collaborators Satoru Kaneko,Takashi Shimomura, Masato Yamanaka,Oscar Vives Physical review D 78, (2008) arXiv:1002.????
Neutrino-induced meson production model for neutrino oscillation experiments Satoshi Nakamura Nuclear Theory Group.
Masato Yamanaka (ICRR, University of Tokyo) Collaborators Junji Hisano, Kazunori Nakayama Shohei Sugiyama, Tomohiro Takesako.
Constraints on the very early universe from thermal WIMP Dark Matter Mitsuru Kakizaki (Bonn Univ.) Mitsuru Kakizaki (Bonn Univ.) July 27, Karlsruhe.
Significant effects of second KK particles on LKP dark matter physics
Significant effects of second KK particles on LKP dark matter physics Mitsuru Kakizaki (Bonn Univ. & ICRR, Univ. of Tokyo) Mitsuru Kakizaki (Bonn Univ.
Sombrero Galaxy (M104, 46 M light years). Long-lived charged massive particle and its effect on cosmology Physics Department, Lancaster University Physics.
Enhancement of Line Gamma Ray Signature from Bino-like Dark Matter Annihilation due to CP Violation Yoshio Sato (Saitama University/Technical University.
Large enhancement of KK dark matter annihilation rate due to threshold singularity Mitsuru Kakizaki (ICRR, University of Tokyo) Dec. Stanford Univ.

Physics 133: Extragalactic Astronomy and Cosmology Lecture 15; March
Isospin Charge independence Accordingly, one can develop a formalism that encompasses this concept. Strong empirical empirical evidence to imply that:
Oct.18, Neutron Field and Induced Radioactivity in IFMIF Environment M. Sugimoto(JAERI) IEA International Work Shop on Fusion Neutronics The Kongreshous.
Significant enhancement of Bino-like dark matter annihilation cross section due to CP violation Yoshio Sato (Saitama University) Collaborated with Shigeki.
Charge-Changing Neutrino Scattering from the Deuteron J. W. Van Orden ODU/Jlab Collaborators: T. W. Donnelly and Oscar Morino MIT W. P. Ford University.
Cold nuclear matter effects on dilepton and photon production Zhong-Bo Kang Los Alamos National Laboratory Thermal Radiation Workshop RBRC, Brookhaven.
Quintessino model and neutralino annihilation to diffuse gamma rays X.J. Bi (IHEP)
1 Primordial nucleosynthesis and New Physics Maxim Pospelov University of Victoria and Perimeter Institute K. Jedamzik and M. Pospelov, arXiv:
A NLO Analysis on Fragility of Dihadron Tomography in High Energy AA Collisions I.Introduction II.Numerical analysis on single hadron and dihadron production.
1 Formation spectra of  -mesic nuclei by (  +,p) reaction at J-PARC and chiral symmetry for baryons Hideko Nagahiro (RCNP) Collaborators : Daisuke Jido.
Masato Yamanaka (Saitama University) collaborators Shigeki Matsumoto Joe Sato Masato Senami arXiv: [hep-ph]Phys.Lett.B647: and Relic abundance.
Masato Yamanaka (Tokyo university, ICRR) Collaborators Shigeki Matsumoto Joe Sato Masato Senami PHYSICAL REVIEW D 80, (2009)
Hypernuclear Production with Hadronic and Electromagnetic Probes Radhey Shyam Saha Institute of Nuclear Physics, Kolkata, India Z.Zt. Institut f. Theo.
1 Identified Particle Dependence of Nuclear Modification Factors in d+Au Collisions at RHIC. Lee Barnby - University of Birmingham For the STAR Collaboration.
Right-handed sneutrino as cold dark matter of the universe Takehiko Asaka (EPFL  Niigata University) Refs: with Ishiwata and Moroi Phys.Rev.D73:061301,2006.
Low-scale Gaugino Mediation in Warped Spacetime Toshifumi Yamada Sokendai, KEK in collaboration with Nobuchika Okada (Univ. of Alabama ) arXiv: May 11,
Flavor induced EDMs with tanbeta enhanced corrections Minoru Nagai (ICRR, Univ. of Tokyo) Aug. 4, 2007 Summer Institute 2007 In collaborated with: J.Hisano.
Interactions of Hadrons and Hadronic Showers
Weak decay of  in nuclear medium FCPPL-2015, USTC, April 8-12, 2015 Institute of High Energy Physics Qiang Zhao Institute of High Energy Physics, CAS.
Significant effects of second KK particles on LKP dark matter physics Collaborated with Mitsuru Kakizaki (ICRR) Mitsuru Kakizaki (ICRR) Shigeki Matsumoto.
Neutrino-Nucleus Reactions at Medium and Low Energies [contents] 1. Neutrino and weak interaction 2. Cross section for ν-A and e-A reactions 3. EMC effect.
K. Tőkési 1 Institute for Nuclear Research, Hungarian Academy of Sciences (ATOMKI), Debrecen, Hungary, EU ATOMIC DATA FOR INTEGRATED TOKAMAC MODELLING.
Photoproduction of Pentaquarks Seung-il Nam *1,2 Atsushi Hosaka 1 Hyun-Chul Kim 2 1.Research Center for Nuclear Physics (RCNP), Osaka University, Japan.
1 Diffractive heavy quark production in AA collisions at the LHC at NLO* Mairon Melo Machado GFPAE – IF – UFRGS
Masato Yamanaka (ICRR, Univ. of Tokyo) Collaborators Masafumi Koike (Saitama Univ.) Yoshitaka Kuno (Osaka Univ.) Joe Sato (Saitama Univ. )  e ee.
Transport properties of nuclear matter within Brueckner-Hartree-Fock Hongfei Zhang ( 张鸿飞) Lanzhou University Aug. 3, 2015 PKU-CUSTIPEN Workshop on " Advances.
1 11/20/13 21/11/2015 Jinniu Hu School of Physics, Nankai University Workshop on “Chiral forces and ab initio calculations” Nov. 20- Nov. 22,
BNL Minjung Kim for the PHENIX Collaboration (SNU/RIKEN) RBRC Workshop: Emerging Spin and Transverse Momentum Effects in p+p and p+A Collisions.
The First Transverse Single Spin Measurement in High Energy Polarized Proton-Nucleus Collision at the PHENIX experiment at RHIC RIKEN/RBRC Itaru Nakagawa.
Collider Signals of Extra Dimension Scenarios
Phys. Lett. B646 (2007) 34, (hep-ph/ ) Non-perturbative effect on thermal relic abundance of dark matter Masato Senami (University of Tokyo, ICRR)
The pp→pp  0  0 reaction and its limiting case, the fusion to quasibound, in search of ABC effect T. Skorodko, University Tuebingen for CELSIUS-WASA.
Observation of Σ + trapping in Gamov states
d(α,ɣ)6Li reaction and second lithium puzzle
Mean free path and transport parameters from Brueckner-Hartree-Fock
Jun Kameda (ICRR) RCCN International workshop at Kashiwa (Dec.10,2004)
A Solution to the Li Problem by the Long Lived Stau
Structure and dynamics from the time-dependent Hartree-Fock model
Yasser Maghrbi Graduiertenkolleg, Todtmoos 2007
Minoru Nagai (ICRR, Univ. of Tokyo)
Guangxi Normal University
Masanori HIRAI 2006, Nov 9, Tokyo-u
Shota Ohnishi (Tokyo Inst. Tech. / RIKEN)
(飛行 K-, n) 反応による K-pp 生成スペクトルと K--核間有効ポテンシャルのエネルギー依存性
MEee SATO, Joe (Saitama University) MPI Heidelberg 2016/Sep/11
Electric Dipole Moments in PseudoDirac Gauginos
Theoretical study of the direct
Breakup of weakly bound nuclei and its influence on fusion
Neutrino-Nucleus Reactions and Nucleosynthesis
Possible solution to the 7Li problem by the long lived stau
Signature of L(1405) in K-dpSn reaction
Big-Bang Nucleosynthesis with Negatively-Charged Massive Particles as a Cosmological Solution to the 6Li and 7Li Problems Motohiko Kusakabe1,2,†, Toshitaka.
Cronin Effect of  K p from d+Au Collisions at 200 GeV
Kazuo MUTO Tokyo Institute of Technology
Sombrero Galaxy (M104, 46 M light years)
(Tokyo university, ICRR)
Probing correlations by use of two-nucleon removal
Presentation transcript:

Impact of nuclear spallation process to the Big-Bang nucleosynthesis induced by long lived charged particle Kenichi Sugai (Saitama University) Collaborators Masafumi Koike, Joe Sato,Toshifumi Jittoh (Saitama University) Kazunori Kohri (Tohoku University) Koichi Yazaki (YITP, RIKEN) Masato Yamanaka (ICRR University of Tokyo) Saturday, February, 20,2010;KEK

Contents Introduction Nuclear spallation process of 4 He Summary

Introduction

The Premordial Lithium Problem

New Destruction process of the Lithium 7 Be ( 7 Li) 7 Li ( 7 He) Bound State Model MSSM LSP: Neutralino,NLSP: Stau Long-lived stau due to quasi- degenerate stau-neutralino Internal Conversion Jittoh et al., PRD (2007, 2008)

New Destruction process of the Lithium Over production of 6 Li Model MSSM LSP: Neutralino,NLSP: Stau Long-lived stau due to quasi- degenerate stau-neutralino Internal Conversion Jittoh et al., PRD (2007, 2008) Excessive 6 Li: Catalyzed Fusion Presence of staus enhances the cross section by 10 8 (Pospelov, PRL (2007))

Competing against the Catalyzed Fusion Overproduction of 6 Li due to catalyzed fusion Overproduction of 6 Li Competing process: Nuclear spallation etc. Over production of 6 Li

Competing against the Catalyzed Fusion Competing process: Nuclear spallation etc. Overproduction of 6 Li due to catalyzed fusion Recovery ?

Nuclear Spallation Proceeds Rapidly Catalyzed fusion K.Hamaguchi et al.,PLB650, 268 (2007) at T = 50 keV n( 4 He-stau) > n( 6 Li) at T~(50-100) keV

Nuclear Spallation Proceeds Rapidly Internal conversion, as a reference to the spallation T.Jittoh et al.,Phys.Rev.D78, (2007) Time Scale of Internal Conversion 7 Be ( 7 Li) 7 Li ( 7 He) Bound State << Spallation would outnumber Catalyzed Fusion Stau can’t survive until the BBN era

Motivation Nuclear spallation will dominate catalyzed fusion!! We investigate the spallation processes Applying the result for the BBN with long- lived stau, we show the allowed region for MSSM

Nuclear spallation process of 4 He

Spallation of the 4 He

How to calculate spallation process Forming wave function of nuclear ・ spin and isospin component → antisymmetric for exchange of inner particles ・ space component → symmetric for exchange of inner particles Calculating the amplitude Integrating the square amplitude over all final state’s momentum As a whole, completely antisymmetric for exchange of inner particles

Wave Function of the 4 He Spin and Isospin Component Space Component

Calculation of the Amplitude and the Cross Section Inner Products

Calculation of the Amplitude and the Cross Section Calculation of the Amplitude Calculation of the Cross Section

Time Scale of 4 He Spallation due to Bound Stau ~30MeV Nuclear Spallation dominates Catalyzed Fusion Order of Time Scale of Catalyzed Fusion m stau = 350 GeV Lifetime[s] Deltam[MeV]

Recovery of the Allowed Region Overproduction of 6 Li

Recovery of the Allowed Region Allowed region recovers!! (expectaition) Overproduction of 6 Li

Summary

Spallation process of 4 He suppresses over production of 6 Li caused by the catalyzed fusion. Prediction to the MSSM parameters Calculation applies to X - particles. Calculation of spallation process of 4 He into a deuterium and two neutrons Calculation of spallation process of 7 Li and 7 Be Future works

Thank you for your attention!

Calculation of the Amplitude and the Cross Section Non-relativistic Approximation The Square Amplitude

Calculation of the Amplitude and the Cross Section Calculation of the Cross Section Calculation of the Rate and the Lifetime RateLifetime

Time Scale of 4 He Spallation due to Bound Stau ~30MeV Nuclear Spallation dominates Catalyzed Fusion Order of Time Scale of Catalyzed Fusion m stau = 350 GeV

Calculation of the Amplitude and the Cross Section The Amplitude Calculation