4.4 Article

Large-scale structure observables in general relativity

Journal

CLASSICAL AND QUANTUM GRAVITY
Volume 32, Issue 4, Pages -

Publisher

IOP PUBLISHING LTD
DOI: 10.1088/0264-9381/32/4/044001

Keywords

large-scale structure; galaxy clustering; weak gravitational lensing

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We review recent studies that rigorously define several key observables of the large-scale structure of the Universe in a general relativistic context. Specifically, we consider (i) redshift perturbation of cosmic clock events; (ii) distortion of cosmic rulers, including weak lensing shear and magnification; and (iii) observed number density of tracers of the large-scale structure. We provide covariant and gauge-invariant expressions of these observables. Our expressions are given for a linearly perturbed flat Friedmann-Robertson-Walker metric including scalar, vector, and tensor metric perturbations. While we restrict ourselves to linear order in perturbation theory, the approach can be straightforwardly generalized to higher order.

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Mavalvala, J. J. McCann, R. McCarthy, D. E. McClelland, P. K. McClincy, S. McCormick, L. McCuller, G. I. McGhee, S. C. McGuire, C. McIsaac, J. McIver, T. McRae, S. T. McWilliams, D. Meacher, M. Mehmet, A. K. Mehta, Q. Meijer, A. Melatos, D. A. Melchor, G. Mendell, A. Menendez-Vazquez, C. S. Menoni, R. A. Mercer, L. Mereni, K. Merfeld, E. L. Merilh, J. D. Merritt, M. Merzougui, S. Meshkov, C. Messenger, C. Messick, P. M. Meyers, F. Meylahn, A. Mhaske, A. Miani, H. Miao, I. Michaloliakos, C. Michel, Y. Michimura, H. Middleton, D. P. Mihaylov, L. Milano, A. L. Miller, A. Miller, B. Miller, M. Millhouse, J. C. Mills, E. Milotti, Y. Minenkov, N. Mio, Ll. M. Mir, M. Miravet-Tenes, A. Mishkin, C. Mishra, T. Mishra, T. Mistry, S. Mitra, V. P. Mitrofanov, G. Mitselmakher, R. Mittleman, O. Miyakawa, K. Miyo, S. Miyoki, Geoffrey Mo, L. M. Modafferi, E. Moguel, K. Mogushi, S. R. P. Mohapatra, S. R. Mohite, I. Molina, M. Molina-Ruiz, M. Mondin, M. Montani, C. J. Moore, J. Moragues, D. Moraru, F. Morawski, A. More, C. Moreno, G. Moreno, Y. Mori, S. Morisaki, N. Morisue, Y. Moriwaki, B. Mours, C. M. Mow-Lowry, S. Mozzon, F. Muciaccia, Arunava Mukherjee, D. Mukherjee, Soma Mukherjee, Subroto Mukherjee, Suvodip Mukherjee, N. Mukund, A. Mullavey, J. Munch, E. A. Muniz, P. G. Murray, R. Musenich, S. Muusse, S. L. Nadji, K. Nagano, A. Nagar, K. Nakamura, H. Nakano, M. Nakano, Y. Nakayama, V. Napolano, I. Nardecchia, T. Narikawa, H. Narola, L. Naticchioni, B. Nayak, R. K. Nayak, B. F. Neil, J. Neilson, A. Nelson, T. J. N. Nelson, M. Nery, P. Neubauer, A. Neunzert, K. Y. Ng, S. W. S. Ng, C. Nguyen, P. Nguyen, T. Nguyen, L. Nguyen Quynh, J. Ni, W. -T. Ni, S. A. Nichols, T. Nishimoto, A. Nishizawa, S. Nissanke, E. Nitoglia, F. Nocera, M. Norman, C. North, S. Nozaki, G. Nurbek, L. K. Nuttall, Y. Obayashi, J. Oberling, B. D. O'Brien, J. O'Dell, E. Oelker, W. Ogaki, G. Oganesyan, J. J. Oh, K. Oh, S. H. Oh, M. Ohashi, T. Ohashi, M. Ohkawa, F. Ohme, H. Ohta, M. A. Okada, Y. Okutani, C. Olivetto, K. Oohara, R. Oram, B. O'Reilly, R. G. Ormiston, N. D. Ormsby, R. O'Shaughnessy, E. O'Shea, S. Oshino, S. Ossokine, C. Osthelder, S. Otabe, D. J. Ottaway, H. Overmier, A. E. Pace, G. Pagano, R. Pagano, M. A. Page, G. Pagliaroli, A. Pai, S. A. Pai, S. Pal, J. R. Palamos, O. Palashov, C. Palomba, H. Pan, K. -C. Pan, P. K. Panda, P. T. H. Pang, C. Pankow, F. Pannarale, B. C. Pant, F. H. Panther, F. Paoletti, A. Paoli, A. Paolone, G. Pappas, A. Parisi, H. Park, J. Park, W. Parker, D. Pascucci, A. Pasqualetti, R. Passaquieti, D. Passuello, M. Patel, M. Pathak, B. Patricelli, A. S. Patron, S. Paul, E. Payne, M. Pedraza, R. Pedurand, M. Pegoraro, A. Pele, F. E. Pena Arellano, S. Penano, S. Penn, A. Perego, A. Pereira, T. Pereira, C. J. Perez, C. Perigois, C. C. Perkins, A. Perreca, S. Perries, D. Pesios, J. Petermann, D. Petterson, H. P. Pfeiffer, H. Pham, K. A. Pham, K. S. Phukon, H. Phurailatpam, O. J. Piccinni, M. Pichot, M. Piendibene, F. Piergiovanni, L. Pierini, V. Pierro, G. Pillant, M. Pillas, F. Pilo, L. Pinard, C. Pineda-Bosque, I. M. Pinto, M. Pinto, B. J. Piotrzkowski, K. Piotrzkowski, M. Pirello, M. D. Pitkin, A. Placidi, E. Placidi, M. L. Planas, W. Plastino, C. Pluchar, R. Poggiani, E. Polini, D. Y. T. Pong, S. Ponrathnam, E. K. Porter, R. Poulton, A. Poverman, J. Powell, M. Pracchia, T. Pradier, A. K. Prajapati, K. Prasai, R. Prasanna, G. Pratten, M. Principe, G. A. Prodi, L. Prokhorov, P. Prosposito, L. Prudenzi, A. Puecher, M. Punturo, F. Puosi, P. Puppo, M. Puerrer, H. Qi, N. Quartey, V. Quetschke, P. J. Quinonez, R. Quitzow-James, F. J. Raab, G. Raaijmakers, H. Radkins, N. Radulesco, P. Raffai, S. X. Rail, S. Raja, C. Rajan, K. E. Ramirez, T. D. Ramirez, A. Ramos-Buades, J. Rana, P. Rapagnani, A. Ray, V. Raymond, N. Raza, M. Razzano, J. Read, L. A. Rees, T. Regimbau, L. Rei, S. Reid, S. W. Reid, D. H. Reitze, P. Relton, A. Renzini, P. Rettegno, B. Revenu, A. Reza, M. Rezac, F. Ricci, D. Richards, J. W. Richardson, L. Richardson, G. Riemenschneider, K. Riles, S. Rinaldi, K. Rink, N. A. Robertson, R. Robie, F. Robinet, A. Rocchi, S. Rodriguez, L. Rolland, J. G. Rollins, M. Romanelli, R. Romano, C. L. Romel, A. Romero, I. M. Romero-Shaw, J. H. Romie, S. Ronchini, L. Rosa, C. A. Rose, D. Rosinska, M. P. Ross, S. Rowan, S. J. Rowlinson, S. Roy, Santosh Roy, Soumen Roy, D. Rozza, P. Ruggi, K. Ruiz-Rocha, K. Ryan, S. Sachdev, T. Sadecki, J. Sadiq, S. Saha, Y. Saito, K. Sakai, M. Sakellariadou, S. Sakon, O. S. Salafia, F. Salces-Carcoba, L. Salconi, M. Saleem, F. Salemi, A. Samajdar, E. J. Sanchez, J. H. Sanchez, L. E. Sanchez, N. Sanchis-Gual, J. R. Sanders, A. Sanuy, T. R. Saravanan, N. Sarin, B. Sassolas, H. Satari, B. S. Sathyaprakash, O. Sauter, R. L. Savage, V. Savant, T. Sawada, H. L. Sawant, S. Sayah, D. Schaetzl, M. Scheel, J. Scheuer, M. G. Schiworski, P. Schmidt, S. Schmidt, R. Schnabel, M. Schneewind, R. M. S. Schofield, A. Schoenbeck, B. W. Schulte, B. F. Schutz, E. Schwartz, J. Scott, S. M. Scott, M. Seglar-Arroyo, Y. Sekiguchi, D. Sellers, A. S. Sengupta, D. Sentenac, E. G. Seo, V. Sequino, A. Sergeev, Y. Setyawati, T. Shaffer, M. S. Shahriar, M. A. Shaikh, B. Shams, L. Shao, A. Sharma, P. Sharma, P. Shawhan, N. S. Shcheblanov, A. Sheela, Y. Shikano, M. Shikauchi, H. Shimizu, K. Shimode, H. Shinkai, T. Shishido, A. Shoda, D. H. Shoemaker, D. M. Shoemaker, S. ShyamSundar, M. Sieniawska, D. Sigg, L. Silenzi, L. P. Singer, D. Singh, M. K. Singh, N. Singh, A. Singha, A. M. Sintes, V. Sipala, V. Skliris, B. J. J. Slagmolen, T. J. Slaven-Blair, J. Smetana, J. R. Smith, L. Smith, R. J. E. Smith, J. Soldateschi, S. N. Somala, K. Somiya, I. Song, K. Soni, V. Sordini, F. Sorrentino, N. Sorrentino, R. Soulard, T. Souradeep, E. Sowell, V. Spagnuolo, A. P. Spencer, M. Spera, P. Spinicelli, A. K. Srivastava, V. Srivastava, K. Staats, C. Stachie, F. Stachurski, D. A. Steer, J. Steinlechner, S. Steinlechner, N. Stergioulas, D. J. Stops, M. Stover, K. A. Strain, L. C. Strang, G. Stratta, M. D. Strong, A. Strunk, R. Sturani, A. L. Stuver, M. Suchenek, S. Sudhagar, V. Sudhir, R. Sugimoto, H. G. Suh, A. G. Sullivan, T. Z. Summerscales, L. Sun, S. Sunil, A. Sur, J. Suresh, P. J. Sutton, Takamasa Suzuki, Takanori Suzuki, Toshikazu Suzuki, B. L. Swinkels, M. J. Szczepanczyk, P. Szewczyk, M. Tacca, H. Tagoshi, S. C. Tait, H. Takahashi, R. Takahashi, S. Takano, H. Takeda, M. Takeda, C. J. Talbot, C. Talbot, K. Tanaka, Taiki Tanaka, Takahiro Tanaka, A. J. Tanasijczuk, S. Tanioka, D. B. Tanner, D. Tao, L. Tao, R. D. Tapia, E. N. Tapia San Martin, C. Taranto, A. Taruya, J. D. Tasson, R. Tenorio, J. E. S. Terhune, L. Terkowski, M. P. Thirugnanasambandam, M. Thomas, P. Thomas, E. E. Thompson, J. E. Thompson, S. R. Thondapu, K. A. Thorne, E. Thrane, Shubhanshu Tiwari, Srishti Tiwari, V. Tiwari, A. M. Toivonen, A. E. Tolley, T. Tomaru, T. Tomura, M. Tonelli, Z. Tornasi, A. Torres-Forne, C. I. Torrie, I. Tosta e Melo, D. Toyra, A. Trapananti, F. Travasso, G. Traylor, M. Trevor, M. C. Tringali, A. Tripathee, L. Troiano, A. Trovato, L. Trozzo, R. J. Trudeau, D. Tsai, K. W. Tsang, T. Tsang, J-S. Tsao, M. Tse, R. Tso, S. Tsuchida, L. Tsukada, D. Tsuna, T. Tsutsui, K. Turbang, M. Turconi, D. Tuyenbayev, A. S. Ubhi, N. Uchikata, T. Uchiyama, R. P. Udall, A. Ueda, T. Uehara, K. Ueno, G. Ueshima, C. S. Unnikrishnan, A. L. Urban, T. Ushiba, A. Utina, G. Vajente, A. Vajpeyi, G. Valdes, M. Valentini, V. Valsan, N. van Bakel, M. van Beuzekom, M. van Dael, J. F. J. van den Brand, C. Van den Broeck, D. C. Vander-Hyde, H. van Haevermaet, J. V. van Heijningen, M. H. P. M. van Putten, N. van Remortel, M. Vardaro, A. F. Vargas, V. Varma, M. Vasuth, A. Vecchio, G. Vedovato, J. Veitch, P. J. Veitch, J. Venneberg, G. Venugopalan, D. Verkindt, P. Verma, Y. Verma, S. M. Vermeulen, D. Veske, F. Vetrano, A. Vicere, S. Vidyant, A. D. Viets, A. Vijaykumar, V. Villa-Ortega, J. -Y. Vinet, A. Virtuoso, S. Vitale, H. Vocca, E. R. G. von Reis, J. S. A. von Wrangel, C. Vorvick, S. P. Vyatchanin, L. E. Wade, M. Wade, K. J. Wagner, R. C. Walet, M. Walker, G. S. Wallace, L. Wallace, J. Wang, J. Z. Wang, W. H. Wang, R. L. Ward, J. Warner, M. Was, T. Washimi, N. Y. Washington, J. Watchi, B. Weaver, C. R. Weaving, S. A. Webster, M. Weinert, A. J. Weinstein, R. Weiss, C. M. Weller, R. A. Weller, F. Wellmann, L. Wen, P. Wessels, K. Wette, J. T. Whelan, D. D. White, B. F. Whiting, C. Whittle, D. Wilken, D. Williams, M. J. Williams, A. R. Williamson, J. L. Willis, B. Willke, D. J. Wilson, C. C. Wipf, T. Wlodarczyk, G. Woan, J. Woehler, J. K. Wofford, D. Wong, I. C. F. Wong, M. Wright, C. Wu, D. S. Wu, H. Wu, D. M. Wysocki, L. Xiao, T. Yamada, H. Yamamoto, K. Yamamoto, T. Yamamoto, K. Yamashita, R. Yamazaki, F. W. Yang, K. Z. Yang, L. Yang, Y. -C. Yang, Y. Yang, Yang Yang, M. J. Yap, D. W. Yeeles, S. -W. Yeh, A. B. Yelikar, M. Ying, J. Yokoyama, T. Yokozawa, J. Yoo, T. Yoshioka, Hang Yu, Haocun Yu, H. Yuzurihara, A. Zadrozny, M. Zanolin, S. Zeidler, T. Zelenova, J. -P. Zendri, M. Zevin, M. Zhan, H. Zhang, J. Zhang, L. Zhang, R. Zhang, T. Zhang, Y. Zhang, C. Zhao, G. Zhao, Y. Zhao, Yue Zhao, R. Zhou, Z. Zhou, X. J. Zhu, Z. -H. Zhu, A. B. Zimmerman, M. E. Zucker, J. Zweizig

Summary: This study reports on a search for compact binary coalescences with at least one component having a mass between 0.2 M-sun and 1.0 M-sun using data from Advanced LIGO and Advanced Virgo, finding no gravitational-wave candidates. Astrophysical constraints are derived on two models that could produce subsolar-mass compact objects, revealing potential for subsolar-mass black holes and suggesting new limits on the fraction of dark matter in such objects. The study represents the first constraints placed on dissipative dark matter models through subsolar-mass analyses.

PHYSICAL REVIEW LETTERS (2022)

Article Astronomy & Astrophysics

Formation and Morphology of the First Galaxies in the Cosmic Morning

Changbom Park, Jaehyun Lee, Juhan Kim, Donghui Jeong, Christophe Pichon, Brad K. Gibson, Owain N. Snaith, Jihye Shin, Yonghwi Kim, Yohan Dubois, C. Gareth Few

Summary: We investigate the formation and morphological evolution of the first galaxies in the cosmic morning using the HR5 simulation. We find that disk-type morphology dominates in the cosmic morning, with almost all first galaxies forming at initial peaks of the matter-density field. The cosmic web of galaxies forms at lower redshifts when most rhizomes globally percolate.

ASTROPHYSICAL JOURNAL (2022)

Article Astronomy & Astrophysics

A Lower Bound on the Mass of Compact Objects from Dissipative Dark Matter

James Gurian, Michael Ryan, Sarah Schon, Donghui Jeong, Sarah Shandera

Summary: This study investigates the fragmentation scale of dark gas formed in dissipative dark-matter halos and presents a simple model consistent with current observations. The results indicate that a significant portion of the parameter space is highly unstable to small-scale fragmentation.

ASTROPHYSICAL JOURNAL LETTERS (2022)

Article Astronomy & Astrophysics

HETDEX Public Source Catalog 1: 220 K Sources Including Over 50 K Lya Emitters from an Untargeted Wide-area Spectroscopic Survey

Erin Mentuch Cooper, Karl Gebhardt, Dustin Davis, Daniel J. J. Farrow, Chenxu Liu, Gregory Zeimann, Robin Ciardullo, John J. J. Feldmeier, Niv Drory, Donghui Jeong, Barbara Benda, William P. P. Bowman, Michael Boylan-Kolchin, Oscar A. Chavez Ortiz, Maya H. H. Debski, Mona Dentler, Maximilian Fabricius, Rameen Farooq, Steven L. L. Finkelstein, Eric Gawiser, Caryl Gronwall, Gary J. J. Hill, Ulrich Hopp, Lindsay R. R. House, Steven Janowiecki, Hasti Khoraminezhad, Wolfram Kollatschny, Eiichiro Komatsu, Martin Landriau, Maja Lujan Niemeyer, Hanshin Lee, Phillip MacQueen, Ken Mawatari, Brianna McKay, Masami Ouchi, Jennifer Poppe, Shun Saito, Donald P. P. Schneider, Jan Snigula, Benjamin P. P. Thomas, Sarah Tuttle, Tanya Urrutia, Laurel Weiss, Lutz Wisotzki, Yechi Zhang

Summary: We release the first catalog of sources obtained from the Hobby-Eberly Telescope Dark Energy Experiment (HETDEX), which is a spectroscopic survey designed to measure the Hubble expansion parameter and angular diameter distance. The catalog includes a large number of Ly alpha-emitting galaxies and [O ii]-emitting galaxies, as well as stars, low-redshift galaxies, and active galactic nuclei. It provides comprehensive information on the identified sources, including coordinates, redshifts, line identifications, classification information, line fluxes, and spectra.

ASTROPHYSICAL JOURNAL (2023)

Article Astronomy & Astrophysics

Using Dark Energy Explorers and Machine Learning to Enhance the Hobby-Eberly Telescope Dark Energy Experiment

Lindsay R. House, Karl Gebhardt, Keely Finkelstein, Erin Mentuch Cooper, Dustin Davis, Robin Ciardullo, Daniel J. Farrow, Steven L. Finkelstein, Caryl Gronwall, Donghui Jeong, L. Clifton Johnson, Chenxu Liu, Benjamin P. Thomas, Gregory Zeimann

Summary: This study analyzes how to enhance cosmological measurements of HETDEX using a citizen science campaign. The Dark Energy Explorers project aims to increase the number of LAEs, reduce false positives caused by noise and [O ii] galaxies. Initial analysis shows that citizen science, combined with unsupervised machine learning, is an efficient tool for accurate classification. The three most impactful aspects of the citizen science campaign are identifying detection problems, providing a clean sample for visual identification, and providing labels for machine learning efforts. Dark Energy Explorers has collected over three and a half million classifications from 11,000 volunteers in 85 countries worldwide. By incorporating the results of Dark Energy Explorers, a 10%-30% improvement in the accuracy of D(A)(z) and H(z) parameters at z=2.4 is expected. While the main goal is to enhance HETDEX, Dark Energy Explorers has already proven to be a uniquely powerful tool for scientific advancement and global accessibility to science.

ASTROPHYSICAL JOURNAL (2023)

Article Astronomy & Astrophysics

Perturbation theory remixed: Improved nonlinearity modeling beyond standard perturbation theory

Zhenyuan Wang, Donghui Jeong, Atsushi Taruya, Takahiro Nishimichi, Ken Osato

Summary: We propose a novel nEPT scheme that models the nonlinear density field by summing up to nth-order density fields in perturbation theory. The analytical power spectrum obtained shows excellent agreement with results from 20 Dark-Quest N-body simulations across a wide range of cosmologies. This method can accelerate the forward modeling of the nonlinear cosmological density field, which is an essential probe of cosmic mysteries such as inflation, dark energy, and dark matter.

PHYSICAL REVIEW D (2023)

Article Astronomy & Astrophysics

Grid-based calculations of redshift-space matter fluctuations from perturbation theory: UV sensitivity and convergence at the field level

Atsushi Taruya, Takahiro Nishimichi, Donghui Jeong

Summary: Perturbation theory is used to interpret the observed nonlinear large-scale structure statistics in the quasilinear regime. The GridSPT algorithm is presented as a grid-based method to compute the nonlinear density and velocity fields in standard perturbation theory. Redshift-space distortions are taken into account in the analysis. The results show that the SPT calculation is more sensitive to UV sensitivity and deviates from N-body results below a certain Fourier wave number.

PHYSICAL REVIEW D (2022)

Article Astronomy & Astrophysics

Gauge-invariant tensor perturbations induced from baryon-CDM relative velocity and the B-mode polarization of the CMB

James Gurian, Donghui Jeong, Jai-chan Hwang, Hyerim Noh

Summary: This study examines the gauge dependence of induced gravitational waves (IGWs) from scalar perturbations and calculates the gravitational wave power spectrum and expected angular power spectrum of B-mode polarization of the cosmic microwave background using relative velocity perturbations. The results show a negligible effect, highlighting the importance of using observable quantities to remove gauge ambiguity and demonstrating the observable consequences of tensor perturbations.

PHYSICAL REVIEW D (2021)

Article Astronomy & Astrophysics

Revealing the Local Cosmic Web from Galaxies by Deep Learning

Sungwook E. Hong, Donghui Jeong, Ho Seong Hwang, Juhan Kim

Summary: This study utilized a deep-learning algorithm to reconstruct the structure of the cosmic web from galaxy distributions, providing insights into the distribution of dark matter and warm-hot intergalactic media in the universe.

ASTROPHYSICAL JOURNAL (2021)

Article Astronomy & Astrophysics

Covariance of the matter power spectrum including the survey window function effect: N-body simulations versus fifth-order perturbation theory on grids

Atsushi Taruya, Takahiro Nishimichi, Donghui Jeong

Summary: A higher-order calculation for the covariance matrix of the matter power spectrum is presented, taking into account the effect of survey window functions. The method quickly generates multiple realizations of nonlinear density fields and computes the covariance originating from the one-loop trispectrum without explicitly computing the trispectrum. Comparing with N-body results, the NNLO GridSPT results reproduce well on quasilinear scales, with the survey window function effect incorporated straightforwardly.

PHYSICAL REVIEW D (2021)

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