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Related papers: CPT-Symmetric Universe

200 papers

We propose simple scoto-seesaw models to account for dark matter and neutrino masses with spontaneous CP violation. This is achieved with a single horizontal $\mathcal{Z}_8$ discrete symmetry, broken to a residual $\mathcal{Z}_2$ subgroup…

High Energy Physics - Phenomenology · Physics 2021-05-12 D. M. Barreiros , F. R. Joaquim , R. Srivastava , J. W. F. Valle

Recent cosmological observations, such as the measurement of the primordial 4He abundance, CMB, and large scale structure, give preference to the existence of extra radiation component, Delta N_nu > 0. The extra radiation may be accounted…

High Energy Physics - Phenomenology · Physics 2011-06-27 Kazunori Nakayama , Fuminobu Takahashi , Tsutomu T. Yanagida

A popular class of theories attributes the matter-antimatter asymmetry of the Universe to CP-violating decays of super-heavy BSM particles in the Early Universe. Recently, we discovered a new source of leptogenesis in these models, namely…

High Energy Physics - Phenomenology · Physics 2017-04-12 J. I. McDonald , G. M. Shore

A simple way to accommodate dark matter is to postulate the existence of a hidden sector. That is, a set of new particles and forces interacting with the known particles predominantly via gravity. In general this leads to a large set of…

Cosmology and Nongalactic Astrophysics · Physics 2014-05-13 R. Foot

We show that a CP-violating interaction induced by a derivative coupling between the running vacuum and a non-conserving baryon current may dynamically break CPT and trigger baryogenesis through an effective chemical potential. By assuming…

General Relativity and Quantum Cosmology · Physics 2017-12-15 J. A. S. Lima , Douglas Singleton

The Standard Model of particle physics fails to explain the important pieces in the standard cosmology, such as inflation, baryogenesis, and dark matter of the Universe. We consider the possibility that the sector to generate small neutrino…

High Energy Physics - Phenomenology · Physics 2015-06-19 Tetsutaro Higaki , Ryuichiro Kitano , Ryosuke Sato

I will give here an overview of the present observational and theoretical situation regarding the question of the matter-antimatter asymmetry of the universe and the related question of the existence of antimatter on a cosmological scale. I…

High Energy Physics - Phenomenology · Physics 2007-05-23 F. W. Stecker

We propose a simple extension of the minimal supersymmetric standard model by introducing a gauge singlet in addition to right-handed neutrinos. The model resolves the strong CP problem by Pecci-Quinn symmetry, explains the origin of…

High Energy Physics - Phenomenology · Physics 2010-08-02 Wan-Il Park

This paper is devoted to the investigation of connection between two apparent asymmetries of the nature --- time-asymmetry and Baryon Asymmetry of the Universe (BAU). The brief review of this subjects is given. We consider the particle…

High Energy Physics - Phenomenology · Physics 2007-05-23 Andro Barnaveli , Merab Gogberashvili

Longstanding anomalies in the Cosmic Microwave Background (CMB), including the low quadrupole moment and hemispherical power asymmetry, have recently been linked to an underlying parity asymmetry. We show here how this parity asymmetry…

General Physics · Physics 2025-07-08 Enrique Gaztañaga , K. Sravan Kumar

The cosmological constant (CC) problem is the biggest enigma of theoretical physics ever. In recent times, it has been rephrased as the dark energy problem in order to encompass a wider spectrum of possibilities. It is, in any case, a…

High Energy Physics - Theory · Physics 2009-07-23 Florian Bauer , Joan Sola , Hrvoje Stefancic

These results represent the solution for the historical problem of the contamination by matter effects on the CPV Asymmetry for neutrino oscillations. Vacuum is CPT-symmetric and matter is T-symmetric, the goal is accomplished by using this…

High Energy Physics - Phenomenology · Physics 2019-10-29 Jose Bernabeu , Alejandro Segarra

Charge-Parity-Time (CPT) symmetry governs that the oscillation parameters for neutrinos and anti-neutrinos are to be identical. Different mass and mixing parameters for these particles may give us a possible hint for CPT violation in the…

High Energy Physics - Experiment · Physics 2020-04-02 Daljeet Kaur

In the minimal gauged B-L extension of the Standard Model, we demonstrate that PeV-scale dark matter (DM) and the baryon asymmetry of the Universe (BAU) can be simultaneously explained through the three right-handed neutrinos (RHNs) present…

High Energy Physics - Phenomenology · Physics 2025-08-05 Basabendu Barman , Arindam Das , Suruj Jyoti Das , Marco Merchand

Conventional thermodynamics, which is formulated for our world populated by radiation and matter, can be extended to describe physical properties of antimatter in two mutually exclusive ways: CP-invariant or CPT-invariant. Here we refer to…

Statistical Mechanics · Physics 2014-04-02 A. Y. Klimenko , U. Maas

For the first time, we have a plausible and complete accounting of matter and energy in the Universe. Expressed a fraction of the critical density it goes like this: neutrinos, between 0.3% and 15%; stars, between 0.3% and 0.6%; baryons…

Astrophysics · Physics 2009-10-31 Michael S. Turner

The Standard Model (SM) of particle physics, being a local, unitary and Lorentz-invariant quantum field theory, remains symmetric under the combined action of Charge, Parity, and Time Reversal (CPT) symmetry. This automatically implies that…

High Energy Physics - Phenomenology · Physics 2023-07-19 Ting Cheng , Manfred Lindner , Manibrata Sen

Motivated by inflation, the theory of big-bang nucleosynthesis and the quest for a deeper understanding of the fundamental forces and particles, a very successful paradigm for the development of structure in the Universe has evolved. It…

Astrophysics · Physics 2009-10-28 Scott Dodelson , Evalyn Gates , Michael S. Turner

Primordial nucleosynthesis provides a probe of the universal abundance of baryons when the universe was only a few minutes old. Recent observations of anisotropy in the cosmic microwave background (CMB) probe the baryon abundance when the…

Astrophysics · Physics 2007-05-23 G. Steigman , J. P. Kneller , A. Zentner

The current laws of physics do not explain the observed imbalance of matter and antimatter in the universe. Sakharov proposed that an explanation would require the violation of CP symmetry between matter and antimatter. The only CP…

High Energy Physics - Experiment · Physics 2021-01-26 K. Abe , R. Akutsu , A. Ali , C. Alt , C. Andreopoulos , L. Anthony , M. Antonova , S. Aoki , A. Ariga , Y. Asada , Y. Ashida , E. T. Atkin , Y. Awataguchi , S. Ban , M. Barbi , G. J. Barker , G. Barr , C. Barry , M. Batkiewicz-Kwasniak , A. Beloshapkin , F. Bench , V. Berardi , S. Berkman , L. Berns , S. Bhadra , S. Bienstock , A. Blondel , S. Bolognesi , B. Bourguille , S. B. Boyd , D. Brailsford , A. Bravar , D. Bravo Berguño , C. Bronner , A. Bubak , M. Buizza Avanzini , J. Calcutt , T. Campbell , S. Cao , S. L. Cartwright , M. G. Catanesi , A. Cervera , A. Chappell , C. Checchia , D. Cherdack , N. Chikuma , G. Christodoulou , J. Coleman , G. Collazuol , L. Cook , D. Coplowe , A. Cudd , A. Dabrowska , G. De Rosa , T. Dealtry , P. F. Denner , S. R. Dennis , C. Densham , F. Di Lodovico , N. Dokania , S. Dolan , O. Drapier , J. Dumarchez , P. Dunne , L. Eklund , S. Emery-Schrenk , A. Ereditato , P. Fernandez , T. Feusels , A. J. Finch , G. A. Fiorentini , G. Fiorillo , C. Francois , M. Friend , Y. Fujii , R. Fujita , D. Fukuda , R. Fukuda , Y. Fukuda , K. Gameil , C. Giganti , T. Golan , M. Gonin , A. Gorin , M. Guigue , D. R. Hadley , J. T. Haigh , P. Hamacher-Baumann , M. Hartz , T. Hasegawa , N. C. Hastings , T. Hayashino , Y. Hayato , A. Hiramoto , M. Hogan , J. Holeczek , N. T. Hong Van , F. Iacob , A. K. Ichikawa , M. Ikeda , T. Ishida , T. Ishii , M. Ishitsuka , K. Iwamoto , A. Izmaylov , B. Jamieson , S. J. Jenkins , C. Jesús-Valls , M. Jiang , S. Johnson , P. Jonsson , C. K. Jung , M. Kabirnezhad , A. C. Kaboth , T. Kajita , H. Kakuno , J. Kameda , D. Karlen , S. P. Kasetti , Y. Kataoka , T. Katori , Y. Kato , E. Kearns , M. Khabibullin , A. Khotjantsev , T. Kikawa , H. Kim , J. Kim , S. King , J. Kisiel , A. Knight , A. Knox , T. Kobayashi , L. Koch , T. Koga , A. Konaka , L. L. Kormos , Y. Koshio , K. Kowalik , H. Kubo , Y. Kudenko , N. Kukita , S. Kuribayashi , R. Kurjata , T. Kutter , M. Kuze , L. Labarga , J. Lagoda , M. Lamoureux , M. Laveder , M. Lawe , M. Licciardi , T. Lindner , R. P. Litchfield , S. L. Liu , X. Li , A. Longhin , L. Ludovici , X. Lu , T. Lux , L. N. Machado , L. Magaletti , K. Mahn , M. Malek , S. Manly , L. Maret , A. D. Marino , J. F. Martin , T. Maruyama , T. Matsubara , K. Matsushita , V. Matveev , K. Mavrokoridis , E. Mazzucato , M. McCarthy , N. McCauley , K. S. McFarland , C. McGrew , A. Mefodiev , C. Metelko , M. Mezzetto , A. Minamino , O. Mineev , S. Mine , M. Miura , L. Molina Bueno , S. Moriyama , J. Morrison , Th. A. Mueller , L. Munteanu , S. Murphy , Y. Nagai , T. Nakadaira , M. Nakahata , Y. Nakajima , A. Nakamura , K. G. Nakamura , K. Nakamura , S. Nakayama , T. Nakaya , K. Nakayoshi , C. Nantais , T. V. Ngoc , K. Niewczas , K. Nishikawa , Y. Nishimura , T. S. Nonnenmacher , F. Nova , P. Novella , J. Nowak , J. C. Nugent , H. M. O'Keeffe , L. O'Sullivan , T. Odagawa , K. Okumura , T. Okusawa , S. M. Oser , R. A. Owen , Y. Oyama , V. Palladino , J. L. Palomino , V. Paolone , W. C. Parker , P. Paudyal , M. Pavin , D. Payne , G. C. Penn , L. Pickering , C. Pidcott , G. Pintaudi , E. S. Pinzon Guerra , C. Pistillo , B. Popov , K. Porwit , M. Posiadala-Zezula , A. Pritchard , B. Quilain , T. Radermacher , E. Radicioni , B. Radics , P. N. Ratoff , E. Reinherz-Aronis , C. Riccio , E. Rondio , S. Roth , A. Rubbia , A. C. Ruggeri , A. Rychter , K. Sakashita , F. Sánchez , C. M. Schloesser , K. Scholberg , J. Schwehr , M. Scott , Y. Seiya , T. Sekiguchi , H. Sekiya , D. Sgalaberna , R. Shah , A. Shaikhiev , F. Shaker , A. Shaykina , M. Shiozawa , W. Shorrock , A. Shvartsman , A. Smirnov , M. Smy , J. T. Sobczyk , H. Sobel , F. J. P. Soler , Y. Sonoda , J. Steinmann , S. Suvorov , A. Suzuki , S. Y. Suzuki , Y. Suzuki , A. A. Sztuc , M. Tada , M. Tajima , A. Takeda , Y. Takeuchi , H. K. Tanaka , H. A. Tanaka , S. Tanaka , L. F. Thompson , W. Toki , C. Touramanis , K. M. Tsui , T. Tsukamoto , M. Tzanov , Y. Uchida , W. Uno , M. Vagins , S. Valder , Z. Vallari , D. Vargas , G. Vasseur , C. Vilela , W. G. S. Vinning , T. Vladisavljevic , V. V. Volkov , T. Wachala , J. Walker , J. G. Walsh , Y. Wang , D. Wark , M. O. Wascko , A. Weber , R. Wendell , M. J. Wilking , C. Wilkinson , J. R. Wilson , R. J. Wilson , K. Wood , C. Wret , Y. Yamada , K. Yamamoto , C. Yanagisawa , G. Yang , T. Yano , K. Yasutome , S. Yen , N. Yershov , M. Yokoyama , T. Yoshida , M. Yu , A. Zalewska , J. Zalipska , K. Zaremba , G. Zarnecki , M. Ziembicki , E. D. Zimmerman , M. Zito , S. Zsoldos , A. Zykova