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Recent BICEP2 results on CMB polarisation B-modes suggest a high value for the inflation scale $V_0^{1/4} \simeq 10^{16}$ GeV, giving experimental evidence for a physical scale in between the EW scale and the Planck mass. We propose that…

High Energy Physics - Phenomenology · Physics 2015-06-19 Luis E. Ibanez , Irene Valenzuela

We briefly review several Higgs inflation models and discuss their cosmological implications. We first classify the inflation models according to the predicted value of the tensor-to-scalar ratio: (i) $r = {\cal O}(0.01-0.1)$, (ii) $r =…

High Energy Physics - Phenomenology · Physics 2015-06-01 Fuminobu Takahashi

Recently, the ATLAS and CMS collaborations have announced exciting hints for a Standard Model-like Higgs boson at a mass of approximately 125 GeV. In this paper, we explore the potential consequences for the MSSM and low scale…

High Energy Physics - Phenomenology · Physics 2013-05-30 Patrick Draper , Patrick Meade , Matthew Reece , David Shih

We investigate an inflation model with the inflaton being identified with a Higgs boson responsible for the breaking of U(1)B-L symmetry. We show that supersymmetry must remain a good symmetry at scales one order of magnitude below the…

High Energy Physics - Phenomenology · Physics 2012-03-13 Kazunori Nakayama , Fuminobu Takahashi

It has been argued that rather generic features of string-inspired inflationary theories with low-energy supersymmetry (SUSY) make it difficult to achieve inflation with a Hubble scale H > m_{3/2}, where m_{3/2} is the gravitino mass in the…

High Energy Physics - Theory · Physics 2015-03-13 Temple He , Shamit Kachru , Alexander Westphal

Combination of Plank and BICEP2 data reported that tensor to scalar ratio $r\simeq 0.16$ and scalar spectral index $n_{s}\simeq 0.96$. In this short note, it is shown that chaotic inflation with quadratic potential, which perfectly accounts…

High Energy Physics - Phenomenology · Physics 2015-02-25 Sibo Zheng

We show that heavy supersymmetric particles around O(100) TeV to O(1) PeV naturally appear in new inflation in which the Higgs boson responsible for the breaking of U(1)B-L plays the role of inflaton. Most important, the supersymmetric…

High Energy Physics - Phenomenology · Physics 2012-05-30 Kazunori Nakayama , Fuminobu Takahashi

The lighter neutral scalar Higgs mass is examined in gauge-mediated supersymmetry-breaking models in which the messenger sector responsible for SUSY breaking is allowed to involve more general sets of $SU(3) \otimes SU(2) \otimes U(1)$…

High Energy Physics - Phenomenology · Physics 2007-05-23 T. A. Kaeding , S. Nandi

A brief review is given of the implications of a 126 GeV Higgs boson for the discovery of supersymmetry. Thus a 126 GeV Higgs boson is problematic within the Standard Model because of vacuum instability pointing to new physics beyond the…

High Energy Physics - Phenomenology · Physics 2016-04-20 Pran Nath

We provide an anthropic reason that the supersymmetry breaking scale is much higher than the electroweak scale as indicated by the null result of collider experiments and observed 125 GeV Higgs boson. We focus on a new inflation model as a…

High Energy Physics - Phenomenology · Physics 2016-03-23 Masahiro Kawasaki , Masaki Yamada , Tsutomu T. Yanagida , Norimi Yokozaki

We consider inflation and supersymmetry breaking in the context of a minimal model of supersymmetry in which the only "low" energy remnant of supersymmetry is the gravitino with a mass of order an EeV. In this theory, the supersymmetry…

High Energy Physics - Phenomenology · Physics 2018-01-03 Emilian Dudas , Tony Gherghetta , Yann Mambrini , Keith A. Olive

I introduce a new low energy effective description of Cosmological SUSY breaking. It requires the existence of a strongly interacting gauge theory at a scale of order $10^3$ GeV, some of whose fields carry standard model quantum numbers.…

High Energy Physics - Phenomenology · Physics 2007-05-23 T. Banks

We consider a SUSY breaking scenario without the Polonyi problem. To solve the problem, the enhanced couplings of the Polonyi field to an inflaton, gauge kinetic functions and itself are assumed. As a result, a gaugino mediated SUSY…

High Energy Physics - Phenomenology · Physics 2015-06-12 Takeo Moroi , Tsutomu T. Yanagida , Norimi Yokozaki

A class of supersymmetric grand unified theories is introduced that has a single scale below the cutoff, that of the supersymmetry breaking masses $\tilde{m}$. For a wide range of the dimensionless parameters, agreement with the observed…

High Energy Physics - Phenomenology · Physics 2015-06-19 Lawrence J. Hall , Yasunori Nomura , Satoshi Shirai

We argue that in the simplest version of the KKLT model, the maximal value of the Hubble constant during inflation cannot exceed the present value of the gravitino mass, H< m_{3/2}. This may have important implications for string cosmology…

High Energy Physics - Theory · Physics 2010-04-06 Renata Kallosh , Andrei Linde

The energy, or mass scale M_SUSY, of the supersymmetry (SUSY) phase transition is, as yet, unknown. If it is very high (i.e., ~ 10^3 GeV), terrestrial accelerators will not be able to measure it. We determine M_SUSY here by combining theory…

Astrophysics · Physics 2007-05-23 Reuven Opher , Ana Pelinson

We show that the gauge mediation models with vector-like matters can explain the Higgs boson mass of 126 GeV without large soft scalar masses nor a large left-right mixing of the stops. The scenario has interesting features: the existence…

High Energy Physics - Phenomenology · Physics 2013-05-09 Norimi Yokozaki

A keV-scale gravitino arsing from a minimal supersymmetric (SUSY) Standard Model (MSSM) is an interesting possibility since the small scale problems that $\Lambda$CDM model encounters in the modern cosmology could be alleviated with the…

High Energy Physics - Phenomenology · Physics 2021-04-08 Gongjun Choi , Tsutomu T. Yanagida , Norimi Yokozaki

It is known that gravitinos are non-thermally produced in inflaton decay processes, which excludes many inflation models for a wide range of the gravitino mass. We find that the constraints from the gravitino overproduction can be greatly…

High Energy Physics - Phenomenology · Physics 2015-06-11 Kazunori Nakayama , Fuminobu Takahashi , Tsutomu T. Yanagida

The large value of the tensor-to-scalar ratio in the cosmic microwave background radiation reported by the BICEP2 collaboration gives strong impact on models of supersymmetry (SUSY). The large ratio indicates inflation with a high-energy…

High Energy Physics - Phenomenology · Physics 2015-06-19 Keisuke Harigaya , Masahiro Ibe , Koji Ichikawa , Kunio Kaneta , Shigeki Matsumoto
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