5,442 research outputs found
PeV scale Supersymmetry breaking and the IceCube neutrino flux
The observation of very high energy neutrino events at IceCube has grasped a
lot of attention in the fields of both astrophysics and particle physics. It
has been speculated that these high energy neutrinos might originate either
from purely conventional astrophysical sources or from the late decay of a
super heavy (PeV scale) dark matter (DM) particle. In order for decaying DM to
be a dominant source of the IceCube high-energy neutrinos, it would require an
unusually suppressed value of the coupling of DM to neutrinos. We attempt to
explain this small coupling in the context of an -parity conserving minimal
supergravity model which has right-handed neutrino superfields. With the main
assumptions of super-partner masses at the PeV scale and also a reheating
temperature not much larger than the PeV scale, we find in our model several
natural order-of-magnitude "miracles", (i) the gravitino is produced via
freeze-in as a DM candidate with the correct relic density (ii) the
right-handed (RH) sneutrino makes up only a tiny fraction (, of the
present day energy density of the universe, yet its decay lifetime to the
gravitino and neutrinos is such that it naturally predicts the right
order-of-magnitude for the IceCube neutrino flux. The long lifetime of the RH
sneutrino is explained by the existence of a global -symmetry which is only
broken due to supersymmetry breaking effects. Our model also predicts a flux of
100 TeV gamma rays from the decaying RH sneutrino which are within the current
observational constraints.Comment: v2: 34 pages, 6 figures, Journal version (published in JHEP
Transport Coefficients of Black MQGP M3-Branes
The SYZ mirror, in the `delocalized limit' of [1], of (M)N
(fractional)D3-branes, and wrapped N_f flavor D7-branes in the presence of a
black-hole resulting in a non-Kaehler resolved warped deformed conifold
(NKRWDC) in [2], was carried out in [3] and resulted in black M3-branes. The
uplift, if valid globally(like [4] for fractional D3 branes in conifolds),
asymptotes to M5-branes wrapping a two-cycle (homologously an (large) integer
sum of two-spheres) in AdS_5xM_6. Interestingly, in the MQGP limit, assuming
the deformation > resolution, by estimating the five SU(3) structure torsion
(\tau) classes W_{1,2,3,4,5} we show that \tau\in W_4+W_5: 2/3
Re(W^3bar_5)=W^3bar_4 in the UV, implying the NKRWDC locally preserves SUSY.
Further, the local T^3 of [3] in the large-r limit and the `MQGP' limit of [3],
satisfies the same conditions as the maximal T^2-invariant special Lagrangian
three-cycle of T^*(S^3) of [6], partly justifying use of local SYZ mirror
symmetry in [3]. Using the Ouyang embedding in the DBI action of a D7-brane or
by dimensionally reducing the 11-dimensional EH action to five (R^{1,3},r)
dimensions, we then calculate a variety of gauge and metric-perturbation-modes'
two-point functions using the prescription of [5], and show: (i) diffusion
constant D~1/T, (ii) the electrical conductivity \sigma~T, (iii) the charge
susceptibility \chi~ T^2, (iv) [using (i) - (iii)] the Einstein's relation
\sigma/\chi=D, is indeed satisfied, (v) the R-charge diffusion constant
D_R~1/T, and (vi) the possibility of generating \eta/s=1/4pi from solutions to
the vector and tensor mode metric perturbations' EOMs, separately. All results
are also valid in the limit of [2].Comment: v4:1+50 pages, correction in torsion classes: type IIB, locally, has
SUSY in the U
Anti-HIV therapy: pipeline approaches and future directions
Human immunodeficiency virus (HIV), with about 30 million deaths and double infections (in developing countries), is an open challenge today for global scientists. Developing safe and effective measurements against it has become the prime need of hour. Though, putting it at health priority, various efforts like chemotherapy, vaccines and others are attempted globally over last decade. Consequently, highly active antiretroviral therapy was introduced but fails to completely block the viral replication due to drug resistance and various other severe side effects. The antigenic variability and lack of appropriate experimental models is the major obstacle in the development of an ever effective treatment against HIV. However, to overcome the present hurdles and to emerge a preventive HIV vaccine efforts at various platforms are done. A renewed, coordinated research, preclinical studies, clinical trials together with sufficient long term scientific and commercial commitments are made. Few of the therapeutic efforts viz. RNA interference (RNAi) based replication arrest of HIV, viral enzymes’ inhibitors, nanotechnology based HIV control and various preclinically trialed vaccines are reviewed in this paper. Also, the observed toxicity of existing therapeutic regimen, key challenges and future prospects for the development of better tolerated prophylactic HIV-1 vaccine are discussed
Towards MQGP
For the Ouyang embedding we calculate the chemical potential mu_C due to a
U(1) gauge field on the w.v. of N_f D7-branes wrapped around a 4-cycle in a
resolved warped deformed conifold with (M)N (fractional)D3-branes of [1], and
show the possible thermodynamical stability up to linear order in the embedding
parameter. In the spirit of [2] we obtain the local type IIA mirror using SYZ
mirror symmetry near (theta_{1,2},psi)=(,{0,2pi,,4pi}) and then
oxidize the same to M theory. We take two limits of this
uplift:(i)g_s,g_sN_f,g_sM^2/N,g_s^2M N_f>1 similar to [1]
effected by M eps^{-3d/2}, N eps^{-19d},g_s epsn^d,d>0 and eps<=O(0.01);(ii)the
`MQGP limit' g_sM^2/N>1 for finite g_s,M, effected by: g_s eps, M
eps^{-3d/2},N eps^{-39d},d>0, eps<~1). The second limit is more suited for the
study of QGP (See [3]) and can only be addressed in M theory. The uplift gives
a black M3-brane solution whose near-horizon geometry near
theta_{1,2}=0,pi-branches, preserves 1/8 SUSY. We obtain eta/s=1/4pi for the
uplift and the diffusion constant for types IIB/IIA backgrounds comes out to be
~1/T, for both limits. The D=11 SUGRA action up to O(R^4,|G_4|^2) is expected
to receive dominant contributions near =0,pi due to poles.
Introducing a small-angle cut-off c and using the =c,(pi-c)-local
uplift the specific heat from the IR-finite part of the action (c-independent)
turns out to be positive indicative of the thermodynamical stability of the
uplift. An ALD-gravity-type interpretation can be given to the counter-terms
for(i). Its verified that the black M3-brane entropy S r_h^3 from M-theoretic
thermodynamical methods and the horizon areas of types IIB/IIA/M3-brane
solutions.Comment: 1+58 pages, LaTeX; v4 some minor corrections, results unchange
On Discovering Electromagnetic Emission from Neutron Star Mergers: The Early Years of Two Gravitational Wave Detectors
We present the first simulation addressing the prospects of finding an
electromagnetic (EM) counterpart to gravitational wave detections (GW) during
the early years of only two advanced interferometers. The perils of such a
search may have appeared insurmountable when considering the coarse ring-shaped
GW localizations spanning thousands of deg^2 using time-of-arrival information
alone. We show that leveraging the amplitude and phase information of the
predicted GW signal narrows the localization to arcs with a median area of only
~250 deg^2, thereby making an EM search tractable. Based on the locations and
orientations of the two LIGO detectors, we find that the GW sensitivity is
limited to one polarization and thus to only two sky quadrants. Thus, the rates
of GW events with two interferometers is only ~40% of the rate with three
interferometers of similar sensitivity. Another important implication of the
sky quadrant bias is that EM observatories in North America and Southern Africa
would be able to systematically respond to GW triggers several hours sooner
than Russia and Chile. Given the larger sky areas and the relative proximity of
detected mergers, 1m-class telescopes with very wide-field cameras are well
positioned for the challenge of finding an EM counterpart. Identification of
the EM counterpart amidst the even larger numbers of false positives further
underscores the importance of building a comprehensive catalog of foreground
stellar sources, background AGN and potential host galaxies in the local
universe.Comment: Submitted to ApJL, 8 pages, 4 figures, 1 tabl
Extranatural Inflation Redux
The success of a given inflationary model crucially depends upon two
features: its predictions for observables such as those of the Cosmic Microwave
background (CMB) and its insensitivity to the unknown ultraviolet (UV) physics
such as quantum gravitational effects. Extranatural inflation is a well
motivated scenario which is insensitive to UV physics by construction. In this
five dimensional model, the fifth dimension is compactified on a circle and the
zero mode of the fifth component of a bulk gauge field acts as the
inflaton. In this work, we study simple variations of the minimal extranatural
inflation model in order to improve its CMB predictions while retaining its
numerous merits. We find that it is possible to obtain CMB predictions
identical to those of e.g. Starobinsky model of
inflation and show that this can be done in the most minimal way by having two
additional extra light fermionic species in the bulk, with the same
charges. We then find the constraints that CMB observations impose on the
parameters of the model.Comment: Journal version (to appear in Phy. Rev. D
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