村山, 斉
Murayama, Hitoshi
Murayama, Hitoshi, 1964-
무라야마 히토시 1964-
VIAF ID: 176789699 (Personal)
Permalink: http://viaf.org/viaf/176789699
Preferred Forms
- 100 1 _ ‡a Murayama, Hitoshi
- 100 1 _ ‡a Murayama, Hitoshi
- 100 1 _ ‡a Murayama, Hitoshi ‡d 1964-
- 100 1 _ ‡a Murayama, Hitoshi, ‡d 1964-
- 100 0 _ ‡a 村山 斉
- 100 1 _ ‡a 村山, 斉
- 100 1 _ ‡a 村山, 斉
- 100 1 _ ‡a 무라야마 히토시 ‡d 1964-
4xx's: Alternate Name Forms (29)
Works
Title | Sources |
---|---|
Ainshutain tsukai uchuron. | |
Atmospheric neutrinos can make beauty strange | |
Baryogenesis from a dark first-order phase transition | |
Can supersymmetric loops correct the fermion mass relations in SU(5)? | |
A compact ultra-clean system for deploying radioactive sources inside the KamLAND detector | |
The Cosmic Evolution Survey (COSMOS): A Large‐Scale Structure atz = 0.73 and the Relation of Galaxy Morphologies to Local Environment | |
COSMOS Morphological Classification with the Zurich Estimator of Structural Types (ZEST) and the Evolution Sincez= 1 of the Luminosity Function of Early, Disk, and Irregular Galaxies | |
COSMOS PHOTOMETRIC REDSHIFTS WITH 30-BANDS FOR 2-deg2 | |
The COSMOS-WIRCam near-infrared imaging survey. I. BzK-selected passive and star-forming galaxy candidates at z {>~} 1.4 | |
Dimensional reduction in anomaly mediation | |
Does the universe have an end? | |
Energy spectra of reactor neutrinos at KamLAND | |
Extragalactic science, cosmology, and Galactic archaeology with the Subaru Prime Focus Spectrograph | |
Family symmetries and proton decay | |
The First Release COSMOS Optical and Near‐IR Data and Catalog | |
Galaxy-scale gravitational lens candidates from the Hyper Suprime-Cam imaging survey and the Galaxy And Mass Assembly spectroscopic survey | |
Hubble space Telescope/Advanced camera for surveys morphology of Ly{alpha} emitters at redshift 5.7 in the COSMOS field | |
The KamLAND full-volume calibration system | |
Kiso kagaku de mirai o tsukuru : Kagakuteki igi to shakaiteki igi. | |
More visible effects of the hidden sector | |
Murayamasan uchu wa dokomade wakattandesuka : Biggu ban kara higgusu ryushi e. | |
The ninth data release of the Sloan Digital Sky Survey: first spectroscopic data from the SDSS-III baryon oscillation spectroscopic survey | |
Not even decoupling can save the minimal supersymmetric SU(5) model | |
The [Oii] λ3727 Luminosity Function and Star Formation Rate atz ≈ 1.2 in the COSMOS 2 Square Degree Field and the Subaru Deep Field | |
On preserving a B + L asymmetry produced in the early universe | |
Partial radiogenic heat model for Earth revealed by geoneutrino measurements | |
Photo-zperformance for precision cosmology - II. Empirical verification1★ | |
Physics at a future Neutrino Factory and super-beam facility | |
practical and consistent parametrization of dark matter self-interactions | |
Precision Measurement of Neutrino Oscillation Parameters with KamLAND | |
Preserving flat directions during inflation | |
Prime Focus Spectrograph for the Subaru telescope: massively multiplexed optical and near-infrared fiber spectrograph | |
Probing the scale of grand unification with gravitational waves | |
Production of radioactive isotopes through cosmic muon spallation in KamLAND | |
Puffy dark matter | |
Realistic Dirac leptogenesis | |
The Redshift Evolution of Early‐Type Galaxies in COSMOS: Do Massive Early‐Type Galaxies Form by Dry Mergers? | |
Regulating the baryon asymmetry in no-scale Affleck-Dine baryogenesis | |
Review of Particle Properties | |
Revisão de Física de Partículas | |
Ryoshi rikigaku fo beibizu. | |
Saikyo ni omoshiroi soryushi. | |
SDSS-III: massive spectroscopic surveys of the distant universe, the Milky Way, and extra-solar planetary systems | |
Search for extraterrestrial antineutrino sources with the KamLAND detector | |
Signatures of baryogenesis in the minimal supersymmetric standard model | |
Sotaisei riron fo beibizu. | |
TheXMM‐NewtonWide‐Field Survey in the COSMOS Field: Statistical Properties of Clusters of Galaxies | |
Top quark forward-backward asymmetry from new t -channel physics | |
Twin SIMPs | |
Uchū ni owari wa arunoka : Soryūshi ga tokiakasu uchū no rekishi | |
Uchu no shiwa to tane : Dai127kai honda zaidan kondankai. | |
Uchū wa hontō ni hitotsu nanoka : Saishin uchūron nyūmon | |
Uchū wa nani de dekiteirunoka : Soryūshi butsurigaku de toku uchū no nazo | |
Uchu wa naze utsukushi noka : Kyukyoku no uchu no hosoku o mezashite. | |
Uju ga jeongmal hana ppun ilkka? | |
Velocity dependence from resonant self-interacting dark matter | |
Wae, uri ga uju e jonjae haneunga? | |
WMAPping out neutrino masses | |
The Zurich Extragalactic Bayesian Redshift Analyzer and its first application: COSMOS | |
왜, 우리가 우주에 존재하는가? 최신 소립자론 입문 | |
우주가 정말 하나뿐일까? 최신 우주론 입문 | |
そうたいせいりろんfor babies | |
アインシュタイン痛快!宇宙論 | |
ニュートンりきがくfor babies | |
ヒッグス粒子素粒子の世界 : 科学界最大の関心事が、みるみる理解できる | |
基礎科学で未来をつくる : 科学的意義と社会的意義 | |
宇宙になぜ我々が存在するのか : 最新素粒子論入門 | |
宇宙に終わりはあるのか? : 素粒子が解き明かす宇宙の歴史 | |
宇宙のしわと種 : 第127回本田財団懇談会 | |
宇宙はなぜこんなにうまくできているのか | |
宇宙はなぜ美しいのか : 究極の「宇宙の法則」を目指して | |
宇宙は何でできているのか : 素粒子物理学で解く宇宙の謎 | |
宇宙は本当にひとつなのか : 最新宇宙論入門 | |
宇宙を創る実験 | |
最強に面白い素粒子 | |
村山さん、宇宙はどこまでわかったんですか? : ビッグバンからヒッグス粒子へ |