BEGIN:VCALENDAR VERSION:2.0 PRODID:-//CERN//INDICO//EN BEGIN:VEVENT SUMMARY:Late-time magnetogenesis DTSTART;VALUE=DATE-TIME:20180213T003000Z DTEND;VALUE=DATE-TIME:20180213T010000Z DTSTAMP;VALUE=DATE-TIME:20210810T020749Z UID:indico-contribution-303-3@conference-indico.kek.jp DESCRIPTION:Speakers: Choi\, Kiwoon (CTPU\, IBS)\nI discuss a late-time ma gnetogenesis scenario\, which takes place after the epoch of electron/posi tron annihilation. It involves an ultralight axion-like particle\, constit uting the dark matter of the Universe\, and a dark U(1) gauge boson introd uced to bypass the obstacle from the relatively high conductivity of the c osmic plasma.\n\nhttps://conference-indico.kek.jp/event/38/contributions/8 29/ LOCATION:KEK Building 3 1F\, Seminar Hall URL:https://conference-indico.kek.jp/event/38/contributions/829/ END:VEVENT BEGIN:VEVENT SUMMARY:Lovely phase space DTSTART;VALUE=DATE-TIME:20180213T010000Z DTEND;VALUE=DATE-TIME:20180213T013000Z DTSTAMP;VALUE=DATE-TIME:20210810T020749Z UID:indico-contribution-303-4@conference-indico.kek.jp DESCRIPTION:Speakers: Melia\, Tom (Kavli IPMU)\nI’ll describe a paramete risation of phase space where the physical (on-shell & momentum conserving ) manifold\, upon which observables have support\, is identified with a co set space for the breaking of a particle number symmetry. I’ll talk abou t its applications to monte carlo simulation and partial wave analyses.\n\ nhttps://conference-indico.kek.jp/event/38/contributions/832/ LOCATION:KEK Building 3 1F\, Seminar Hall URL:https://conference-indico.kek.jp/event/38/contributions/832/ END:VEVENT BEGIN:VEVENT SUMMARY:Axion coupled to hidden sector DTSTART;VALUE=DATE-TIME:20180213T020000Z DTEND;VALUE=DATE-TIME:20180213T023000Z DTSTAMP;VALUE=DATE-TIME:20210810T020749Z UID:indico-contribution-304-5@conference-indico.kek.jp DESCRIPTION:Speakers: Takahashi\, Fuminobu (Tohoku University)\nThe QCD ax ion may be coupled to a hidden sector. As an example\, I will discuss two scenarios in which the QCD axion is coupled to a hidden photon. In the fir st case\, the axion is coupled to massless hidden photons\, and such a cou pling is known to induce tachyonic instabilities if the coupling is suffic iently strong. I will explain how the tachyonic preheating affects the fin al axion abundance based on the lattice simulations. In the second case\, the axion is coupled to hidden photons in the presence of hidden monopoles . In this case the axion acquires an extra mass due to the Witten effect\, which suppresses the final axion abundance.\n\nhttps://conference-indico. kek.jp/event/38/contributions/831/ LOCATION:KEK Building 3 1F\, Seminar Hall URL:https://conference-indico.kek.jp/event/38/contributions/831/ END:VEVENT BEGIN:VEVENT SUMMARY:Multi-Messenger Astrophysics in the Gravitational Wave Era DTSTART;VALUE=DATE-TIME:20180213T023000Z DTEND;VALUE=DATE-TIME:20180213T030000Z DTSTAMP;VALUE=DATE-TIME:20210810T020749Z UID:indico-contribution-304-6@conference-indico.kek.jp DESCRIPTION:Speakers: Ioka\, Kunihito (YITP\, Kyoto University)\nhttps://c onference-indico.kek.jp/event/38/contributions/834/ LOCATION:KEK Building 3 1F\, Seminar Hall URL:https://conference-indico.kek.jp/event/38/contributions/834/ END:VEVENT BEGIN:VEVENT SUMMARY:Recent PandaX-II Results on Dark Matter Search and PandaX-4T Upgra de Plan DTSTART;VALUE=DATE-TIME:20180214T010000Z DTEND;VALUE=DATE-TIME:20180214T013000Z DTSTAMP;VALUE=DATE-TIME:20210810T020749Z UID:indico-contribution-307-18@conference-indico.kek.jp DESCRIPTION:Speakers: Zhou\, Ning (Shanghai Jiao Tong University)\nPandaX experiment\, located at China JinPing underground Laboratory (CJPL)\, is a 500kg scale liquid xenon dark matter direct detection experiment. With th e first 98.7-day data\, PandaX-II experiment obtained stringent upper limi ts on the spin-independent (SI) and spin-dependent (SD) WIMP-nucleon elast ic scattering cross sections. Alternative models of dark matter are also e xplored using this data. Meanwhile\, PandaX collaboration has launched an upgrade plan to build PandaX-4T detector with 4-ton liquid xenon in the ac tive volume. The PandaX-4T experiment will be relocated to CJPL-II and is expected to run after 2020. Detailed simulation indicates that the sensiti vity on SI WIMP-nucleon scattering cross section could reach 10^{-47} cm^2 after two-year's running\n\nhttps://conference-indico.kek.jp/event/38/con tributions/837/ LOCATION:KEK Building 3 1F\, Seminar Hall URL:https://conference-indico.kek.jp/event/38/contributions/837/ END:VEVENT BEGIN:VEVENT SUMMARY:Addressing theoretical uncertainties in direct dark matter searche s DTSTART;VALUE=DATE-TIME:20180214T003000Z DTEND;VALUE=DATE-TIME:20180214T010000Z DTSTAMP;VALUE=DATE-TIME:20210810T020749Z UID:indico-contribution-307-17@conference-indico.kek.jp DESCRIPTION:Speakers: Alejandro\, Ibarra (Technical University of Munich)\ nThe interpretation of any experiment probing the dark matter distribution inside the Solar System is subject to our ignorance of the local dark mat ter density and velocity distribution\, as well as our ignorance of the na ture and strength of the dark matter-nucleon interaction. In this talk we present new ideas to interpret the outcome of direct detection experiments without making assumptions of the velocity distribution\, and to confront a positive signal to a null search experiment in a halo-independent and m odel-independent manner.\n\nhttps://conference-indico.kek.jp/event/38/cont ributions/848/ LOCATION:KEK Building 3 1F\, Seminar Hall URL:https://conference-indico.kek.jp/event/38/contributions/848/ END:VEVENT BEGIN:VEVENT SUMMARY:Colored Dark Matter DTSTART;VALUE=DATE-TIME:20180214T000000Z DTEND;VALUE=DATE-TIME:20180214T003000Z DTSTAMP;VALUE=DATE-TIME:20210810T020749Z UID:indico-contribution-307-16@conference-indico.kek.jp DESCRIPTION:Speakers: Strumia\, Alessandro (Pisa U &\; INFN &\; CERN )\nWe explore the possibility that Dark Matter is the lightest hadron made of two stable color octet Dirac fermions $\\Q$. The cosmological DM abund ance is reproduced for $M_\\Q\\approx 9.5 \\TeV$\, compatibly with direct searches (the Rayleigh cross section\, suppressed by $1/M_\\Q^6$\, is clos e to present bounds)\, indirect searches (enhanced by $\\Q\\Q+\\bar\\Q\\b ar\\Q\\to \\Q\\bar\\Q+\\Q\\bar\\Q$ recombination)\, and with collider sear ches (where $\\Q$ manifests as tracks\, pair produced via QCD). Hybrid had rons\, made of $\\Q$ and of SM quarks and gluons\, have large QCD cross se ctions\, and do not reach underground detectors. Their cosmological abunda nce is $10^5$ times smaller than DM\, such that their unusual signals seem compatible with bounds. Those in the Earth and stars sank to their center s\; the Earth crust and meteorites later accumulate a secondary abundance\ , although their present abundance depends on nuclear and geological prope rties that we cannot compute from first principles.\n\nhttps://conference- indico.kek.jp/event/38/contributions/849/ LOCATION:KEK Building 3 1F\, Seminar Hall URL:https://conference-indico.kek.jp/event/38/contributions/849/ END:VEVENT BEGIN:VEVENT SUMMARY:Analytic Boosted Boson Discrimination at the LHC DTSTART;VALUE=DATE-TIME:20180214T023000Z DTEND;VALUE=DATE-TIME:20180214T030000Z DTSTAMP;VALUE=DATE-TIME:20210810T020749Z UID:indico-contribution-308-20@conference-indico.kek.jp DESCRIPTION:Speakers: Moult\, Ian (Berkeley)\nIn this talk I will discuss recent progress in the area of jet substructure at the LHC\, focusing in p articular on analytic calculations of jet substructure observables of curr ent interest.\n\nhttps://conference-indico.kek.jp/event/38/contributions/8 15/ LOCATION:KEK Building 3 1F\, Seminar Hall URL:https://conference-indico.kek.jp/event/38/contributions/815/ END:VEVENT BEGIN:VEVENT SUMMARY:Higgs precision: a window to new physics DTSTART;VALUE=DATE-TIME:20180214T020000Z DTEND;VALUE=DATE-TIME:20180214T023000Z DTSTAMP;VALUE=DATE-TIME:20210810T020749Z UID:indico-contribution-308-19@conference-indico.kek.jp DESCRIPTION:Speakers: Mawatari\, Kentarou ()\nhttps://conference-indico.ke k.jp/event/38/contributions/850/ LOCATION:KEK Building 3 1F\, Seminar Hall URL:https://conference-indico.kek.jp/event/38/contributions/850/ END:VEVENT BEGIN:VEVENT SUMMARY:Latest SM results with the ATLAS detector (including SM-Higgs) DTSTART;VALUE=DATE-TIME:20180214T052000Z DTEND;VALUE=DATE-TIME:20180214T055500Z DTSTAMP;VALUE=DATE-TIME:20210810T020749Z UID:indico-contribution-309-1@conference-indico.kek.jp DESCRIPTION:Speakers: Sforza\, Federico (Tufts University)\nThe precise me asurement of SM observables is a key element of the LHC programme\, both a s a probe of the fundamental properties of Nature and as a tool to improve future experimental and theoretical studies. This talk reviews the recent highlights in the measurement of SM processes\, including the SM-Higgs pr operties\, performed thanks to the ATLAS experiment.\n\nhttps://conference -indico.kek.jp/event/38/contributions/827/ LOCATION:KEK Building 3 1F\, Seminar Hall URL:https://conference-indico.kek.jp/event/38/contributions/827/ END:VEVENT BEGIN:VEVENT SUMMARY:SM\, Higgs\, and BSM Physics at CMS DTSTART;VALUE=DATE-TIME:20180214T043000Z DTEND;VALUE=DATE-TIME:20180214T052000Z DTSTAMP;VALUE=DATE-TIME:20210810T020749Z UID:indico-contribution-309-0@conference-indico.kek.jp DESCRIPTION:Speakers: Neu\, Christopher (University of Virginia)\nhttps:// conference-indico.kek.jp/event/38/contributions/828/ LOCATION:KEK Building 3 1F\, Seminar Hall URL:https://conference-indico.kek.jp/event/38/contributions/828/ END:VEVENT BEGIN:VEVENT SUMMARY:Latest BSM results with the ATLAS detector DTSTART;VALUE=DATE-TIME:20180214T055500Z DTEND;VALUE=DATE-TIME:20180214T063000Z DTSTAMP;VALUE=DATE-TIME:20210810T020749Z UID:indico-contribution-309-2@conference-indico.kek.jp DESCRIPTION:Speakers: Sanchez Pineda\, Arturo (Universita di Udine\, ICTP and CERN)\nhttps://conference-indico.kek.jp/event/38/contributions/830/ LOCATION:KEK Building 3 1F\, Seminar Hall URL:https://conference-indico.kek.jp/event/38/contributions/830/ END:VEVENT BEGIN:VEVENT SUMMARY:Distinguishing axions from WIMPs as CDM DTSTART;VALUE=DATE-TIME:20180215T003000Z DTEND;VALUE=DATE-TIME:20180215T010000Z DTSTAMP;VALUE=DATE-TIME:20210810T020749Z UID:indico-contribution-312-34@conference-indico.kek.jp DESCRIPTION:Speakers: Davidson\, Sacha (IN2P3/CNRS)\nhttps://conference-in dico.kek.jp/event/38/contributions/809/ LOCATION:KEK Building 3 1F\, Seminar Hall URL:https://conference-indico.kek.jp/event/38/contributions/809/ END:VEVENT BEGIN:VEVENT SUMMARY:Hidden sector behind the quark mixing DTSTART;VALUE=DATE-TIME:20180215T010000Z DTEND;VALUE=DATE-TIME:20180215T013000Z DTSTAMP;VALUE=DATE-TIME:20210810T020749Z UID:indico-contribution-312-35@conference-indico.kek.jp DESCRIPTION:Speakers: Omura\, Yuji (KMI\, Nagoya Univ.)\nThe small quark m ixing\, described by the Cabibbo-Kobayashi-Maskawa (CKM) matrix in the Sta ndard Model\, may be a clue to reveal new physics around the TeV scale. We consider a simple scenario that extra particles in a hidden sector radiat ively mediate the flavor violation to the quark sector around the TeV scal e and effectively realize the observed CKM matrix. The lightest particle i n the hidden sector\, whose contribution to the CKM matrix is expected to be dominant\, is a good dark matter (DM) candidate\, so we focus on the co ntribution\, and discuss the DM physics. In this scenario\, there is an ex plicit relation between the CKM matrix and flavor violating couplings\, su ch as four-quark couplings\, because both are radiatively induced by the p articles in the hidden sector. Then\, we can explicitly find the DM mass r egion and the size of Yukawa couplings between the DM and quarks\, based o n the study of flavor physics and DM physics. In conclusion\, we show that DM mass in our scenario is around the TeV scale\, and the Yukawa coupling s are between O(0.01) and O(1). The spin-independent DM scattering cross s ection is estimated as O(10^-9) [pb]. We also introduce the light dark mat ter scenario.\n\nhttps://conference-indico.kek.jp/event/38/contributions/8 56/ LOCATION:KEK Building 3 1F\, Seminar Hall URL:https://conference-indico.kek.jp/event/38/contributions/856/ END:VEVENT BEGIN:VEVENT SUMMARY:Naturalizing SUSY with the Relaxion and the Inflaton DTSTART;VALUE=DATE-TIME:20180215T000000Z DTEND;VALUE=DATE-TIME:20180215T003000Z DTSTAMP;VALUE=DATE-TIME:20210810T020749Z UID:indico-contribution-312-33@conference-indico.kek.jp DESCRIPTION:Speakers: Gherghetta\, Tony (University of Minnesota)\nThe LHC Run II superpartner mass limits have exacerbated the tuning in supersymme tric extensions of the Standard Model. A possible way to explain this tuni ng is via a two-field relaxion mechanism\, where the second field is ident ified with the inflaton. I will discuss the implications of the relaxion-i nflaton dynamics for supersymmetry and inflation\, as well as the prospect s for detecting this new invisible sector in future experiments.\n\nhttps: //conference-indico.kek.jp/event/38/contributions/858/ LOCATION:KEK Building 3 1F\, Seminar Hall URL:https://conference-indico.kek.jp/event/38/contributions/858/ END:VEVENT BEGIN:VEVENT SUMMARY:Recent developments on rare B-decays DTSTART;VALUE=DATE-TIME:20180215T020000Z DTEND;VALUE=DATE-TIME:20180215T023000Z DTSTAMP;VALUE=DATE-TIME:20210810T020749Z UID:indico-contribution-313-36@conference-indico.kek.jp DESCRIPTION:Speakers: Bobeth\, Christoph (Technical University Munich)\nAf ter a review of tensions in charged-current and rare B decays and their in terpretation in beyond SM scenarios\, we focus on some developments that a im to improve theoretical control. Progress on QED corrections to leptonic decays B_s -> mu mu and B_u -> mu nu has been made\, that was required in view of the current accuracy providing in the future precision at the per cent level to short-distance quantities. A novel approach to the hadronic charm contribution in rare b-> s ll decays builds on a combined analysis o f b->s ll and b-> s (ccbar) -> ll decays to separate hadronic contributio ns from new physics signals.\n\nhttps://conference-indico.kek.jp/event/38/ contributions/855/ LOCATION:KEK Building 3 1F\, Seminar Hall URL:https://conference-indico.kek.jp/event/38/contributions/855/ END:VEVENT BEGIN:VEVENT SUMMARY:Neutrino Oscillation Experiments and Recent Results from T2K DTSTART;VALUE=DATE-TIME:20180215T023000Z DTEND;VALUE=DATE-TIME:20180215T030000Z DTSTAMP;VALUE=DATE-TIME:20210810T020749Z UID:indico-contribution-313-37@conference-indico.kek.jp DESCRIPTION:Speakers: Iwamoto\, Konosuke (University of Tokyo)\nNon-zero m ass of the neutrinos was proved by the discovery of neutrino oscillations in 1998. Further precision measurements of the neutrino oscillations lead to understanding the matter-antimatter asymmetry of the universe. This tal k provides overview of neutrino oscillations and the experimental results that contribute to measuring the oscillation parameters. Recent results an d the future prospects of T2K will be given.\n\nhttps://conference-indico. kek.jp/event/38/contributions/860/ LOCATION:KEK Building 3 1F\, Seminar Hall URL:https://conference-indico.kek.jp/event/38/contributions/860/ END:VEVENT BEGIN:VEVENT SUMMARY:Cosmology of a Fine-Tuned SUSY Higgs DTSTART;VALUE=DATE-TIME:20180216T003000Z DTEND;VALUE=DATE-TIME:20180216T010000Z DTSTAMP;VALUE=DATE-TIME:20210810T020749Z UID:indico-contribution-316-28@conference-indico.kek.jp DESCRIPTION:Speakers: Reece\, Matthew (Harvard University)\nI will discuss some work in progress that explores whether a mildly fine-tuned Higgs bos on\, as in (mini-)split supersymmetry\, can have interesting or observable cosmological consequences. As moduli fields oscillate\, the Higgs can res pond and perhaps acquire very large values along a D-flat direction. Possi ble consequences involve a burst of gravitational wave production and an a ltered estimate of the number of e-folds of inflation.\n\nhttps://conferen ce-indico.kek.jp/event/38/contributions/798/ LOCATION:KEK Building 3 1F\, Seminar Hall URL:https://conference-indico.kek.jp/event/38/contributions/798/ END:VEVENT BEGIN:VEVENT SUMMARY:An Update on Supersymmetric String Landscape DTSTART;VALUE=DATE-TIME:20180216T010000Z DTEND;VALUE=DATE-TIME:20180216T013000Z DTSTAMP;VALUE=DATE-TIME:20210810T020749Z UID:indico-contribution-316-29@conference-indico.kek.jp DESCRIPTION:Speakers: Watari\, Taizan (Kavli IPMU\, the University of Toky o)\nhttps://conference-indico.kek.jp/event/38/contributions/800/ LOCATION:KEK Building 3 1F\, Seminar Hall URL:https://conference-indico.kek.jp/event/38/contributions/800/ END:VEVENT BEGIN:VEVENT SUMMARY:Unification from Scattering Amplitudes DTSTART;VALUE=DATE-TIME:20180216T000000Z DTEND;VALUE=DATE-TIME:20180216T003000Z DTSTAMP;VALUE=DATE-TIME:20210810T020749Z UID:indico-contribution-316-27@conference-indico.kek.jp DESCRIPTION:Speakers: Cheung\, Clifford (Caltech)\nhttps://conference-indi co.kek.jp/event/38/contributions/814/ LOCATION:KEK Building 3 1F\, Seminar Hall URL:https://conference-indico.kek.jp/event/38/contributions/814/ END:VEVENT BEGIN:VEVENT SUMMARY:Beyond the LHC: physics goals and CERN's plans for future collider s DTSTART;VALUE=DATE-TIME:20180216T053500Z DTEND;VALUE=DATE-TIME:20180216T060500Z DTSTAMP;VALUE=DATE-TIME:20210810T020749Z UID:indico-contribution-318-22@conference-indico.kek.jp DESCRIPTION:Speakers: Mangano\, Michelangelo (CERN)\nThe LHC performance c ontinues to exceed expectations\, and the experiments are entering a new h igh-statistics phase for their studies. The projections for the ultimate p hysics output of the LHC are being updated\, and new plans are being drawn for next steps\, with scenarios ranging from an energy upgrade of the LHC \, to the construction of a new 100km circular collider facility. I will r eview the physics motivations that justify these future plans\, and the st atus of the project definition.\n\nhttps://conference-indico.kek.jp/event/ 38/contributions/799/ LOCATION:KEK Building 3 1F\, Seminar Hall URL:https://conference-indico.kek.jp/event/38/contributions/799/ END:VEVENT BEGIN:VEVENT SUMMARY:Theoretical uncertainties of monojet signatures from compressed ma ss spectra DTSTART;VALUE=DATE-TIME:20180216T044500Z DTEND;VALUE=DATE-TIME:20180216T051000Z DTSTAMP;VALUE=DATE-TIME:20210810T020749Z UID:indico-contribution-318-21@conference-indico.kek.jp DESCRIPTION:Speakers: Sung Hak\, Lim (KEK)\nhttps://conference-indico.kek. jp/event/38/contributions/816/ LOCATION:KEK Building 3 1F\, Seminar Hall URL:https://conference-indico.kek.jp/event/38/contributions/816/ END:VEVENT BEGIN:VEVENT SUMMARY:Probing flavour-violating decays of squarks at the LHC DTSTART;VALUE=DATE-TIME:20180216T051000Z DTEND;VALUE=DATE-TIME:20180216T053500Z DTSTAMP;VALUE=DATE-TIME:20210810T020749Z UID:indico-contribution-318-49@conference-indico.kek.jp DESCRIPTION:Speakers: Chakraborty\, Amit (KEK)\nWe study squark decays bey ond the Minimal Flavor Violation framework at the LHC. Considering mixing between the second and third generation squarks\, we first provide the cov erage of the current searches at the Run-1 and Run-2 of LHC in the context of a simplified model containing two active squark flavours. We then stud y the sensitivity of a dedicated search strategy involving leptons\, jets\ , and missing transverse energy at the high luminosity run of LHC.\n\nhttp s://conference-indico.kek.jp/event/38/contributions/818/ LOCATION:KEK Building 3 1F\, Seminar Hall URL:https://conference-indico.kek.jp/event/38/contributions/818/ END:VEVENT END:VCALENDAR