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The Real Space Power Spectrum of the PSCz Survey from 0.01 to 300 h/Mpc
We report a measurement of the real space (not redshift space) power spectrum of galaxies over four and a half decades of wavenumber, 0.01 to 300 h/Mpc, from the IRAS Point Source Catalog Redshift Sur...
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Science and ultimate reality
First published in 2004...
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Tegmark, Max Viata 3.0. Omul In Epoca Inteligentei Artificiale Scan
Tegmark, Max Viata 3.0. Omul In Epoca Inteligentei Artificiale Scan...
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Karhunen-Loeve eigenvalue problems in cosmology: how should we tackle large data sets?
Since cosmology is no longer "the data-starved science", the problem of how to best analyze large data sets has recently received considerable attention, and Karhunen-Loeve eigenvalue methods have bee...
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Large-Scale Sunyaev-Zel'dovich Effect: Measuring Statistical Properties with Multifrequency Maps
We study the prospects for extracting detailed statistical properties of the Sunyaev-Zel'dovich (SZ) effect associated with large scale structure using upcoming multifrequency CMB experiments. The gre...
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What should we be worried about?
First published in 2014...
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Consciousness as a State of Matter
We examine the hypothesis that consciousness can be understood as a state of matter, "perceptronium", with distinctive information processing abilities. We explore five basic principles that may disti...
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Nuclear War from a Cosmic Perspective
I discuss the impact of computer progress on nuclear war policy, both by enabling more accurate nuclear winter simulations and by affecting the probability of war starting accidentally. I argue that f...
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The Quest for Microwave Foreground X
The WMAP team has produced a foreground map that can account for most of the low-frequency Galactic microwave emission in the WMAP maps, tentatively interpreting it as synchrotron emission. Finkbeiner...
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Spherical Harmonic Analysis of the Angular Distribution of Gamma-Ray Bursts
We compute the angular power spectrum C_l of the BATSE 3B catalog, and find no evidence for clustering on any scale. These constraints bridge the entire range from small scales, probing source cluster...
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An icosahedron-based method for pixelizing the celestial sphere
For power spectrum estimation it's important that the pixelization of a CMB sky map be smooth and regular to high degree. With this criterion in mind the ``COBE sky cube" was defined. This paper has a...
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A measurement of the polarization-temperature angular cross power spectrum of the Cosmic Microwave B
We present a measurement of the temperature-polarization angular cross power spectrum, , of the Cosmic Microwave Background. The result is based on $\sim 200$ hours of data from 8 polarization sensiti...
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Measuring quantum states: an experimental setup for measuring the spatial density matrix
To quantify the effect of decoherence in quantum measurements, it is desirable to measure not merely the square modulus of the spatial wavefunction, but the entire density matrix, whose phases carry i...
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What Are You Optimistic About?
First published in 2007...
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Combined multi-frequency map for point source substraction
A method is proposed for combining multi-frequency maps in order to produce a catalogue of extragalactic point sources using data from future high-precision satellite experiments. We have found the op...
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The best American science and nature writing 2004
First published in 2004...
View Book →Improved limits on gamma-ray burst repetition from BATSE
First published in 1996...
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Measuring the galaxy power spectrum with future redshift surveys
Precision measurements of the galaxy power spectrum P(k) require a data analysis pipeline that is both fast enough to be computationally feasible and accurate enough to take full advantage of high-qua...
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The Angular Power Spectrum of Galaxies from Early SDSS Data
We compute the angular power spectrum C_l from 1.5 million galaxies in early SDSS data on large angular scales, l...
View Book →¿Hay un Cisne Negro para Max Tegmark?
First published in 2022...
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Halo stochasticity in global clustering analysis
In the present work we study the statistics of haloes, which in the halo model determines the distribution of galaxies. Haloes are known to be biased tracer of dark matter, and at large scales it is u...
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Forecasting Cosmic Parameter Errors from Microwave Background Anisotropy Experiments
Accurate measurements of the cosmic microwave background (CMB) anisotropies with an angular resolution of a few arcminutes can be used to determine fundamental cosmological parameters such as the dens...
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Cosmology and the Halo Occupation Distribution from Small-Scale Galaxy Clustering in the Sloan Digit
We use the projected correlation function w_p(r_p) of a volume-limited subsample of the Sloan Digital Sky Survey (SDSS) main galaxy redshift catalogue to measure the halo occupation distribution (HOD)...
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Our Mathematical Universe Max Tegmark
Theoretical physics and cosmology...
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The angular power spectrum of BATSE 3B gamma-ray bursts
First published in 1996...
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Accelerating dark energy models with anisotropic fluid in Bianchi type-$VI_{0}$ space-time
Motivated by the increasing evidence for the need of a geometry that resembles Bianchi morphology to explain the observed anisotropy in the WMAP data, we have discussed some features of the Bianchi ty...
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Superhuman Brain Albert Einstein Galileo Galilei Isaac Newton Johannes Kepler And Stephen Hawking
Superhuman Brain Albert Einstein Galileo Galilei Isaac Newton Johannes Kepler and Stephen Hawking. Albert Einstein, the Nobel prize-winning physicist who gave the world the theory of relativity, E = m...
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