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Nova · Professor Researcher · re-ranking top 20…

Cumrun Vafa

· Chair, Department of Physics; Timken University Professor

Harvard University · Physics

Active 1984–2026

h-index143
Citations75.1k
Papers52077 last 5y
Funding$1.3M
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About

Cumrun Vafa is the Chair of the Department of Physics and the Timken University Professor at Harvard University, located at Jefferson Lab 467. His primary research area is string theory, a field that aims to develop a unified fundamental theory of nature. String theory seeks to describe all particles and forces within a single quantum framework, addressing phenomena across scales from subatomic to cosmological. Vafa's work involves building new mathematical tools to explore the implications of string theory, which intersects with fields such as mathematics, particle phenomenology, and astrophysics. Throughout his career, Vafa has contributed to various aspects of string theory, including topological strings, mirror symmetry, and the study of black holes, particularly the Bekenstein-Hawking entropy. He has worked on geometrically engineering quantum field theories, solving strong coupling dynamics of confining theories, and geometrizing string theory defects through F-theory. His recent research involves applying string theory concepts to predict the nature of dark energy and the fate of the universe. Vafa's work is characterized by its interdisciplinary nature and its focus on uncovering new laws of physics through advanced mathematical techniques.

Research topics

  • Philosophy
  • Theoretical physics
  • Physics
  • Theology
  • Astronomy

Selected publications

  • On the finiteness of 6d supergravity Landscape

    Journal of High Energy Physics · 2026-05-04 · 14 citations

    preprintOpen accessSenior author

    A bstract We consider supergravity theories with 8 supercharges in d = 6. We show that all the proposed anomaly free theories with unbounded number of massless modes are restricted to a finite subset and thus argue that there is an upper bound on the number of massless modes, consistent with the String Lamppost Principle.

  • Finite landscape of 6d N=(1,0) supergravity

    SciPost Physics · 2026-01-21 · 4 citations

    preprintOpen access

    We present a bottom-up argument showing that the number of massless fields in six-dimensional quantum gravitational theories with eight supercharges is uniformly bounded. Specifically, we show that the number of tensor multiplets is bounded by T≤ 193 <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"> <mml:mrow> <mml:mi>T</mml:mi> <mml:mo>≤</mml:mo> <mml:mn>193</mml:mn> </mml:mrow> </mml:math> , and the rank of the gauge group is restricted to r(V)≤ 480 <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"> <mml:mrow> <mml:mi>r</mml:mi> <mml:mo stretchy="false" form="prefix">(</mml:mo> <mml:mi>V</mml:mi> <mml:mo stretchy="false" form="postfix">)</mml:mo> <mml:mo>≤</mml:mo> <mml:mn>480</mml:mn> </mml:mrow> </mml:math> . Given that F-theory compactifications on elliptic CY 3-folds are a subset, this provides a bound on the Hodge numbers of elliptic CY 3-folds: h^{1,1}({\rm CY_3})≤ 491 , h^{1,1}({\rm Base})≤ 194 which are saturated by special elliptic CY 3-folds. This establishes that our bounds are sharp and also provides further evidence for the string lamppost principle. These results are derived by a comprehensive examination of the boundaries of the tensor moduli branch, showing that any consistent supergravity theory with T≠0 <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"> <mml:mrow> <mml:mi>T</mml:mi> <mml:mo>≠</mml:mo> <mml:mn>0</mml:mn> </mml:mrow> </mml:math> must include a BPS string in its spectrum corresponding to a “little string theory” (LST) or a critical heterotic string. From this tensor branch analysis, we establish a containment relationship between SCFTs and LSTs embedded within a gravitational theory. Combined with the classification of 6d SCFTs and LSTs, this then leads to the above bounds. Together with previous works, this establishes a bound on the number of massless fields in the supergravity for d≥ 6 <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"> <mml:mrow> <mml:mi>d</mml:mi> <mml:mo>≥</mml:mo> <mml:mn>6</mml:mn> </mml:mrow> </mml:math> .

  • On the Origin and Fate of Our Universe

    arXiv (Cornell University) · 2025-01-01

    preprintOpen access1st authorCorresponding

    This brief review, intended for high energy and astrophysics researchers, explores the implications of recent theoretical advances in string theory and the Swampland program for understanding bounds on the structure of positive potentials allowed in quantum gravity. This has a bearing on both inflationary models for the early universe as well as the fate of our universe. The paper includes a review of the dS conjecture as well as the TransPlanckian Censorship Conjecture (TCC) and its relation to the species scale. We provide evidence for these principles as well as what they may lead to in terms of phenomenological predictions. (Talk presented at Lemaitre Conference 2024)

  • Bounds on Discrete Gauge Symmetries in Supergravity

    arXiv (Cornell University) · 2025-11-12

    preprintOpen access

    We place bounds on the order of enhanced discrete gauge symmetries that act on massless fields and thus arise at subloci of the moduli space in supergravity theories. We focus on supersymmetric theories with 8 or more supercharges which in some cases lead to sharp upper bounds realized by specific string constructions.

  • Quasicrystalline string landscape

    Physical review. D/Physical review. D. · 2025-04-22 · 11 citations

    articleOpen accessSenior author

    In this work, we investigate a largely unexplored nongeometric corner of the string landscape: the quasicrystalline orbifolds. These exist at special points of the Narain moduli, leading to frozen moduli and large quantum symmetries. Here, we complete the classification and construction of quasicrystalline Narain lattices and use this to explore supersymmetric compactifications in <a:math xmlns:a="http://www.w3.org/1998/Math/MathML" display="inline"><a:mn>4</a:mn><a:mo>≤</a:mo><a:mi>D</a:mi><a:mo>≤</a:mo><a:mn>6</a:mn></a:math> and with <c:math xmlns:c="http://www.w3.org/1998/Math/MathML" display="inline"><c:mn>4</c:mn><c:mo>≤</c:mo><c:mi>Q</c:mi><c:mo>≤</c:mo><c:mn>16</c:mn></c:math> supercharges, leading to novel theories, including theories with large quantum symmetries at all points in the moduli space. We anticipate that these constructions will have many applications, and in subsequent work, we apply these techniques to construct new nonsupersymmetric tachyon-free models. Similarly, these constructions can lead to constructing exotic matter representations in the string landscape.

  • Neutrinos, B-L Symmetry and the Dark Dimension

    arXiv (Cornell University) · 2025-12-09

    preprintOpen access

    We consider realizations of a gauged B-L symmetry in the context of the Dark Dimension scenario, where the SM lives on a codimension one brane in 5d spacetime. The B-L can naturally be a bulk gauge symmetery leading to a global symmetry on the SM brane, and have its gauge anomaly canceled by charged bulk modes. This naturally leads to the existence of 3 right-handed neutrinos propagating in the dark dimension. Allowing for Higgsing of B-L by a bulk scalar at the Higgs scale, results in a massive gauge field with $m_{B-L}\sim 100$ GeV and weak coupling $g_{B-L}\sim 10^{-10}$ which is allowed by current bounds. The model also predicts a natural matching $m_ν\sim m_{KK}\simΛ^{1/4}$, thereby providing a theoretical explanation for the observed coincidence between neutrino masses and the Dark Energy scale. It also predicts a tower of sterile right-handed neutrinos in the $keV$ mass range.

  • Symmetries and M-theory-like Vacua in Four Dimensions

    ArXiv.org · 2025-03-20

    preprintOpen accessSenior author

    Non-geometric flux vacua have recently been revisited, leading to the remarkable discovery of isolated 4D ${\mathcal N}=1$ supersymmetric Minkowski vacua. These constructions rely on the non-renormalization of the superpotential, which is supported by heuristic arguments. Given the significance of verifying the existence of these isolated M-theory-like vacua, we present alternative symmetry-based arguments that arrive at the same conclusion. Additionally, we leverage these symmetries to argue for the existence of unstable dS solutions as well as supersymmetric AdS solutions.

  • On the origin and fate of our universe

    General Relativity and Gravitation · 2025-01-01 · 5 citations

    article1st authorCorresponding
  • Counting AdS Vacua

    ArXiv.org · 2025-12-03

    preprintOpen accessSenior author

    We study the 'number' $\mathfrak{N}(μ)$ of AdS vacua with a UV cut off $ μ$. It has been proposed that this number is finite. We find evidence that $\mathfrak{N}(μ)\sim a \ μ^{-b}$ as $μ\rightarrow 0$ for some constants $a$ and $b$ of $O(1)$ in Planck units that may depend on dimension and the number of supercharges. For this result to hold it is crucial to integrate over the volume of massless and tachyonic directions of AdS which corresponds to the volume of the space of marginal and relevant deformations of the dual CFT. We are led to the surprising prediction that theories with large number of light moduli contribute very little to the volume measure among all theories. We also speculate about the dS case leading to the number of quasi-dS vacua of the order of $Λ^{-α}$ for some $O(1)$ parameter $α$.

  • Dark dimension and the grand unification of forces

    Physical review. D/Physical review. D. · 2025-02-10 · 7 citations

    articleOpen access

    The dark dimension scenario, predicting one extra mesoscopic dimension in the micron range, has emerged by applying various swampland principles to the dark energy. In this note we find that realizing the grand unification of gauge forces is highly constraining in this context. Without actually constructing any grand unified theory (GUT) models, we argue that the mere assumption of grand unification of forces in this scenario, together with the experimental bounds on massive replicas of the Standard Model gauge bosons, predicts an upper bound for the GUT scale, <a:math xmlns:a="http://www.w3.org/1998/Math/MathML" display="inline"><a:msub><a:mi>M</a:mi><a:mi>GUT</a:mi></a:msub><a:mo>≲</a:mo><a:msup><a:mn>10</a:mn><a:mn>16</a:mn></a:msup><a:mtext> </a:mtext><a:mtext> </a:mtext><a:mi>GeV</a:mi></a:math>. Combined with the experimental bound on the proton lifetime, this predicts that the <c:math xmlns:c="http://www.w3.org/1998/Math/MathML" display="inline"><c:mi>X</c:mi></c:math> gauge boson mediating proton decay is a 5D solitonic string of Planckian tension stretched across a length scale <e:math xmlns:e="http://www.w3.org/1998/Math/MathML" display="inline"><e:mi>L</e:mi><e:mo>∼</e:mo><e:mo stretchy="false">(</e:mo><e:mn>1</e:mn><e:mi>–</e:mi><e:mn>10</e:mn><e:mtext> </e:mtext><e:mtext> </e:mtext><e:mi>TeV</e:mi><e:msup><e:mo stretchy="false">)</e:mo><e:mrow><e:mo>−</e:mo><e:mn>1</e:mn></e:mrow></e:msup></e:math> ending on gauge branes of the same diameter <i:math xmlns:i="http://www.w3.org/1998/Math/MathML" display="inline"><i:mo>∼</i:mo><i:mi>L</i:mi></i:math>. This leads to a mass of <k:math xmlns:k="http://www.w3.org/1998/Math/MathML" display="inline"><k:msub><k:mi>M</k:mi><k:mi>X</k:mi></k:msub><k:mo>∼</k:mo><k:msup><k:mn>10</k:mn><k:mn>15</k:mn></k:msup><k:mi>–</k:mi><k:msup><k:mn>10</k:mn><k:mn>16</k:mn></k:msup><k:mtext> </k:mtext><k:mtext> </k:mtext><k:mi>GeV</k:mi></k:math>. In particular assuming grand unification in the dark dimension scenario results in a tower of Kaluza-Klein excitations of Standard Model gauge bosons on the gauge branes in the 1–10 TeV range. This suggests that the diameter/separation <m:math xmlns:m="http://www.w3.org/1998/Math/MathML" display="inline"><m:mi>L</m:mi></m:math> of the gauge branes correlates with both the weak scale <o:math xmlns:o="http://www.w3.org/1998/Math/MathML" display="inline"><o:mo>∼</o:mo><o:mn>1</o:mn><o:mo>/</o:mo><o:mi>L</o:mi></o:math> near a TeV the GUT scale <q:math xmlns:q="http://www.w3.org/1998/Math/MathML" display="inline"><q:mo>∼</q:mo><q:msubsup><q:mi>M</q:mi><q:mn>5</q:mn><q:mn>2</q:mn></q:msubsup><q:mi>L</q:mi></q:math> at <s:math xmlns:s="http://www.w3.org/1998/Math/MathML" display="inline"><s:msup><s:mn>10</s:mn><s:mn>16</s:mn></s:msup><s:mtext> </s:mtext><s:mtext> </s:mtext><s:mi>GeV</s:mi></s:math>.

Recent grants

Frequent coauthors

  • Hirosi Ooguri

    The University of Tokyo

    73 shared
  • Mina Aganagic

    57 shared
  • Jonathan J. Heckman

    43 shared
  • Sergio Cecotti

    Beijing Institute of Mathematical Sciences and Applications

    40 shared
  • Sheldon Katz

    University of Illinois Urbana-Champaign

    29 shared
  • Albrecht Klemm

    29 shared
  • Robbert Dijkgraaf

    27 shared
  • Masahito Yamazaki

    The University of Tokyo

    26 shared

Education

  • Ph.D., Mathematics

    Princeton University

    1984
  • B.A., Mathematics

    Harvard University

    1979
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