Yuhsin Tsai
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View article: A cosmological case study of a tower of warm dark matter states: Nnaturalness
A cosmological case study of a tower of warm dark matter states: Nnaturalness Open
In this work, we study the cosmological effects of a tower of warm dark matter states on the cosmic microwave background (CMB) and on large-scale structure (LSS). For concreteness, we consider the Nnaturalness model, which is a proposed me…
View article: Feebly Interacting Particles: FIPs at LHCb
Feebly Interacting Particles: FIPs at LHCb Open
With the establishment and maturation of the experimental programs searching for new physics with sizeable couplings at the LHC, there is an increasing interest in the broader particle and astrophysics community for exploring the physics o…
View article: Boiling After the Dust Settles: Constraining First-Order Phase Transitions During Dark Energy Domination
Boiling After the Dust Settles: Constraining First-Order Phase Transitions During Dark Energy Domination Open
A first-order phase transition could occur in the late universe when vacuum energy begins dominating the energy density ($z \lesssim 0.3$) and convert some latent heat into other forms such as invisible radiation. This generic possibility …
View article: MATHUSLA: An External Long-Lived Particle Detector to Maximize the Discovery Potential of the HL-LHC
MATHUSLA: An External Long-Lived Particle Detector to Maximize the Discovery Potential of the HL-LHC Open
We present the current status of the MATHUSLA (MAssive Timing Hodoscope for Ultra-Stable neutraL pArticles) long-lived particle (LLP) detector at the HL-LHC, covering the design, fabrication and installation at CERN Point 5. MATHUSLA40 is …
View article: Conceptual Design Report for the MATHUSLA Long-Lived Particle Detector near CMS
Conceptual Design Report for the MATHUSLA Long-Lived Particle Detector near CMS Open
We present the Conceptual Design Report (CDR) for the MATHUSLA (MAssive Timing Hodoscope for Ultra-Stable neutraL pArticles) long-lived particle detector at the HL-LHC, covering the design, fabrication and installation at CERN Point 5. MAT…
View article: Echoes of Self-Interacting Dark Matter from Binary Black Hole Mergers
Echoes of Self-Interacting Dark Matter from Binary Black Hole Mergers Open
Dark matter (DM) environments around black holes (BHs) can influence their mergers through dynamical friction, causing gravitational wave (GW) dephasing during the inspiral phase. While this effect is well studied for collisionless dark ma…
View article: Light in the shadows: primordial black holes making dark matter shine
Light in the shadows: primordial black holes making dark matter shine Open
View article: Dark matter-radiation scattering enhances CMB phase shift through dark matter-loading
Dark matter-radiation scattering enhances CMB phase shift through dark matter-loading Open
A phase shift in the acoustic oscillations of cosmic microwave background (CMB) spectra is a characteristic signature for the presence of non-photon radiation propagating differently from photons, even when the radiation couples to the Sta…
View article: The Sound of Dark Sectors in Pulsar Timing Arrays
The Sound of Dark Sectors in Pulsar Timing Arrays Open
A phase transition in the dark sector (DS) presents a promising explanation for the stochastic gravitational wave (GW) signals detected in recent observations by Pulsar Timing Arrays (PTAs). Instead of focusing solely on fitting data with …
View article: Detector-size upper bounds on dark hadron lifetime from cosmology
Detector-size upper bounds on dark hadron lifetime from cosmology Open
We show that in a confining hidden valley model where the lightest hidden particles are dark hadrons that have mass splittings larger than \\( \\mathcal{O}(0.1) \\) GeV, if the lightest dark hadron is either stable or decays i…
View article: Finite Bubble Statistics Constrain Late Cosmological Phase Transitions
Finite Bubble Statistics Constrain Late Cosmological Phase Transitions Open
We consider first order cosmological phase transitions (PTs) happening at late times below standard model temperatures TPT≲GeV. The inherently stochastic nature of bubble nucleation and the finite number of bubbles associated with a late-t…
View article: Hawking radiation of nonrelativistic scalars: applications to pion and axion production
Hawking radiation of nonrelativistic scalars: applications to pion and axion production Open
A bstract In studying secondary gamma-ray emissions from Primordial Black Holes (PBHs), the production of scalar particles like pions and axion-like particles (ALPs) via Hawking radiation is crucial. While previous analyses assumed relativ…
View article: Observable CMB B-modes from Cosmological Phase Transitions
Observable CMB B-modes from Cosmological Phase Transitions Open
A B-mode polarization signal in the cosmic microwave background (CMB) is widely regarded as smoking gun evidence for gravitational waves produced during inflation. Here we demonstrate that tensor perturbations from a cosmological phase tra…
View article: Biomarker potential of nuclear Nrf2 activation in the ABC subtype of diffuse large B‑cell lymphoma
Biomarker potential of nuclear Nrf2 activation in the ABC subtype of diffuse large B‑cell lymphoma Open
Diffuse large B-cell lymphoma (DLBCL) is an aggressive B-cell lymphoma characterized by distinct subtypes and heterogeneous treatment outcomes. Oxidative stress and the dysregulation of related regulatory genes are prevalent in DLBCL, prom…
View article: A cosmological case study of a tower of warm dark matter states: $N$naturalness
A cosmological case study of a tower of warm dark matter states: $N$naturalness Open
In this work, we study the cosmological effects of a tower of warm dark matter states on the cosmic microwave background (CMB) and on large-scale structure (LSS). For concreteness, we consider the $N$naturalness model, which is a proposed …
View article: Hawking Radiation of Nonrelativistic Scalars: Applications to Pion and Axion Production
Hawking Radiation of Nonrelativistic Scalars: Applications to Pion and Axion Production Open
In studying secondary gamma-ray emissions from Primordial Black Holes (PBHs), the production of scalar particles like pions and axion-like particles (ALPs) via Hawking radiation is crucial. While previous analyses assumed relativistic prod…
View article: Dark Matter-Radiation Scattering Enhances CMB Phase Shift through Dark Matter-loading
Dark Matter-Radiation Scattering Enhances CMB Phase Shift through Dark Matter-loading Open
A phase shift in the acoustic oscillations of CMB spectra is a characteristic signature for the presence of non-photon radiation propagating differently from photons, even when the radiation couples to SM particles solely gravitationally. …
View article: Challenges in interpreting the NANOGrav 15-year dataset as early Universe gravitational waves produced by an ALP induced instability
Challenges in interpreting the NANOGrav 15-year dataset as early Universe gravitational waves produced by an ALP induced instability Open
In this paper, we study a possible early universe source for the recent observation of a stochastic gravitational wave background at the NANOGrav pulsar timing array. The source is a tachyonic instability in a dark gauge field induced by a…
View article: Finite Bubble Statistics Constrain Late Cosmological Phase Transitions
Finite Bubble Statistics Constrain Late Cosmological Phase Transitions Open
We consider first order cosmological phase transitions (PT) happening at late times, below Standard Model (SM) temperatures $T_{\rm PT} \lesssim$ GeV. The inherently stochastic nature of bubble nucleation and the finite number of bubbles a…
View article: Precision cosmological constraints on atomic dark matter
Precision cosmological constraints on atomic dark matter Open
A bstract Atomic dark matter is a simple but highly theoretically motivated possibility for an interacting dark sector that could constitute some or all of dark matter. We perform a comprehensive study of precision cosmological observables…
View article: Unraveling cosmological anisotropies within stochastic gravitational wave backgrounds
Unraveling cosmological anisotropies within stochastic gravitational wave backgrounds Open
Identifying the anisotropies in a cosmologically sourced stochastic gravitational wave background (SGWB) would be of significance in shedding light on the nature of primordial inhomogeneities. For example, if SGWB carries isocurvature fluc…
View article: Probing cosmological particle production and pairwise hotspots with deep neural networks
Probing cosmological particle production and pairwise hotspots with deep neural networks Open
Particles with masses much larger than the inflationary Hubble scale, ${H}_{I}$, can be pair-produced nonadiabatically during inflation. Due to their large masses, the produced particles modify the curvature perturbation around their locat…
View article: High G9a Expression in DLBCL and Its Inhibition by Niclosamide to Induce Autophagy as a Therapeutic Approach
High G9a Expression in DLBCL and Its Inhibition by Niclosamide to Induce Autophagy as a Therapeutic Approach Open
Background: Diffuse large B-cell lymphoma (DLBCL) is a malignant lymphoid tumor disease that is characterized by heterogeneity, but current treatment does not benefit all patients, which highlights the need to identify oncogenic genes and …
View article: Unraveling Cosmological Anisotropies within Stochastic Gravitational Wave Backgrounds
Unraveling Cosmological Anisotropies within Stochastic Gravitational Wave Backgrounds Open
Identifying the anisotropies in a cosmologically sourced stochastic gravitational wave background (SGWB) would be of significance in shedding light on the nature of primordial inhomogeneities. For example, if SGWB carries isocurvature fluc…
View article: Detecting axionlike particles with primordial black holes
Detecting axionlike particles with primordial black holes Open
Future gamma-ray experiments, such as the e-ASTROGAM and AMEGO telescopes, can detect the Hawking radiation of photons from primordial black holes (PBHs) if they make up a fraction or all of dark matter. PBHs can analogously also Hawking r…
View article: Challenges in Interpreting the NANOGrav 15-Year Data Set as Early Universe Gravitational Waves Produced by ALP Induced Instability
Challenges in Interpreting the NANOGrav 15-Year Data Set as Early Universe Gravitational Waves Produced by ALP Induced Instability Open
In this paper, we study a possible early universe source for the recent observation of a stochastic gravitational wave background at the NANOGrav pulsar timing array. The source is a tachyonic instability in a dark gauge field induced by a…
View article: Displaced lepton jet signatures from self-interacting dark matter bound states
Displaced lepton jet signatures from self-interacting dark matter bound states Open
We study self-interacting dark matter signatures at the Large Hadron Collider. A light dark photon, mediating dark matter self-interactions, can bind dark matter particles to form a bound state when they are produced via a heavy pseduoscal…
View article: Exploring Mirror Twin Higgs Cosmology with Present and Future Weak Lensing Surveys
Exploring Mirror Twin Higgs Cosmology with Present and Future Weak Lensing Surveys Open
We explore the potential of precision cosmological data to study non-minimal dark sectors by updating the cosmological constraint on the mirror twin Higgs model (MTH). The MTH model addresses the Higgs little hierarchy problem by introduci…
View article: Probing Cosmological Particle Production and Pairwise Hotspots with Deep Neural Networks
Probing Cosmological Particle Production and Pairwise Hotspots with Deep Neural Networks Open
Particles with masses much larger than the inflationary Hubble scale, $H_I$, can be pair-produced non-adiabatically during inflation. Due to their large masses, the produced particles modify the curvature perturbation around their location…
View article: Improved cosmological constraints on the neutrino mass and lifetime
Improved cosmological constraints on the neutrino mass and lifetime Open
We present cosmological constraints on the sum of neutrino masses as a function of the neutrino lifetime, in a framework in which neutrinos decay into dark radiation after becoming non-relativistic. We find that in this regime the cosmic m…