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Related papers: The weak anthropic principle and the landscape of …

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Anthropic arguments in multiverse cosmology and string theory rely on the weak anthropic principle (WAP). We show that the principle, though ultimately a tautology, is nevertheless ambiguous. It can be reformulated in one of two unambiguous…

High Energy Physics - Theory · Physics 2007-05-23 Steven Weinstein

In this lecture I make some educated guesses, about the landscape of string theory vacua. Based on the recent work of a number of authors, it seems plausible that the lanscape is unimaginably large and diverse. Whether we like it or not,…

High Energy Physics - Theory · Physics 2007-05-23 Leonard Susskind

I examine some non-anthropic approaches to the string landscape. These approaches are based on finding the initial conditions of the universe using the wavefunction of the multiverse to select the most probable vacuum out of this landscape.…

High Energy Physics - Theory · Physics 2008-11-26 Edward Tetteh-Lartey

Recent developments in string theory suggest that string theory landscape of vacua is vast. It is natural to ask if this landscape is as vast as allowed by consistent-looking effective field theories. We use universality ideas from string…

High Energy Physics - Theory · Physics 2007-05-23 Cumrun Vafa

We argue that the study of the statistics of the landscape of string vacua provides the first potentially predictive -- and also falsifiable -- framework for string theory. The question of whether the theory does or does not predict low…

High Energy Physics - Theory · Physics 2017-08-23 Michael Dine

After reviewing the cosmological constant problem - why is Lambda not huge? - I outline the two basic approaches that had emerged by the late 1980s, and note that each made a clear prediction. Precision cosmological experiments now indicate…

High Energy Physics - Theory · Physics 2007-05-23 Raphael Bousso

We revisit anthropic arguments purporting to explain the measured value of the cosmological constant. We argue that different ways of assigning probabilities to candidate universes lead to totally different anthropic predictions. As an…

Astrophysics · Physics 2007-07-23 Glenn D. Starkman , Roberto Trotta

This paper is a synthesis of talks I gave at the Cargese Workshop in June 2004 and the Munich Conference on Superstring Vacua in November 2004. I present arguments which show that the landscape of string theory is not a well established…

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

There is evidence that string theory possesses a large discretuum of stable and/or metastable ground states, with zero or four supersymmetries in four dimensions. I discuss critically the nature of this evidence. Assuming this "landscape"…

High Energy Physics - Theory · Physics 2017-08-23 Michael Dine

It is explained in detail why the Anthropic Principle (AP) cannot yield any falsifiable predictions, and therefore cannot be a part of science. Cases which have been claimed as successful predictions from the AP are shown to be not that.…

High Energy Physics - Theory · Physics 2007-05-23 Lee Smolin

Progress in string theory has resulted in a whole landscape of vacua solutions.In this talk I describe a proposal for exploring the cosmological implications of the landscape, based on the dynamics of the wavefunction of the universe…

High Energy Physics - Phenomenology · Physics 2009-11-11 Laura Mersini-Houghton

Selection effects in cosmology are often invoked to "explain" why some of the fundamental constant of Nature, and in particular the cosmological constant, take on the value they do in our Universe. We briefly review this probabilistic…

Astrophysics · Physics 2009-11-11 Roberto Trotta , Glenn D. Starkman

The anthropic principle implies that life can emerge and be sustained only in a narrow range of values of fundamental constants. Here we show that anthropic arguments can set powerful constraints on {\em transient} variations of the…

We argue that if string theory as an approach to the fundamental laws of physics is correct, then there is almost no room for anthropic arguments in cosmology. The quark and lepton masses and interaction strengths are determined.

Astrophysics · Physics 2009-10-31 Gordon L. Kane , Malcolm J. Perry , Anna N. Zytkow

We show that anthropic selection emerges inevitably in the general framework for prediction in quantum cosmology. There the predictions of anthropic reasoning depend on the prior implied by the universe's quantum state. To illustrate this…

Cosmology and Nongalactic Astrophysics · Physics 2013-12-16 James Hartle , Thomas Hertog

Identifying string theory vacua with desired physical properties at low energies requires searching through high-dimensional solution spaces - collectively referred to as the string landscape. We highlight that this search problem is…

High Energy Physics - Theory · Physics 2021-11-24 Alex Cole , Sven Krippendorf , Andreas Schachner , Gary Shiu

We review some basic flux vacua counting techniques and results, focusing on the distributions of properties over different regions of the landscape of string vacua and assessing the phenomenological implications. The topics we discuss…

High Energy Physics - Theory · Physics 2009-11-11 Jason Kumar

Superstring flux compactifications can stabilize all moduli while leading to an enormous number of vacua solutions, each leading to different $4-d$ laws of physics. While the string landscape provides at present the only plausible…

High Energy Physics - Phenomenology · Physics 2024-02-29 Howard Baer , Vernon Barger , Dakotah Martinez , Shadman Salam

We examine several issues pertaining to statistical predictivity of the string theory landscape for weak scale supersymmetry (SUSY). We work within a predictive landscape wherein super-renormalizable terms scan while renormalizable terms do…

High Energy Physics - Phenomenology · Physics 2020-10-21 Howard Baer , Vernon Barger , Shadman Salam , Dibyashree Sengupta

The usage of the anthropic principle in modern cosmology is reviewed. It is argued that its recent use to explain the observedvalues of cosmological parameters as most probable values for an ensemble of universes, is not justified. However,…

Astrophysics · Physics 2016-11-23 Berndt Müller
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