Sambuddha Sanyal
Tata Institute of Fundamental Research
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Featured researches published by Sambuddha Sanyal.
Journal of High Energy Physics | 2017
Chethan Krishnan; Sambuddha Sanyal; P. N. Bala Subramanian
A bstractA class of tensor models were recently outlined as potentially calculable examples of holography: their perturbative large-N behavior is similar to the Sachdev-Ye-Kitaev (SYK) model, but they are fully quantum mechanical (in the sense that there is no quenched disorder averaging). These facts make them intriguing tentative models for quantum black holes. In this note, we explicitly diagonalize the simplest non-trivial Gurau-Witten tensor model and study its spectral and late-time properties. We find parallels to (a single sample of) SYK where some of these features were recently attributed to random matrix behavior and quantum chaos. In particular, the spectral form factor exhibits a dip-ramp-plateau structure after a running time average, in qualitative agreement with SYK. But we also observe that even though the spectrum has a unique ground state, it has a huge (quasi-?)degeneracy of intermediate energy states, not seen in SYK. If one ignores the delta function due to the degeneracies however, there is level repulsion in the unfolded spacing distribution hinting chaos. Furthermore, there are gaps in the spectrum. The system also has a spectral mirror symmetry which we trace back to the presence of a unitary operator with which the Hamiltonian anticommutes. We use it to argue that to the extent that the model exhibits random matrix behavior, it is controlled not by the Dyson ensembles, but by the BDI (chiral orthogonal) class in the Altland-Zirnbauer classification.
Journal of High Energy Physics | 2017
Chethan Krishnan; K.V. Pavan Kumar; Sambuddha Sanyal
A bstractWe further explore the connection between holographic O(n) tensor models and random matrices. First, we consider the simplest non-trivial uncolored tensor model and show that the results for the density of states, level spacing and spectral form factor are qualitatively identical to the colored case studied in arXiv:1612.06330. We also explain an overall 16-fold degeneracy by identifying various symmetries, some of which were unavailable in SYK and the colored models. Secondly, and perhaps more interestingly, we systematically identify the Spectral Mirror Symmetry and the Time-Reversal Symmetry of both the colored and uncolored models for all values of n, and use them to identify the Andreev ensembles that control their random matrix behavior. We find that the ensembles that arise exhibit a refined version of Bott periodicity in n.
European Physical Journal A | 2009
Amruta Mishra; Arvind Kumar; Sambuddha Sanyal; Stefan Schramm
The medium modifications of the energies of kaons and antikaons in isospin asymmetric hyperonic matter are investigated using a chiral SU(3) model. The isospin-dependent medium effects are important for asymmetric heavy-ion collision experiments, as well as relevant for the neutron star phenomenology as the bulk matter in the interior of the neutron star is highly isospin asymmetric. The effects of hyperons on the medium modifications of the kaons and antikaons in the strange hadronic matter are investigated in the present work and are seen to be appreciable for hadronic matter with large strangeness fractions. The study of the K -mesons in the asymmetric strange hadronic matter can be especially relevant for the compressed strange baryonic matter which can result from asymmetric heavy-ion collision experiments in the future accelerator facility FAIR at GSI.
European Physical Journal A | 2010
Amruta Mishra; Arvind Kumar; Sambuddha Sanyal; V. Dexheimer; Stefan Schramm
Abstract.The modification of kaon and antikaon properties in the interior of (proto-)neutron stars is investigated using a chiral SU(3) model. The parameters of the model are fitted to nuclear-matter saturation properties, baryon octet vacuum masses, hyperon optical potentials and low-energy kaon-nucleon scattering lengths. We study the kaon/antikaon medium modification and explore the possibility of antikaon condensation in (proto-)neutron star matter at zero as well as finite temperature/entropy and neutrino content. The effect of hyperons on kaon and antikaon optical potentials is also investigated at different stages of the neutron star evolution.
Physical Review B | 2011
Sambuddha Sanyal; Argha Banerjee; Kedar Damle
We study the effect of a missing spin in a one dimensional
Physical Review Letters | 2016
Sambuddha Sanyal; Kedar Damle; Olexei I. Motrunich
S=1/2
Physical Review B | 2012
Sambuddha Sanyal; Argha Banerjee; Kedar Damle; Anders W. Sandvik
antiferromagnet with nearest neighbour Heisenberg exchange
Bulletin of the American Physical Society | 2018
Archak Purkayastha; Sambuddha Sanyal; Abhishek Dhar; Manas Kulkarni
J
arXiv: Strongly Correlated Electrons | 2018
Sambuddha Sanyal; Kusum Dhochak; Subhro Bhattacharjee
and six-spin coupling
Physical Review B | 2018
Archak Purkayastha; Sambuddha Sanyal; Abhishek Dhar; Manas Kulkarni
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